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{{Short description|A list of systems with multiple planets}} {{Short description|A list of systems with multiple planets}}
{{further|Planetary system}} {{further|Planetary system}}
[[File:Confirmed exoplanets by methods EPE.svg|right|thumb|350px|Number of extrasolar planet discoveries per year through 2021. Colors indicate method of detection. [[File:Confirmed exoplanets by methods EPE.svg|right|thumb|350px|Number of extrasolar planet discoveries per year through 2023. Colors indicate method of detection.
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From the total of {{Extrasolar planet counts|system_count}} stars known to have ] (as of {{Extrasolar planet counts|asof|mdy}}), there are a total of {{Extrasolar planet counts|multiplanetsystem_count}} known multiplanetary systems,<ref name="Encyclopaedia">{{cite encyclopedia|title=Interactive Extra-solar Planets Catalog |encyclopedia=] |url=http://exoplanet.eu/catalog.php |last=Schneider |first=Jean |date=6 December 2016 |access-date=2016-12-06}}</ref> or stars with at least two confirmed planets, beyond the ]. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are ] (the Solar System's star, also referred to as the Sun) and ] with 8 confirmed planets each, followed by ] with 7 planets. From the total of {{Extrasolar planet counts|system_count}} stars known to have ] (as of {{Extrasolar planet counts|asof|mdy}}), there are a total of {{Extrasolar planet counts|multiplanetsystem_count}} known multiplanetary systems,<ref name="Encyclopaedia">{{cite encyclopedia |title=Interactive Extra-solar Planets Catalog |url=https://exoplanet.eu/catalog/ |last=Schneider |first=Jean |date=6 December 2016 |encyclopedia=] |access-date=2016-12-06 |archive-date=2016-12-09 |archive-url=https://web.archive.org/web/20161209220644/http://exoplanet.eu/catalog/ |url-status=live }}</ref> or stars with at least two confirmed planets, beyond the ]. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are the ] (the Solar System's star) and ], with 8 confirmed planets each, followed by ] with 7 planets.


The {{Extrasolar planet counts|multiplanetsystem_count}} multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (], ] and ]). The nearest system with four or more confirmed planets is ], with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 ly away.{{citation needed|date=March 2022}}]] The {{Extrasolar planet counts|multiplanetsystem_count}} multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (], ] and ]). The nearest system with four or more confirmed planets is ], with four known.{{citation needed|date=February 2024}}{{Efn|] at closer distance has a candidate four-planet system, of which one planet has been confirmed so far.<ref>{{cite journal
| title=A sub-Earth-mass planet orbiting Barnard's star
| first1=J. I. | last1=González Hernández | first2=A. | last2=Suárez Mascareño
| first3=A. M. | last3=Silva | first4=A. K. | last4=Stefanov
| first5=J. P. | last5=Faria | first6=H. M. | last6=Tabernero
| first7=A. | last7=Sozzetti | first8=R. | last8=Rebolo
| first9=F. | last9=Pepe | first10=N. C. | last10=Santos
| first11=S. | last11=Cristiani | first12=C. | last12=Lovis
| first13=X. | last13=Dumusque | first14=P. | last14=Figueira
| first15=J. | last15=Lillo-Box | first16=N. | last16=Nari
| first17=S. | last17=Benatti | first18=M. J. | last18=Hobson
| first19=A. | last19=Castro-González | first20=R. | last20=Allart
| first21=V. M. | last21=Passegger | first22=M.-R. | last22=Zapatero Osorio
| first23=V. | last23=Adibekyan | first24=Y. | last24=Alibert
| first25=C. | last25=Allende Prieto | first26=F. | last26=Bouchy
| first27=M. | last27=Damasso | first28=V. | last28=D’Odorico
| first29=P. | last29=Di Marcantonio | first30=D. | last30=Ehrenreich
| first31=G. | last31=Lo Curto | first32=R. | last32=Génova Santos
| first33=C. J. A. P. | last33=Martins | first34=A. | last34=Mehner
| first35=G. | last35=Micela | first36=P. | last36=Molaro
| first37=N. | last37=Nunes15 | first38=E. | last38=Palle
| first39=S. G. | last39=Sousa | first40=S. | last40=Udry
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=690 | id=A79 | date=October 2024
| pages=A79 | doi=10.1051/0004-6361/202451311
| arxiv=2410.00569 | bibcode=2024A&A...690A..79G }}</ref>}} The farthest confirmed multiplanetary system is ], at {{convert|13,300|ly|pc}} away.<ref>{{Cite web |first1=Jean-Philippe |last1=Beaulieu |first2=D. P. |last2=Bennett |first3=Virginie |last3=Batista |first4=A.
|last4=Fukui |date=January 2016 |title=Revisiting the microlensing event OGLE 2012-BLG-0026: A solar mass star with two cold giant planets |url=https://www.researchgate.net/publication/290028818 |website=researchgate.net}}</ref>


The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important ] are ] and ] because they determine how these ]s form. Systems with higher mass and metallicity tend to have more planets and more massive planets.{{citation needed|date=April 2022}} However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 AU.<ref name="JMBrewer2018">{{cite journal |last1=Brewer |first1=John M. |last2=Wang |first2=Songhu |last3=Fischer |first3=Debra A. |last4=Foreman-Mackey |first4=Daniel |title=Compact multi-planet systems are more common around metal poor hosts|journal=The Astrophysical Journal |volume=867 |at=L3 |arxiv=1810.10009 |doi=10.3847/2041-8213/aae710 |date=2018-10-24 |issue=1 |bibcode=2018ApJ...867L...3B |s2cid=67832557 }}</ref> The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important ] are ] and ] because they determine how these ]s form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 AU.<ref name="JMBrewer2018">{{cite journal |last1=Brewer |first1=John M. |last2=Wang |first2=Songhu |last3=Fischer |first3=Debra A. |last4=Foreman-Mackey |first4=Daniel |title=Compact multi-planet systems are more common around metal poor hosts|journal=The Astrophysical Journal |volume=867 |at=L3 |arxiv=1810.10009 |doi=10.3847/2041-8213/aae710 |date=2018-10-24 |issue=1 |bibcode=2018ApJ...867L...3B |s2cid=67832557 |doi-access=free }}</ref>


==Multiplanetary systems== ==Multiplanetary systems==
{{Dynamic list}}
<div style="float: left; margin: 5px;"> <div style="float: left; margin: 5px;">
{| class="wikitable" {| class="wikitable"
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| bgcolor="#f76879" width=30 style="text-align: center" |9 | bgcolor="#f76879" width=30 style="text-align: center" |9
|}</div> |}</div>
<!------ Stars with only one or two planets should not be added here, but at ] instead ---> <!------ Stars with only one planet should not be added here, but at ] instead --->
{{clear}} {{clear}}
{{Multiplanetary systems list/Top}} {{Multiplanetary systems list/Top}}
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| Apparent magnitude = 10.43 to 11.11<ref name="VizieRproximac">{{cite journal |bibcode=2009yCat....102025S |title=VizieR online data catalog: General catalogue of variable stars (Samus+ 2007–2013) |journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S |volume=1 |display-authors=etal |last1=Samus |first1=N. N. |last2=Durlevich |first2=O. V. |year=2009}}</ref> | Apparent magnitude = 10.43 to 11.11<ref name="VizieRproximac">{{cite journal |bibcode=2009yCat....102025S |title=VizieR online data catalog: General catalogue of variable stars (Samus+ 2007–2013) |journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S |volume=1 |display-authors=etal |last1=Samus |first1=N. N. |last2=Durlevich |first2=O. V. |year=2009}}</ref>
| Distance = 4.244 | Distance = 4.244
| Spectral type = M5.5Ve<ref>{{cite journal |bibcode=1991AJ....101..662B |title=The late-M dwarfs |journal=The Astronomical Journal |volume=101 |pages=662 |last1=Bessell |first1=M. S. |year=1991 |doi=10.1086/115714}}</ref> | Spectral type = M5.5Ve<ref>{{cite journal |bibcode=1991AJ....101..662B |title=The late-M dwarfs |journal=The Astronomical Journal |volume=101 |pages=662 |last1=Bessell |first1=M. S. |year=1991 |doi=10.1086/115714|doi-access=free }}</ref>
| Mass = 0.1221 | Mass = 0.1221
| Radius = 0.1542 | Radius = 0.1542
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| Confirmed planets = 2 | Confirmed planets = 2
|Unconfirmed planets = 1 |Unconfirmed planets = 1
| Notes = Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable.<ref name=ProximaESPRESSO>{{cite journal |last1=Mascareño |first1=A. Suárez |last2=Faria |first2=J. P. |last3=Figueira |first3=P. |last4=Lovis |first4=C. |last5=Damasso |first5=M. |last6=Hernández |first6=J. I. González |last7=Rebolo |first7=R. |last8=Cristiani |first8=S. |last9=Pepe |first9=F. |last10=Santos |first10=N. C. |last11=Osorio |first11=M. R. Zapatero |last12=Adibekyan |first12=V. |last13=Hojjatpanah |first13=S. |last14=Sozzetti |first14=A. |last15=Murgas |first15=F. |last16=Abreu |first16=M. |last17=Affolter |first17=M. |last18=Alibert |first18=Y. |last19=Aliverti |first19=M. |last20=Allart |first20=R. |last21=Prieto |first21=C. Allende |last22=Alves |first22=D. |last23=Amate |first23=M. |last24=Avila |first24=G. |last25=Baldini |first25=V. |last26=Bandi |first26=T. |last27=Barros |first27=S. C. C. |last28=Bianco |first28=A. |last29=Benz |first29=W. |last30=Bouchy |first30=F. |last31=Broeng |first31=C. |last32=Cabral |first32=A. |last33=Calderone |first33=G. |last34=Cirami |first34=R. |last35=Coelho |first35=J. |last36=Conconi |first36=P. |last37=Coretti |first37=I. |last38=Cumani |first38=C. |last39=Cupani |first39=G. |last40=D’Odorico |first40=V. |last41=Deiries |first41=S. |last42=Delabre |first42=B. |last43=Marcantonio |first43=P. Di |last44=Dumusque |first44=X. |last45=Ehrenreich |first45=D. |last46=Fragoso |first46=A. |last47=Genolet |first47=L. |last48=Genoni |first48=M. |last49=Santos |first49=R. Génova |last50=Hughes |first50=I. |last51=Iwert |first51=O. |last52=Kerber |first52=F. |last53=Knusdstrup |first53=J. |last54=Landoni |first54=M. |last55=Lavie |first55=B. |last56=Lillo-Box |first56=J. |last57=Lizon |first57=J. |last58=Curto |first58=G. Lo |last59=Maire |first59=C. |last60=Manescau |first60=A. |last61=Martins |first61=C. J. a. P. |last62=Mégevand |first62=D. |last63=Mehner |first63=A. |last64=Micela |first64=G. |last65=Modigliani |first65=A. |last66=Molaro |first66=P. |last67=Monteiro |first67=M. A. |last68=Monteiro |first68=M. J. P. F. G. |last69=Moschetti |first69=M. |last70=Mueller |first70=E. |last71=Nunes |first71=N. J. |last72=Oggioni |first72=L. |last73=Oliveira |first73=A. |last74=Pallé |first74=E. |last75=Pariani |first75=G. |last76=Pasquini |first76=L. |last77=Poretti |first77=E. |last78=Rasilla |first78=J. L. |last79=Redaelli |first79=E. |last80=Riva |first80=M. |last81=Tschudi |first81=S. Santana |last82=Santin |first82=P. |last83=Santos |first83=P. |last84=Segovia |first84=A. |last85=Sosnowska |first85=D. |last86=Sousa |first86=S. |last87=Spanò |first87=P. |last88=Tenegi |first88=F. |last89=Udry |first89=S. |last90=Zanutta |first90=A. |last91=Zerbi |first91=F. |title=Revisiting Proxima with ESPRESSO |journal=Astronomy & Astrophysics |date=1 July 2020 |volume=639 |pages=A77 |doi=10.1051/0004-6361/202037745 |arxiv=2005.12114 |bibcode=2020A&A...639A..77S |s2cid=218869742 |url=https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |language=en |issn=0004-6361}}</ref><ref>{{cite journal |last1=Del Genio |first1=Anthony D. |last2=Way |first2=Michael J. |last3=Amundsen |first3=David S. |last4=Aleinov |first4=Igor |last5=Kelley |first5=Maxwell |last6=Kiang |first6=Nancy Y. |last7=Clune |first7=Thomas L. |title=Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean |journal=Astrobiology |date=January 2019 |volume=19 |issue=1 |pages=99–125 |doi=10.1089/ast.2017.1760 |pmid=30183335 |arxiv=1709.02051 |bibcode=2019AsBio..19...99D |s2cid=52165056 |url=https://www.liebertpub.com/doi/full/10.1089/ast.2017.1760 |issn=1531-1074}}</ref> Planet c initially appeared likely but has since been disputed.<ref name="Artigau2022">{{cite journal|last1=Artigau|first1=Étienne|last2=Cadieux|first2=Charles|last3=Cook|first3=Neil J.|last4=Doyon|first4=René|last5=Vandal|first5=Thomas|last6=Donati|first6=Jean-Françcois|last7=Moutou|first7=Claire|last8=Delfosse|first8=Xavier|last9=Fouqué|first9=Pascal|last10=Martioli|first10=Eder|last11=Bouchy|first11=François|last12=Parsons|first12=Jasmine|last13=Carmona|first13=Andres|last14=Dumusque|first14=Xavier|last15=Astudillo-Defru|first15=Nicola|last16=Bonfils|first16=Xavier|last17=Mignon|first17=Lucille|display-authors=5|title=Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry|journal=The Astronomical Journal|volume=164:84|issue=3|pages=18pp|arxiv=2207.13524|bibcode=2022AJ....164...84A|doi=10.3847/1538-3881/ac7ce6|doi-access=free|date=June 23, 2022|publication-date=August 8, 2022}}</ref> | Notes = Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable.<ref name=ProximaESPRESSO>{{cite journal |last1=Mascareño |first1=A. Suárez |last2=Faria |first2=J. P. |last3=Figueira |first3=P. |last4=Lovis |first4=C. |last5=Damasso |first5=M. |last6=Hernández |first6=J. I. González |last7=Rebolo |first7=R. |last8=Cristiani |first8=S. |last9=Pepe |first9=F. |last10=Santos |first10=N. C. |last11=Osorio |first11=M. R. Zapatero |last12=Adibekyan |first12=V. |last13=Hojjatpanah |first13=S. |last14=Sozzetti |first14=A. |last15=Murgas |first15=F. |last16=Abreu |first16=M. |last17=Affolter |first17=M. |last18=Alibert |first18=Y. |last19=Aliverti |first19=M. |last20=Allart |first20=R. |last21=Prieto |first21=C. Allende |last22=Alves |first22=D. |last23=Amate |first23=M. |last24=Avila |first24=G. |last25=Baldini |first25=V. |last26=Bandi |first26=T. |last27=Barros |first27=S. C. C. |last28=Bianco |first28=A. |last29=Benz |first29=W. |last30=Bouchy |first30=F. |last31=Broeng |first31=C. |last32=Cabral |first32=A. |last33=Calderone |first33=G. |last34=Cirami |first34=R. |last35=Coelho |first35=J. |last36=Conconi |first36=P. |last37=Coretti |first37=I. |last38=Cumani |first38=C. |last39=Cupani |first39=G. |last40=D’Odorico |first40=V. |last41=Deiries |first41=S. |last42=Delabre |first42=B. |last43=Marcantonio |first43=P. Di |last44=Dumusque |first44=X. |last45=Ehrenreich |first45=D. |last46=Fragoso |first46=A. |last47=Genolet |first47=L. |last48=Genoni |first48=M. |last49=Santos |first49=R. Génova |last50=Hughes |first50=I. |last51=Iwert |first51=O. |last52=Kerber |first52=F. |last53=Knusdstrup |first53=J. |last54=Landoni |first54=M. |last55=Lavie |first55=B. |last56=Lillo-Box |first56=J. |last57=Lizon |first57=J. |last58=Curto |first58=G. Lo |last59=Maire |first59=C. |last60=Manescau |first60=A. |last61=Martins |first61=C. J. a. P. |last62=Mégevand |first62=D. |last63=Mehner |first63=A. |last64=Micela |first64=G. |last65=Modigliani |first65=A. |last66=Molaro |first66=P. |last67=Monteiro |first67=M. A. |last68=Monteiro |first68=M. J. P. F. G. |last69=Moschetti |first69=M. |last70=Mueller |first70=E. |last71=Nunes |first71=N. J. |last72=Oggioni |first72=L. |last73=Oliveira |first73=A. |last74=Pallé |first74=E. |last75=Pariani |first75=G. |last76=Pasquini |first76=L. |last77=Poretti |first77=E. |last78=Rasilla |first78=J. L. |last79=Redaelli |first79=E. |last80=Riva |first80=M. |last81=Tschudi |first81=S. Santana |last82=Santin |first82=P. |last83=Santos |first83=P. |last84=Segovia |first84=A. |last85=Sosnowska |first85=D. |last86=Sousa |first86=S. |last87=Spanò |first87=P. |last88=Tenegi |first88=F. |last89=Udry |first89=S. |last90=Zanutta |first90=A. |last91=Zerbi |first91=F. |title=Revisiting Proxima with ESPRESSO |journal=Astronomy & Astrophysics |date=1 July 2020 |volume=639 |pages=A77 |doi=10.1051/0004-6361/202037745 |arxiv=2005.12114 |bibcode=2020A&A...639A..77S |s2cid=218869742 |url=https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |language=en |issn=0004-6361 |access-date=9 May 2022 |archive-date=27 June 2022 |archive-url=https://web.archive.org/web/20220627141045/https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |url-status=live }}</ref><ref>{{cite journal |last1=Del Genio |first1=Anthony D. |last2=Way |first2=Michael J. |last3=Amundsen |first3=David S. |last4=Aleinov |first4=Igor |last5=Kelley |first5=Maxwell |last6=Kiang |first6=Nancy Y. |last7=Clune |first7=Thomas L. |title=Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean |journal=Astrobiology |date=January 2019 |volume=19 |issue=1 |pages=99–125 |doi=10.1089/ast.2017.1760 |pmid=30183335 |arxiv=1709.02051 |bibcode=2019AsBio..19...99D |s2cid=52165056 |url=https://www.liebertpub.com/doi/full/10.1089/ast.2017.1760 |issn=1531-1074}}</ref> Planet c initially appeared likely but has since been disputed.<ref name="Artigau2022">{{cite journal|last1=Artigau|first1=Étienne|last2=Cadieux|first2=Charles|last3=Cook|first3=Neil J.|last4=Doyon|first4=René|last5=Vandal|first5=Thomas|last6=Donati|first6=Jean-Françcois|last7=Moutou|first7=Claire|last8=Delfosse|first8=Xavier|last9=Fouqué|first9=Pascal|last10=Martioli|first10=Eder|last11=Bouchy|first11=François|last12=Parsons|first12=Jasmine|last13=Carmona|first13=Andres|last14=Dumusque|first14=Xavier|last15=Astudillo-Defru|first15=Nicola|last16=Bonfils|first16=Xavier|last17=Mignon|first17=Lucille|display-authors=5|title=Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry|journal=The Astronomical Journal|volume=164:84|issue=3|pages=18pp|arxiv=2207.13524|bibcode=2022AJ....164...84A|doi=10.3847/1538-3881/ac7ce6|doi-access=free|date=June 23, 2022|publication-date=August 8, 2022}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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| date =2015-12-23 | date =2015-12-23
| publisher =Universe Today | publisher =Universe Today
| access-date =2016-12-04}}</ref><ref>{{cite web | access-date =2016-12-04
| archive-date =2021-02-11
| archive-url =https://web.archive.org/web/20210211185356/https://www.universetoday.com/111716/14-red-dwarf-stars-to-view-with-backyard-telescopes/
| url-status =live
}}</ref><ref>{{cite web
| url =http://kencroswell.com/thebrightestreddwarf.html | url =http://kencroswell.com/thebrightestreddwarf.html
| title =The Brightest Red Dwarf | title =The Brightest Red Dwarf
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| date =July 2002 | date =July 2002
| website =KenCroswell.com | website =KenCroswell.com
| access-date =2016-12-04}}</ref> | access-date =2016-12-04
| archive-date =2018-10-20
| archive-url =https://web.archive.org/web/20181020223954/http://www.kencroswell.com/thebrightestreddwarf.html
| url-status =live
}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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|volume=641 |pages=A23 |volume=641 |pages=A23
|doi=10.1051/0004-6361/202038047 |arxiv=2006.09403 |doi=10.1051/0004-6361/202038047 |arxiv=2006.09403
|bibcode=2020A&A...641A..23P |s2cid=219721292 |quote=<span style="font-family:LatinModern;"><small>GJ 273 is a planetary system orbiting an M&nbsp;dwarf only 3.75&nbsp;pc away, composed of two confirmed planets, GJ&nbsp;273b and GJ&nbsp;273c, and two promising candidates, GJ&nbsp;273d and GJ&nbsp;273e ... the system remained stable only for values of inclinations ranging from 90◦ to ∼72◦</small></span> |bibcode=2020A&A...641A..23P |s2cid=219721292 |quote=<span style="font-family:LatinModern;"><small>GJ 273 is a planetary system orbiting an M&nbsp;dwarf only 3.75&nbsp;pc away, composed of two confirmed planets, GJ&nbsp;273b and GJ&nbsp;273c, and two promising candidates, GJ&nbsp;273d and GJ&nbsp;273e ... the system remained stable only for values of inclinations ranging from 90◦ to ~72◦</small></span>
}} }}
</ref> Planet b is potentially habitable.<ref name="Astudillo-Defru2017">{{cite journal | doi=10.1051/0004-6361/201630153 </ref> Planet b is potentially habitable.<ref name="Astudillo-Defru2017">{{cite journal
|doi = 10.1051/0004-6361/201630153
|last1 = Astudillo-Defru
| last1=Astudillo-Defru | first1=Nicola | last2=Forveille | first2=Thierry
|first1 = Nicola
| last3=Bonfils | first3=Xavier | last4=Ségransan | first4=Damien
|last2 = Forveille
| last5=Bouchy | first5=François | last6=Delfosse | first6=Xavier
|first2 = Thierry
| last7=Lovis | first7=Christophe | last8=Mayor | first8=Michel
|last3 = Bonfils
| last9=Murgas | first9=Felipe | last10=Pepe | first10=Francesco
|first3 = Xavier
| last11=Santos | first11=Nuno C. | last12=Udry | first12=Stéphane
|last4 = Ségransan
| last13=Wünsche | first13=Anaël | display-authors=6
|first4 = Damien
| year=2017
|last5 = Bouchy
| title=The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
|first5 = François
| journal=Astronomy and Astrophysics
|last6 = Delfosse
| volume=602 | at=A88
|first6 = Xavier
| arxiv=1703.05386 | bibcode=2017A&A...602A..88A | s2cid=119418595
|last7 = Lovis
| url=https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|first7 = Christophe
}}
|last8 = Mayor
</ref>
|first8 = Michel
|last9 = Murgas
|first9 = Felipe
|last10 = Pepe
|first10 = Francesco
|last11 = Santos
|first11 = Nuno C.
|last12 = Udry
|first12 = Stéphane
|last13 = Wünsche
|first13 = Anaël
|display-authors = 6
|year = 2017
|title = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
|journal = Astronomy and Astrophysics
|volume = 602
|at = A88
|arxiv = 1703.05386
|bibcode = 2017A&A...602A..88A
|s2cid = 119418595
|url = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|access-date = 2022-02-25
|archive-date = 2022-09-28
|archive-url = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|url-status = live
}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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|Unconfirmed planets = 1 |Unconfirmed planets = 1
| Notes = Flare star.<ref name=gcvsyzceti>{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}</ref> | Notes = Flare star.<ref name=gcvsyzceti>{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}</ref>
}}
{{Multiplanetary systems list
| Star = Tau Ceti
| Constellation = Cetus
| Right ascension = {{RA|01|44|05.13}}
| Declination = {{DEC|−15|56|22.4}}
| Apparent magnitude = 3.49
| Distance = 11.905
| Spectral type = G8V
| Mass = 0.783
| Radius = 0.793
| Temperature = 5344
| Metallicity = -0.55
| Age = 5.8
| Confirmed planets = 4
|Unconfirmed planets = 4
| Notes = Were planets b, c, d, i, PxP-4 and PxP-5 confirmed, would have a total of 10 planets. <ref name="Dietrich Apai 2020">{{cite journal|last1=Dietrich|first1=Jeremy|last2=Apai | first2=Dániel |author-link2=Daniel Apai|title=An Integrated Analysis with Predictions on the Architecture of the tau Ceti Planetary System, Including a Habitable Zone Planet|journal=The Astronomical Journal|arxiv=2010.14675|date=2020-10-27|volume=161|page=17|doi=10.3847/1538-3881/abc560|s2cid=225094415}}</ref>Planets e and f are potentially habitable, but the habitability of e is disputed.<ref name=TauCetiHabitable>{{Cite web|title=Two Nearby Habitable Worlds? - Planetary Habitability Laboratory @ UPR Arecibo|url=http://phl.upr.edu/press-releases/twonearbyhabitableworlds|access-date=2020-10-07|website=phl.upr.edu}}</ref><ref>{{Cite web|title=Four Exoplanets Detected around Nearby Star Tau Ceti {{!}} Astronomy {{!}} Sci-News.com|url=http://www.sci-news.com/astronomy/tau-ceti-exoplanets-05117.html|access-date=2020-10-07|website=Breaking Science News {{!}} Sci-News.com|language=en-US}}</ref><ref>{{Cite journal|last1=Feng|first1=Fabo|last2=Tuomi|first2=Mikko|last3=Jones|first3=Hugh R. A.|last4=Barnes|first4=John|last5=Anglada-Escude|first5=Guillem|last6=Vogt|first6=Steven S.|last7=Butler|first7=R. Paul|date=2017-09-05|title=Color difference makes a difference: four planet candidates around tau Ceti|journal=The Astronomical Journal|volume=154|issue=4|pages=135|doi=10.3847/1538-3881/aa83b4|arxiv=1708.02051|bibcode=2017AJ....154..135F|s2cid=53500995|issn=1538-3881}}</ref><ref>{{Cite book|last1=Guedel|first1=M.|last2=Dvorak|first2=R.|last3=Erkaev|first3=N.|last4=Kasting|first4=J.|last5=Khodachenko|first5=M.|last6=Lammer|first6=H.|last7=Pilat-Lohinger|first7=E.|last8=Rauer|first8=H.|last9=Ribas|first9=I.|last10=Wood|first10=B. E.|title=Protostars and Planets VI|date=2014|chapter=Astrophysical Conditions for Planetary Habitability|doi=10.2458/azu_uapress_9780816531240-ch038|arxiv=1407.8174|isbn=9780816531240|s2cid=118447677}}</ref> Closest system to the Sun with exactly four confirmed planets, and closest ] to the Sun with confirmed exoplanets.<ref>{{cite web
| last=Henry | first=Todd J.
| date=October 1, 2006
| url=http://www.chara.gsu.edu/RECONS/TOP100.htm
| title=The One Hundred Nearest Star Systems
| publisher=Research Consortium on Nearby Stars
| access-date=2006-12-11 | archive-url = https://web.archive.org/web/20061128221321/http://www.chara.gsu.edu/RECONS/TOP100.htm| archive-date = November 28, 2006}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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|last18=Reiners |first18=Ansgar |last18=Reiners |first18=Ansgar
|last19=Anglada-Escudé |first19=G. |last19=Anglada-Escudé |first19=G.
|date=2019-08-13 |title=Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061 |doi=10.1093/mnras/staa248 |arxiv=1908.04717| s2cid=199551874 |language=en}}</ref> |date=2019-08-13 |title=Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061 |volume=493 |issue=1 |pages=536–550 |doi=10.1093/mnras/staa248 |doi-access=free |arxiv=1908.04717| s2cid=199551874 |language=en}}</ref>
}} }}
{{Multiplanetary systems list
| Star = ]
| Constellation = Aries (constellation){{!}}Aries
| Right ascension = {{RA|02|53|00.89}}
| Declination = {{DEC|+16|52|53}}
| Apparent magnitude = 15.13
| Distance = 12.497
| Spectral type = M7V
| Mass = 0.097
| Radius = 0.120
| Temperature = 3034
| Metallicity = -0.11±0.28
| Age = 8
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Teegarden's Star b and Teegarden's Star c are likely Earth-mass planets that orbit in the habitable zone.<ref name="CARMENES">{{cite journal |last1=Caballero |first1=J. A. |last2=Reiners |first2=Ansgar |last3=Ribas |first3=I. |last4=Dreizler |first4=S. |last5=Zechmeister |first5=M. |display-authors=etal |date=12 June 2019 |title=The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star |journal=Astronomy & Astrophysics |volume=627 |pages=A49 |language=en |doi=10.1051/0004-6361/201935460 |arxiv=1906.07196 |issn=0004-6361 |bibcode=2019A&A...627A..49Z |s2cid=189999121 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = Wolf 1061 | Star = Wolf 1061
Line 259: Line 313:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet c is potentially habitable.<ref name="unswpaper">{{cite journal |last1=Davison |first1=Cassy L. |last2=White |first2=Russel J. |last3=Henry |first3=Todd J. |last4=Riedel |first4=Adric R. |last5=Jao |first5=Wei-Chun |last6=Bailey III |first6=John I. |last7=Quinn |first7=Samuel N. |last8=Justin R. |first8=Cantrell |last9=John P. |first9=Subasavage |last10=Jen G. |first10=Winters |title=A 3D Search for Companions to 12 Nearby M-Dwarfs |year=2015 |arxiv=1501.05012 |doi=10.1088/0004-6256/149/3/106 |volume=149 |issue=3 |journal=The Astronomical Journal |page=106|bibcode = 2015AJ....149..106D |s2cid=9719725 }}</ref><ref>{{cite web|author=Stuart Gary |url=http://www.abc.net.au/news/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824 |title=Potentially habitable super-Earth discovered orbiting star 14 light years from Earth|publisher=ABC News (Australia)|date=17 December 2015}}</ref><ref name=Wolf1061kane>{{citation | Notes = Planet c is potentially habitable.<ref name="unswpaper">{{cite journal |last1=Davison |first1=Cassy L. |last2=White |first2=Russel J. |last3=Henry |first3=Todd J. |last4=Riedel |first4=Adric R. |last5=Jao |first5=Wei-Chun |last6=Bailey III |first6=John I. |last7=Quinn |first7=Samuel N. |last8=Justin R. |first8=Cantrell |last9=John P. |first9=Subasavage |last10=Jen G. |first10=Winters |title=A 3D Search for Companions to 12 Nearby M-Dwarfs |year=2015 |arxiv=1501.05012 |doi=10.1088/0004-6256/149/3/106 |volume=149 |issue=3 |journal=The Astronomical Journal |page=106|bibcode = 2015AJ....149..106D |s2cid=9719725 }}</ref><ref>{{cite web|author=Stuart Gary|url=http://www.abc.net.au/news/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|title=Potentially habitable super-Earth discovered orbiting star 14 light years from Earth|publisher=ABC News (Australia)|date=17 December 2015|access-date=2022-05-10|archive-date=2017-06-09|archive-url=https://web.archive.org/web/20170609122527/http://www.abc.net.au/news/science/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|url-status=live}}</ref><ref name=Wolf1061kane>{{citation
| title=Characterization of the Wolf 1061 Planetary System | title=Characterization of the Wolf 1061 Planetary System
| last1=Kane | first1=Stephen R. | last2=von Braun | first2=Kaspar | last1=Kane | first1=Stephen R. | last2=von Braun | first2=Kaspar
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| volume=835 | issue=2 | id=200 | pages=9 | date=February 2017 | volume=835 | issue=2 | id=200 | pages=9 | date=February 2017
| doi=10.3847/1538-4357/835/2/200 | bibcode=2017ApJ...835..200K | doi=10.3847/1538-4357/835/2/200 | bibcode=2017ApJ...835..200K
| arxiv=1612.09324 | s2cid=30738573 | postscript=. }}</ref> | arxiv=1612.09324 | s2cid=30738573 | postscript=. | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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|volume=424 |issue=2 |pages=1206 |title = Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems |volume=424 |issue=2 |pages=1206 |title = Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
|arxiv = 1206.2370 | doi=10.1111/j.1365-2966.2012.21298.x |arxiv = 1206.2370 | doi=10.1111/j.1365-2966.2012.21298.x
|bibcode=2012MNRAS.424.1206W |s2cid=54056835 }}</ref> with a semi-major axis at approximately 19 AU.<ref name="Kennedy_2015">{{Cite journal | doi = 10.1093/mnras/stv511| title = Kuiper belt structure around nearby super-Earth host stars| journal = Monthly Notices of the Royal Astronomical Society| volume = 449| issue = 3| pages = 3121| year = 2015| last1 = Kennedy | first1 = G. M.| last2 = Matra | first2 = L.| last3 = Marmier | first3 = M.| last4 = Greaves | first4 = J. S.| last5 = Wyatt | first5 = M. C.| last6 = Bryden | first6 = G.| last7 = Holland | first7 = W.| last8 = Lovis | first8 = C.| last9 = Matthews | first9 = B. C.| last10 = Pepe | first10 = F.| last11 = Sibthorpe | first11 = B.| last12 = Udry | first12 = S.|arxiv = 1503.02073 |bibcode = 2015MNRAS.449.3121K | s2cid = 53638901}}</ref> |doi-access=free |bibcode=2012MNRAS.424.1206W |s2cid=54056835 }}</ref> with a semi-major axis at approximately 19 AU.<ref name="Kennedy_2015">{{Cite journal | doi = 10.1093/mnras/stv511| title = Kuiper belt structure around nearby super-Earth host stars| journal = Monthly Notices of the Royal Astronomical Society| volume = 449| issue = 3| pages = 3121| year = 2015| last1 = Kennedy | first1 = G. M.| last2 = Matra | first2 = L.| last3 = Marmier | first3 = M.| last4 = Greaves | first4 = J. S.| last5 = Wyatt | first5 = M. C.| last6 = Bryden | first6 = G.| last7 = Holland | first7 = W.| last8 = Lovis | first8 = C.| last9 = Matthews | first9 = B. C.| last10 = Pepe | first10 = F.| last11 = Sibthorpe | first11 = B.| last12 = Udry | first12 = S.| doi-access = free|arxiv = 1503.02073 |bibcode = 2015MNRAS.449.3121K | s2cid = 53638901}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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| Age = 4.326 | Age = 4.326
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = 2 |Unconfirmed planets = 1
| Notes = The unconfirmed planets d and g are potentially habitable.<ref name="AstronomyNowGliese581">{{cite news |title=Reanalysis of data suggests 'habitable' planet GJ 581d really could exist |url=http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |date=9 March 2015 |work=] |access-date=27 May 2015 }}</ref> | Notes = The disputed planet d is potentially habitable.<ref name="AstronomyNowGliese581">{{cite news |title=Reanalysis of data suggests 'habitable' planet GJ 581d really could exist |url=http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |date=9 March 2015 |work=] |access-date=27 May 2015 |archive-date=20 May 2015 |archive-url=https://web.archive.org/web/20150520175016/http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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| Confirmed planets = 6 | Confirmed planets = 6
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Closest star to the Sun with exactly six<ref name="Vogt2015HD219134">{{cite journal |arxiv=1509.07912 |last1=Vogt |first1=Steven S. |display-authors=etal |title=Six Planets Orbiting HD 219134 |date=November 2015 |doi=10.1088/0004-637X/814/1/12 |volume=814 |issue=1 |journal=] |page=12 |bibcode=2015ApJ...814...12V|s2cid=45438051 }}</ref> exoplanets, and closest ] to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.<ref>{{cite journal |author-link= |arxiv=2112.05337 |title= An Integrative Analysis of the HD 219134 Planetary System and the Inner solar system: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria|last1= Dietrich|first1= Jeremy|last2= Apai|first2= Dániel|last3= Malhotra|first3= Renu|journal=The Astronomical Journal |year= 2022|volume=163 |issue=2 |page=88 |doi=10.3847/1538-3881/ac4166 |bibcode=2022AJ....163...88D |s2cid=245117944 }}</ref> | Notes = Closest star to the Sun with exactly six<ref name="Vogt2015HD219134">{{cite journal |arxiv=1509.07912 |last1=Vogt |first1=Steven S. |display-authors=etal |title=Six Planets Orbiting HD 219134 |date=November 2015 |doi=10.1088/0004-637X/814/1/12 |volume=814 |issue=1 |journal=] |page=12 |bibcode=2015ApJ...814...12V|s2cid=45438051 }}</ref> exoplanets, and closest ] to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.<ref>{{cite journal |author-link= |arxiv=2112.05337 |title= An Integrative Analysis of the HD 219134 Planetary System and the Inner solar system: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria|last1= Dietrich|first1= Jeremy|last2= Apai|first2= Dániel|last3= Malhotra|first3= Renu|journal=The Astronomical Journal |year= 2022|volume=163 |issue=2 |page=88 |doi=10.3847/1538-3881/ac4166 |bibcode=2022AJ....163...88D |s2cid=245117944 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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| Confirmed planets = 2 | Confirmed planets = 2
|Unconfirmed planets = 1 |Unconfirmed planets = 1
| Notes = Planet d remains unconfirmed,<ref name=debris61Vir>{{Cite journal | last1=Wyatt | first1=M. C. | last2=Kennedy | first2=G. | last3=Sibthorpe | first3=B. | last4=Moro-Martín | first4=A. | last5=Lestrade | first5=J.-F. | last6=Ivison | first6=R. J. | last7=Matthews | first7=B. | last8=Udry | first8=S. | last9=Greaves | first9=J. S. | last10=Kalas | first10=P. | last11=Lawler | first11=S. | last12=Su | first12=K. Y. L. | last13=Rieke | first13=G. H. | last14=Booth | first14=M. | last15=Bryden | first15=G. | last16=Horner | first16=J. | last17=Kavelaars | first17=J. J. | last18=Wilner | first18=D. | display-authors=1 | title=Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems | journal=MNRAS | date=2012 | bibcode = 2012MNRAS.424.1206W | doi = 10.1111/j.1365-2966.2012.21298.x | arxiv=1206.2370 | volume=424 | issue=2 | pages=1206–1223| s2cid=54056835 }}</ref> and a 2021 study found that it was likely a false positive.<ref name=Rosenthal2021_61VirD>{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973}}</ref> 61 Virginis also has a debris disk. | Notes = Planet d remains unconfirmed,<ref name=debris61Vir>{{Cite journal | last1=Wyatt | first1=M. C. | last2=Kennedy | first2=G. | last3=Sibthorpe | first3=B. | last4=Moro-Martín | first4=A. | last5=Lestrade | first5=J.-F. | last6=Ivison | first6=R. J. | last7=Matthews | first7=B. | last8=Udry | first8=S. | last9=Greaves | first9=J. S. | last10=Kalas | first10=P. | last11=Lawler | first11=S. | last12=Su | first12=K. Y. L. | last13=Rieke | first13=G. H. | last14=Booth | first14=M. | last15=Bryden | first15=G. | last16=Horner | first16=J. | last17=Kavelaars | first17=J. J. | last18=Wilner | first18=D. | display-authors=1 | title=Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems | journal=MNRAS | date=2012 | bibcode = 2012MNRAS.424.1206W | doi = 10.1111/j.1365-2966.2012.21298.x | arxiv=1206.2370 | volume=424 | issue=2 | pages=1206–1223| doi-access=free | s2cid=54056835 }}</ref> and a 2021 study found that it was likely a false positive.<ref name=Rosenthal2021_61VirD>{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973 |doi-access=free }}</ref> 61 Virginis also has a debris disk.
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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| journal=Monthly Notices of the Royal Astronomical Society | journal=Monthly Notices of the Royal Astronomical Society
| volume=476 | issue=4 | pages=4584–4591 | date=June 2018 | volume=476 | issue=4 | pages=4584–4591 | date=June 2018
| doi=10.1093/mnras/sty492 | arxiv=1803.02832 | doi=10.1093/mnras/sty492 | doi-access=free | arxiv=1803.02832
| bibcode=2018MNRAS.476.4584K }}</ref> | bibcode=2018MNRAS.476.4584K }}</ref>
}} }}
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| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet d is a potentially habitable Super-Earth.<ref>Falconer, Rebecca, '''', Axios, August 1, 2019</ref><ref name="TESSGliese357d">{{Cite web|url=https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|title=TESS Discovers Habitable Zone Planet in GJ 357 System|last1=Reddy|first1=Francis|last2=Center|first2=NASA’s Goddard Space Flight|date=2019-07-31|website=SciTechDaily|language=en-US|access-date=2019-08-01}}</ref><ref>{{Cite web|url=https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|title=Potentially habitable 'super-Earth' discovered just 31 light-years away|website=NBC News|language=en|access-date=2019-08-01}}</ref><ref>{{Cite web|url=http://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world|title=NASA's TESS Helps Find Intriguing New World|last=Garner|first=Rob|date=2019-07-30|website=NASA|access-date=2019-08-01}}</ref> | Notes = Planet d is a potentially habitable Super-Earth.<ref>Falconer, Rebecca, '' {{Webarchive|url=https://web.archive.org/web/20191218061126/https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html |date=2019-12-18 }}'', Axios, August 1, 2019</ref><ref name="TESSGliese357d">{{Cite web|url=https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|title=TESS Discovers Habitable Zone Planet in GJ 357 System|last1=Reddy|first1=Francis|last2=Center|first2=NASA’s Goddard Space Flight|date=2019-07-31|website=SciTechDaily|language=en-US|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801162521/https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|url-status=live}}</ref><ref>{{Cite web|url=https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|title=Potentially habitable 'super-Earth' discovered just 31 light-years away|website=NBC News|date=31 July 2019|language=en|access-date=2019-08-01|archive-date=2019-07-31|archive-url=https://web.archive.org/web/20190731230808/https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|url-status=live}}</ref><ref>{{Cite web|url=http://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world|title=NASA's TESS Helps Find Intriguing New World|last=Garner|first=Rob|date=2019-07-30|website=NASA|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801045621/https://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world/|url-status=live}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = ] | Star = ]
| Constellation = Volans (constellation){{!}}Volans | Constellation = Volans
| Right ascension = {{RA|08|18|07.62}} | Right ascension = {{RA|08|18|07.62}}
| Declination = {{DEC|-68|18|46.8}} | Declination = {{DEC|-68|18|46.8}}
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| Notes = The unconfirmed planet f orbits in the habitable zone.<ref name="Demangeon2021L98-59">{{cite journal | Notes = The unconfirmed planet f orbits in the habitable zone.<ref name="Demangeon2021L98-59">{{cite journal
|display-authors = etal |display-authors = etal
|first1 = Oliver D. S. |last1 = Demangeon |first1 = Oliver D. S.
|last1 = Demangeon
|first2 = M. R. |last2 = Zapatero Osorio |first2 = M. R.
|last2 = Zapatero Osorio
|first3 = Y. |last3 = Alibert |first3 = Y.
|last3 = Alibert
|first4 = S. C. C. |last4 = Barros |first4 = S. C. C.
|last4 = Barros
|first5 = V. |last5 = Adibekyan |first5 = V.
|last5 = Adibekyan
|first6 = H. M. |last6 = Tabernero |first6 = H. M.
|last6 = Tabernero
|title = A warm terrestrial planet with half the mass of Venus transiting a nearby star |title = A warm terrestrial planet with half the mass of Venus transiting a nearby star
|url = https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf |url = https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
|date = July 2021 |date = July 2021
|journal = Astronomy & Astrophysics |journal = Astronomy & Astrophysics
|volume = 653 |pages = 38 |volume = 653
|pages = 38
|doi = 10.1051/0004-6361/202140728|s2cid = 236957385 |arxiv = 2108.03323 |doi = 10.1051/0004-6361/202140728
|s2cid = 236957385
|arxiv = 2108.03323
|bibcode = 2021A&A...653A..41D }}</ref> |bibcode = 2021A&A...653A..41D
|access-date = 2022-03-03
|archive-date = 2021-11-13
|archive-url = https://web.archive.org/web/20211113184620/https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
|url-status = live
}}</ref>
}}
{{Multiplanetary systems list
| Star = ] A
| Constellation = Ursa Major
| Right ascension = {{RA|11|11|05.88}}
| Declination = {{DEC|30|26|42.61}}
| Apparent magnitude = 8.31
| Distance = 38.76
| Spectral type = K7V
| Mass = 0.65
| Radius = 0.679
| Temperature = 4120
| Metallicity = 0.24
| Age = 12.4
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes = <ref>{{Cite journal |last1=Dedrick |first1=Cayla M. |last2=Fulton |first2=Benjamin J. |last3=Knutson |first3=Heather A. |last4=Howard |first4=Andrew W. |last5=Beatty |first5=Thomas G. |last6=Cargile |first6=Phillip A. |last7=Gaudi |first7=B. Scott |last8=Hirsch |first8=Lea A. |last9=Kuhn |first9=Rudolf B. |last10=Lund |first10=Michael B. |last11=James |first11=David J. |last12=Kosiarek |first12=Molly R. |last13=Pepper |first13=Joshua |last14=Petigura |first14=Erik A. |last15=Rodriguez |first15=Joseph E. |date=January 2021 |title=Two Planets Straddling the Habitable Zone of the Nearby K Dwarf Gl 414A |journal=The Astronomical Journal |language=en |volume=161 |issue=2 |pages=86 |doi=10.3847/1538-3881/abd0ef |doi-access=free |arxiv=2009.06503 |bibcode=2021AJ....161...86D |issn=1538-3881}}</ref><ref>{{Cite web |title=GJ 414 Overview |url=https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |access-date=January 4, 2024 |website=NASA Exoplanet Archive |archive-date=December 9, 2023 |archive-url=https://web.archive.org/web/20231209091347/https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = 55 Cancri | Star = 55 Cancri|Copernicus
| Constellation = Cancer (constellation){{!}}Cancer | Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|52|35.81}} | Right ascension = {{RA|08|52|35.81}}
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| journal=] | journal=]
| volume=92 | pages=139–165 | date=July 1986 | volume=92 | pages=139–165 | date=July 1986
| bibcode=1986AJ.....92..139S | doi=10.1086/114146 }}</ref> | bibcode=1986AJ.....92..139S | doi=10.1086/114146 | doi-access=free }}</ref>
| Mass = 0.39 | Mass = 0.39
| Radius = 0.42 | Radius = 0.42
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| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = The habitability of planets b and c is disputed.<ref>{{cite news | last=Sutherland | first=Paul | date=March 5, 2014 | title=Habitable planets common around red dwarf stars | url=http://sen.com/news/habitable-planets-common-around-red-dwarf-stars | website=Sen | publisher=Sen Corporation Ltd. | access-date=July 28, 2022 | archive-date=November 12, 2020 | archive-url=https://web.archive.org/web/20201112041601/https://www.sen.com/news/habitable-planets-common-around-red-dwarf-stars | url-status=live }}</ref><ref>{{citation
| Notes = The habitability of planets b and c is disputed.<ref>{{cite web
| last=Sutherland | first=Paul | date=March 5, 2014
| title=Habitable planets common around red dwarf stars
| url=http://sen.com/news/habitable-planets-common-around-red-dwarf-stars
| website=Sen | publisher=Sen Corporation Ltd. }}</ref><ref>{{citation
| title=Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics | title=Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics
| display-authors=1 | last1=Tuomi | first1=Mikko | display-authors=1 | last1=Tuomi | first1=Mikko
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| journal=Monthly Notices of the Royal Astronomical Society | journal=Monthly Notices of the Royal Astronomical Society
| volume=441 | issue=2 | pages=1545–1569 | year=2014 | volume=441 | issue=2 | pages=1545–1569 | year=2014
| doi=10.1093/mnras/stu358 | arxiv=1403.0430 | postscript=. | doi=10.1093/mnras/stu358 | doi-access=free | arxiv=1403.0430 | postscript=.
| bibcode=2014MNRAS.441.1545T | s2cid=32965505 }}</ref> | bibcode=2014MNRAS.441.1545T | s2cid=32965505 }}</ref>
}} }}
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| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = 2 |Unconfirmed planets = 2
| Notes = The existence of planets e and g are disputed.<ref name=Diaz2016HD40307>{{cite journal | title=The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles | url=https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | last1=Díaz | first1=R. F. | last2=Ségransan | first2=D. | last3=Udry | first3=S. | last4=Lovis | first4=C. | last5=Pepe | first5=F. | last6=Dumusque | first6=X. | last7=Marmier | first7=M. | last8=Alonso | first8=R. | last9=Benz | first9=W. | last10=Bouchy | first10=F. | last11=Coffinet | first11=A. | last12=Collier Cameron | first12=A. | last13=Deleuil | first13=M. | last14=Figueira | first14=P. | last15=Gillon | first15=M. | last16=Lo Curto | first16=G. | last17=Mayor | first17=M. | last18=Mordasini | first18=C. | last19=Motalebi | first19=F. | last20=Moutou | first20=C. | last21=Pollacco | first21=D. | last22=Pompei | first22=E. | last23=Queloz | first23=D. | last24=Santos | first24=N. | last25=Wyttenbach | first25=A. | display-authors=1 | journal=Astronomy and Astrophysics | volume=585 | at=A134 | year=2016 | arxiv=1510.06446 | bibcode=2016A&A...585A.134D | doi=10.1051/0004-6361/201526729 | s2cid=118531921 }}</ref> If confirmed, planet g is potentially habitable.<ref name="tuomi12HD40307g">{{cite journal |doi=10.1051/0004-6361/201220268 |last1=Tuomi |first1=Mikko |last2=Anglada-Escudé |first2=Guillem |last3=Gerlach |first3=Enrico |last4=Jones |first4=Hugh R. A. |last5=Reiners |first5=Ansgar |last6=Rivera |first6=Eugenio J. |last7=Vogt |first7=Steven S. |last8=Butler |first8=R. Paul |title=Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307 |journal=Astronomy & Astrophysics |date=17 December 2012 |volume=549 |pages=A48 |arxiv=1211.1617 |bibcode=2013A&A...549A..48T |s2cid=7424216 }}</ref> | Notes = The existence of planets e and g are disputed.<ref name=Diaz2016HD40307>{{cite journal | title=The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles | url=https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | last1=Díaz | first1=R. F. | last2=Ségransan | first2=D. | last3=Udry | first3=S. | last4=Lovis | first4=C. | last5=Pepe | first5=F. | last6=Dumusque | first6=X. | last7=Marmier | first7=M. | last8=Alonso | first8=R. | last9=Benz | first9=W. | last10=Bouchy | first10=F. | last11=Coffinet | first11=A. | last12=Collier Cameron | first12=A. | last13=Deleuil | first13=M. | last14=Figueira | first14=P. | last15=Gillon | first15=M. | last16=Lo Curto | first16=G. | last17=Mayor | first17=M. | last18=Mordasini | first18=C. | last19=Motalebi | first19=F. | last20=Moutou | first20=C. | last21=Pollacco | first21=D. | last22=Pompei | first22=E. | last23=Queloz | first23=D. | last24=Santos | first24=N. | last25=Wyttenbach | first25=A. | display-authors=1 | journal=Astronomy and Astrophysics | volume=585 | at=A134 | year=2016 | arxiv=1510.06446 | bibcode=2016A&A...585A.134D | doi=10.1051/0004-6361/201526729 | s2cid=118531921 | access-date=2022-02-24 | archive-date=2021-02-24 | archive-url=https://web.archive.org/web/20210224090311/https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | url-status=live }}</ref> If confirmed, planet g is potentially habitable.<ref name="tuomi12HD40307g">{{cite journal |doi=10.1051/0004-6361/201220268 |last1=Tuomi |first1=Mikko |last2=Anglada-Escudé |first2=Guillem |last3=Gerlach |first3=Enrico |last4=Jones |first4=Hugh R. A. |last5=Reiners |first5=Ansgar |last6=Rivera |first6=Eugenio J. |last7=Vogt |first7=Steven S. |last8=Butler |first8=R. Paul |title=Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307 |journal=Astronomy & Astrophysics |date=17 December 2012 |volume=549 |pages=A48 |arxiv=1211.1617 |bibcode=2013A&A...549A..48T |s2cid=7424216 }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = Upsilon Andromedae | Star = Upsilon Andromedae|Titawin
| Constellation = Andromeda (constellation){{!}}Andromeda | Constellation = Andromeda (constellation){{!}}Andromeda
| Right ascension = {{RA|01|36|47.84}} | Right ascension = {{RA|01|36|47.84}}
Line 605: Line 686:
| Age = 3.781 | Age = 3.781
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = 1 |Unconfirmed planets =
| Notes = Nearest ] star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after ]. All exoplanets orbit around star A in the binary system. | Notes = Nearest ] star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after ]. All exoplanets orbit around star A in the binary system.
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = 47 Ursae Majoris | Star = 47 Ursae Majoris|Chalawan
| Constellation = Ursa Major | Constellation = Ursa Major
| Right ascension = {{RA|10|59|27.97}} | Right ascension = {{RA|10|59|27.97}}
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| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet b was discovered in 1996 and was one of the first exoplanets to be discovered.<ref> | Notes = Planet Taphao Thong was discovered in 1996 and was one of the first exoplanets to be discovered.<ref>
{{cite journal {{cite journal
| author=R. P. Butler | author=R. P. Butler
Line 644: Line 725:
|volume=403 |issue=2 |pages=731–747 |volume=403 |issue=2 |pages=731–747
|doi=10.1111/j.1365-2966.2009.16233.x |doi=10.1111/j.1365-2966.2009.16233.x
|doi-access=free
|bibcode=2010MNRAS.403..731G
|bibcode=2010MNRAS.403..731G
|arxiv = 1003.5549 |s2cid=16722873 |arxiv = 1003.5549 |s2cid=16722873
}}</ref> }}</ref>
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{{Multiplanetary systems list {{Multiplanetary systems list
| Star = ] | Star = ]
| Constellation = Lupus | Constellation = Lupus (constellation){{!}}Lupus
| Right ascension = {{RA|15|21|49.57}} | Right ascension = {{RA|15|21|49.57}}
| Declination = {{DEC|−48|19|01.1}} | Declination = {{DEC|−48|19|01.1}}
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{{Multiplanetary systems list {{Multiplanetary systems list
| Star = ] | Star = ]
| Constellation = Draco (constellation){{!}}Draco | Constellation = Cetus (constellation){{!}}Cetus
| Right ascension = {{RA|00|44|59.31}} | Right ascension = {{RA|00|44|59.31}}
| Declination = {{DEC|-15|16|16.7}} | Declination = {{DEC|-15|16|16.7}}
Line 681: Line 763:
| Confirmed planets = 2 | Confirmed planets = 2
|Unconfirmed planets = 1 |Unconfirmed planets = 1
| Notes = Planet b is a potentially habitable Super-Earth.<ref name="NYT-20170419">{{cite news |last=Overbye |first=Dennis |author-link=Dennis Overbye |title=A new exoplanet may be most promising yet in search for life |url=https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |date=19 April 2017 |work=] |access-date=20 April 2017}}</ref> | Notes = Planet b is a potentially habitable Super-Earth.<ref name="NYT-20170419">{{cite news |last=Overbye |first=Dennis |author-link=Dennis Overbye |title=A new exoplanet may be most promising yet in search for life |url=https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |date=19 April 2017 |work=] |access-date=20 April 2017 |archive-date=11 November 2020 |archive-url=https://web.archive.org/web/20201111202355/https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 699: Line 781:
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.<ref name="PHL-20120829">{{cite web | Notes = Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.<ref name="PHL-20120829">{{cite web
| last=Méndez | first=Abel | date=August 29, 2012 | last=Méndez
| first=Abel
| date=August 29, 2012
| title=A Hot Potential Habitable Exoplanet around Gliese 163 | title=A Hot Potential Habitable Exoplanet around Gliese 163
| url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163 | url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
| publisher=] (Planetary Habitability Laboratory) | publisher=] (Planetary Habitability Laboratory)
| accessdate=September 20, 2012 }}</ref><ref name="Space-20120920">{{cite web | accessdate=September 20, 2012
| archive-date=October 21, 2019
| last=Redd | first=Nola Taylor
| archive-url=https://web.archive.org/web/20191021202448/http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
| url-status=dead
}}</ref><ref name="Space-20120920">{{cite web
| last=Redd
| first=Nola Taylor
| title=Newfound Alien Planet a Top Contender to Host Life | title=Newfound Alien Planet a Top Contender to Host Life
| url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html | url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
| date=September 20, 2012 | publisher=] | date=September 20, 2012
| publisher=]
| accessdate=September 20, 2012 }}</ref> | accessdate=September 20, 2012
| archive-date=December 26, 2019
| archive-url=https://web.archive.org/web/20191226102330/https://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
| url-status=live
}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = Mu Arae | Star = Mu Arae|Cervantes
| Constellation = Ara (constellation){{!}}Ara | Constellation = Ara (constellation){{!}}Ara
| Right ascension = {{RA|17|44|08.70}} | Right ascension = {{RA|17|44|08.70}}
Line 725: Line 819:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet b orbits in the ]. However, it is a ], so it itself is uninhabitable although a large moon orbiting around it may be habitable. | Notes = Planet Quijote orbits in the ]. However, it is a ], so it itself is uninhabitable although a large moon orbiting around it may be ].
}} }}
{{Multiplanetary systems list
| Star = ]
| Constellation = Corona Borealis
| Right ascension = {{RA|15|58|18.8}}
| Declination = {{DEC|35|24|24.3}}
| Apparent magnitude = 12.67
| Distance = 51.58
| Spectral type = M3.5V
| Mass = 0.313
| Radius = 0.32
| Temperature = 3384
| Metallicity = -0.02
| Age =
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes = <ref>{{Cite web |title=Simbad - Object view |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=G%20180-18 |access-date=2024-01-04 |website=simbad.cds.unistra.fr}}</ref><ref>{{Cite journal |last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Lubin |first4=Jack |last5=Cañas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Libby-Roberts |first9=Jessica E. |last10=Lin |first10=Andrea S. J. |last11=Mahadevan |first11=Suvrath |last12=Stefánsson |first12=Guđmundur |last13=Bender |first13=Chad F. |last14=Blake |first14=Cullen H. |last15=Cochran |first15=William D. |date=2022-08-30 |title=GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion |journal=The Astrophysical Journal |volume=936 |issue=1 |pages=55 |doi=10.3847/1538-4357/ac8480 |doi-access=free |arxiv=2207.10672 |bibcode=2022ApJ...936...55B |issn=0004-637X}}</ref>
}}


{{Multiplanetary systems list {{Multiplanetary systems list
| Star = ] A | Star = ] A
Line 743: Line 856:
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Held the record for widest range of masses in a planetary system in 2012.<ref name="4-planet Gj676A">{{cite journal | Notes = Held the record for widest range of masses in a planetary system in 2012.<ref name="4-planet Gj676A">{{cite journal
|last = Anglada-Escudé |first=Guillem |last=Anglada-Escudé
|first=Guillem
|author2=Tuomi, Mikko |author2=Tuomi, Mikko
|date = 2012 |date=2012
|title = A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems |title=A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems
|arxiv = 1206.7118 |arxiv=1206.7118
|bibcode = 2012A&A...548A..58A |bibcode=2012A&A...548A..58A
|doi=10.1051/0004-6361/201219910 |doi=10.1051/0004-6361/201219910
|volume=548 |volume=548
|journal=Astronomy |journal=Astronomy
|pages=A58 |pages=A58
|s2cid=17115882 |s2cid=17115882
|url=http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2 |url=http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2
}}{{Dead link|date=February 2024 |bot=InternetArchiveBot |fix-attempted=yes }}</ref>
}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 816: Line 930:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planets b and d orbit in the habitable zone.<ref name="arxiv.org_Gliese3293">{{cite journal | doi=10.1051/0004-6361/201630153 | Notes = Planets b and d orbit in the habitable zone.<ref name="arxiv.org_Gliese3293">{{cite journal
|doi = 10.1051/0004-6361/201630153
|last1 = Astudillo-Defru
| last1=Astudillo-Defru | first1=Nicola | last2=Forveille | first2=Thierry
|first1 = Nicola
| last3=Bonfils | first3=Xavier | last4=Ségransan | first4=Damien
|last2 = Forveille
| last5=Bouchy | first5=François | last6=Delfosse | first6=Xavier
|first2 = Thierry
| last7=Lovis | first7=Christophe | last8=Mayor | first8=Michel
|last3 = Bonfils
| last9=Murgas | first9=Felipe | last10=Pepe | first10=Francesco
|first3 = Xavier
| last11=Santos | first11=Nuno C. | last12=Udry | first12=Stéphane
|last4 = Ségransan
| last13=Wünsche | first13=Anaël | display-authors=6
|first4 = Damien
| year=2017
|last5 = Bouchy
| title=The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
|first5 = François
| journal=Astronomy and Astrophysics
|last6 = Delfosse
| volume=602 | at=A88
|first6 = Xavier
| arxiv=1703.05386 | bibcode=2017A&A...602A..88A | s2cid=119418595
|last7 = Lovis
| url=https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|first7 = Christophe
|last8 = Mayor
|first8 = Michel
|last9 = Murgas
|first9 = Felipe
|last10 = Pepe
|first10 = Francesco
|last11 = Santos
|first11 = Nuno C.
|last12 = Udry
|first12 = Stéphane
|last13 = Wünsche
|first13 = Anaël
|display-authors = 6
|year = 2017
|title = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
|journal = Astronomy and Astrophysics
|volume = 602
|at = A88
|arxiv = 1703.05386
|bibcode = 2017A&A...602A..88A
|s2cid = 119418595
|url = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|access-date = 2022-02-25
|archive-date = 2022-09-28
|archive-url = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|url-status = live
}}</ref> }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = HD 142|37 G. Phe | Star = LHS 1678
| Constellation = Caelum
| Right ascension = {{Ra|04|32|43}}
| Declination = {{Dec|-39|47|21}}
| Apparent magnitude = 12
| Distance = 64.8
| Spectral type = M2V
| Mass = 0.345
| Radius = 0.329
| Temperature = 3490
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 0
| Notes = <ref>{{cite web | url=https://exoplanet.eu/catalog/lhs_1678_d--8971/ | title=Planet LHS 1678 D | date=2024 }}</ref>
}}
{{Multiplanetary systems list
| Star = ]
| Constellation = Corvus (constellation){{!}}Corvus
| Right ascension = {{RA|11|59|10.0}}
| Declination = {{DEC|-20|21|13.6}}
| Apparent magnitude = 7.92
| Distance = 66.3
| Spectral type = K3V
| Mass = 0.82
| Radius = 0.77
| Temperature = 4942
| Metallicity = 0.11
| Age = 4.8
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = The innermost planet, which is unconfirmed, might suffer from significant ].<ref name="Kane2024">{{cite journal |last1=Kane |first1=Stephen R. |last2=Fetherolf |first2=Tara |display-authors=etal |date=March 2024 |title=A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World |journal=] |volume= 167|issue= 5|page=239 |doi= 10.3847/1538-3881/ad3820|doi-access=free |arxiv=2403.17062|bibcode=2024AJ....167..239K }}</ref>
}}
{{Multiplanetary systems list
| Star = HD 142
| Constellation = Phoenix (constellation){{!}}Phoenix | Constellation = Phoenix (constellation){{!}}Phoenix
| Right ascension = {{RA|00|06|19.0}} | Right ascension = {{RA|00|06|19.0}}
Line 863: Line 1,039:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = A debris disk candidate as it has an infrared excess.<ref name=apjl710_1_L26>{{citation | display-authors=1 | last1=Koerner | first1=D. W. | last2=Kim | first2=S. | last3=Trilling | first3=D. E. | last4=Larson | first4=H. | last5=Cotera | first5=A. | last6=Stapelfeldt | first6=K. R. | last7=Wahhaj | first7=Z. | last8=Fajardo-Acosta | first8=S. | last9=Padgett | first9=D. | last10=Backman | first10=D. | title=New Debris Disk Candidates Around 49 Nearby Stars | journal=The Astrophysical Journal Letters | volume=710 | issue=1 | pages=L26–L29 | date=February 2010 | doi=10.1088/2041-8205/710/1/L26 | bibcode=2010ApJ...710L..26K | s2cid=122844702 | postscript=. | url=http://openknowledge.nau.edu/449/7/Koerner_DW_etal_2010_New_debris_disk_candidates_around_49_nearby_stars%281%29.pdf | access-date=2022-02-25 | archive-date=2020-09-15 | archive-url=https://web.archive.org/web/20200915161129/http://openknowledge.nau.edu/449/7/Koerner_DW_etal_2010_New_debris_disk_candidates_around_49_nearby_stars%281%29.pdf | url-status=live }}</ref>
| Notes = A debris disk candidate as it has an infrared excess.<ref name=apjl710_1_L26>{{citation
| display-authors=1
| last1=Koerner | first1=D. W. | last2=Kim | first2=S.
| last3=Trilling | first3=D. E. | last4=Larson | first4=H.
| last5=Cotera | first5=A. | last6=Stapelfeldt | first6=K. R.
| last7=Wahhaj | first7=Z. | last8=Fajardo-Acosta | first8=S.
| last9=Padgett | first9=D. | last10=Backman | first10=D.
| title=New Debris Disk Candidates Around 49 Nearby Stars
| journal=The Astrophysical Journal Letters
| volume=710 | issue=1 | pages=L26–L29 | date=February 2010
| doi=10.1088/2041-8205/710/1/L26 | bibcode=2010ApJ...710L..26K
| s2cid=122844702 | postscript=. | url=http://openknowledge.nau.edu/449/7/Koerner_DW_etal_2010_New_debris_disk_candidates_around_49_nearby_stars%281%29.pdf}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 883: Line 1,048:
| Apparent magnitude = 7.01 | Apparent magnitude = 7.01
| Distance = 72 | Distance = 72
| Spectral type = G9V<ref name="Spectype164922">{{cite journal|arxiv=1607.00007|last1= Fulton|first1= Benjamin J.|title= Three Temperate Neptunes Orbiting Nearby Stars|last2= Howard|first2= Andrew W.|last3= Weiss|first3= Lauren M.|last4= Sinukoff|first4= Evan|last5= Petigura|first5= Erik A.|last6= Isaacson|first6= Howard|last7= Hirsch|first7= Lea|last8= Marcy|first8= Geoffrey W.|last9= Henry|first9= Gregory W.|last10= Grunblatt|first10= Samuel K.|last11= Huber|first11= Daniel|author12= Kaspar von Braun|last13= Boyajian|first13= Tabetha S.|last14= Kane|first14= Stephen R.|last15= Wittrock|first15= Justin|last16= Horch|first16= Elliott P.|last17= Ciardi|first17= David R.|last18= Howell|first18= Steve B.|last19= Wright|first19= Jason T.|last20= Ford|first20= Eric B.|year= 2016|doi=10.3847/0004-637X/830/1/46|volume=830|issue= 1|journal=The Astrophysical Journal|page=46|bibcode = 2016ApJ...830...46F |s2cid= 36666883}}</ref> | Spectral type = G9V<ref name="Spectype164922">{{cite journal|arxiv=1607.00007|last1= Fulton|first1= Benjamin J.|title= Three Temperate Neptunes Orbiting Nearby Stars|last2= Howard|first2= Andrew W.|last3= Weiss|first3= Lauren M.|last4= Sinukoff|first4= Evan|last5= Petigura|first5= Erik A.|last6= Isaacson|first6= Howard|last7= Hirsch|first7= Lea|last8= Marcy|first8= Geoffrey W.|last9= Henry|first9= Gregory W.|last10= Grunblatt|first10= Samuel K.|last11= Huber|first11= Daniel|author12= Kaspar von Braun|last13= Boyajian|first13= Tabetha S.|last14= Kane|first14= Stephen R.|last15= Wittrock|first15= Justin|last16= Horch|first16= Elliott P.|last17= Ciardi|first17= David R.|last18= Howell|first18= Steve B.|last19= Wright|first19= Jason T.|last20= Ford|first20= Eric B.|year= 2016|doi=10.3847/0004-637X/830/1/46|volume=830|issue= 1|journal=The Astrophysical Journal|page=46|bibcode = 2016ApJ...830...46F |s2cid= 36666883|doi-access= free}}</ref>
| Mass = 0.874 | Mass = 0.874
| Radius = 0.999 | Radius = 0.999
Line 892: Line 1,057:
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.<ref name="Spectype164922"/> | Notes = Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.<ref name="Spectype164922"/>
}}
{{Multiplanetary systems list
| Star = HD 63433
| Constellation = Gemini (constellation){{!}}Gemini
| Right ascension = {{RA|07|49|55.0}}
| Declination = {{DEC|+27|21|47.4}}
| Apparent magnitude = 6.92
| Distance = 73
| Spectral type = G5V
| Mass = 0.99
| Radius = 0.912
| Temperature =5640
| Metallicity = 0.03
| Age = 0.4
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 927: Line 1,109:
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = HD 184010 | Star = LP 791-18
| Constellation = Vulpecula | Constellation = Crater
| Right ascension = {{RA|19|31|22.0}} | Right ascension = {{RA|11|02|45.95}}
| Declination = {{DEC|+26|37|02}} | Declination = {{DEC|-16|24|22.3}}
| Apparent magnitude = 5.9 | Apparent magnitude = 16.9
| Distance = 200 | Distance = 86.9
| Spectral type = KOIII-IV | Spectral type = M6V/M7V
| Mass = 1.35 | Mass = 0.139
| Radius = 4.86 | Radius = 0.17
| Temperature = 4971 | Temperature =2960
| Metallicity = -0.17 | Metallicity =-0.09
| Age = 2.76 | Age = 0.5
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes =
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 971: Line 1,154:
| Metallicity = | Metallicity =
| Age = | Age =
| Confirmed planets = 3 | Confirmed planets = 5
|Unconfirmed planets = |Unconfirmed planets =
| Notes = The planets have moderately eccentric orbits.<ref name=Mayor2011>{{citation | Notes = The planets have moderately eccentric orbits.<ref name=Mayor2011>{{citation
Line 1,016: Line 1,199:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planets b and c are in a 2:1 orbital resonance.<ref name="Lee2006">{{cite journal | title=On the 2:1 Orbital Resonance in the HD 82943 Planetary System | last1=Lee | first1=Man Hoi | last2=Butler | first2=R. Paul | last3=Fischer | first3=Debra A. | last4=Marcy | first4=Geoffrey W. | last5=Vogt | first5=Steven S. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=641 | issue=2 | pages=1178–1187 | arxiv=astro-ph/0512551 | bibcode=2006ApJ...641.1178L | doi=10.1086/500566 | s2cid=119432579 }}</ref> Planet b orbits in the habitable zone, but it and planet c are massive enough to be ]s. HD 82943 has an unusual ] abundance.<ref name="eso0118">{{cite press release | title=The Harsh Destiny of a Planet? | date=May 9, 2001 | publisher=] | location=Garching, Germany | url=http://www.eso.org/public/news/eso0118/ | access-date=December 30, 2012 }}</ref> | Notes = Planets b and c are in a 2:1 orbital resonance.<ref name="Lee2006">{{cite journal | title=On the 2:1 Orbital Resonance in the HD 82943 Planetary System | last1=Lee | first1=Man Hoi | last2=Butler | first2=R. Paul | last3=Fischer | first3=Debra A. | last4=Marcy | first4=Geoffrey W. | last5=Vogt | first5=Steven S. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=641 | issue=2 | pages=1178–1187 | arxiv=astro-ph/0512551 | bibcode=2006ApJ...641.1178L | doi=10.1086/500566 | s2cid=119432579 }}</ref> Planet b orbits in the habitable zone, but it and planet c are massive enough to be ]s. HD 82943 has an unusual ] abundance.<ref name="eso0118">{{cite press release | title=The Harsh Destiny of a Planet? | date=May 9, 2001 | publisher=] | location=Garching, Germany | url=http://www.eso.org/public/news/eso0118/ | access-date=December 30, 2012 | archive-date=September 21, 2020 | archive-url=https://web.archive.org/web/20200921074543/https://www.eso.org/public/news/eso0118/ | url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,050: Line 1,233:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.<ref>{{cite journal | bibcode=2018AJ....155...72R | doi=10.3847/1538-3881/aaa292 | arxiv=1709.01957| title=A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc| journal=The Astronomical Journal| volume=155| issue=2| pages=72| year=2018| last1=Rodriguez| first1=Joseph E| last2=Vanderburg| first2=Andrew| last3=Eastman| first3=Jason D| last4=Mann| first4=Andrew W| last5=Crossfield| first5=Ian J. M| last6=Ciardi| first6=David R| last7=Latham| first7=David W| last8=Quinn| first8=Samuel N| s2cid=55459523 }}</ref> | Notes = Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.<ref>{{cite journal | bibcode=2018AJ....155...72R | doi=10.3847/1538-3881/aaa292 | arxiv=1709.01957| title=A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc| journal=The Astronomical Journal| volume=155| issue=2| pages=72| year=2018| last1=Rodriguez| first1=Joseph E| last2=Vanderburg| first2=Andrew| last3=Eastman| first3=Jason D| last4=Mann| first4=Andrew W| last5=Crossfield| first5=Ian J. M| last6=Ciardi| first6=David R| last7=Latham| first7=David W| last8=Quinn| first8=Samuel N| s2cid=55459523 | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
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}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = ] | Star = ]
| Constellation = Dorado (constellation){{!}}Dorado | Constellation = Dorado (constellation){{!}}Dorado
| Right ascension = {{RA|06|28|22.97}} | Right ascension = {{RA|06|28|22.97}}
Line 1,084: Line 1,267:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planets d and e are potentially habitable.<ref name="NASA-20200106">{{cite news |last1=Andreolo |first1=Claire |last2=Cofield |first2=Calla |last3=Kazmierczak |first3=Jeanette |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.jpl.nasa.gov/news/news.php?feature=7569 |date=6 January 2020 |work=] |access-date=6 January 2020 }}</ref><ref name="NASA-20200106b">{{cite news |last1=Garner |first1=Rob |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |date=6 January 2020 |work=] |access-date=6 January 2020 }}</ref><ref name="SPC-20200106">{{cite news |last=Wall |first=Mike |title=NASA's TESS Planet Hunter Finds Its 1st Earth-Size World in 'Habitable Zone' |url=https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |date=6 January 2020 |work=] |access-date=6 January 2020 }}</ref> | Notes = Planets d and e are potentially habitable.<ref name="NASA-20200106">{{cite news |last1=Andreolo |first1=Claire |last2=Cofield |first2=Calla |last3=Kazmierczak |first3=Jeanette |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.jpl.nasa.gov/news/news.php?feature=7569 |date=6 January 2020 |work=] |access-date=6 January 2020 |archive-date=14 April 2020 |archive-url=https://web.archive.org/web/20200414070820/https://www.jpl.nasa.gov/news/news.php?feature=7569 |url-status=live }}</ref><ref name="NASA-20200106b">{{cite news |last1=Garner |first1=Rob |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |date=6 January 2020 |work=] |access-date=6 January 2020 |archive-date=5 April 2020 |archive-url=https://web.archive.org/web/20200405004715/https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |url-status=live }}</ref><ref name="SPC-20200106">{{cite news |last=Wall |first=Mike |title=NASA's TESS Planet Hunter Finds Its 1st Earth-Size World in 'Habitable Zone' |url=https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |date=6 January 2020 |work=] |access-date=6 January 2020 |archive-date=8 April 2020 |archive-url=https://web.archive.org/web/20200408031443/https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,119: Line 1,302:
| last29=Mengel | first29=Matthew W. | last30=Morton | first30=Timothy D. | last29=Mengel | first29=Matthew W. | last30=Morton | first30=Timothy D.
| display-authors=1 | year=2019 | display-authors=1 | year=2019
| arxiv=1905.05193 | doi=10.3847/2041-8213/ab322d | bibcode=2019ApJ...881L..19V | s2cid=153311715 }}</ref> | arxiv=1905.05193 | doi=10.3847/2041-8213/ab322d | bibcode=2019ApJ...881L..19V | s2cid=153311715 | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,136: Line 1,319:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet c orbits at the outer edge of the habitable zone.<ref name="Vogt2005">{{cite journal | title=Five New Multicomponent Planetary Systems | last1=Vogt | first1=Steven S. | last2=Butler | first2=R. Paul | last3=Marcy | first3=Geoffrey W. | last4=Fischer | first4=Debra A. | last5=Henry | first5=Gregory W. | last6=Laughlin | first6=Greg | last7=Wright | first7=Jason T. | last8=Johnson | first8=John A. | display-authors=1 | journal=The Astrophysical Journal | volume=632 | issue=1 | pages=638–658 | year=2005 | bibcode=2005ApJ...632..638V | doi=10.1086/432901 | s2cid=16509245 | access-date=2020-12-11 | url=https://authors.library.caltech.edu/36250/1/0004-637X_632_1_638.pdf | archive-date=2018-07-22 | archive-url=https://web.archive.org/web/20180722000634/https://authors.library.caltech.edu/36250/1/0004-637X_632_1_638.pdf | url-status=live }}</ref>
| Notes = Planet c orbits at the outer edge of the habitable zone.<ref name="Vogt2005">{{cite journal
| title=Five New Multicomponent Planetary Systems
| last1=Vogt | first1=Steven S. | last2=Butler | first2=R. Paul
| last3=Marcy | first3=Geoffrey W. | last4=Fischer | first4=Debra A.
| last5=Henry | first5=Gregory W. | last6=Laughlin | first6=Greg
| last7=Wright | first7=Jason T. | last8=Johnson | first8=John A.
| display-authors=1 | journal=The Astrophysical Journal
| volume=632 | issue=1 | pages=638–658 | year=2005
| bibcode=2005ApJ...632..638V | doi=10.1086/432901 | s2cid=16509245 | access-date=2020-12-11
| url=https://authors.library.caltech.edu/36250/1/0004-637X_632_1_638.pdf }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,196: Line 1,370:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet c orbits in the habitable zone.<ref name=Hebrard2016HD141399c>{{Cite journal |doi=10.1051/0004-6361/201527585 |last1=Hébrard |first1=Guillaume |last2=Arnold |first2=Luc |last3=Forveille |first3=Thierry |last4=Correia |first4=Alexandre C. M. |last5=Laskar |first5=Jacques |last6=Bonfils |first6=Xavier |last7=Boisse |first7=Isabelle |last8=Díaz |first8=Rodrigo F. |last9=Hagelberg |first9=Janis |last10=Sahlmann |first10=Johannes |last11=Santos |first11=Nuno C. |display-authors=11 |author12=Nicola Astudillo-Defru |author13=Simon Borgniet |author14=François Bouchy |author15=Vincent Bourrier |author16=Bastien Courcol |author17=Xavier Delfosse |author18=Magali Deleuil |author19=Olivier D. S. Demangeon |author20=David Ehrenreich |author21=João Gregório |author22=N. Jovanovic |author23=Olivier Labrevoir |author24=Anne-Marie Lagrange |author25=Christophe Lovis |author26=J. Lozi |author27=Claire Moutou |author28=Guillaume Montagnier |author29=Francesco Pepe |author30=Javiera Rey |author31=Alexandre Santerne |author32=Damien Ségransan |author33=Stéphane Udry |author34=Michael Vanhuysse |author35=A. Vigan |author36=Paul A. Wilson |date=2016-04-01 |title=The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen |url=http://adsabs.harvard.edu/abs/2016A%26A...588A.145H |journal=Astronomy and Astrophysics |volume=588 |pages=A145 |issn=0004-6361 |arxiv=1602.04622 |bibcode=2016A&A...588A.145H |s2cid=55138055 }}</ref> | Notes = Planet c orbits in the habitable zone.<ref name=Hebrard2016HD141399c>{{Cite journal |doi=10.1051/0004-6361/201527585 |last1=Hébrard |first1=Guillaume |last2=Arnold |first2=Luc |last3=Forveille |first3=Thierry |last4=Correia |first4=Alexandre C. M. |last5=Laskar |first5=Jacques |last6=Bonfils |first6=Xavier |last7=Boisse |first7=Isabelle |last8=Díaz |first8=Rodrigo F. |last9=Hagelberg |first9=Janis |last10=Sahlmann |first10=Johannes |last11=Santos |first11=Nuno C. |display-authors=11 |author12=Nicola Astudillo-Defru |author13=Simon Borgniet |author14=François Bouchy |author15=Vincent Bourrier |author16=Bastien Courcol |author17=Xavier Delfosse |author18=Magali Deleuil |author19=Olivier D. S. Demangeon |author20=David Ehrenreich |author21=João Gregório |author22=N. Jovanovic |author23=Olivier Labrevoir |author24=Anne-Marie Lagrange |author25=Christophe Lovis |author26=J. Lozi |author27=Claire Moutou |author28=Guillaume Montagnier |author29=Francesco Pepe |author30=Javiera Rey |author31=Alexandre Santerne |author32=Damien Ségransan |author33=Stéphane Udry |author34=Michael Vanhuysse |author35=A. Vigan |author36=Paul A. Wilson |date=2016-04-01 |title=The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen |url=http://adsabs.harvard.edu/abs/2016A%26A...588A.145H |journal=Astronomy and Astrophysics |volume=588 |pages=A145 |issn=0004-6361 |arxiv=1602.04622 |bibcode=2016A&A...588A.145H |s2cid=55138055 |access-date=2022-02-26 |archive-date=2019-04-10 |archive-url=https://web.archive.org/web/20190410043711/http://adsabs.harvard.edu/abs/2016A%26A...588A.145H |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,330: Line 1,504:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = The outermost planet orbits in the habitable zone.<ref name=ScienceNewsK2-3></ref> | Notes = The outermost planet orbits in the habitable zone.<ref name=ScienceNewsK2-3>{{Cite web |url=http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |title=Three Super-Earths Found Circling Nearby Red Dwarf |access-date=2022-02-27 |archive-date=2019-01-02 |archive-url=https://web.archive.org/web/20190102064436/http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,347: Line 1,521:
| Confirmed planets = 1 | Confirmed planets = 1
|Unconfirmed planets = 5 |Unconfirmed planets = 5
| Notes = Some planets were not detected or inferred to be false positives in a later study.<ref name=Rosenthal2021>{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973}}</ref> | Notes = Some planets were not detected or inferred to be false positives in a later study.<ref name=Rosenthal2021>{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,413: Line 1,587:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
|Notes = 2 planets around primary, and 1 planet around secondary star.<ref name=TeskeHD>{{cite journal|bibcode=2016AJ....152..167T|doi=10.3847/0004-6256/152/6/167|arxiv=1608.06216|title=The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B|journal=The Astronomical Journal|volume=152|issue=6|pages=167|year=2016|last1=Teske|first1=Johanna K|last2=Shectman|first2=Stephen A|last3=Vogt|first3=Steve S|last4=Díaz|first4=Matías|last5=Butler|first5=R. Paul|last6=Crane|first6=Jeffrey D|last7=Thompson|first7=Ian B|last8=Arriagada|first8=Pamela|s2cid=118852162}}</ref> |Notes = 2 planets around primary, and 1 planet around secondary star.<ref name=TeskeHD>{{cite journal|bibcode=2016AJ....152..167T|doi=10.3847/0004-6256/152/6/167|arxiv=1608.06216|title=The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B|journal=The Astronomical Journal|volume=152|issue=6|pages=167|year=2016|last1=Teske|first1=Johanna K|last2=Shectman|first2=Stephen A|last3=Vogt|first3=Steve S|last4=Díaz|first4=Matías|last5=Butler|first5=R. Paul|last6=Crane|first6=Jeffrey D|last7=Thompson|first7=Ian B|last8=Arriagada|first8=Pamela|s2cid=118852162 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,479: Line 1,653:
| Metallicity = 0.244 | Metallicity = 0.244
| Age = 2.150 | Age = 2.150
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 184010
| Constellation = Vulpecula
| Right ascension = {{RA|19|31|22.0}}
| Declination = {{DEC|+26|37|02}}
| Apparent magnitude = 5.9
| Distance = 200
| Spectral type = KOIII-IV
| Mass = 1.35
| Radius = 4.86
| Temperature = 4971
| Metallicity = -0.17
| Age = 2.76
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
Line 1,554: Line 1,744:
| Apparent magnitude = 9.77 | Apparent magnitude = 9.77
| Distance = 215 | Distance = 215
| Spectral type = G | Spectral type = G8V
| Mass = 0.803 | Mass = 0.803
| Radius = 0.770 | Radius = 0.770
Line 1,560: Line 1,750:
| Metallicity = −0.32 | Metallicity = −0.32
| Age = 6 | Age = 6
| Confirmed planets = 4 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets = 1
| Notes = The existence of Kepler-37e is dubious.<ref name=Rajpaul2021>{{citation|arxiv=2107.13900|year=2021|title=A HARPS-N mass for the elusive Kepler-37d: A case study in disentangling stellar activity and planetary signals|doi=10.1093/mnras/stab2192|last1=Rajpaul|first1=V. M.|last2=Buchhave|first2=L. A.|last3=Lacedelli|first3=G.|last4=Rice|first4=K.|last5=Mortier|first5=A.|last6=Malavolta|first6=L.|last7=Aigrain|first7=S.|last8=Borsato|first8=L.|last9=Mayo|first9=A. W.|last10=Charbonneau|first10=D.|last11=Damasso|first11=M.|last12=Dumusque|first12=X.|last13=Ghedina|first13=A.|last14=Latham|first14=D. W.|last15=López-Morales|first15=M.|last16=Magazzù|first16=A.|last17=Micela|first17=G.|last18=Molinari|first18=E.|last19=Pepe|first19=F.|last20=Piotto|first20=G.|last21=Poretti|first21=E.|last22=Rowther|first22=S.|last23=Sozzetti|first23=A.|last24=Udry|first24=S.|last25=Watson|first25=C. A.|journal=Monthly Notices of the Royal Astronomical Society|volume=507|issue=2|pages=1847–1868 |doi-access=free |bibcode=2021MNRAS.507.1847R}} Kepler-37e is discussed in sections 2.2.2 & 6.4.</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,713: Line 1,904:
| Age = 0.7 | Age = 0.7
| Confirmed planets = 6 | Confirmed planets = 6
|Unconfirmed planets = |Unconfirmed planets = 1
| Notes = | Notes =
}} }}
Line 1,730: Line 1,921:
| Age = 5 | Age = 5
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets = 1
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,805: Line 1,996:
| Apparent magnitude = 10.31 | Apparent magnitude = 10.31
| Distance = 354 | Distance = 354
| Spectral type = K0-1.5<ref name="David_et_al_V1298Taurispectype">{{Cite journal|last1=David|first1=Trevor J.|last2=Cody|first2=Ann Marie|last3=Hedges|first3=Christina L.|last4=Mamajek|first4=Eric E.|last5=Hillenbrand|first5=Lynne A.|last6=Ciardi|first6=David R.|last7=Beichman|first7=Charles A.|last8=Petigura|first8=Erik A.|last9=Fulton|first9=Benjamin J.|last10=Isaacson|first10=Howard T.|last11=Howard|first11=Andrew W.|date=August 2019|title=A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau|journal=The Astronomical Journal|language=en|volume=158|issue=2|pages=79|doi=10.3847/1538-3881/ab290f|arxiv=1902.09670|bibcode=2019AJ....158...79D|s2cid=119003936|issn=0004-6256}}</ref> | Spectral type = K0-1.5<ref name="David_et_al_V1298Taurispectype">{{Cite journal|last1=David|first1=Trevor J.|last2=Cody|first2=Ann Marie|last3=Hedges|first3=Christina L.|last4=Mamajek|first4=Eric E.|last5=Hillenbrand|first5=Lynne A.|last6=Ciardi|first6=David R.|last7=Beichman|first7=Charles A.|last8=Petigura|first8=Erik A.|last9=Fulton|first9=Benjamin J.|last10=Isaacson|first10=Howard T.|last11=Howard|first11=Andrew W.|date=August 2019|title=A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau|journal=The Astronomical Journal|language=en|volume=158|issue=2|pages=79|doi=10.3847/1538-3881/ab290f|arxiv=1902.09670|bibcode=2019AJ....158...79D|s2cid=119003936|issn=0004-6256 |doi-access=free }}</ref>
| Mass = 1.101 | Mass = 1.101
| Radius = 1.345 | Radius = 1.345
Line 1,813: Line 2,004:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = This star is a young ].<ref name="David et al 2">{{Cite journal|last1=David|first1=Trevor J.|last2=Petigura|first2=Erik A.|last3=Luger|first3=Rodrigo|last4=Foreman-Mackey|first4=Daniel|last5=Livingston|first5=John H.|last6=Mamajek|first6=Eric E.|last7=Hillenbrand|first7=Lynne A.|date=2019-10-29|title=Four Newborn Planets Transiting the Young Solar Analog V1298 Tau|journal=The Astrophysical Journal|volume=885|issue=1|pages=L12|arxiv=1910.04563|bibcode=2019ApJ...885L..12D|doi=10.3847/2041-8213/ab4c99|s2cid=204008446|issn=2041-8213}}</ref> | Notes = This star is a young ].<ref name="David et al 2">{{Cite journal|last1=David|first1=Trevor J.|last2=Petigura|first2=Erik A.|last3=Luger|first3=Rodrigo|last4=Foreman-Mackey|first4=Daniel|last5=Livingston|first5=John H.|last6=Mamajek|first6=Eric E.|last7=Hillenbrand|first7=Lynne A.|date=2019-10-29|title=Four Newborn Planets Transiting the Young Solar Analog V1298 Tau|journal=The Astrophysical Journal|volume=885|issue=1|pages=L12|arxiv=1910.04563|bibcode=2019ApJ...885L..12D|doi=10.3847/2041-8213/ab4c99|s2cid=204008446|issn=2041-8213 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,881: Line 2,072:
| Confirmed planets = 5 | Confirmed planets = 5
|Unconfirmed planets = 2 |Unconfirmed planets = 2
| Notes = Planet f has an unusually low density, and might have rings or an extended atmosphere.<ref name=HIP_41378_f>{{Cite journal|last1=Akinsanmi|first1=B.|last2=Santos|first2=N. C.|last3=Faria|first3=J. P.|last4=Oshagh|first4=M.|last5=Barros|first5=S. C. C.|last6=Santerne|first6=A.|last7=Charnoz|first7=S.|date=2020-03-01|title=Can planetary rings explain the extremely low density of HIP 41378 𝑓?|url=https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|journal=Astronomy & Astrophysics|language=en|volume=635|pages=L8|doi=10.1051/0004-6361/202037618| arxiv=2002.11422|issn=0004-6361|doi-access=free}}</ref><ref name=santerneHIP41378f>{{cite arXiv|eprint=1911.07355|last1=Santerne|first1=A.|title=An extremely low-density and temperate giant exoplanet|last2=Malavolta|first2=L.|last3=Kosiarek|first3=M. R.|last4=Dai|first4=F.|last5=Dressing|first5=C. D.|last6=Dumusque|first6=X.|last7=Hara|first7=N. C.|last8=Lopez|first8=T. A.|last9=Mortier|first9=A.|last10=Vanderburg|first10=A.|last11=Adibekyan|first11=V.|last12=Armstrong|first12=D. J.|last13=Barrado|first13=D.|last14=Barros|first14=S. C. C.|last15=Bayliss|first15=D.|last16=Berardo|first16=D.|last17=Boisse|first17=I.|last18=Bonomo|first18=A. S.|last19=Bouchy|first19=F.|last20=Brown|first20=D. J. A.|last21=Buchhave|first21=L. A.|last22=Butler|first22=R. P.|last23=Collier Cameron|first23=A.|last24=Cosentino|first24=R.|last25=Crane|first25=J. D.|last26=Crossfield|first26=I. J. M.|last27=Damasso|first27=M.|last28=Deleuil|first28=M. R.|last29=Delgado Mena|first29=E.|last30=Demangeon|first30=O.|display-authors=29|class=astro-ph.EP|year=2019}}</ref> More planets are still suspected.<ref name="Vanderburg_HIP_41378">{{Cite journal| author = Andrew Vanderburg|display-authors=etal | Notes = Planet f has an unusually low density, and might have rings or an extended atmosphere.<ref name=HIP_41378_f>{{Cite journal|last1=Akinsanmi|first1=B.|last2=Santos|first2=N. C.|last3=Faria|first3=J. P.|last4=Oshagh|first4=M.|last5=Barros|first5=S. C. C.|last6=Santerne|first6=A.|last7=Charnoz|first7=S.|date=2020-03-01|title=Can planetary rings explain the extremely low density of HIP 41378 𝑓?|url=https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|journal=Astronomy & Astrophysics|language=en|volume=635|pages=L8|doi=10.1051/0004-6361/202037618|arxiv=2002.11422|issn=0004-6361|doi-access=free|access-date=2022-03-19|archive-date=2021-10-28|archive-url=https://web.archive.org/web/20211028001745/https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|url-status=live}}</ref><ref name=santerneHIP41378f>{{cite arXiv|eprint=1911.07355|last1=Santerne|first1=A.|title=An extremely low-density and temperate giant exoplanet|last2=Malavolta|first2=L.|last3=Kosiarek|first3=M. R.|last4=Dai|first4=F.|last5=Dressing|first5=C. D.|last6=Dumusque|first6=X.|last7=Hara|first7=N. C.|last8=Lopez|first8=T. A.|last9=Mortier|first9=A.|last10=Vanderburg|first10=A.|last11=Adibekyan|first11=V.|last12=Armstrong|first12=D. J.|last13=Barrado|first13=D.|last14=Barros|first14=S. C. C.|last15=Bayliss|first15=D.|last16=Berardo|first16=D.|last17=Boisse|first17=I.|last18=Bonomo|first18=A. S.|last19=Bouchy|first19=F.|last20=Brown|first20=D. J. A.|last21=Buchhave|first21=L. A.|last22=Butler|first22=R. P.|last23=Collier Cameron|first23=A.|last24=Cosentino|first24=R.|last25=Crane|first25=J. D.|last26=Crossfield|first26=I. J. M.|last27=Damasso|first27=M.|last28=Deleuil|first28=M. R.|last29=Delgado Mena|first29=E.|last30=Demangeon|first30=O.|display-authors=29|class=astro-ph.EP|year=2019}}</ref> More planets are still suspected.<ref name="Vanderburg_HIP_41378">{{Cite journal| author = Andrew Vanderburg|display-authors=etal
| author-link = | author-link =
| arxiv =1606.08441 | arxiv =1606.08441
Line 1,894: Line 2,085:
| bibcode =2016ApJ...827L..10V | bibcode =2016ApJ...827L..10V
|s2cid=8794583 |s2cid=8794583
|doi-access=free
}}</ref> }}</ref>
}} }}
Line 1,927: Line 2,119:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Giant host star | Notes = Host star is
a giant star with spectral type of K0III.<ref>{{Cite web |last=Martin |first=Pierre-Yves |date=2022 |title=Planet HD 33142 c |url=https://exoplanet.eu/catalog/hd_33142_c--6882/ |access-date=2024-02-03 |website=exoplanet.eu |language=en |archive-date=2024-02-03 |archive-url=https://web.archive.org/web/20240203050836/https://exoplanet.eu/catalog/hd_33142_c--6882/ |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,944: Line 2,137:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = A secondary red dwarf is gravitationally bound to K2-148.<ref name=K2-148>{{Cite journal |arxiv = 1710.03239|doi = 10.3847/1538-3881/aaa9c1|title = Exoplanets around Low-mass Stars Unveiled by K2|journal = The Astronomical Journal|volume = 155|issue = 3|pages = 127|year = 2018|last1 = Hirano|first1 = Teruyuki|last2 = Dai|first2 = Fei|last3 = Gandolfi|first3 = Davide|last4 = Fukui|first4 = Akihiko|last5 = Livingston|first5 = John H.|last6 = Miyakawa|first6 = Kohei|last7 = Endl|first7 = Michael|last8 = Cochran|first8 = William D.|last9 = Alonso-Floriano|first9 = Francisco J.|last10 = Kuzuhara|first10 = Masayuki|last11 = Montes|first11 = David|last12 = Ryu|first12 = Tsuguru|last13 = Albrecht|first13 = Simon|last14 = Barragan|first14 = Oscar|last15 = Cabrera|first15 = Juan|last16 = Csizmadia|first16 = Szilard|last17 = Deeg|first17 = Hans|last18 = Eigmüller|first18 = Philipp|last19 = Erikson|first19 = Anders|last20 = Fridlund|first20 = Malcolm|last21 = Grziwa|first21 = Sascha|last22 = Guenther|first22 = Eike W.|last23 = Hatzes|first23 = Artie P.|last24 = Korth|first24 = Judith|last25 = Kudo|first25 = Tomoyuki|last26 = Kusakabe|first26 = Nobuhiko|last27 = Narita|first27 = Norio|last28 = Nespral|first28 = David|last29 = Nowak|first29 = Grzegorz|last30 = Pätzold|first30 = Martin|display-authors = 29|bibcode = 2018AJ....155..127H| s2cid=54590874 }}</ref> | Notes = A secondary red dwarf is gravitationally bound to K2-148.<ref name=K2-148>{{Cite journal |arxiv = 1710.03239|doi = 10.3847/1538-3881/aaa9c1|title = Exoplanets around Low-mass Stars Unveiled by K2|journal = The Astronomical Journal|volume = 155|issue = 3|pages = 127|year = 2018|last1 = Hirano|first1 = Teruyuki|last2 = Dai|first2 = Fei|last3 = Gandolfi|first3 = Davide|last4 = Fukui|first4 = Akihiko|last5 = Livingston|first5 = John H.|last6 = Miyakawa|first6 = Kohei|last7 = Endl|first7 = Michael|last8 = Cochran|first8 = William D.|last9 = Alonso-Floriano|first9 = Francisco J.|last10 = Kuzuhara|first10 = Masayuki|last11 = Montes|first11 = David|last12 = Ryu|first12 = Tsuguru|last13 = Albrecht|first13 = Simon|last14 = Barragan|first14 = Oscar|last15 = Cabrera|first15 = Juan|last16 = Csizmadia|first16 = Szilard|last17 = Deeg|first17 = Hans|last18 = Eigmüller|first18 = Philipp|last19 = Erikson|first19 = Anders|last20 = Fridlund|first20 = Malcolm|last21 = Grziwa|first21 = Sascha|last22 = Guenther|first22 = Eike W.|last23 = Hatzes|first23 = Artie P.|last24 = Korth|first24 = Judith|last25 = Kudo|first25 = Tomoyuki|last26 = Kusakabe|first26 = Nobuhiko|last27 = Narita|first27 = Norio|last28 = Nespral|first28 = David|last29 = Nowak|first29 = Grzegorz|last30 = Pätzold|first30 = Martin|display-authors = 29|bibcode = 2018AJ....155..127H| s2cid=54590874 | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 1,961: Line 2,154:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = 1 |Unconfirmed planets = 1
| Notes = Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone.<ref name="Gilliland2013Kepler-68">{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }}</ref> Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.<ref name="Mills2019Kepler-68">{{cite journal | title=Long-period Giant Companions to Three Compact, Multiplanet Systems | last1=Mills | first1=Sean M. | last2=Howard | first2=Andrew W. | last3=Weiss | first3=Lauren M. | last4=Steffen | first4=Jason H. | last5=Isaacson | first5=Howard | last6=Fulton | first6=Benjamin J. | last7=Petigura | first7=Erik A. | last8=Kosiarek | first8=Molly R. | last9=Hirsch | first9=Lea A. | last10=Boisvert | first10=John H. | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=145 | year=2019 | arxiv=1903.07186 | bibcode=2019AJ....157..145M | doi=10.3847/1538-3881/ab0899 | s2cid=119197547 }}</ref> | Notes = Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone.<ref name="Gilliland2013Kepler-68">{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }}</ref> Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.<ref name="Mills2019Kepler-68">{{cite journal | title=Long-period Giant Companions to Three Compact, Multiplanet Systems | last1=Mills | first1=Sean M. | last2=Howard | first2=Andrew W. | last3=Weiss | first3=Lauren M. | last4=Steffen | first4=Jason H. | last5=Isaacson | first5=Howard | last6=Fulton | first6=Benjamin J. | last7=Petigura | first7=Erik A. | last8=Kosiarek | first8=Molly R. | last9=Hirsch | first9=Lea A. | last10=Boisvert | first10=John H. | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=145 | year=2019 | arxiv=1903.07186 | bibcode=2019AJ....157..145M | doi=10.3847/1538-3881/ab0899 | s2cid=119197547 | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,012: Line 2,205:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Binary with each star orbited by two planets.<ref name="Desidera2014">{{cite journal | title=The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S | url=https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | last1=Desidera | first1=S. | last2=Bonomo | first2=A. S. | last3=Claudi | first3=R. U. | last4=Damasso | first4=M. | last5=Biazzo | first5=K. | last6=Sozzetti | first6=A. | last7=Marzari | first7=F. | last8=Benatti | first8=S. | last9=Gandolfi | first9=D. | last10=Gratton | first10=R. | last11=Lanza | first11=A. F. | last12=Nascimbeni | first12=V. | last13=Andreuzzi | first13=G. | last14=Affer | first14=L. | last15=Barbieri | first15=M. | last16=Bedin | first16=L. R. | last17=Bignamini | first17=A. | last18=Bonavita | first18=M. | last19=Borsa | first19=F. | last20=Calcidese | first20=P. | last21=Christille | first21=J. M. | last22=Cosentino | first22=R. | last23=Covino | first23=E. | last24=Esposito | first24=M. | last25=Giacobbe | first25=P. | last26=Harutyunyan | first26=A. | last27=Latham | first27=D. | last28=Lattanzi | first28=M. | last29=Leto | first29=G. | last30=Lodato | first30=G. | display-authors=1 | journal=Astronomy and Astrophysics | volume=567 | issue=6 | at=L6 | year=2014 | arxiv=1407.0251 | bibcode=2014A&A...567L...6D | doi=10.1051/0004-6361/201424339 | s2cid=118567085 }}</ref><ref name="Damasso et al">{{cite journal | title=A comprehensive analysis of the XO-2 stellar and planetary systems | last1=Damasso | first1=M. | last2=Biazzo | first2=K. | last3=Bonomo | first3=A. S. | last4=Desidera | first4=S. | last5=Lanza | first5=A. F. | last6=Nascimbeni | first6=V. | last7=Esposito | first7=M. | last8=Scandariato | first8=G. | last9=Sozzetti | first9=A. | last10=Cosentino | first10=R. | last11=Gratton | first11=R. | last12=Malavolta | first12=L. | last13=Rainer | first13=M. | last14=Gandolfi | first14=D. | last15=Poretti | first15=E. | last16=Zanmar Sanchez | first16=R. | last17=Ribas | first17=I. | last18=Santos | first18=N. | last19=Affer | first19=L. | last20=Andreuzzi | first20=G. | last21=Barbieri | first21=M. | last22=Bedin | first22=L. R. | last23=Benatti | first23=S. | last24=Bernagozzi | first24=A. | last25=Bertolini | first25=E. | last26=Bonavita | first26=M. | last27=Borsa | first27=F. | last28=Borsato | first28=L. | last29=Boschin | first29=W. | last30=Calcidese | first30=P. | last31=Carbognani | first31=A. | last32=Cenadelli | first32=D. | last33=Christille | first33=J. M. | last34=Claudi | first34=R. U. | last35=Covino | first35=E. | last36=Cunial | first36=A. | last37=Giacobbe | first37=P. | last38=Granata | first38=V. | last39=Harutyunyan | first39=A. | last40=Lattanzi | first40=M. G. | last41=Leto | first41=G. | last42=Libralato | first42=M. | last43=Lodato | first43=G. | last44=Lorenzi | first44=V. | last45=Mancini | first45=L. | last46=Martinez Fiorenzano | first46=A. F. | last47=Marzari | first47=F. | last48=Masiero | first48=S. | last49=Micela | first49=G. | last50=Molinari | first50=E. | last51=Molinaro | first51=M. | last52=Munari | first52=U. | last53=Murabito | first53=S. | last54=Pagano | first54=I. | last55=Pedani | first55=M. | last56=Piotto | first56=G. | last57=Rosenberg | first57=A. | last58=Silvotti | first58=R. | last59=Southworth | first59=J. | display-authors=1 | journal=Astronomy & Astrophysics | volume=575 | at=A111 | year=2015 | doi=10.1051/0004-6361/201425332 | doi-access=free }}</ref> | Notes = Binary with each star orbited by two planets.<ref name="Desidera2014">{{cite journal | title=The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S | url=https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | last1=Desidera | first1=S. | last2=Bonomo | first2=A. S. | last3=Claudi | first3=R. U. | last4=Damasso | first4=M. | last5=Biazzo | first5=K. | last6=Sozzetti | first6=A. | last7=Marzari | first7=F. | last8=Benatti | first8=S. | last9=Gandolfi | first9=D. | last10=Gratton | first10=R. | last11=Lanza | first11=A. F. | last12=Nascimbeni | first12=V. | last13=Andreuzzi | first13=G. | last14=Affer | first14=L. | last15=Barbieri | first15=M. | last16=Bedin | first16=L. R. | last17=Bignamini | first17=A. | last18=Bonavita | first18=M. | last19=Borsa | first19=F. | last20=Calcidese | first20=P. | last21=Christille | first21=J. M. | last22=Cosentino | first22=R. | last23=Covino | first23=E. | last24=Esposito | first24=M. | last25=Giacobbe | first25=P. | last26=Harutyunyan | first26=A. | last27=Latham | first27=D. | last28=Lattanzi | first28=M. | last29=Leto | first29=G. | last30=Lodato | first30=G. | display-authors=1 | journal=Astronomy and Astrophysics | volume=567 | issue=6 | at=L6 | year=2014 | arxiv=1407.0251 | bibcode=2014A&A...567L...6D | doi=10.1051/0004-6361/201424339 | s2cid=118567085 | access-date=2022-06-25 | archive-date=2021-05-11 | archive-url=https://web.archive.org/web/20210511170517/https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | url-status=live }}</ref><ref name="Damasso et al">{{cite journal | title=A comprehensive analysis of the XO-2 stellar and planetary systems | last1=Damasso | first1=M. | last2=Biazzo | first2=K. | last3=Bonomo | first3=A. S. | last4=Desidera | first4=S. | last5=Lanza | first5=A. F. | last6=Nascimbeni | first6=V. | last7=Esposito | first7=M. | last8=Scandariato | first8=G. | last9=Sozzetti | first9=A. | last10=Cosentino | first10=R. | last11=Gratton | first11=R. | last12=Malavolta | first12=L. | last13=Rainer | first13=M. | last14=Gandolfi | first14=D. | last15=Poretti | first15=E. | last16=Zanmar Sanchez | first16=R. | last17=Ribas | first17=I. | last18=Santos | first18=N. | last19=Affer | first19=L. | last20=Andreuzzi | first20=G. | last21=Barbieri | first21=M. | last22=Bedin | first22=L. R. | last23=Benatti | first23=S. | last24=Bernagozzi | first24=A. | last25=Bertolini | first25=E. | last26=Bonavita | first26=M. | last27=Borsa | first27=F. | last28=Borsato | first28=L. | last29=Boschin | first29=W. | last30=Calcidese | first30=P. | last31=Carbognani | first31=A. | last32=Cenadelli | first32=D. | last33=Christille | first33=J. M. | last34=Claudi | first34=R. U. | last35=Covino | first35=E. | last36=Cunial | first36=A. | last37=Giacobbe | first37=P. | last38=Granata | first38=V. | last39=Harutyunyan | first39=A. | last40=Lattanzi | first40=M. G. | last41=Leto | first41=G. | last42=Libralato | first42=M. | last43=Lodato | first43=G. | last44=Lorenzi | first44=V. | last45=Mancini | first45=L. | last46=Martinez Fiorenzano | first46=A. F. | last47=Marzari | first47=F. | last48=Masiero | first48=S. | last49=Micela | first49=G. | last50=Molinari | first50=E. | last51=Molinaro | first51=M. | last52=Munari | first52=U. | last53=Murabito | first53=S. | last54=Pagano | first54=I. | last55=Pedani | first55=M. | last56=Piotto | first56=G. | last57=Rosenberg | first57=A. | last58=Silvotti | first58=R. | last59=Southworth | first59=J. | display-authors=1 | journal=Astronomy & Astrophysics | volume=575 | at=A111 | year=2015 | doi=10.1051/0004-6361/201425332 | doi-access=free | arxiv=1501.01424 }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,078: Line 2,271:
| Metallicity = -0.02 | Metallicity = -0.02
| Age = 7.9 | Age = 7.9
| Confirmed planets = 5 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = The planets are likely in a 1:2:5:7 orbital resonance.<ref name="Heller2019K2-32">{{cite journal | title=Transit least-squares survey. I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance | url=https://www.aanda.org/articles/aa/full_html/2019/05/aa35276-19/aa35276-19.html | last1=Heller | first1=René | last2=Rodenbeck | first2=Kai | last3=Hippke | first3=Michael | journal=Astronomy and Astrophysics | volume=625 | at=A31 | year=2019 | arxiv=1904.00651 | bibcode=2019A&A...625A..31H | bibcode-access=free | doi=10.1051/0004-6361/201935276 | doi-access=free }}</ref> | Notes = The planets are likely in a 1:2:5:7 orbital resonance.<ref name="Heller2019K2-32">{{cite journal | title=Transit least-squares survey. I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance | url=https://www.aanda.org/articles/aa/full_html/2019/05/aa35276-19/aa35276-19.html | last1=Heller | first1=René | last2=Rodenbeck | first2=Kai | last3=Hippke | first3=Michael | journal=Astronomy and Astrophysics | volume=625 | at=A31 | year=2019 | arxiv=1904.00651 | bibcode=2019A&A...625A..31H | bibcode-access=free | doi=10.1051/0004-6361/201935276 | doi-access=free | access-date=2022-03-04 | archive-date=2022-01-25 | archive-url=https://web.archive.org/web/20220125190022/https://www.aanda.org/articles/aa/full_html/2019/05/aa35276-19/aa35276-19.html | url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,139: Line 2,332:
| Right ascension = {{RA|19|54|36.6}} | Right ascension = {{RA|19|54|36.6}}
| Declination = {{DEC|+43|57|18}} | Declination = {{DEC|+43|57|18}}
| Apparent magnitude = 15.29<ref name="Souto2017">{{Cite journal|arxiv=1612.01598|last1=Souto|first1=Diogo|title=Chemical Abundances of M-dwarfs from the APOGEE Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186|journal=The Astrophysical Journal|volume=835|issue=2|pages=239|last2=Cunha|first2=Katia|last3= Garcia-Hernandez|first3=D. A.|last4=Zamora|first4=Olga|last5= Allende Prieto|first5=C.|last6=Smith|first6=Verne|last7=Mahadevan|first7=Suvrath|last8=Blake|first8=Cullen|last9= Johnson|first9=J. A.|last10=Jonsson|first10=Henrik|last11=Pinsonneault|first11=Marc|last12=Holtzman|first12=Jon|last13= Majewski|first13=S. R.|last14=Shetrone|first14=Matthew|last15=Teske|first15=Johanna|last16=Nidever|first16=David|last17=Schiavon|first17=Ricardo|last18=Sobeck|first18=Jennifer|last19= Garcia Perez|first19=A. E.|last20= Gomez Maqueo Chew|first20=Y.|last21=Stassun|first21=Keivan|display-authors=1|year=2017|bibcode=2017ApJ...835..239S|doi=10.3847/1538-4357/835/2/239|s2cid=73634716}}</ref> | Apparent magnitude = 15.29<ref name="Souto2017">{{Cite journal|arxiv=1612.01598|last1=Souto|first1=Diogo|title=Chemical Abundances of M-dwarfs from the APOGEE Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186|journal=The Astrophysical Journal|volume=835|issue=2|pages=239|last2=Cunha|first2=Katia|last3= Garcia-Hernandez|first3=D. A.|last4=Zamora|first4=Olga|last5= Allende Prieto|first5=C.|last6=Smith|first6=Verne|last7=Mahadevan|first7=Suvrath|last8=Blake|first8=Cullen|last9= Johnson|first9=J. A.|last10=Jonsson|first10=Henrik|last11=Pinsonneault|first11=Marc|last12=Holtzman|first12=Jon|last13= Majewski|first13=S. R.|last14=Shetrone|first14=Matthew|last15=Teske|first15=Johanna|last16=Nidever|first16=David|last17=Schiavon|first17=Ricardo|last18=Sobeck|first18=Jennifer|last19= Garcia Perez|first19=A. E.|last20= Gomez Maqueo Chew|first20=Y.|last21=Stassun|first21=Keivan|display-authors=1|year=2017|bibcode=2017ApJ...835..239S|doi=10.3847/1538-4357/835/2/239|s2cid=73634716 |doi-access=free }}</ref>
| Distance = 579.23<ref name="GaiaDR2Specific4DistancesKepler-186">{{cite journal |title=Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2 |journal=The Astronomical Journal |last1=Bailer-Jones |first1=C. A. L. |last2=Rybizki |first2=J. |last3=Fouesneau |first3=M. |last4=Mantelet |first4=G. |last5=Andrae |first5=R. |display-authors=1 |volume=156 |issue=2 |pages=58 |date=August 2018 |doi=10.3847/1538-3881/aacb21 |bibcode=2018AJ....156...58B |arxiv=1804.10121|s2cid=119289017 }}</ref> | Distance = 579.23<ref name="GaiaDR2Specific4DistancesKepler-186">{{cite journal |title=Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2 |journal=The Astronomical Journal |last1=Bailer-Jones |first1=C. A. L. |last2=Rybizki |first2=J. |last3=Fouesneau |first3=M. |last4=Mantelet |first4=G. |last5=Andrae |first5=R. |display-authors=1 |volume=156 |issue=2 |pages=58 |date=August 2018 |doi=10.3847/1538-3881/aacb21 |bibcode=2018AJ....156...58B |arxiv=1804.10121|s2cid=119289017 |doi-access=free }} {{Webarchive|url=https://web.archive.org/web/20220511093334/http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-ref=VIZ5d5b5b10086b&-out.add=.&-source=I/347/gaia2dis&-c=298.65273597008%20%2b43.95498841816,eq=ICRS,rs=2&-out.orig=o |date=2022-05-11 }}</ref>
| Spectral type = M1V<ref name=NASAExoplanetKepler-186f>{{cite web|url=http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-186+f|title=Kepler-186 f|work=NASA Exoplanet Archive|access-date=19 July 2016}}</ref> | Spectral type = M1V<ref name=NASAExoplanetKepler-186f>{{cite web|url=http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-186+f|title=Kepler-186 f|work=NASA Exoplanet Archive|access-date=19 July 2016|archive-date=18 March 2022|archive-url=https://web.archive.org/web/20220318185724/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-186+f|url-status=live}}</ref>
| Mass = 0.478 | Mass = 0.478
| Radius = 0.472 | Radius = 0.472
Line 2,149: Line 2,342:
| Confirmed planets = 5 | Confirmed planets = 5
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.<ref name="SCI-20140418">{{Cite journal| doi = 10.1126/science.1249403| title = An Earth-Sized Planet in the Habitable Zone of a Cool Star| journal = ]| volume = 344| issue = 6181| pages = 277–280| date = 2014-04-18| arxiv=1404.5667| last1 = Quintana | first1 = E. V.| last2 = Barclay | first2 = T.| last3 = Raymond | first3 = S. N.| last4 = Rowe | first4 = J. F.| last5 = Bolmont | first5 = E.| last6 = Caldwell | first6 = D. A.| last7 = Howell | first7 = S. B.| last8 = Kane | first8 = S. R.| last9 = Huber | first9 = D.| last10 = Crepp | first10 = J. R.| last11 = Lissauer | first11 = J. J. | author-link11=Jack J. Lissauer| last12 = Ciardi | first12 = D. R.| last13 = Coughlin | first13 = J. L.| last14 = Everett | first14 = M. E.| last15 = Henze | first15 = C. E.| last16 = Horch | first16 = E.| last17 = Isaacson | first17 = H.| last18 = Ford | first18 = E. B.| last19 = Adams | first19 = F. C.| last20 = Still | first20 = M.| last21 = Hunter | first21 = R. C.| last22 = Quarles | first22 = B.| last23 = Selsis | first23 = F.|bibcode = 2014Sci...344..277Q | pmid=24744370| s2cid = 1892595}} free version = http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf</ref> | Notes = Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.<ref name="SCI-20140418">{{Cite journal| doi = 10.1126/science.1249403| title = An Earth-Sized Planet in the Habitable Zone of a Cool Star| journal = ]| volume = 344| issue = 6181| pages = 277–280| date = 2014-04-18| arxiv=1404.5667| last1 = Quintana | first1 = E. V.| last2 = Barclay | first2 = T.| last3 = Raymond | first3 = S. N.| last4 = Rowe | first4 = J. F.| last5 = Bolmont | first5 = E.| last6 = Caldwell | first6 = D. A.| last7 = Howell | first7 = S. B.| last8 = Kane | first8 = S. R.| last9 = Huber | first9 = D.| last10 = Crepp | first10 = J. R.| last11 = Lissauer | first11 = J. J. | author-link11=Jack J. Lissauer| last12 = Ciardi | first12 = D. R.| last13 = Coughlin | first13 = J. L.| last14 = Everett | first14 = M. E.| last15 = Henze | first15 = C. E.| last16 = Horch | first16 = E.| last17 = Isaacson | first17 = H.| last18 = Ford | first18 = E. B.| last19 = Adams | first19 = F. C.| last20 = Still | first20 = M.| last21 = Hunter | first21 = R. C.| last22 = Quarles | first22 = B.| last23 = Selsis | first23 = F.|bibcode = 2014Sci...344..277Q | pmid=24744370| s2cid = 1892595}} free version = http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf {{Webarchive|url=https://web.archive.org/web/20140418183443/http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf |date=2014-04-18 }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,200: Line 2,393:
| Confirmed planets = 6 | Confirmed planets = 6
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planet g was not fully verified, or could be two long-period planets instead.<ref name="Christiansen">{{Cite journal|first1=Jessie L. |last1=Christiansen |first2=Ian J. M. |last2=Crossfield |first3=Geert |last3=Barentsen |first4=Chris J. |last4=Lintott |first5=Thomas |last5=Barclay |first6=Brooke D. |last6=Simmons |first7=Erik |last7=Petigura |first8=Joshua E. |last8=Schlieder |first9=Courtney D. |last9=Dressing |first10=Andrew |last10=Vanderburg |first11=David R. |last11=Ciardi |first12=Campbell |last12=Allen |first13=Adam |last13=McMaster |first14=Grant |last14=Miller |first15=Martin |last15=Veldthuis |first16=Sarah |last16=Allen |first17=Zach |last17=Wolfenbarger |first18=Brian |last18=Cox |first19=Julia |last19=Zemiro |first20=Andrew W. |last20=Howard |first21=John |last21=Livingston |first22=Evan |last22=Sinukoff |first23=Timothy |last23=Catron |first24=Andrew |last24=Grey |first25=Joshua J. E. |last25=Kusch |first26=Ivan |last26=Terentev |first27=Martin |last27=Vales |first28=Martti H. |last28=Kristiansen|date=2018-01-11|title=The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists|journal=The Astronomical Journal|language=en|volume=155|issue=2|pages=57|arxiv=1801.03874|doi=10.3847/1538-3881/aa9be0|issn=1538-3881|bibcode=2018AJ....155...57C |s2cid=52971376 }}</ref> | Notes = Planet g was not fully verified, or could be two long-period planets instead.<ref name="Christiansen">{{Cite journal|first1=Jessie L. |last1=Christiansen |first2=Ian J. M. |last2=Crossfield |first3=Geert |last3=Barentsen |first4=Chris J. |last4=Lintott |first5=Thomas |last5=Barclay |first6=Brooke D. |last6=Simmons |first7=Erik |last7=Petigura |first8=Joshua E. |last8=Schlieder |first9=Courtney D. |last9=Dressing |first10=Andrew |last10=Vanderburg |first11=David R. |last11=Ciardi |first12=Campbell |last12=Allen |first13=Adam |last13=McMaster |first14=Grant |last14=Miller |first15=Martin |last15=Veldthuis |first16=Sarah |last16=Allen |first17=Zach |last17=Wolfenbarger |first18=Brian |last18=Cox |first19=Julia |last19=Zemiro |first20=Andrew W. |last20=Howard |first21=John |last21=Livingston |first22=Evan |last22=Sinukoff |first23=Timothy |last23=Catron |first24=Andrew |last24=Grey |first25=Joshua J. E. |last25=Kusch |first26=Ivan |last26=Terentev |first27=Martin |last27=Vales |first28=Martti H. |last28=Kristiansen|date=2018-01-11|title=The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists|journal=The Astronomical Journal|language=en|volume=155|issue=2|pages=57|arxiv=1801.03874|doi=10.3847/1538-3881/aa9be0|issn=1538-3881|bibcode=2018AJ....155...57C |s2cid=52971376 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,234: Line 2,427:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = One planet is a gas giant which orbits in the habitable zone.<ref name="WASP-47habzone">{{Cite journal|last1=Becker|first1=Juliette C.|last2=Vanderburg|first2=Andrew|last3=Adams|first3=Fred C.|last4=Rappaport|first4=Saul A.|last5=Schwengeler|first5=Hans Martin|title=Wasp-47: A Hot Jupiter System with Two Additional Planets Discovered by K2|date=2015-10-12|journal=The Astrophysical Journal|language=en|volume=812|issue=2|pages=L18|doi=10.1088/2041-8205/812/2/L18|issn=2041-8213|arxiv=1508.02411|bibcode=2015ApJ...812L..18B|s2cid=14681933}}</ref><ref name="Neveu-VanMalle2016">{{cite journal | title=Hot Jupiters with relatives: Discovery of additional planets in orbit around WASP-41 and WASP-47 | url=https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | last1=Neveu-VanMalle | first1=M. | last2=Queloz | first2=D. | last3=Anderson | first3=D. R. | last4=Brown | first4=D. J. A. | last5=Collier Cameron | first5=A. | last6=Delrez | first6=L. | last7=Díaz | first7=R. F. | last8=Gillon | first8=M. | last9=Hellier | first9=C. | last10=Jehin | first10=E. | last11=Lister | first11=T. | last12=Pepe | first12=F. | last13=Rojo | first13=P. | last14=Ségransan | first14=D. | last15=Triaud | first15=A. H. M. J. | last16=Turner | first16=O. D. | last17=Udry | first17=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=586 | at=A93 | year=2016 | arxiv=1509.07750 | bibcode=2016A&A...586A..93N | doi=10.1051/0004-6361/201526965 | s2cid=53354547 }}</ref> WASP-47 is the only planetary system known to have both planets near the hot Jupiter and another planet much further out.<ref name="caltech.eduWASP-47">{{cite web|url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|title=WASP-47|website=exoplanetarchive.ipac.caltech.edu}}</ref> | Notes = One planet is a gas giant which orbits in the habitable zone.<ref name="WASP-47habzone">{{Cite journal|last1=Becker|first1=Juliette C.|last2=Vanderburg|first2=Andrew|last3=Adams|first3=Fred C.|last4=Rappaport|first4=Saul A.|last5=Schwengeler|first5=Hans Martin|title=Wasp-47: A Hot Jupiter System with Two Additional Planets Discovered by K2|date=2015-10-12|journal=The Astrophysical Journal|language=en|volume=812|issue=2|pages=L18|doi=10.1088/2041-8205/812/2/L18|issn=2041-8213|arxiv=1508.02411|bibcode=2015ApJ...812L..18B|s2cid=14681933}}</ref><ref name="Neveu-VanMalle2016">{{cite journal | title=Hot Jupiters with relatives: Discovery of additional planets in orbit around WASP-41 and WASP-47 | url=https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | last1=Neveu-VanMalle | first1=M. | last2=Queloz | first2=D. | last3=Anderson | first3=D. R. | last4=Brown | first4=D. J. A. | last5=Collier Cameron | first5=A. | last6=Delrez | first6=L. | last7=Díaz | first7=R. F. | last8=Gillon | first8=M. | last9=Hellier | first9=C. | last10=Jehin | first10=E. | last11=Lister | first11=T. | last12=Pepe | first12=F. | last13=Rojo | first13=P. | last14=Ségransan | first14=D. | last15=Triaud | first15=A. H. M. J. | last16=Turner | first16=O. D. | last17=Udry | first17=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=586 | at=A93 | year=2016 | arxiv=1509.07750 | bibcode=2016A&A...586A..93N | doi=10.1051/0004-6361/201526965 | s2cid=53354547 | access-date=2022-05-08 | archive-date=2022-02-28 | archive-url=https://web.archive.org/web/20220228025245/https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | url-status=live }}</ref> WASP-47 is the only planetary system known to have both planets near the ] and another planet much further out.<ref name="caltech.eduWASP-47">{{cite web|url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|title=WASP-47|website=exoplanetarchive.ipac.caltech.edu|access-date=2022-05-08|archive-date=2022-05-08|archive-url=https://web.archive.org/web/20220508114227/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|url-status=live}}</ref>
}} }}


Line 2,332: Line 2,525:
|last1=Schneider |last1=Schneider
|title=Star: Kepler-25 |title=Star: Kepler-25
|encyclopedia=]
|publisher=Paris Observatory
|url=http://exoplanet.eu/star.php?st=Kepler-25 |url=http://exoplanet.eu/star.php?st=Kepler-25
|access-date=2013-12-18 |access-date=2013-12-18
|url-status=dead |url-status=dead
|archive-url=https://web.archive.org/web/20120616125118/http://exoplanet.eu/star.php?st=Kepler-25 |archive-url=https://web.archive.org/web/20120616125118/http://exoplanet.eu/star.php?st=Kepler-25
|encyclopedia=]
|archive-date=2012-06-16 |archive-date=2012-06-16
}}</ref> }}</ref>
Line 2,407: Line 2,599:
| Apparent magnitude = 13.002 | Apparent magnitude = 13.002
| Distance = 976 | Distance = 976
| Spectral type = K0V<ref name="Nespral2017">{{cite journal | title=Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations | url=https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | last1=Nespral | first1=D. | last2=Gandolfi | first2=D. | last3=Deeg | first3=H. J. | last4=Borsato | first4=L. | last5=Fridlund | first5=M. C. V. | last6=Barragán | first6=O. | last7=Alonso | first7=R. | last8=Grziwa | first8=S. | last9=Korth | first9=J. | last10=Albrecht | first10=S. | last11=Cabrera | first11=J. | last12=Csizmadia | first12=Sz. | last13=Nowak | first13=G. | last14=Kuutma | first14=T. | last15=Saario | first15=J. | last16=Eigmüller | first16=P. | last17=Erikson | first17=A. | last18=Guenther | first18=E. W. | last19=Hatzes | first19=A. P. | last20=Montañés Rodríguez | first20=P. | last21=Palle | first21=E. | last22=Pätzold | first22=M. | last23=Prieto-Arranz | first23=J. | last24=Rauer | first24=H. | last25=Sebastian | first25=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=601 | at=A128 | year=2017 | arxiv=1604.01265 | bibcode=2017A&A...601A.128N | doi=10.1051/0004-6361/201628639 | s2cid=55978628 }}</ref> or G9V<ref name="Sinukoff2016">{{cite journal | title=Eleven Multiplanet Systems From K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths | last1=Sinukoff | first1=Evan | last2=Howard | first2=Andrew W. | last3=Petigura | first3=Erik A. | last4=Schlieder | first4=Joshua E. | last5=Crossfield | first5=Ian J. M. | last6=Ciardi | first6=David R. | last7=Fulton | first7=Benjamin J. | last8=Isaacson | first8=Howard | last9=Aller | first9=Kimberly M. | last10=Baranec | first10=Christoph | last11=Beichman | first11=Charles A. | last12=Hansen | first12=Brad M. S. | last13=Knutson | first13=Heather A. | last14=Law | first14=Nicholas M. | last15=Liu | first15=Michael C. | last16=Riddle | first16=Reed | last17=Dressing | first17=Courtney D. | display-authors=1 | journal=The Astrophysical Journal | volume=827 | issue=1 | at=78 | year=2016 | arxiv=1511.09213 | bibcode=2016ApJ...827...78S | doi=10.3847/0004-637X/827/1/78 | doi-access=free }}</ref> | Spectral type = K0V<ref name="Nespral2017">{{cite journal | title=Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations | url=https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | last1=Nespral | first1=D. | last2=Gandolfi | first2=D. | last3=Deeg | first3=H. J. | last4=Borsato | first4=L. | last5=Fridlund | first5=M. C. V. | last6=Barragán | first6=O. | last7=Alonso | first7=R. | last8=Grziwa | first8=S. | last9=Korth | first9=J. | last10=Albrecht | first10=S. | last11=Cabrera | first11=J. | last12=Csizmadia | first12=Sz. | last13=Nowak | first13=G. | last14=Kuutma | first14=T. | last15=Saario | first15=J. | last16=Eigmüller | first16=P. | last17=Erikson | first17=A. | last18=Guenther | first18=E. W. | last19=Hatzes | first19=A. P. | last20=Montañés Rodríguez | first20=P. | last21=Palle | first21=E. | last22=Pätzold | first22=M. | last23=Prieto-Arranz | first23=J. | last24=Rauer | first24=H. | last25=Sebastian | first25=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=601 | at=A128 | year=2017 | arxiv=1604.01265 | bibcode=2017A&A...601A.128N | doi=10.1051/0004-6361/201628639 | s2cid=55978628 | access-date=2022-03-18 | archive-date=2022-05-04 | archive-url=https://web.archive.org/web/20220504003941/https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | url-status=live }}</ref> or G9V<ref name="Sinukoff2016">{{cite journal | title=Eleven Multiplanet Systems From K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths | last1=Sinukoff | first1=Evan | last2=Howard | first2=Andrew W. | last3=Petigura | first3=Erik A. | last4=Schlieder | first4=Joshua E. | last5=Crossfield | first5=Ian J. M. | last6=Ciardi | first6=David R. | last7=Fulton | first7=Benjamin J. | last8=Isaacson | first8=Howard | last9=Aller | first9=Kimberly M. | last10=Baranec | first10=Christoph | last11=Beichman | first11=Charles A. | last12=Hansen | first12=Brad M. S. | last13=Knutson | first13=Heather A. | last14=Law | first14=Nicholas M. | last15=Liu | first15=Michael C. | last16=Riddle | first16=Reed | last17=Dressing | first17=Courtney D. | display-authors=1 | journal=The Astrophysical Journal | volume=827 | issue=1 | at=78 | year=2016 | arxiv=1511.09213 | bibcode=2016ApJ...827...78S | doi=10.3847/0004-637X/827/1/78 | doi-access=free }}</ref>
| Mass = 0.918 | Mass = 0.918
| Radius = 0.881±0.111 | Radius = 0.881±0.111
Line 2,417: Line 2,609:
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
| Star = PSR B1257+12 | Star = PSR B1257+12|Lich
| Constellation = Virgo (constellation){{!}}Virgo | Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|13|00|03.58}} | Right ascension = {{RA|13|00|03.58}}
Line 2,448: Line 2,640:
| Confirmed planets = 5 | Confirmed planets = 5
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Planets e and f orbit in the habitable zone.<ref name = "BoruckiKepler-62">{{Cite journal | last=Borucki | first=William J. | author-link=William J. Borucki |display-authors=etal | title=Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone | journal=Science Express| date=18 April 2013 | doi=10.1126/science.1234702 | access-date=18 March 2022|url=https://www.science.org/doi/10.1126/science.1234702|arxiv = 1304.7387 |bibcode = 2013Sci...340..587B | pmid=23599262 | volume=340 | issue=6132 | pages=587–90| hdl=1721.1/89668 | s2cid=21029755 }}</ref><ref name="NASA-20130418">{{cite web |last1=Johnson |first1=Michele |last2=Harrington |first2=J.D. |title=NASA's Kepler Discovers Its Smallest 'Habitable Zone' Planets to Date |url=http://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |date=18 April 2013 |work=] |access-date=18 March 2022}}</ref> | Notes = Planets e and f orbit in the habitable zone.<ref name = "BoruckiKepler-62">{{Cite journal | last=Borucki | first=William J. | author-link=William J. Borucki | display-authors=etal | title=Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone | journal=Science Express | date=18 April 2013 | doi=10.1126/science.1234702 | access-date=18 March 2022 | url=https://www.science.org/doi/10.1126/science.1234702 | arxiv=1304.7387 | bibcode=2013Sci...340..587B | pmid=23599262 | volume=340 | issue=6132 | pages=587–90 | hdl=1721.1/89668 | s2cid=21029755 | archive-date=2 May 2022 | archive-url=https://web.archive.org/web/20220502115940/https://www.science.org/doi/10.1126/science.1234702 | url-status=live }}</ref><ref name="NASA-20130418">{{cite web |last1=Johnson |first1=Michele |last2=Harrington |first2=J.D. |title=NASA's Kepler Discovers Its Smallest 'Habitable Zone' Planets to Date |url=http://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |date=18 April 2013 |work=] |access-date=18 March 2022 |archive-date=8 May 2020 |archive-url=https://web.archive.org/web/20200508010029/https://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |url-status=dead }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,463: Line 2,655:
| Metallicity = -0.216 | Metallicity = -0.216
| Age = | Age =
| Confirmed planets = 4 | Confirmed planets = 5
|Unconfirmed planets = |Unconfirmed planets =
| Notes = | Notes =
Line 2,480: Line 2,672:
| Metallicity = 0.02 | Metallicity = 0.02
| Age = 6.5 | Age = 6.5
| Confirmed planets = 3 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = | Notes =
Line 2,650: Line 2,842:
| Confirmed planets = 4 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Transiting exoplanets<ref name=Steffen2012>{{citation|arxiv=1201.5412|title=Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations|year=2012|doi=10.1111/j.1365-2966.2012.20467.x|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Ford|first3=Eric B.|last4=Carter|first4=Joshua A.|last5=Desert|first5=Jean-Michel|last6=Fressin|first6=Francois|last7=Holman|first7=Matthew J.|last8=Lissauer|first8=Jack J.|last9=Moorhead|first9=Althea V.|last10=Rowe|first10=Jason F.|last11=Ragozzine|first11=Darin|last12=Welsh|first12=William F.|last13=Batalha|first13=Natalie M.|last14=Borucki|first14=William J.|last15=Buchhave|first15=Lars A.|last16=Bryson|first16=Steve|last17=Caldwell|first17=Douglas A.|last18=Charbonneau|first18=David|last19=Ciardi|first19=David R.|last20=Cochran|first20=William D.|last21=Endl|first21=Michael|last22=Everett|first22=Mark E.|last23=Gautier III|first23=Thomas N.|last24=Gilliland|first24=Ron L.|last25=Girouard|first25=Forrest R.|last26=Jenkins|first26=Jon M.|last27=Horch|first27=Elliott|last28=Howell|first28=Steve B.|last29=Isaacson|first29=Howard|last30=Klaus|first30=Todd C.|journal=Monthly Notices of the Royal Astronomical Society |volume=421 |issue=3 |bibcode=2012MNRAS.421.2342S |s2cid=11898578|display-authors=29}}</ref> which are low-density planets below the size of ].<ref name=Cubillos2016>{{citation|arxiv=1611.09236|title=An overabundance of low-density Neptune-like planets|year=2016|doi=10.1093/mnras/stw3103|last1=Cubillos|first1=Patricio|last2=Erkaev|first2=Nikolai V.|last3=Juvan|first3=Ines|last4=Fossati|first4=Luca|last5=Johnstone|first5=Colin P.|last6=Lammer|first6=Helmut|last7=Lendl|first7=Monika|last8=Odert|first8=Petra|last9=Kislyakova|first9=Kristina G.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|issue=2|pages=1868–1879|s2cid=119408956}}</ref><ref name=Jontof2015>{{citation|arxiv=1512.02003|title=Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M<sub>🜨</sub> with Diverse Densities and Incident Fluxes|year=2015|doi=10.3847/0004-637X/820/1/39|last1=Jontof-Hutter|first1=Daniel|last2=Ford|first2=Eric B.|last3=Rowe|first3=Jason F.|last4=Lissauer|first4=Jack J.|last5=Fabrycky|first5=Daniel C.|author6=Christa Van Laerhoven|last7=Agol|first7=Eric|last8=Deck|first8=Katherine M.|last9=Holczer|first9=Tomer|last10=Mazeh|first10=Tsevi|s2cid=11322397}}</ref> | Notes = Transiting exoplanets<ref name=Steffen2012>{{citation|arxiv=1201.5412|title=Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations|year=2012|doi=10.1111/j.1365-2966.2012.20467.x|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Ford|first3=Eric B.|last4=Carter|first4=Joshua A.|last5=Desert|first5=Jean-Michel|last6=Fressin|first6=Francois|last7=Holman|first7=Matthew J.|last8=Lissauer|first8=Jack J.|last9=Moorhead|first9=Althea V.|last10=Rowe|first10=Jason F.|last11=Ragozzine|first11=Darin|last12=Welsh|first12=William F.|last13=Batalha|first13=Natalie M.|last14=Borucki|first14=William J.|last15=Buchhave|first15=Lars A.|last16=Bryson|first16=Steve|last17=Caldwell|first17=Douglas A.|last18=Charbonneau|first18=David|last19=Ciardi|first19=David R.|last20=Cochran|first20=William D.|last21=Endl|first21=Michael|last22=Everett|first22=Mark E.|last23=Gautier III|first23=Thomas N.|last24=Gilliland|first24=Ron L.|last25=Girouard|first25=Forrest R.|last26=Jenkins|first26=Jon M.|last27=Horch|first27=Elliott|last28=Howell|first28=Steve B.|last29=Isaacson|first29=Howard|last30=Klaus|first30=Todd C.|journal=Monthly Notices of the Royal Astronomical Society |volume=421 |issue=3 |doi-access=free |bibcode=2012MNRAS.421.2342S |s2cid=11898578|display-authors=29}}</ref> which are low-density planets below the size of ].<ref name=Cubillos2016>{{citation|arxiv=1611.09236|title=An overabundance of low-density Neptune-like planets|year=2016|doi=10.1093/mnras/stw3103|last1=Cubillos|first1=Patricio|last2=Erkaev|first2=Nikolai V.|last3=Juvan|first3=Ines|last4=Fossati|first4=Luca|last5=Johnstone|first5=Colin P.|last6=Lammer|first6=Helmut|last7=Lendl|first7=Monika|last8=Odert|first8=Petra|last9=Kislyakova|first9=Kristina G.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|issue=2|pages=1868–1879|doi-access=free |s2cid=119408956}}</ref><ref name=Jontof2015>{{citation|arxiv=1512.02003|title=Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M<sub>🜨</sub> with Diverse Densities and Incident Fluxes|year=2015|doi=10.3847/0004-637X/820/1/39|last1=Jontof-Hutter|first1=Daniel|last2=Ford|first2=Eric B.|last3=Rowe|first3=Jason F.|last4=Lissauer|first4=Jack J.|last5=Fabrycky|first5=Daniel C.|author6=Christa Van Laerhoven|last7=Agol|first7=Eric|last8=Deck|first8=Katherine M.|last9=Holczer|first9=Tomer|last10=Mazeh|first10=Tsevi|journal=The Astrophysical Journal |volume=820 |issue=1 |page=39 |s2cid=11322397 |doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,718: Line 2,910:
| Confirmed planets = 6 | Confirmed planets = 6
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Red dwarf star with six confirmed planets.<ref name="Xie2013Kepler-80">{{cite journal|last1=Xie|first1=J.-W.|year=2013|title=Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems|journal=Astrophysical Journal Supplement Series|volume=208|issue=2|pages=22|arxiv=1208.3312|bibcode=2013ApJS..208...22X|doi=10.1088/0067-0049/208/2/22|s2cid=17160267}}</ref><ref name="Shallue2017">{{cite journal|last1=Shallue|first1=C. J.|last2=Vanderburg|first2=A.|date=2017|title=Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90|url=https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|journal=]|volume=155|issue=2|pages=94|arxiv=1712.05044|bibcode=2018AJ....155...94S|doi=10.3847/1538-3881/aa9e09|s2cid=4535051|access-date=2017-12-15}}</ref> Five of them are in an ].<ref name="MacDonald2016">{{Cite journal|last1=MacDonald|first1=Mariah G.|last2=Ragozzine|first2=Darin|last3=Fabrycky|first3=Daniel C.|last4=Ford|first4=Eric B.|last5=Holman|first5=Matthew J.|last6=Isaacson|first6=Howard T.|last7=Lissauer|first7=Jack J.|last8=Lopez|first8=Eric D.|last9=Mazeh|first9=Tsevi|date=2016-01-01|title=A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets|url=http://stacks.iop.org/1538-3881/152/i=4/a=105|journal=The Astronomical Journal|volume=152|issue=4|pages=105|doi=10.3847/0004-6256/152/4/105|arxiv = 1607.07540 |bibcode = 2016AJ....152..105M |s2cid=119265122}}</ref><ref name="Shallue2017" /> | Notes = Red dwarf star with six confirmed planets.<ref name="Xie2013Kepler-80">{{cite journal|last1=Xie|first1=J.-W.|year=2013|title=Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems|journal=Astrophysical Journal Supplement Series|volume=208|issue=2|pages=22|arxiv=1208.3312|bibcode=2013ApJS..208...22X|doi=10.1088/0067-0049/208/2/22|s2cid=17160267}}</ref><ref name="Shallue2017">{{cite journal|last1=Shallue|first1=C. J.|last2=Vanderburg|first2=A.|date=2017|title=Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90|url=https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|journal=]|volume=155|issue=2|pages=94|arxiv=1712.05044|bibcode=2018AJ....155...94S|doi=10.3847/1538-3881/aa9e09|s2cid=4535051|access-date=2017-12-15|doi-access=free|archive-date=2017-12-24|archive-url=https://web.archive.org/web/20171224094458/https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|url-status=live}}</ref> Five of them are in an ].<ref name="MacDonald2016">{{Cite journal|last1=MacDonald|first1=Mariah G.|last2=Ragozzine|first2=Darin|last3=Fabrycky|first3=Daniel C.|last4=Ford|first4=Eric B.|last5=Holman|first5=Matthew J.|last6=Isaacson|first6=Howard T.|last7=Lissauer|first7=Jack J.|last8=Lopez|first8=Eric D.|last9=Mazeh|first9=Tsevi|date=2016-01-01|title=A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets|url=http://stacks.iop.org/1538-3881/152/i=4/a=105|journal=The Astronomical Journal|volume=152|issue=4|pages=105|doi=10.3847/0004-6256/152/4/105|arxiv = 1607.07540 |bibcode = 2016AJ....152..105M |s2cid=119265122 |doi-access=free }}</ref><ref name="Shallue2017" />
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 2,819: Line 3,011:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-1338
| Constellation = Pictor
| Right ascension = {{RA|06|08|31.97}}
| Declination = {{DEC|+59|32|28.1}}
| Apparent magnitude = 11.72
| Distance = 1318
| Spectral type = F8 <br> M
| Mass = 1.127
| Radius = 1.331/0.309
| Temperature = 6160
| Metallicity = 0.01
| Age = 4.4
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes = | Notes =
}} }}
Line 2,862: Line 3,071:
| Apparent magnitude = | Apparent magnitude =
| Distance = 1340 | Distance = 1340
| Spectral type = ]+M | Spectral type = ] <br> M
| Mass = 0.48+0.12 | Mass = 0.48+0.12
| Radius = | Radius =
Line 2,870: Line 3,079:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Three circumbinary planets orbit around the Kepler-451 binary pair.<ref name=Esmer2022_Kepler-451>{{citation|arxiv=2202.02118|year=2022|title=Detection of two additional circumbinary planets around Kepler-451|author1=Ekrem Murat Esmer|last2=Baştürk|first2=Özgür|author3=Selim Osman Selam|last4=Aliş|first4=Sinan|journal=Monthly Notices of the Royal Astronomical Society |volume=511 |issue=4 |pages=5207–5216 |doi=10.1093/mnras/stac357 }}</ref> | Notes = Three circumbinary planets orbit around the Kepler-451 binary pair.<ref name=Esmer2022_Kepler-451>{{citation|arxiv=2202.02118|year=2022|title=Detection of two additional circumbinary planets around Kepler-451|author1=Ekrem Murat Esmer|last2=Baştürk|first2=Özgür|author3=Selim Osman Selam|last4=Aliş|first4=Sinan|journal=Monthly Notices of the Royal Astronomical Society |volume=511 |issue=4 |pages=5207–5216 |doi=10.1093/mnras/stac357 |doi-access=free |bibcode=2022MNRAS.511.5207E }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,203: Line 3,412:
| Metallicity = -0.079 | Metallicity = -0.079
| Age = | Age =
| Confirmed planets = 3 | Confirmed planets = 4
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Super-puff planets with some of the lowest densities known.<ref name="Kepler-51">{{cite journal | Notes = Super-puff planets with some of the lowest densities known.<ref name="Kepler-51">{{cite journal
Line 3,213: Line 3,422:
| first9=Jonathan J. | last9=Fortney | first10=Michael R. | last10=Line | first9=Jonathan J. | last9=Fortney | first10=Michael R. | last10=Line
| first11=Roberto | last11=Sanchis-Ojeda | first12=Joshua N. | last12=Winn | first11=Roberto | last11=Sanchis-Ojeda | first12=Joshua N. | last12=Winn
| journal=The Astronomical Journal | year=2020 | volume=159 | issue=2 | page=57 | display-authors=1 | doi=10.3847/1538-3881/ab5d36 | arxiv=1910.12988 | bibcode=2020AJ....159...57L | s2cid=204950000 }}</ref> | journal=The Astronomical Journal | year=2020 | volume=159 | issue=2 | page=57 | display-authors=1 | doi=10.3847/1538-3881/ab5d36 | arxiv=1910.12988 | bibcode=2020AJ....159...57L | s2cid=204950000 | doi-access=free }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,247: Line 3,456:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = First multiplanetary system to discovered by the Kepler Space Telescope.<ref>{{cite web |url=http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |title=Kepler Discovers Multi-Planet System |author=Nancy Atkinson |date=26 August 2010 |publisher=Universe Today |access-date=13 January 2011}}</ref><ref name="Holman2010Kepler-9">{{Cite journal | title=Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations | url=http://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | last1=Holman | first1=M. J. | last2=Fabrycky | first2=D. C. | last3=Ragozzine | first3=D. | last4=Ford | first4=E. B. | last5=Steffen | first5=J. H. | last6=Welsh | first6=W. F. | last7=Lissauer | first7=J. J. | last8=Latham | first8=D. W. | last9=Marcy | first9=G. W. | last10=Walkowicz | first10=L. M. | last11=Batalha | first11=N. M. | last12=Jenkins | first12=J. M. | last13=Rowe | first13=J. F. | last14=Cochran | first14=W. D. | last15=Fressin | first15=F. | last16=Torres | first16=G. | last17=Buchhave | first17=L. A. | last18=Sasselov | first18=D. D. | last19=Borucki | first19=W. J. | last20=Koch | first20=D. G. | last21=Basri | first21=G. | last22=Brown | first22=T. M. | last23=Caldwell | first23=D. A. | last24=Charbonneau | first24=D. | last25=Dunham | first25=E. W. | last26=Gautier | first26=T. N. | last27=Geary | first27=J. C. | last28=Gilliland | first28=R. L. | last29=Haas | first29=M. R. | last30=Howell | first30=S. B. | display-authors=1 | journal=Science | volume=330 | issue=6000 | pages=51–54 | year=2010 | bibcode=2010Sci...330...51H | doi=10.1126/science.1195778 | pmid=20798283 | s2cid=8141085 }}</ref> | Notes = First multiplanetary system to be discovered by the Kepler Space Telescope.<ref>{{cite web |url=http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |title=Kepler Discovers Multi-Planet System |author=Nancy Atkinson |date=26 August 2010 |publisher=Universe Today |access-date=13 January 2011 |archive-date=24 February 2012 |archive-url=https://web.archive.org/web/20120224041800/http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |url-status=live }}</ref><ref name="Holman2010Kepler-9">{{Cite journal | title=Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations | url=http://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | last1=Holman | first1=M. J. | last2=Fabrycky | first2=D. C. | last3=Ragozzine | first3=D. | last4=Ford | first4=E. B. | last5=Steffen | first5=J. H. | last6=Welsh | first6=W. F. | last7=Lissauer | first7=J. J. | last8=Latham | first8=D. W. | last9=Marcy | first9=G. W. | last10=Walkowicz | first10=L. M. | last11=Batalha | first11=N. M. | last12=Jenkins | first12=J. M. | last13=Rowe | first13=J. F. | last14=Cochran | first14=W. D. | last15=Fressin | first15=F. | last16=Torres | first16=G. | last17=Buchhave | first17=L. A. | last18=Sasselov | first18=D. D. | last19=Borucki | first19=W. J. | last20=Koch | first20=D. G. | last21=Basri | first21=G. | last22=Brown | first22=T. M. | last23=Caldwell | first23=D. A. | last24=Charbonneau | first24=D. | last25=Dunham | first25=E. W. | last26=Gautier | first26=T. N. | last27=Geary | first27=J. C. | last28=Gilliland | first28=R. L. | last29=Haas | first29=M. R. | last30=Howell | first30=S. B. | display-authors=1 | journal=Science | volume=330 | issue=6000 | pages=51–54 | year=2010 | bibcode=2010Sci...330...51H | doi=10.1126/science.1195778 | pmid=20798283 | s2cid=8141085 | access-date=2022-06-17 | archive-date=2022-12-07 | archive-url=https://web.archive.org/web/20221207160620/https://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,313: Line 3,522:
| Confirmed planets = 8 | Confirmed planets = 8
|Unconfirmed planets = |Unconfirmed planets =
| Notes = All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets.<ref name="NASA-20171214a">{{cite web |last1=Chou |first1=Felicia |last2=Hawkes |first2=Alison |last3=Landau |first3=Elizabeth |title=Artificial Intelligence, NASA Data Used to Discover Eighth Planet Circling Distant Star |url=https://www.jpl.nasa.gov/news/news.php?feature=7026 |date=14 December 2017 |work=] |access-date=15 December 2017 }}</ref> A ] test shows that the system is stable.<ref name="Schmitt2014">{{cite journal|last1= Schmitt|first1=J. R.|last2= Wang|first2= J.|last3= Fischer|first3=D. A.|last4= Jek|first4=K. J.|last5= Moriarty|first5=J. C.|last6= Boyajian|first6=T. S.|last7= Schwamb|first7=M. E.|last8= Lintott|first8= C.|last9= Lynn|first9=S.|last10= Smith|first10=A. M.|last11= Parrish|first11= M.|last12= Schawinski|first12= K.|last13= Simpson|first13= R.|last14= LaCourse|first14= D.|last15= Omohundro|first15=M. R.|last16= Winarski|first16= T.|last17= Goodman|first17=S. J.|last18= Jebson|first18= T.|last19= Schwengeler|first19=H. M.|last20= Paterson|first20=D. A.|last21= Sejpka|first21= J.|last22= Terentev|first22= I.|last23= Jacobs|first23= T.|last24= Alsaadi|first24 =N.|last25= Bailey|first25=R. C.|last26= Ginman|first26= T.|last27= Granado|first27= P.|last28= Guttormsen|first28=K. V.|last29= Mallia|first29= F.|last30= Papillon|first30=A. L.|last31= Rossi|first31= F.|last32= Socolovsky|first32= M.|last33= Stiak|first33= L.|title= Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates From the Kepler Archival Data|journal= The Astronomical Journal|volume= 148|issue= 28|date= 2014-06-26|page=28|doi= 10.1088/0004-6256/148/2/28 |arxiv= 1310.5912|bibcode=2014AJ....148...28S|s2cid=119238163}}</ref> Planet h orbits in the habitable zone. | Notes = All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets.<ref name="NASA-20171214a">{{cite web |last1=Chou |first1=Felicia |last2=Hawkes |first2=Alison |last3=Landau |first3=Elizabeth |title=Artificial Intelligence, NASA Data Used to Discover Eighth Planet Circling Distant Star |url=https://www.jpl.nasa.gov/news/news.php?feature=7026 |date=14 December 2017 |work=] |access-date=15 December 2017 |archive-date=5 May 2020 |archive-url=https://web.archive.org/web/20200505042830/https://www.jpl.nasa.gov/news/news.php?feature=7026 |url-status=live }}</ref> A ] test shows that the system is stable.<ref name="Schmitt2014">{{cite journal|last1= Schmitt|first1=J. R.|last2= Wang|first2= J.|last3= Fischer|first3=D. A.|last4= Jek|first4=K. J.|last5= Moriarty|first5=J. C.|last6= Boyajian|first6=T. S.|last7= Schwamb|first7=M. E.|last8= Lintott|first8= C.|last9= Lynn|first9=S.|last10= Smith|first10=A. M.|last11= Parrish|first11= M.|last12= Schawinski|first12= K.|last13= Simpson|first13= R.|last14= LaCourse|first14= D.|last15= Omohundro|first15=M. R.|last16= Winarski|first16= T.|last17= Goodman|first17=S. J.|last18= Jebson|first18= T.|last19= Schwengeler|first19=H. M.|last20= Paterson|first20=D. A.|last21= Sejpka|first21= J.|last22= Terentev|first22= I.|last23= Jacobs|first23= T.|last24= Alsaadi|first24 =N.|last25= Bailey|first25=R. C.|last26= Ginman|first26= T.|last27= Granado|first27= P.|last28= Guttormsen|first28=K. V.|last29= Mallia|first29= F.|last30= Papillon|first30=A. L.|last31= Rossi|first31= F.|last32= Socolovsky|first32= M.|last33= Stiak|first33= L.|title= Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates From the Kepler Archival Data|journal= The Astronomical Journal|volume= 148|issue= 28|date= 2014-06-26|page=28|doi= 10.1088/0004-6256/148/2/28 |arxiv= 1310.5912|bibcode=2014AJ....148...28S|s2cid=119238163}}</ref> Planet h orbits in the habitable zone.
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,415: Line 3,624:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-160
| Constellation = Lyra
| Right ascension = {{RA|19|11|05.65}}
| Declination = {{DEC|+42|52|09.5}}
| Apparent magnitude = 13.101
| Distance = 3140
| Spectral type = G2V
| Mass =
| Radius = 1.18
| Temperature =5470
| Metallicity =-0.361
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes = The unconfirmed planet Kepler-160e (or KOI-456.04) is a potentially habitable planet.<ref>{{Cite web|last=Patel|first=Neel V.|date=2020-06-05|title=Astronomers have found a planet like Earth orbiting a star like the sun|url=https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|access-date=2020-06-07|website=MIT Technology Review|language=en|archive-date=2023-05-25|archive-url=https://web.archive.org/web/20230525031722/https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|url-status=live}}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,550: Line 3,776:
| Confirmed planets = 3 | Confirmed planets = 3
|Unconfirmed planets = |Unconfirmed planets =
| Notes = Circumbinary planets, with one of the planets orbiting in the habitable zone.<ref name=discoveryKepler-47>{{Cite journal|arxiv= 1208.5489 |title= Kepler-47: A Transiting Circumbinary Multi-Planet System|journal= Science|volume= 337|issue= 6101|pages= 1511–4|last1= Orosz|first1= Jerome A.|last2= Welsh|first2= William F.|last3= Carter|first3= Joshua A.|last4= Fabrycky|first4= Daniel C.|last5= Cochran|first5= William D.|last6= Endl|first6= Michael|last7= Ford|first7= Eric B.|last8= Haghighipour|first8= Nader|last9= MacQueen|first9= Phillip J.|last10= Mazeh|first10= Tsevi|last11= Sanchis-Ojeda|first11= Roberto|last12= Short|first12= Donald R.|last13= Torres|first13= Guillermo|last14= Agol|first14= Eric|last15= Buchhave|first15= Lars A.|last16= Doyle|first16= Laurance R.|last17= Isaacson|first17= Howard|last18= Lissauer|first18= Jack J.|last19= Marcy|first19= Geoffrey W.|last20= Shporer|first20= Avi|last21= Windmiller|first21= Gur|last22= Barclay|first22= Thomas|last23= Boss|first23= Alan P.|last24= Clarke|first24= Bruce D.|last25= Fortney|first25= Jonathan|last26= Geary|first26= John C.|last27= Holman|first27= Matthew J.|last28= Huber|first28= Daniel|last29= Jenkins|first29= Jon M.|last30= Kinemuchi|first30= Karen|display-authors= 29|year= 2012|doi= 10.1126/science.1228380 |pmid=22933522|bibcode = 2012Sci...337.1511O |s2cid= 44970411 }}</ref><ref name=NASAKepler-47>{{cite news|url=http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|title=NASA's Kepler Discovers Multiple Planets Orbiting a Pair of Stars|date=28 August 2012|publisher=]|website=exoplanets.nasa.gov|quote=Kepler mission has discovered multiple transiting planets orbiting two suns for the first time|access-date=2 September 2012}}</ref><ref name="ScienceDaily2012Kepler-47">{{cite journal|url=https://www.sciencedaily.com/releases/2012/08/120828190127.htm |title=NASA's Kepler discovers multiple planets orbiting a pair of stars |doi=10.1126/science.1228380 |publisher=] |date=28 August 2012 |access-date=4 November 2012|arxiv = 1208.5489 |bibcode = 2012Sci...337.1511O |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Carter |first3=Joshua A. |last4=Fabrycky |first4=Daniel C. |last5=Cochran |first5=William D. |last6=Endl |first6=Michael |last7=Ford |first7=Eric B. |last8=Haghighipour |first8=Nader |last9=MacQueen |first9=Phillip J. |last10=Mazeh |first10=Tsevi |last11=Sanchis-Ojeda |first11=Roberto |last12=Short |first12=Donald R. |last13=Torres |first13=Guillermo |last14=Agol |first14=Eric |last15=Buchhave |first15=Lars A. |last16=Doyle |first16=Laurance R. |last17=Isaacson |first17=Howard |last18=Lissauer |first18=Jack J. |last19=Marcy |first19=Geoffrey W. |last20=Shporer |first20=Avi |last21=Windmiller |first21=Gur |last22=Barclay |first22=Thomas |last23=Boss |first23=Alan P. |last24=Clarke |first24=Bruce D. |last25=Fortney |first25=Jonathan |last26=Geary |first26=John C. |last27=Holman |first27=Matthew J. |last28=Huber |first28=Daniel |last29=Jenkins |first29=Jon M. |last30=Kinemuchi |first30=Karen |journal=Science |volume=337 |issue=6101 |pages=1511–4 |pmid=22933522 |s2cid=44970411 |display-authors=29 }}</ref> | Notes = Circumbinary planets, with one of the planets orbiting in the habitable zone.<ref name=discoveryKepler-47>{{Cite journal|arxiv= 1208.5489 |title= Kepler-47: A Transiting Circumbinary Multi-Planet System|journal= Science|volume= 337|issue= 6101|pages= 1511–4|last1= Orosz|first1= Jerome A.|last2= Welsh|first2= William F.|last3= Carter|first3= Joshua A.|last4= Fabrycky|first4= Daniel C.|last5= Cochran|first5= William D.|last6= Endl|first6= Michael|last7= Ford|first7= Eric B.|last8= Haghighipour|first8= Nader|last9= MacQueen|first9= Phillip J.|last10= Mazeh|first10= Tsevi|last11= Sanchis-Ojeda|first11= Roberto|last12= Short|first12= Donald R.|last13= Torres|first13= Guillermo|last14= Agol|first14= Eric|last15= Buchhave|first15= Lars A.|last16= Doyle|first16= Laurance R.|last17= Isaacson|first17= Howard|last18= Lissauer|first18= Jack J.|last19= Marcy|first19= Geoffrey W.|last20= Shporer|first20= Avi|last21= Windmiller|first21= Gur|last22= Barclay|first22= Thomas|last23= Boss|first23= Alan P.|last24= Clarke|first24= Bruce D.|last25= Fortney|first25= Jonathan|last26= Geary|first26= John C.|last27= Holman|first27= Matthew J.|last28= Huber|first28= Daniel|last29= Jenkins|first29= Jon M.|last30= Kinemuchi|first30= Karen|display-authors= 29|year= 2012|doi= 10.1126/science.1228380 |pmid=22933522|bibcode = 2012Sci...337.1511O |s2cid= 44970411 }}</ref><ref name=NASAKepler-47>{{cite news|url=http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|title=NASA's Kepler Discovers Multiple Planets Orbiting a Pair of Stars|date=28 August 2012|publisher=]|website=exoplanets.nasa.gov|quote=Kepler mission has discovered multiple transiting planets orbiting two suns for the first time|access-date=2 September 2012|archive-date=31 October 2012|archive-url=https://web.archive.org/web/20121031024345/http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|url-status=dead}}</ref><ref name="ScienceDaily2012Kepler-47">{{cite journal |url=https://www.sciencedaily.com/releases/2012/08/120828190127.htm |title=NASA's Kepler discovers multiple planets orbiting a pair of stars |doi=10.1126/science.1228380 |publisher=] |date=28 August 2012 |access-date=4 November 2012 |arxiv=1208.5489 |bibcode=2012Sci...337.1511O |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Carter |first3=Joshua A. |last4=Fabrycky |first4=Daniel C. |last5=Cochran |first5=William D. |last6=Endl |first6=Michael |last7=Ford |first7=Eric B. |last8=Haghighipour |first8=Nader |last9=MacQueen |first9=Phillip J. |last10=Mazeh |first10=Tsevi |last11=Sanchis-Ojeda |first11=Roberto |last12=Short |first12=Donald R. |last13=Torres |first13=Guillermo |last14=Agol |first14=Eric |last15=Buchhave |first15=Lars A. |last16=Doyle |first16=Laurance R. |last17=Isaacson |first17=Howard |last18=Lissauer |first18=Jack J. |last19=Marcy |first19=Geoffrey W. |last20=Shporer |first20=Avi |last21=Windmiller |first21=Gur |last22=Barclay |first22=Thomas |last23=Boss |first23=Alan P. |last24=Clarke |first24=Bruce D. |last25=Fortney |first25=Jonathan |last26=Geary |first26=John C. |last27=Holman |first27=Matthew J. |last28=Huber |first28=Daniel |last29=Jenkins |first29=Jon M. |last30=Kinemuchi |first30=Karen |journal=Science |volume=337 |issue=6101 |pages=1511–4 |pmid=22933522 |s2cid=44970411 |display-authors=29 |archive-date=21 September 2022 |archive-url=https://web.archive.org/web/20220921182959/https://www.sciencedaily.com/releases/2012/08/120828190127.htm |url-status=live }}</ref>
}} }}
{{Multiplanetary systems list {{Multiplanetary systems list
Line 3,650: Line 3,876:
| Age = 7.5 | Age = 7.5
| Confirmed planets = 2 | Confirmed planets = 2
|Unconfirmed planets = 1 |Unconfirmed planets = 2
| Notes = Farthest system from the Sun with an unconfirmed exoplanet candidate. | Notes = Farthest system from the Sun with an unconfirmed exoplanet candidate.
}} }}
Line 3,753: Line 3,979:
| Confirmed planets = 5 | Confirmed planets = 5
|Unconfirmed planets = |Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = ]
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|37|21.23}}
| Declination = {{DEC|+50|20|11.55}}
| Apparent magnitude = 15.76
| Distance = 4900
| Spectral type = F8V
| Mass = 0.99
| Radius = 1.09
| Temperature = 5835
| Metallicity = 0.010
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 4
| Notes = | Notes =
}} }}
Line 4,467: Line 4,710:


==Stars orbited by both planets and brown dwarfs== ==Stars orbited by both planets and brown dwarfs==
Stars orbited by objects on both sides of the 13 ] dividing line. Stars orbited by objects on both sides of the ~13 ] dividing line.


* ] (HD 3651)<ref>{{cite journal | display-authors=1 | last1=Mugrauer | first1=M. | last2=Seifahrt | first2=A. | last3=Neuhäuser | first3=R. | last4=Mazeh | first4=T. | title=HD 3651 B: the first directly imaged brown dwarf companion of an exoplanet host star | journal=Monthly Notices of the Royal Astronomical Society: Letters | volume=373 | issue=1 | pages=L31–L35 | date=2006 | doi=10.1111/j.1745-3933.2006.00237.x | doi-access=free | type=abstract | arxiv=astro-ph/0608484 | bibcode=2006MNRAS.373L..31M | s2cid=15608344 }}</ref>
* ] (HD 3651)
* ] * ]<ref>{{cite journal
| title=Two New Planets in Eccentric Orbits
* ] A
| last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
* ]
| last3=Vogt | first3=Steven S. | last4=Fischer | first4=Debra
* ]
| last5=Liu | first5=Michael C. | display-authors=1
* ]
| journal=The Astrophysical Journal
| volume=520 | issue=1 | pages=239–247 | year=1999
| arxiv=astro-ph/9904275 | bibcode=1999ApJ...520..239M
| doi=10.1086/307451 | s2cid=16827678 }}</ref><ref>{{cite journal
| title=Two Substellar Companions Orbiting HD 168443
| last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
| last3=Vogt | first3=Steven S. | last4=Liu | first4=Michael C.
| last5=Laughlin | first5=Gregory | last6=Apps | first6=Kevin
| last7=Graham | first7=J. R. | last8=Lloyd | first8=J.
| last9=Luhman | first9=Kevin L. | first10=Ray | last10=Jayawardhana
| display-authors=1 | journal=The Astrophysical Journal
| volume=555 | issue=1 | pages=418–425 | year=2001
| bibcode=2001ApJ...555..418M | doi=10.1086/321445 | doi-access=free }}</ref>
* ] A<ref name=Cheetham2018>{{cite journal
| title=Direct imaging of an ultracool substellar companion to the exoplanet host star HD 4113 A
| last1=Cheetham | first1=A. | last2=Ségransan | first2=D.
| last3=Peretti | first3=S. | last4=Delisle | first4=J. -B.
| last5=Hagelberg | first5=J. | last6=Beuzit | first6=J. -L.
| last7=Forveille | first7=T. | last8=Marmier | first8=M.
| last9=Udry | first9=S. | last10=Wildi | first10=F.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=614 | id=A16 | pages=19 | date=June 2018
| arxiv=1712.05217 | bibcode=2018A&A...614A..16C
| doi=10.1051/0004-6361/201630136 | s2cid=119084543 }}</ref>
* ] A<ref>{{cite web|title=Astronomers Announce First Clear Evidence of a Brown Dwarf|url=http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/48/|publisher=] news release STScI-1995-48|date=November 29, 1995|access-date=24 September 2013|archive-date=9 July 2008|archive-url=https://web.archive.org/web/20080709002411/http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/48/|url-status=live}}</ref><ref>{{cite encyclopedia |title=Planet GJ 229 A b |url=https://exoplanet.eu/catalog/gj_229_a_b--1533/ |date=1995 |encyclopedia=] |access-date=7 September 2022}}</ref><ref>{{cite encyclopedia |title=Planet GJ 229 A c|url=https://exoplanet.eu/catalog/gj_229_a_c--7263/ |date=1995 |encyclopedia=]|access-date=7 September 2022}}</ref>
* ] A<ref>{{Citation | title=Detection of the nearest Jupiter analog in radial velocity and astrometry data | first1=Fabo | last1=Feng | first2=Guillem | last2=Anglada-Escudé | first3=Mikko | last3=Tuomi | first4=Hugh R. A. | last4=Jones | first5=Julio | last5=Chanamé | first6=Paul R. | last6=Butler | first7=Markus | last7=Janson | journal=Monthly Notices of the Royal Astronomical Society | arxiv=1910.06804 | date=14 October 2019 | volume=490 | issue=4 | pages=5002–5016 | doi=10.1093/mnras/stz2912 | doi-access=free | bibcode=2019MNRAS.490.5002F | s2cid=204575783 }}</ref><ref>{{cite news|last=Scholz |first=Ralf-Dieter |author2=McCaughrean, Mark |date=2003-01-13 |title=Discovery of Nearest Known Brown Dwarf: Bright Southern Star Epsilon Indi Has Cool, Substellar Companion |publisher=European Southern Observatory |url=http://www.eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |access-date=2006-05-24 |url-status=dead |archive-url=https://web.archive.org/web/20071014191814/http://eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |archive-date=October 14, 2007 }}</ref><ref>{{cite journal | last=Scholz | first=R.-D. | author2=McCaughrean, M. J. | author3=Lodieu, N. | author4=Kuhlbrodt, B. | title=ε Indi B: A new benchmark T dwarf | journal=Astronomy and Astrophysics | date=February 2003 | volume=398 | issue=3 | pages=L29–L33 | bibcode=2003A&A...398L..29S | doi=10.1051/0004-6361:20021847 | arxiv=astro-ph/0212487 | s2cid=119474823 }}</ref>
* ]<ref>{{cite journal | title=Catalog of Nearby Exoplanets | last1=Butler | first1=R. P. | last2=Wright | first2=J. T. | last3=Marcy | first3=G. W. | last4=Fischer | first4=D. A. | last5=Vogt | first5=S. S. | last6=Tinney | first6=C. G. | last7=Jones | first7=H. R. A. | last8=Carter | first8=B. D. | last9=Johnson | first9=J. A. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=646 | issue=1 | pages=505–522 | arxiv=astro-ph/0607493 | bibcode=2006ApJ...646..505B | doi=10.1086/504701 | s2cid=119067572 }}</ref>
* ]<ref>{{cite journal |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |display-authors=etal |date=August 2022 |title=3D Selection of 167 Substellar Companions to Nearby Stars |journal=] |volume=262 |issue=21 |page=21 |doi=10.3847/1538-4365/ac7e57 |arxiv=2208.12720 |bibcode=2022ApJS..262...21F|s2cid=251864022 |doi-access=free }}</ref><ref>{{cite journal | arxiv=2203.01018| doi=10.3847/1538-3881/ac5dcb| title=A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit| year=2022| last1=Hatzes| first1=Artie P.| last2=Gandolfi| first2=Davide| last3=Korth| first3=Judith| last4=Rodler| first4=Florian| last5=Sabotta| first5=Silvia| last6=Esposito| first6=Massimiliano| last7=Barragán| first7=Oscar| last8=Van Eylen| first8=Vincent| last9=Livingston| first9=John H.| last10=Serrano| first10=Luisa Maria| last11=Luque| first11=Rafael| last12=Smith| first12=Alexis M. S.| last13=Redfield| first13=Seth| last14=Persson| first14=Carina M.| last15=Pätzold| first15=Martin| last16=Palle| first16=Enric| last17=Nowak| first17=Grzegorz| last18=Osborne| first18=Hannah L. M.| last19=Narita| first19=Norio| last20=Mathur| first20=Savita| last21=Lam| first21=Kristine W. F.| last22=Kabáth| first22=Petr| last23=Johnson| first23=Marshall C.| last24=Guenther| first24=Eike W.| last25=Grziwa| first25=Sascha| last26=Goffo| first26=Elisa| last27=Fridlund| first27=Malcolm| last28=Endl| first28=Michael| last29=Deeg| first29=Hans J.| last30=Csizmadia| first30=Szilard| journal=The Astronomical Journal| volume=163| issue=5| page=223| bibcode=2022AJ....163..223H| s2cid=247218413| display-authors=1| doi-access=free}}</ref>
* ]<ref>{{cite journal | title=A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529 | last1=Fischer | first1=Debra A. | last2=Marcy | first2=Geoffrey W. | last3=Butler | first3=R. Paul | last4=Vogt | first4=Steven S. | last5=Henry | first5=Gregory W. | last6=Pourbaix | first6=Dimitri | last7=Walp | first7=Bernard | last8=Misch | first8=Anthony A. | last9=Wright | first9=Jason T. | display-authors=1 | journal=The Astrophysical Journal | volume=586 | issue=2 | pages=1394–1408 | year=2003 | bibcode=2003ApJ...586.1394F | bibcode-access=free | doi=10.1086/367889 | doi-access=free }}</ref>
* ]<ref>{{Cite journal |last1=Khandelwal |first1=Akanksha |last2=Sharma |first2=Rishikesh |last3=Chakraborty |first3=Abhijit |last4=Chaturvedi |first4=Priyanka |last5=Ulmer-Moll |first5=Solène |last6=Ciardi |first6=David R. |last7=Boyle |first7=Andrew W. |last8=Baliwal |first8=Sanjay |last9=Bieryla |first9=Allyson |last10=Latham |first10=David W. |last11=Prasad |first11=Neelam J. S. S. V. |last12=Nayak |first12=Ashirbad |last13=Lendl |first13=Monika |last14=Mordasini |first14=Christoph |date=2023-04-01 |title=Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603 |url=https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |journal=Astronomy & Astrophysics |language=en |volume=672 |pages=L7 |doi=10.1051/0004-6361/202245608 |issn=0004-6361 |doi-access=free |arxiv=2303.11841 |bibcode=2023A&A...672L...7K |access-date=2023-12-15 |archive-date=2024-02-28 |archive-url=https://web.archive.org/web/20240228142329/https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |url-status=live }}</ref>
* ]<ref name="Zhang2024">{{cite journal |last1=Zhang |first1=Keming |last2=Zang |first2=Weicheng |last3=El-Badry |first3=Kareem |last4=Lu |first4=Jessica R. |display-authors=etal |date=September 2024 |title=An Earth-mass planet and a brown dwarf in orbit around a white dwarf |journal=] |volume= 8|issue= 12|pages= 1575–1582|doi=10.1038/s41550-024-02375-9 |arxiv=2409.02157 |bibcode=2024NatAs.tmp..237Z}}</ref>


==See also== ==See also==
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* ] * ]
* ] * ]
* ] * ]
* ] * ]
* ] * ]
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<!-- ==Notes== <!-- ==Notes==
{{Reflist|group=note}} --> {{Reflist|group=note}} -->

==Notes==
{{notelist}}


==References== ==References==
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{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}} {{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}


{{DEFAULTSORT:Multiplanetary systems}}
] ]
] ]

Latest revision as of 00:28, 22 December 2024

A list of systems with multiple planets Further information: Planetary system
Number of extrasolar planet discoveries per year through 2023. Colors indicate method of detection.
  Direct imaging   Microlensing   Transit   Radial velocity   Timing

From the total of 4,949 stars known to have exoplanets (as of July 24, 2024), there are a total of 1007 known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets.

The 1007 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d). The nearest system with four or more confirmed planets is Gliese 876, with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 light-years (4,100 pc) away.

The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important stellar properties are mass and metallicity because they determine how these planetary systems form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 AU.

Multiplanetary systems

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.
Color indicates number of planets
2 (x) 3 4 5 6 7 8 9
Star
 Constellation
 Right
ascension
 Declination
 Apparent
magnitude
 Distance (ly)
 Spectral
type
 Mass
(M☉)
 Temperature (K)
 Age
(Gyr)
 Confirmed
(unconfirmed)
planets
 Notes
Sun – - - −26.74 0.000016 G2V 1 5778 4.572 8 (1) The hypothesised Planet Nine remains unconfirmed.
Proxima Centauri Centaurus 14 29 42.94853 −62° 40′ 46.1631″ 10.43 to 11.11 4.244 M5.5Ve 0.122 3042 4.85 2 (1) Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable. Planet c initially appeared likely but has since been disputed.
Lalande 21185 Ursa Major 11 03 20.1940 +35° 58′ 11.5682″ 7.520 8.3044±0.0007 M2V 0.39 3601±51 8.047 2 (1) Brightest red dwarf star in the northern celestial hemisphere.
Lacaille 9352 Piscis Austrinus 23 05 52.04 −35° 51′ 11.05″ 7.34 10.721 M0.5V 0.486 3688±86 4.57 2 (1) The unconfirmed planet d is potentially habitable.
Luyten's Star Canis Minor 07 27 24.4991 05° 13′ 32.827″ 9.872 11.20 M3.5V 0.26 3150 unknown 2 (2) Stellar activity level and rotational rate suggest an age higher than 8 billion years. Planet b is potentially habitable.
YZ Ceti Cetus 01 12 30.64 −16° 59′ 56.3″ 12.07 11.74 M4.5V 0.13 3056 4 3 (1) Flare star.
Gliese 1061 Horologium 03 35 59.69 −44° 30′ 45.3″ 13.03 12.04 M5.5V 0.113 2953 unknown 3 Planets c and d are potentially habitable.
Teegarden's Star Aries 02 53 00.89 +16° 52′ 53″ 15.13 12.497 M7V 0.097 3034 8 3 Teegarden's Star b and Teegarden's Star c are likely Earth-mass planets that orbit in the habitable zone.
Wolf 1061 Ophiuchus 16 30 18.0584 −12° 39′ 45.325″ 10.07 14.050 ± 0.002 M3.5V 0.294 3342 unknown 3 Planet c is potentially habitable.
Gliese 876 Aquarius 22 53 16.73 −14° 15′ 49.3″ 10.17 15.25 M4V 0.334 3348 4.893 4 Planet b is a gas giant which orbits in the habitable zone.
82 G. Eridani Eridanus 03 19 55.65 −43° 04′ 11.2″ 4.254 19.71 G8V 0.7 5401 5.76 3 (3) This star also has a dust disk with a semi-major axis at approximately 19 AU.
Gliese 581 Libra 15 19 26.83 −07° 43′ 20.2″ 10.56 20.56 M3V 0.311 3484 4.326 3 (1) The disputed planet d is potentially habitable.
Gliese 667 C Scorpius 17 18 57.16 −34° 59′ 23.14″ 10.20 21 M1.5V 0.31 3700 2 2 (1) Triple star system - all exoplanets orbit around Star C. Planet c is potentially habitable, and there are more unconfirmed planets.
HD 219134 Cassiopeia 23 13 14.74 57° 10′ 03.5″ 5.57 21 K3Vvar 0.794 4699 12.66 6 Closest star to the Sun with exactly six exoplanets, and closest K-type main sequence star to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.
61 Virginis Virgo 13 18 24.31 −18° 18′ 40.3″ 4.74 28 G5V 0.954 5531 8.96 2 (1) Planet d remains unconfirmed, and a 2021 study found that it was likely a false positive. 61 Virginis also has a debris disk.
Gliese 433 Hydra 11 35 26.9485 −25° 10′ 08.9″ 9.79 29.8±0.1 M1.5V 0.48 3550±100 unknown 3 An infrared excess around this star suggests a circumstellar disk.
Gliese 357 Hydra 09 36 01.6373 −21° 39′ 38.878″ 10.906 30.776 M2.5V 0.362 3488 unknown 3 Planet d is a potentially habitable Super-Earth.
L 98-59 Volans 08 18 07.62 −68° 18′ 46.8″ 11.69 34.6 M3V 0.312 3412 unknown 4 (1) The unconfirmed planet f orbits in the habitable zone.
Gliese 414 A Ursa Major 11 11 05.88 30° 26′ 42.61″ 8.31 38.76 K7V 0.65 4120 12.4 2 (0)
Gliese 806 Cygnus 20 45 04.099 +44° 29′ 56.6″ 10.79 39.3 M1.5V 0.423 3586 3 2 (1) -
TRAPPIST-1 Aquarius 23 06 29.283 −05° 02′ 28.59″ 18.80 39.5 M8V 0.089 2550 7.6 7 Planets d, e, f and g are potentially habitable. Only star known with exactly seven confirmed planets. All seven terrestrial planets lie within only 0.07 AU of the star.
55 Cancri Cancer 08 52 35.81 +28° 19′ 50.9″ 5.95 40 K0IV-V 1.026 5217 7.4 5 All five known planets orbit around star A (none are circumbinary or orbit around star B). Closest system with exactly five confirmed planets.
Gliese 180 Eridanus 04 53 49.9798 −17° 46′ 24.294″ 10.894 40.3 M2V or M3V 0.39 3562 unknown 3 The habitability of planets b and c is disputed.
HD 69830 Puppis 08 18 23.95 −12° 37′ 55.8″ 5.95 41 K0V 0.856 5385 7.446 3 A debris disk exterior to the three exoplanets was detected by the Spitzer Space Telescope in 2005.
HD 40307 Pictor 05 54 04.24 −60° 01′ 24.5″ 7.17 42 K2.5V 0.752 4977 1.198 4 (2) The existence of planets e and g are disputed. If confirmed, planet g is potentially habitable.
Upsilon Andromedae Andromeda 01 36 47.84 +41° 24′ 19.7″ 4.09 44 F8V 1.27 6107 3.781 3 Nearest F-type main sequence star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after 7 Canis Majoris. All exoplanets orbit around star A in the binary system.
47 Ursae Majoris Ursa Major 10 59 27.97 +40° 25′ 48.9″ 5.10 46 G0V 1.029 5892 7.434 3 Planet Taphao Thong was discovered in 1996 and was one of the first exoplanets to be discovered. The planet was the first long-period extrasolar planet discovered. The other planets were discovered later.
Nu Lupi Lupus 15 21 49.57 −48° 19′ 01.1″ 5.65 47 G2V 0.906 5664 10.36 3 One of the oldest stars in the solar neighbourhood.
LHS 1140 Cetus 00 44 59.31 −15° 16′ 16.7″ 14.18 48.9 M4.5V 0.179 3216±39 5 2 (1) Planet b is a potentially habitable Super-Earth.
Gliese 163 Dorado 04 09 16 −53° 22′ 25″ 11.8 49 M3.5V 0.4 unknown 3 5 Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.
Mu Arae Ara 17 44 08.70 −51° 50′ 02.6″ 5.15 51 G3IV-V 1.077 5704 6.413 4 Planet Quijote orbits in the circumstellar habitable zone. However, it is a gas giant, so it itself is uninhabitable although a large moon orbiting around it may be habitable.
GJ 3929 Corona Borealis 15 58 18.8 35° 24′ 24.3″ 12.67 51.58 M3.5V 0.313 3384 unknown 2 (0)
Gliese 676 A Ara 17 30 11.2042 −51° 38′ 13.116″ 9.59 53 M0V 0.71 unknown unknown 4 Held the record for widest range of masses in a planetary system in 2012.
HD 7924 Cassiopeia 01 21 59.12 +76° 42′ 37.0″ 7.19 55 K0V 0.832 5177 unknown 3 These planets may be potentially habitable Super-Earths.
Pi Mensae Mensa 05 37 09.8851 −80° 28′ 08.8313″ 5.65 59.62±0.07 G0V 1.11 6013 3.4 3 Outer planet is likely a brown dwarf.
Gliese 3293 Eridanus 04 28 35.72 −25° 10′ 08.9″ 11.96 59 M2.5V 0.42 3466±49 unknown 4 Planets b and d orbit in the habitable zone.
LHS 1678 Caelum 04 32 43 −39° 47′ 21″ 12 64.8 M2V 0.345 3490 unknown 3 (0)
HD 104067 Corvus 11 59 10.0 −20° 21′ 13.6″ 7.92 66.3 K3V 0.82 4942 4.8 2 (1) The innermost planet, which is unconfirmed, might suffer from significant tidal heating.
HD 142 Phoenix 00 06 19.0 −49° 04′ 30″ 5.70 67 G1 IV 1.1 6180 5.93 3 -
HD 215152 Aquarius 22 43 21 −06° 24′ 03″ 8.13 70 G8IV 1.019 5646 7.32 4 A debris disk candidate as it has an infrared excess.
HD 164922 Hercules 18 02 30.86 +26° 18′ 46.8″ 7.01 72 G9V 0.874 5293 13.4 4 Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.
HD 63433 Gemini 07 49 55.0 +27° 21′ 47.4″ 6.92 73 G5V 0.99 5640 0.4 3
HIP 57274 Ursa Major 11 44 41 +30° 57′ 33″ 8.96 85 K5V 0.73 4640 7.87 3 -
HD 39194 Mensa 05 44 32 −70° 08′ 37″ 8.08 86.2 K0V unknown 5205 unknown 3 The planets have eccentric orbits.
LP 791-18 Crater 11 02 45.95 −16° 24′ 22.3″ 16.9 86.9 M6V/M7V 0.139 2960 0.5 3
HD 181433 Pavo 19 25 09.57 −66° 28′ 07.7″ 8.38 87 K5V 0.777 4962 8.974 3 -
HD 134606 Apus 15 15 15 −70° 31′ 11″ 6.85 87 G6IV unknown unknown unknown 5 The planets have moderately eccentric orbits.
HD 158259 Draco 17 25 24.0 +52° 47′ 26″ 6.46 89 G0 1.08 unknown unknown 5 (1) A G-type star slightly more massive than the Sun. Planet g remains unconfirmed.
HD 82943 Hydra 09 34 50.74 −12° 07′ 46.4″ 6.54 90 F9V Fe+0.5 1.175 5874 3.08 3 Planets b and c are in a 2:1 orbital resonance. Planet b orbits in the habitable zone, but it and planet c are massive enough to be brown dwarfs. HD 82943 has an unusual lithium-6 abundance.
Gliese 3138 Cetus 02 09 10.90 −16° 20′ 22.53″ 10.877 92.9 0.681 3717±49 unknown 3
GJ 9827 Pisces 23 27 04.84 −01° 17′ 10.59″ 10.10 96.8±0.2 K6V 0.593 4294±52 unknown 3 Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.
K2-239 Sextans 10 42 22.63 +04° 26′ 28.86″ 14.5 101.5 M3V 0.4 3420 unknown 3
TOI-700 Dorado 06 28 22.97 −65° 34′ 43.01″ 13.10 101.61 M2V 0.416 3480 1.5 4 Planets d and e are potentially habitable.
HD 17926 Fornax 02 51 56.16 −30° 48′ 53.2″ 6.38 105 F6V 1.145 6201 unknown 3 The star has a red dwarf companion.
HD 37124 Taurus 05 37 02.49 +20° 43′ 50.8″ 7.68 110 G4V 0.83 5606 3.327 3 Planet c orbits at the outer edge of the habitable zone.
HD 20781 Fornax 03 20 03 −28° 47′ 02″ 8.44 115 G9.5V 0.7 5256±29 unknown 4 Located in binary star system.
Kepler-444 Lyra 19 19 01 41° 38′ 05″ 9.0 117 K0V 0.758 5040 11.23 5 Nearest multiplanetary system where the planets were discovered by the Kepler space telescope.
HD 141399 Boötes 15 46 54.0 +46° 59′ 11″ 7.2 118 K0V 1.07 5600 unknown 4 Planet c orbits in the habitable zone.
Kepler-42 Cygnus 19 28 53 +44° 37′ 10″ 16.12 126 M5V 0.13 3068 unknown 3 -
HD 31527 Lepus 04 55 38 −23° 14′ 31″ 7.48 126 G0V unknown unknown unknown 3 -
HD 10180 Hydrus 01 37 53.58 −60° 30′ 41.5″ 7.33 127 G1V 1.055 5911 4.335 6 (3) Has three unconfirmed candidates. If these candidate exoplanets were confirmed, HD 10180 would have the largest planetary system of any star.
HD 23472 Reticulum 03 41 50.3988 −62° 46′ 01.4772″ 9.72 127.48 K3.5V 0.67 4684±99 unknown 5
HR 8799 Pegasus 23 07 28.72 +21° 08′ 03.3″ 5.96 129 A5V 1.472 7429 0.064 4 Only A-type main sequence star with a multiplanetary system, and hottest and most massive single main sequence star with a multiplanetary system. All four planets are massive super-Jupiters.
HD 27894 Reticulum 04 20 47.05 −59° 24′ 39.0″ 9.42 138 K2V 0.8 4875 3.9 3 -
HD 93385 Vela 10 46 15.1160 −41° 27′ 51.7261″ 7.486 141.6 G2V 1.07 5823 4.13 3
K2-3 Leo 11 29 20.3918 −01° 27′ 17.280″ 12.168 143.9±0.4 M0V 0.601 3835±70 1 3 The outermost planet orbits in the habitable zone.
HD 34445 Orion 05 17 41.0 +07° 21′ 12″ 7.31 152 G0V 1.07 5836 8.5 1 (5) Some planets were not detected or inferred to be false positives in a later study.
HD 204313 Capricornus 21 28 12.21 –21° 43′ 34.5″ 7.99 154 G5V 1.045 5767 3.38 3 -
HD 3167 Pisces 00 34 57.5 +04° 22′ 53″ 8.97 154.4 K0V 0.852 5300 10.2 4 -
HIP 34269 Puppis 07 06 13.98 −47° 35′ 13.87″ 10.59 154.81 0.74 4440±100 unknown 4
HD 133131 Libra 15 03 35.80651 −27° 50′ 27.5520″ 8.4 168 G2V+G2V 0.95 5799±19 6 3 2 planets around primary, and 1 planet around secondary star.
K2-136 [ru] Taurus 04 29 38.99 +22° 52′ 57.80″ 11.2 173 K5V 0.71 4364±70 0.7 3
HIP 14810 Aries 03 11 14.23 +21° 05′ 50.5″ 8.51 174 G5V 0.989 5485 5.271 3 -
HD 191939 Draco 20 08 05.75 +66° 51′ 2.1″ 8.971 175 G9V 0.81 5348 8.7 6
HD 125612 Virgo 14 20 53.51 −17° 28′ 53.5″ 8.33 177 G3V 1.099 5897 2.15 3 -
HD 184010 Vulpecula 19 31 22.0 +26° 37′ 02″ 5.9 200 KOIII-IV 1.35 4971 2.76 3 -
HD 109271 Virgo 12 33 36.0 −11° 37′ 19″ 8.05 202 G5 1.047 5783 7.3 2 (1) -
HD 38677 Orion 05 47 06.0 −10° 37′ 49″″ 8.0 202 F8V 1.21 6196.0 2.01 4 -
TOI-178 Sculptor 00 29 12.30 30° 27′ 13.46″ 11.95 205.16 K7V 0.65 4316±70 7.1 6 The planets are in an orbital resonance.
HD 108236 Centaurus 12 26 17.89 −51° 21′ 46.21″ 9.24 211 G3V 0.97 5730 5.8 5 -
Kepler-37 Lyra 18 58 23.1 44° 31′ 05″ 9.77 215 G8V 0.803 5417 6 3 (1) The existence of Kepler-37e is dubious.
K2-72 Aquarius 22 18 29.2548 −09° 36′ 44.3824″ 15.04 217 M2V 0.27 3497 unknown 4 2 planets in habitable zone
Kepler-138 Lyra 19 21 32.0 +43° 17′ 35″ 13.5 218.5 M1V 0.57 3871 unknown 3 (1)
K2-233 Libra 15 21 55.2 −20° 13′ 54″ 10.0 221 K3 0.8 4950 0.36 3
TOI-1260 Ursa Major 10 28 35.03 +65° 51′ 16.38″ 11.973 239.5 0.66 4227±85 6.7 3
LP 358-499 Taurus 04 40 35.64 +25° 00′ 36.05″ 13.996 245.3 0.46 3655±80 unknown 4 Also known as K2-133
K2-266 Sextans 10 31 44.5 +00° 56′ 15″ 252 K 0.69 4285 8.4 4 (2)
K2-155 Taurus 04 21 52.5 +21° 21′ 13″ 12.8 267 K7 0.65 4258 unknown 3
K2-384 Cetus 01 21 59.86 00° 45′ 04.41″ 16.12 270 M?V 0.33 3623±138 unknown 5
TOI-1136 Draco 12 48 44.38 +64° 51′ 18.99″ 9.534 275.8 1.022 5770±50 0.7 6 (1)
TOI-561 Sextans 09 52 44.44 +06° 12′ 57.97″ 10.252 279 G9V 0.785 5455 5 4 (1) -
Kepler-445 Cygnus 19 54 57.0 +46° 29′ 55″ 18 294 0.18 3157 unknown 3 -
TOI-763 Centaurus 12 57 52.45 −39° 45′ 27.71″ 10.156 311 0.917 5444 6.2 2 (1) -
K2-229 Virgo 12 27 29.5848 −06° 43′ 18.7660″ 10.985 335 K2V 0.837 5185 5.4 3
Kepler-102 Lyra 18 45 55.9 +47° 12′ 29″ 11.492 340 K3V 0.81 4809 1.41 5
V1298 Tauri Taurus 04 05 19.5912 +20° 09′ 25.5635″ 10.31 354 K0-1.5 1.101 4970 0.023 4 This star is a young T Tauri variable.
K2-302 Aquarius 22 20 22.7764 −09° 30′ 34.2934″ 11.98 359.3 unknown 3297±73 unknown 3
K2-198 Virgo 13 15 22.5 −06° 27′ 54″ 11.0 362 0.8 5213 unknown 3
TOI-125 Hydrus 01 34 22.73 −66° 40′ 32.95″ 11.02 363 0.859 5320 unknown 3 (2)
HIP 41378 Cancer 08 26 28.0 +10° 04′ 49″ 8.9 378 F8 1.15 6199 unknown 5 (2) Planet f has an unusually low density, and might have rings or an extended atmosphere. More planets are still suspected.
Kepler-446 Lyra 18 49 00.0 +44° 55′ 16″ 16.5 391 M4V 0.22 3359 unknown 3 -
HD 33142 Lepus 05 07 35.54 −13° 59′ 11.34″ 7.96 394.3 1.52 5025
−16		 unknown 3 Host star is a giant star with spectral type of K0III.
K2-148 Cetus 00 58 04.28 −00° 11′ 35.36″ 13.05 407 K7V 0.65 4079±70 unknown 3 A secondary red dwarf is gravitationally bound to K2-148.
Kepler-68 Cygnus 19 24 07.76 +49° 02′ 25.0″ 8.588 440 G1V 1.079 5793 6.3 3 (1) Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone. Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.
HD 28109 Hydrus 04 20 57.13 −68° 06′ 09.51″ 9.38 457 1.26 6120±50 unknown 3
COROT-7 Monoceros 06 43 49.47 −01° 03′ 46.9″ 11.73 489 K0V 0.93 5275 1.5 3
XO-2 Lynx 07 48 07.4814 +50° 13′ 03.2578″ 11.18 496±3 K0V+K0V unknown unknown 6.3 4 Binary with each star orbited by two planets.
Kepler-411 Cygnus 19 10 25.3 +49° 31′ 24″ 12.5 499.4 K3V 0.83 4974 unknown 5
K2-381 Sagittarius 19 12 06.46 −21° 00′ 27.51″ 13.01 505 K2 0.754 4473±138 unknown 3
K2-285 Pisces 23 17 32.2 +01° 18′ 01″ 12.03 508 K2V 0.83 4975 unknown 4
K2-32 Ophiuchus 16 49 42.2602 −19° 32′ 34.151″ 12.31 510 G9V 0.856 5275 7.9 4 The planets are likely in a 1:2:5:7 orbital resonance.
TOI-1246 Draco 16 44 27.96 70° 25′ 46.70″ 11.6 558 1.12 5217±50 unknown 4
K2-352 Cancer 09 21 46.8434 +18° 28′ 10.34710″ 11.12 577 G2V 0.98 5791 unknown 3
Kepler-398 Lyra 19 25 52.5 +40° 20′ 38″ 578 K5V 0.72 4493 unknown 3
Kepler-186 Cygnus 19 54 36.6 +43° 57′ 18″ 15.29 579.23 M1V 0.478 3788 unknown 5 Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.
K2-37 Scorpius 16 13 48.2445 −24° 47′ 13.4279″ 12.52 590 G3V 0.9 5413 unknown 3
K2-58 Aquarius 22 15 17.2364 −14° 02′ 59.3151″ 12.13 596 K2V 0.89 5038 unknown 3
K2-138 Aquarius 23 15 47.77 −10° 50′ 58.91″ 12.21 597±55 K1V 0.93 5378±60 2.3 6 Planet g was not fully verified, or could be two long-period planets instead.
K2-38 Scorpius 16 00 08.06 −23° 11′ 21.33″ 11.34 630 G3V 1.03 5731±66 unknown 2 (1) Dust disk in system
WASP-47 Aquarius 22 04 49.0 −12° 01′ 08″ 11.9 652 G9V 1.084 5400 unknown 4 One planet is a gas giant which orbits in the habitable zone. WASP-47 is the only planetary system known to have both planets near the hot Jupiter and another planet much further out.
K2-368 Aquarius 22 10 32.58 −11° 09′ 58.02″ 13.54 674 K3 0.746 4663±138 unknown 3 (1)
HAT-P-13 Ursa Major 08 39 31.81 +47° 21′ 07.3″ 10.62 698 G4 1.22 5638 5 2 (1) -
Kepler-19 Cygnus 19 21 41 +37° 51′ 06″ 15.178 717 G 0.936 5541 1.9 3 System consists of a thick-envelope Super-Earth and two Neptune-mass planets.
Kepler-296 Lyra 19 06 09.6 +49° 26′ 14.4″ 12.6 737.113 K7V + M1V unknown 4249 unknown 5 All planets orbit around the primary star. Planets e and f are potentially habitable.
Kepler-454 Lyra 19 09 55.0 +38° 13′ 44″ 11.57 753 G 1.028 5687 5.25 3
Kepler-25 Lyra 19 06 33.0 +39° 29′ 16″ 11 799 F 1.22 6190 unknown 3 Two planets were discovered by transit-timing variations, and the third planet was discovered by follow-up radial velocity measurements.
Kepler-114 Cygnus 19 36 29.0 +48° 20′ 58″ 13.7 846 K 0.71 4450 unknown 3
Kepler-54 Cygnus 19 39 06.0 +43° 03′ 23″ 16.3 886 M 0.52 3705 unknown 3
Kepler-20 Lyra 19 10 47.524 42° 20′ 19.30″ 12.51 950 G8V 0.912 5466 8.8 6 Planets e and f were the first Earth-sized planets to be discovered.
K2-19 Virgo 11 39 50.4804 +00° 36′ 12.8773″ 13.002 976 K0V or G9V 0.918 5250±70 8 3 -
PSR B1257+12 Virgo 13 00 03.58 +12° 40′ 56.5″ 24.31 980 pulsar 1.444 28856 0.797 3 Only pulsar with a multiplanetary system, and first exoplanets and multiplanetary system to be confirmed. Star with dimmest apparent magnitude to have a multiplanetary system.
Kepler-62 Lyra 18 52 51.060 +45° 20′ 59.507″ 13.75 990 K2V 0.69 4925 7 5 Planets e and f orbit in the habitable zone.
Kepler-48 Cygnus 19 56 33.41 +40° 56′ 56.47″ 13.04 1000 K 0.88 5190 unknown 5
Kepler-100 Lyra 19 25 32.6 +41° 59′ 24″ 1011 G1IV 1.109 5825 6.5 4
Kepler-49 Cygnus 19 29 11.0 +40° 35′ 30″ 15.5 1015 K 0.55 3974 unknown 4
Kepler-65 Lyra 19 14 45.3 +41° 09′ 04.2″ 11.018 1019 F6IV 1.199 6211 unknown 4 -
Kepler-52 Draco 19 06 57.0 +49° 58′ 33″ 15.5 1049 K 0.58 4075 unknown 3
K2-314 Libra 15 13 00.0 −16° 43′ 29″ 11.4 1059 G8IV/V 1.05 5430 9 3
K2-219 Pisces 00 51 22.9 +08° 52′ 04″ 12.09 1071 G2 1.02 5753±50 unknown 3
K2-268 Cancer 08 54 50.2862 +11° 50′ 53.7745″ 13.85 1079 unknown unknown unknown 5
K2-183 Cancer 08 20 01.7184 14° 01′ 10.0711″ 12.85 1083 unknown 5482±50 unknown 3
K2-187 Cancer 08 50 05.6682 23° 11′ 33.3712″ 12.864 1090 G?V 0.967 5438±63 unknown 4
Kepler-1542 Lyra 19 02 54.8 +42° 39′ 16″ 1096 G5V 0.94 5564 unknown 4 -
Kepler-26 Lyra 18 59 46 +46° 34′ 00″ 16 1100 M0V 0.65 4500 unknown 4 Transiting exoplanets which are low-density planets below the size of Neptune.
Kepler-167 Cygnus 19 30 38.0 +38° 20′ 43″ 1119 ± 6 0.76 4796 unknown 4
Kepler-81 Cygnus 19 34 32.9 +42° 49′ 30″ 15.56 1136 K?V 0.648 4391 unknown 3
Kepler-132 Lyra 18 52 56.6 +41° 20′ 35″ 1140 F9 0.98 6003 unknown 4
Kepler-80 Cygnus 19 44 27.0 +39° 58′ 44″ 14.804 1218 M0V 0.73 4250 unknown 6 Red dwarf star with six confirmed planets. Five of them are in an orbital resonance.
Kepler-159 Cygnus 19 48 16.8 +40° 52′ 08″ 1219 K 0.63 4625 unknown 2 (1) Star has a very low metallicity.
K2-299 Aquarius 22 05 06.5342 −14° 07′ 18.0135″ 13.12 1220 unknown 5724±72 unknown 3
Kepler-88 Lyra 19 24 35.5431 +40° 40′ 09.8098″ 13.5 1243 G8IV 1.022 5513±67 2.45 3
Kepler-174 Lyra 19 09 45.4 +43° 49:56′ 1269 K unknown 4880 unknown 3 Planet d may orbit in the habitable zone.
Kepler-32 Cygnus 19 51 22.0 +46° 34′ 27″ 16 1301.1 M1V 0.58 3900 unknown 3 (2) -
Kepler-83 Lyra 18 48 55.8 +43° 39′ 56″ 16.51 1306 K7V 0.664 4164 unknown 3
TOI-1338 Pictor 06 08 31.97 +59° 32′ 28.1″ 11.72 1318 F8
M		 1.127 6160 4.4 2 (0)
Kepler-271 Lyra 18 52 00.7 +44° 17′ 03″ 1319 G7V 0.9 5524 unknown 3 Metal-poor star
Kepler-169 19 03 60.0 +40° 55:10′ 12.186 1326 K2V 0.86 4997 unknown 5
Kepler-451 Cygnus 19 38 32.61 46° 03′ 59.1″ 1340 sdB
M		 0.6 29564 6 3 Three circumbinary planets orbit around the Kepler-451 binary pair.
Kepler-304 Cygnus 19 37 46.0 +40° 33′ 27″ 1418 K 0.8 4731 unknown 4
Kepler-18 Cygnus 19 52 19.06 +44° 44′ 46.76″ 13.549 1430 G7V 0.97 5345 10 3
Kepler-106 Cygnus 20 03 27.4 +44° 20′ 15″ 12.882 1449 G1V 1 5858 4.83 4
Kepler-92 Lyra 19 16 21.0 +41° 33′ 47″ 11.6 1463 G1IV 1.209 5871 5.52 3
Kepler-450 Cygnus 19 41 56.8 +51° 00′ 49″ 11.684 1487 F 1.19 6152 unknown 3
Kepler-89 Cygnus 19 49 20.0 +41° 53′ 28″ 12.4 1580 F8V 1.25 6116 3.9 4 Farthest F-type main sequence star from the Sun with a multiplanetary system. One study found hints of additional planets orbiting Kepler-89.
Kepler-1388 Lyra 18 53 20.6 +47° 10′ 28″ 1604 0.63 4098 unknown 4 -
K2-282 Pisces 00 53 43.6833 07° 59′ 43.1397″ 14.04 1638 G?V 0.94 5499±109 unknown 3
Kepler-107 Cygnus 19 48 06.8 +48° 12′ 31″ 12.7 1714 G2V 1.238 5851 4.29 4 -
Kepler-1047 Cygnus 19 14 35.1 +50° 47′ 20″ 1846 G2V 1.08 5754 unknown 3 -
Kepler-55 Lyra 19 00 40.0 +44° 01′ 35″ 16.3 1888 K 0.62 4362 unknown 5 Planet c may orbit in the inner habitable zone.
Kepler-166 Cygnus 19 32 38.4 +48° 52′ 52″ 1968 G 0.88 5413 unknown 3
Kepler-11 Cygnus 19 48 27.62 +41° 54′ 32.9″ 13.69 2150 ±20 G6V 0.954 5681 7.834 6 Farthest star from the Sun with exactly six exoplanets. First system discovered with six transiting planets. The planets have low densities.
Kepler-1254 Draco 19 34 59.3 +45° 06′ 26″ 2205 0.78 4985 unknown 3 -
Kepler-289 Cygnus 19 49 51.7 +42° 52′ 58″ 12.9 2283 G0V 1.08 5990 0.65 3 -
Kepler-85 Cygnus 19 23 54.0 +45° 17′ 25″ 15.0 2495 G 0.92 5666 unknown 4
Kepler-157 Lyra 19 24 23.3 +38° 52′ 32″ 2523 G2V 1.02 5774 unknown 3
Kepler-342 Cygnus 19 24 23.3 +38° 52′ 32″ 2549 F 1.13 6175 unknown 4
Kepler-148 Cygnus 19 19 08.7 +46° 51′ 32″ 2580 K?V 0.83 5019.0±122.0 unknown 3
Kepler-51 Cygnus 19 45 55.0 +49° 56′ 16″ 15.0 2610 G?V 1 5803 unknown 4 Super-puff planets with some of the lowest densities known.
Kepler-403 Cygnus 19 19 41.1 +46° 44′ 40″ 2741 F9IV-V 1.25 6090 unknown 3
Kepler-9 Lyra 19 02 17.76 +38° 24′ 03.2″ 13.91 2754 G2V 0.998 5722 3.008 3 First multiplanetary system to be discovered by the Kepler Space Telescope.
Kepler-23 Cygnus 19 36 52.0 +49° 28′ 45″ 14 2790 G5V 1.11 5760 unknown 3 -
Kepler-46 Cygnus 19 17 05.0 +42° 36′ 15″ 15.3 2795 K?V 0.902 5155 9.9 3 -
Kepler-305 Cygnus 19 56 53.83 +40° 20′ 35.46″ 15.812 2833 K 0.85 4918 unknown 3 (1)
Kepler-90 Draco 18 57 44.0 +49° 18′ 19″ 14.0 2840 ± 40 G0V 1.13 5930 2 8 All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets. A Hill stability test shows that the system is stable. Planet h orbits in the habitable zone.
Kepler-150 Lyra 19 12 56.2 +40° 31′ 15″ 2906 G?V 0.97 5560 unknown 5 Planet f orbits in the habitable zone.
Kepler-82 Cygnus 19 31 29.61 +42° 57′ 58.09″ 15.158 2949 G?V 0.91 5512 unknown 4
Kepler-154 Cygnus 19 19 07.3 +49° 53′ 48″ 2985 G3V 0.98 5690 unknown 5
Kepler-56 Cygnus 19 35 02.0 +41° 52′ 19″ 13 3060 K?III 1.32 4840 3.5 3
Kepler-350 Lyra 19 01 41.0 +39° 42′ 22″ 13.8 3121 F 1.03 6215 unknown 3
Kepler-603 Cygnus 19 37 07.4 +42° 17′ 27″ 3134 G2V 1.01 5808 unknown 3 -
Kepler-160 Lyra 19 11 05.65 +42° 52′ 09.5″ 13.101 3140 G2V unknown 5470 unknown 3 (1) The unconfirmed planet Kepler-160e (or KOI-456.04) is a potentially habitable planet.
Kepler-401 Cygnus 19 20 19.9 +50° 51′ 49″ 3149 F8V 1.17 6117 unknown 3
Kepler-58 Cygnus 19 45 26.0 +39° 06′ 55″ 15.3 3161 G1V 1.04 5843 unknown 3
Kepler-79 Cygnus 20 02 04.11 +44° 22′ 53.69″ 13.914 3329 F 1.17 6187 unknown 4
Kepler-60 Cygnus 19 15 50.70 +42° 15′ 54.04″ 13.959 3343 G 1.04 5915 unknown 3
Kepler-122 19 24 26.9 +39° 56′ 57″ 3351 F 1.08 6050 unknown 4
Kepler-279 Lyra 19 09 34.0 +42° 11′ 42″ 13.7 3383 F 1.1 6562 unknown 3
Kepler-255 Cygnus 19 44 15.4 +45° 58′ 37″ 3433 G6V 0.9 5573 unknown 3
Kepler-47 Cygnus 19 41 11.5 +46° 55′ 13.69″ 15.178 3442 G
M		 1.043 5636(A)
(B is unknown)		 4.5 3 Circumbinary planets, with one of the planets orbiting in the habitable zone.
Kepler-292 19 43 03.84 +43° 25′ 27.4″ 13.97 3446 K0V 0.85 5299 unknown 5
Kepler-27 Cygnus 19 28 56.82 +41° 05′ 9.15″ 15.855 3500 G5V 0.65 5400 unknown 3
Kepler-351 Lyra 19 05 48.6 +42° 39′ 28″ 3535 G?V 0.89 5643 unknown 3
Kepler-276 Cygnus 19 34 16 +39° 02′ 11″ 15.368 3734 G?V 1.1 5812 unknown 3
Kepler-24 Lyra 19 21 39.18 +38° 20′ 37.51″ 14.925 3910 G1V 1.03 5800 unknown 4 -
Kepler-87 Cygnus 19 51 40.0 +46° 57′ 54″ 15 4021 G4IV 1.1 5600 7.5 2 (2) Farthest system from the Sun with an unconfirmed exoplanet candidate.
Kepler-33 Lyra 19 16 18.61 +46° 00′ 18.8″ 13.988 4090 G1IV 1.164 5849 4.27 5
Kepler-282 Lyra 18 58 43.0 +44° 47′ 51″ 15.2 4363 G?V 0.97 5876 unknown 4
Kepler-758 Cygnus 19 32 20.3 +41° 08′ 08″ 4413 1.16 6228 unknown 4 Farthest system from the Sun with exactly four confirmed exoplanets.
Kepler-53 Lyra 19 21 51.0 +40° 33′ 45″ 16 4455 G?V 0.98 5858 unknown 3
Kepler-30 Lyra 19 01 08.07 +38° 56′ 50.21″ 15.403 4560 G6V 0.99 5498 unknown 3
Kepler-84 Cygnus 19 53 00.49 +40° 29′ 45.87″ 14.764 4700 G3IV 1 5755 unknown 5
Kepler-385 Cygnus 19 37 21.23 +50° 20′ 11.55″ 15.76 4900 F8V 0.99 5835 unknown 3 (4)
Kepler-31 Cygnus 19 36 06.0 +45° 51′ 11″ 15.5 5429 F 1.21 6340 unknown 3 The three planets are in an orbital resonance.
Kepler-238 Lyra 19 11 35 +40° 38′ 16″ 15.084 5867 G5IV 1.06 5614 unknown 5 One of the farthest systems from the Sun with a multiplanetary system, and the farthest system where exoplanets were discovered by the Kepler space telescope.
Kepler-245 Cygnus 19 26 33.4 +42° 26′ 11″ 0.8 5100 unknown 4
Kepler-218 Cygnus 19 41 39.1 +46° 15′ 59″ unknown 5502 unknown 3
Kepler-217 Cygnus 19 32 09.1 +46° 16′ 39″ unknown 6171 unknown 3
Kepler-192 Lyra 19 11 40.3 +45° 35′ 34″ unknown 5479 unknown 3
Kepler-191 Cygnus 19 24 44.0 +45° 19′ 23″ 0.85 5282 unknown 3
Kepler-176 Cygnus 19 38 40.3 +43° 51′ 12″ unknown 5232 unknown 4
Kepler-431 Lyra 18 44 26.9 +43° 13′ 40″ 1.071 6004 unknown 3
Kepler-338 Lyra 18 51 54.9 +40° 47′ 04″ 1.1 5923 unknown 4
Kepler-197 Cygnus 19 40 54.3 +50° 33′ 32″ unknown 6004 unknown 4
Kepler-247 Lyra 19 14 34.2 +43° 02′ 21″ 0.884 5094 unknown 3
Kepler-104 Lyra 19 10 25.1 +42° 10′ 00″ 0.81 5711 unknown 3 -
Kepler-126 Cygnus 19 17 23.4 +44° 12′ 31″ unknown 6239 unknown 3 -
Kepler-127 Lyra 19 00 45.6 +46° 01′ 41″ unknown 6106 unknown 3 -
Kepler-130 Lyra 19 13 48.2 +40° 14′ 43″ 1 5884 unknown 3 -
Kepler-164 Lyra 19 11 07.4 +47° 37′ 48″ 1.11 5888 unknown 3 -
Kepler-171 Cygnus 19 47 05.3 +41° 45′ 20″ unknown 5642 unknown 3 -
Kepler-172 Lyra 19 47 05.3 +41° 45′ 20″ 0.86 5526 unknown 4 -
Kepler-149 Lyra 19 03 24.9 +38° 23′ 03″ unknown 5381 unknown 3
Kepler-142 Cygnus 19 40 28.5 +48° 28′ 53″ 0.99 5790 unknown 3
Kepler-124 Draco 19 07 00.7 +49° 03′ 54″ unknown 4984 unknown 3
Kepler-402 Lyra 19 13 28.9 +43° 21′ 17″ unknown 6090 unknown 4
Kepler-399 Cygnus 19 58 00.4 +40° 40′ 15″ unknown 5502 unknown 3
Kepler-374 Cygnus 19 36 33.1 +42° 22′ 14″ 0.84 5977 unknown 3
Kepler-372 Cygnus 19 25 01.5 +49° 15′ 32″ 1.15 6509 unknown 3
Kepler-363 Lyra 18 52 46.1 +41° 18′ 19″ 1.23 5593 unknown 3
Kepler-359 Cygnus 19 33 10.5 +42° 11′ 47″ 1.07 6248 unknown 3
Kepler-357 Cygnus 19 24 58.3 +44° 00′ 31″ 0.78 5036 unknown 3
Kepler-354 Lyra 19 03 00.4 +41° 20′ 08″ 0.65 4648 unknown 3
Kepler-206 Lyra 19 26 32.3 +41° 50′ 02″ 0.94 5764 unknown 3
Kepler-203 Cygnus 19 01 23.3 +41° 45′ 43″ 0.98 5821 unknown 3
Kepler-194 Cygnus 19 27 53.1 +47° 51′ 51″ unknown 6089 unknown 3
Kepler-184 Lyra 19 27 48.5 +43° 04′ 29″ unknown 5788 unknown 3
Kepler-178 Lyra 19 08 24.3 +46° 53′ 47″ unknown 5676 unknown 3
Kepler-336 Lyra 19 20 57.0 +41° 19′ 53″ 0.89 5867 unknown 3
Kepler-334 Lyra 19 08 33.8 +47° 06′ 55″ 1 5828 unknown 3
Kepler-332 Lyra 19 06 39.1 +47° 24′ 49″ 0.8 4955 unknown 3
Kepler-331 Lyra 19 27 20.2 +39° 18′ 26″ 0.51 4347 unknown 3
Kepler-327 Cygnus 19 30 34.2 44° 05′ 16″ 0.55 3799 unknown 3
Kepler-326 Cygnus 19 37 18.1 +46° 00′ 08″ 0.98 5105 unknown 3
Kepler-325 Cygnus 19 19 20.5 +49° 49′ 32″ 0.87 5752 unknown 3

Stars orbited by both planets and brown dwarfs

Stars orbited by objects on both sides of the ~13 Jupiter mass dividing line.

See also

For links to specific lists of exoplanets see:

Online archives:


Notes

  1. Barnard's Star at closer distance has a candidate four-planet system, of which one planet has been confirmed so far.

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