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==Data Table== ==Data Table==
{{sticky header}}
{| class="wikitable sortable" style="text-align:center" {| class="wikitable sortable sticky-header" style="text-align:center"
! Name
! M🜨
! R🜨
! g
! Ts
! ''a''
! ''e''
! class="unsortable" |
! D
|- class="sorttop"
! !
! {{Vertical header|Mass (in Earth masses)}} ! {{Vertical header|Mass (in Earth masses)}}
Line 103: Line 114:
! {{Vertical header|Main source}} ! {{Vertical header|Main source}}
! {{Vertical header|Distance from the Sun in lightyears}} ! {{Vertical header|Distance from the Sun in lightyears}}
|-
! Name
! M🜨
! R🜨
! g
! Ts
! ''a''
! ''e''
! class="unsortable" |
! D
|- |-
| ]|| ≥1.27 || ~1.1|| || {{free|234 K <br />-39°C}} || 0.05||<0.35 || <ref name="nature_paper" />||4.22 | ]|| ≥1.27 || ~1.1|| || {{free|234 K <br />-39°C}} || 0.05||<0.35 || <ref name="nature_paper" />||4.22
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| ]|| ≥2.89||≥1.35|| || {{free|259 K<br />-14&nbsp;°C}}|| 0.091 || 0.10 || ||12.20 | ]|| ≥2.89||≥1.35|| || {{free|259 K<br />-14&nbsp;°C}}|| 0.091 || 0.10 || ||12.20
|- |-
| ]|| ≥4.3||≥1.64|| ||{{free| -<br /> -}} || || ||<ref name="ReferenceA">{{Cite web|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|title = HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo}}</ref> ||13.8 | ]|| ≥4.3||≥1.64|| ||{{free| -<br /> -}} || || ||<ref name="ReferenceA">{{Cite web|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|title=HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo|access-date=2013-01-26|archive-date=2012-06-01|archive-url=https://web.archive.org/web/20120601044944/http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|url-status=dead}}</ref> ||13.8
|- |-
| ]|| ≥5.21||≥2.04|| ||{{free| -<br /> -}} || || || ||13.8 | ]|| ≥5.21||≥2.04|| ||{{free| -<br /> -}} || || || ||13.8
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|- |-
| ]||≥5.4 || || || {{won|251 K<br />-22 °C}} | ]||≥5.4 || || || {{won|251 K<br />-22 °C}}
|| 0.162 || 0.03 || <ref name="phl.upr.edu"/><ref>{{cite web|url=http://phl.upr.edu/press-releases/gliese832|title=A Nearby Super-Earth with the Right Temperature but Extreme Seasons - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015}}</ref>||16.16 || 0.162 || 0.03 || <ref name="phl.upr.edu"/><ref>{{cite web|url=http://phl.upr.edu/press-releases/gliese832|title=A Nearby Super-Earth with the Right Temperature but Extreme Seasons - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015|archive-date=13 May 2019|archive-url=https://web.archive.org/web/20190513221647/http://phl.upr.edu/press-releases/gliese832|url-status=dead}}</ref>||16.16
|- |-
| ]|| ≥2.7 || || || {{bad|660 K<br /> 387&nbsp;°C<ref name="aaa534"/> }} || 0.1207 || 0||<ref name=epe_HD_20794/>||19.71 | ]|| ≥2.7 || || || {{bad|660 K<br /> 387&nbsp;°C<ref name="aaa534"/> }} || 0.1207 || 0||<ref name=epe_HD_20794/>||19.71
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|| 0.05 || 0.09 || <ref name="hec"/> || 22 || 0.05 || 0.09 || <ref name="hec"/> || 22
|- |-
|]<ref>{{cite journal |doi=10.1051/0004-6361/201014704 |last1=Bonfils |first1=Xavier |last2=Delfosse |first2=Xavier |last3=Udry |first3=Stéphane |last4=Forveille |first4=Thierry |last5=Mayor |first5=Michel |last6=Perrier |first6=Christian |last7=Bouchy |first7=François |last8=Gillon |first8=Michaël |last9=Lovis |first9=Christophe |last10=Pepe |first10=Francesco |last11=Queloz |first11=Didier |last12=Santos |first12=Nuno C. |last13=Ségransan |first13=Damien |last14=Bertaux |first14=Jean-Loup |title=The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample |journal=Astronomy and Astrophysics |date=2011 |volume=549 |bibcode=2013A&A...549A.109B |arxiv = 1111.5019 |pages=A109 |s2cid=119288366 }}</ref><ref>{{cite web|url=http://phl.upr.edu/press-releases/apotentialhabitableexoplanetinanearbytriplestarsystem|title=A Potential Habitable Exoplanet in a Nearby Triple Star System - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015}}</ref>|| 3.8 || || 1.32 ||{{won|302 K <br />29&nbsp;°C }} |]<ref>{{cite journal |doi=10.1051/0004-6361/201014704 |last1=Bonfils |first1=Xavier |last2=Delfosse |first2=Xavier |last3=Udry |first3=Stéphane |last4=Forveille |first4=Thierry |last5=Mayor |first5=Michel |last6=Perrier |first6=Christian |last7=Bouchy |first7=François |last8=Gillon |first8=Michaël |last9=Lovis |first9=Christophe |last10=Pepe |first10=Francesco |last11=Queloz |first11=Didier |last12=Santos |first12=Nuno C. |last13=Ségransan |first13=Damien |last14=Bertaux |first14=Jean-Loup |title=The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample |journal=Astronomy and Astrophysics |date=2011 |volume=549 |bibcode=2013A&A...549A.109B |arxiv = 1111.5019 |pages=A109 |s2cid=119288366 }}</ref><ref>{{cite web|url=http://phl.upr.edu/press-releases/apotentialhabitableexoplanetinanearbytriplestarsystem|title=A Potential Habitable Exoplanet in a Nearby Triple Star System - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015|archive-date=25 February 2021|archive-url=https://web.archive.org/web/20210225032824/http://phl.upr.edu/press-releases/apotentialhabitableexoplanetinanearbytriplestarsystem|url-status=dead}}</ref>|| 3.8 || || 1.32 ||{{won|302 K <br />29&nbsp;°C }}
|| 0.13 || 0.34 || <ref name="hec"/> || 22 || 0.13 || 0.34 || <ref name="hec"/> || 22
|- |-
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|- |-
| ]|| ≥2.3 || || ||{{won|312 K<br />39&nbsp;°C }} | ]|| ≥2.3 || || ||{{won|312 K<br />39&nbsp;°C }}
|| || ||<ref name="arxiv.org"/><ref name="phl.upr.edu">{{cite web|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|title=HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015}}</ref> ||38 || || ||<ref name="arxiv.org"/><ref name="phl.upr.edu">{{cite web|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|title=HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo|access-date=3 October 2015|archive-date=1 June 2012|archive-url=https://web.archive.org/web/20120601044944/http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|url-status=dead}}</ref> ||38


|- |-
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|| 0.247 ||0.02|| <ref name="tuomi12"/>||42 || 0.247 ||0.02|| <ref name="tuomi12"/>||42
|- |-
| ]|| ≥7.1 || || || {{free|284 K<br />11&nbsp;°C<ref>{{cite web |title=HEC: Data of Potential Habitable Worlds |url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data |date=November 12, 2012 |publisher=] (Planetary Habitability Laboratory)}}</ref>}} | ]|| ≥7.1 || || || {{free|284 K<br />11&nbsp;°C<ref>{{cite web |title=HEC: Data of Potential Habitable Worlds |url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data |date=November 12, 2012 |publisher=] (Planetary Habitability Laboratory) |access-date=January 26, 2013 |archive-date=June 1, 2012 |archive-url=https://web.archive.org/web/20120601044944/http://phl.upr.edu/projects/habitable-exoplanets-catalog/data |url-status=dead }}</ref>}}
|| 0.600 ||0.29||<ref name="tuomi12"/>||42 || 0.600 ||0.29||<ref name="tuomi12"/>||42
|- |-
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'''Note''': There is no ] about terrestrial composition of most of the planets in the list. Sources in the "Main source" column confirm the ''possibility'' of terrestrial composition. '''Note''': There is no ] about terrestrial composition of most of the planets in the list. Sources in the "Main source" column confirm the ''possibility'' of terrestrial composition.


In September 2012, the discovery of two planets orbiting ]<ref name="Simbad-20120920">{{cite web|author=Staff |title=LHS 188 -- High proper-motion Star |url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HIP+19394 |date=September 20, 2012 |publisher=](Strasbourg astronomical Data Center) |access-date=September 20, 2012 }}</ref> was announced.<ref name="PHL-20120829">{{cite web |last=Méndez |first=Abel |title=A Hot Potential Habitable Exoplanet around Gliese 163|url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163 |date=August 29, 2012|publisher=] (Planetary Habitability Laboratory)|access-date=September 20, 2012 }}</ref><ref name="Space-20120920">{{cite news |last=Redd |first = Nola Taylor|title=Newfound Alien Planet a Top Contender to Host Life|url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html|date=September 20, 2012|work=] |access-date=September 20, 2012 }}</ref> One of the planets, ], about 6.9 times the mass of Earth and somewhat hotter, was considered to be within the ], but is probably not terrestrial.<ref name="PHL-20120829"/><ref name="Space-20120920"/> In September 2012, the discovery of two planets orbiting ]<ref name="Simbad-20120920">{{cite web|author=Staff |title=LHS 188 -- High proper-motion Star |url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HIP+19394 |date=September 20, 2012 |publisher=](Strasbourg astronomical Data Center) |access-date=September 20, 2012 }}</ref> was announced.<ref name="PHL-20120829">{{cite web |last=Méndez |first=Abel |title=A Hot Potential Habitable Exoplanet around Gliese 163 |url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163 |date=August 29, 2012 |publisher=] (Planetary Habitability Laboratory) |access-date=September 20, 2012 |archive-date=October 21, 2019 |archive-url=https://web.archive.org/web/20191021202448/http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163 |url-status=dead }}</ref><ref name="Space-20120920">{{cite news |last=Redd |first = Nola Taylor|title=Newfound Alien Planet a Top Contender to Host Life|url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html|date=September 20, 2012|work=] |access-date=September 20, 2012 }}</ref> One of the planets, ], about 6.9 times the mass of Earth and somewhat hotter, was considered to be within the ], but is probably not terrestrial.<ref name="PHL-20120829"/><ref name="Space-20120920"/>


In May 2016, the finding of three Earth-like planets of ultracool dwarf ] has been released. In May 2016, the finding of three Earth-like planets of ultracool dwarf ] has been released.


The existence of the planet ] was refuted in 2022, when a study found that the ] signal shows characteristics of a signal originating from stellar activity, and not from a planet. The existence of the planet ] was refuted in 2022, when a study found that the ] signal shows characteristics of a signal originating from stellar activity, and not from a planet.<ref>https://www.aanda.org/articles/aa/abs/2022/08/aa43063-22/aa43063-22.html</ref>


==Statistics== ==Statistics==

Latest revision as of 03:29, 24 December 2024

This article needs to be updated. The reason given is: The article does not yet include recent discoveries such as Teegarden b and c, the planets of L 98-59, Gliese 486 b and Wolf 1069 b.. Please help update this article to reflect recent events or newly available information. (February 2024)

This list of nearest terrestrial exoplanet candidates contains possible terrestrial ("rocky") exoplanets spaced at a distance of up to 50 light-years from the Solar System, ordered by increasing distance.

They may be composed primarily of silicate rocks and/or metals. Within the Solar System, the terrestrial planets are the inner planets closest to the Sun.

Exoplanets discovered (incomplete)

This list is incomplete, currently containing 34 exoplanets, 11 of which probably lie inside their star's habitable zone.

There are roughly 2,000 stars at a distance of up to 50 light-years from the Solar System (64 of them are yellow-orange "G" stars like the Sun). As many as 15% of them could have Earth-sized planets in the habitable zones.

On November 4, 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarf stars within the Milky Way galaxy. Eleven billion of these estimated planets may be orbiting Sun-like stars. The nearest such planet was then as close as 12 light-years away but (see below) is now estimated slightly above four light-years away.

On August 24, 2016, astronomers announced the discovery of a rocky planet in the habitable zone of Proxima Centauri, the closest star to Earth (not counting the Sun). Called Proxima b, the planet is 1.3 times the mass of Earth and has an orbital period of roughly 11.2 Earth days. However, Proxima Centauri's classification as a red dwarf casts doubts on the habitability of any exoplanets in its orbit due to low stellar flux, high probability of tidal locking, small circumstellar habitable zones and high stellar variation. Another likely candidate is Alpha Centauri, Earth's nearest Sun-like star system 4.37 light-years away. Estimates place the probability of finding a habitable planet around Alpha Centauri A or B at roughly 75%. Alpha Centauri is the target of several exoplanet-finding missions, including Breakthrough Starshot and Mission Centaur, the latter of which is chronicled in the 2016 documentary film The Search for Earth Proxima.

In 2023, astronomers used the radial velocity method to confirm that the exoplanet Wolf 1069 b sits in the habitable zone of Wolf 1069. Located 31 light years from Earth, this planet is 1.26 times the mass of Earth and has a radius of 1.08 times the Earth's. Though Wolf 1069 b is likely tidally locked, its daylight side may still be habitable. It has similar characteristics to Proxima Centauri b and is one of the nearest discovered potentially habitable exoplanets to Earth. Wolf 1069 b is likely rocky, with an Earth-like composition, and climate models suggest that it is habitable for a broad range of possible atmospheres although the nature of its true atmosphere is unknown. Characterizing its atmosphere is more difficult than with a transiting exoplanet as transmission spectroscopy is inapplicable, and instruments for alternative techniques such as analysis of thermal emission and reflected light are not yet available. The angular separation between Wolf 1069 b and its star is also small, which further complicates these measurements.

Data Table

Name M🜨 R🜨 g Ts a e D
Mass (in Earth masses) Radius (in Earth radii) Surface gravity (1 – standard Earth gravity) Surface temperature Semi-major axis in astronomical units Orbital eccentricity Main source Distance from the Sun in lightyears
Proxima Centauri b ≥1.27 ~1.1 234 K
-39°C
0.05 <0.35 4.22
Proxima Centauri c ~7 39 K
-234 °C
~1.489 ~0.04 4.22
Ross 128 b ≥1.40 213 to 301 K
-60 to 28 °C
11.03
Luyten b ≥2.89 ≥1.35 259 K
-14 °C
0.091 0.10 12.20
Wolf 1061c ≥4.3 ≥1.64 -
-
13.8
Wolf 1061d ≥5.21 ≥2.04 -
-
13.8
Wolf 1069 b 1.26 1.08 250.1 K
-23.1 °C
0.0672 31
Gliese 876 d 6.8 650 K
377 °C
0.021 0.21 15
Gliese 682 b ≥2 -
-


16
Gliese 832 c ≥5.4 251 K
-22 °C
0.162 0.03 16.16
82 G. Eridani b ≥2.7 660 K
387 °C
0.1207 0 19.71
82 G. Eridani c ≥2.4 508 K
235 °C
0.2036 0 19.71
82 G. Eridani d ≥4.8 388 K
115 °C
0.3499 0 19.71
Gliese 581 e ≥1.7 -
-
0.029 0 20
Gliese 581 c ≥5.6 -
-
0.072 0 20
Gliese 581 d ≥5.6 2.34 1.27 233 K
-41 °C
0.218 0 20
HD 219134 b 4.5 1.6 700 K
427 °C
21
Gliese 667 Cb 6.30 1.44 445 K

172 °C

0.05 0.09 22
Gliese 667 Cc 3.8 1.32 302 K
29 °C
0.13 0.34 22
61 Virginis b ≥5.1 -
-
0.050 0.12 28
HD 85512 b ≥3.6 1.74 1.33 351 K
78 °C
0.26 0.11 36
GJ 180 b ≥2.3 312 K
39 °C
38
TRAPPIST-1b -
-
39.5
TRAPPIST-1c -
-
39.5
TRAPPIST-1d 0.48 282.1 K
9 °C
39.5
TRAPPIST-1e 246.1 K
-27.1 °C
39.5
TRAPPIST-1f 219 K
-54 °C
39.5
TRAPPIST-1g 198.6 K
-75 °C
39.5
TRAPPIST-1h 169 K
-104 °C
39.5
55 Cancri e
(Janssen)
8.6 -
-
0.016 0.17 40
HD 40307 b ≥4.2 -
-
0.047 0.2 42
HD 40307 c ≥6.8 -
-
0.081 0.06 42
HD 40307 d ≥9.2 -
-
0.134 0.07 42
HD 40307 e ≥3.5 -
-
0.1886 0.15 42
HD 40307 f ≥5.2 385 K
112 °C
0.247 0.02 42
HD 40307 g ≥7.1 284 K
11 °C
0.600 0.29 42

Note: There is no scientific consensus about terrestrial composition of most of the planets in the list. Sources in the "Main source" column confirm the possibility of terrestrial composition.

In September 2012, the discovery of two planets orbiting Gliese 163 was announced. One of the planets, Gliese 163 c, about 6.9 times the mass of Earth and somewhat hotter, was considered to be within the habitable zone, but is probably not terrestrial.

In May 2016, the finding of three Earth-like planets of ultracool dwarf TRAPPIST-1 has been released.

The existence of the planet Gliese 832 c was refuted in 2022, when a study found that the radial velocity signal shows characteristics of a signal originating from stellar activity, and not from a planet.

Statistics

Distance from the Solar System
Distance Lying within
the habitable zone
All
< 10 light-years 0 (2?) 2
< 20 light-years 6 15
< 30 light-years 8 22
< 40 light-years 10 24
< 50 light-years 11 31

Note: in most cases the composition of the atmosphere and atmosphere pressure of exoplanets are unknown, so surface temperatures are estimates based on computer models and expert opinions.

See also

References

  1. ^ Pepe, F.; et al. (2011), "The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310", Astronomy & Astrophysics, 534: A58, arXiv:1108.3447, Bibcode:2011A&A...534A..58P, doi:10.1051/0004-6361/201117055, S2CID 15088852
  2. ^ Schneider, Jean, "Star: HD 20794", Extrasolar Planets Encyclopaedia, archived from the original on October 8, 2011, retrieved 2011-12-05
  3. ^ Tuomi, Mikko; Anglada-Escudé, Guillem; Gerlach, Enrico; Jones, Hugh R. A.; Reiners, Ansgar; Rivera, Eugenio J.; Vogt, Steven S.; Butler, R. Paul (17 December 2012). "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307". Astronomy & Astrophysics. 549: A48. arXiv:1211.1617. Bibcode:2013A&A...549A..48T. doi:10.1051/0004-6361/201220268. S2CID 7424216.
  4. "Stars within 50 light years". Retrieved 3 October 2015.
  5. "G stars within 100 light-years". Retrieved 3 October 2015.
  6. ^ Tuomi, Mikko; Jones, Hugh R. A.; Barnes, John R.; Anglada-Escudé, Guillem; Jenkins, James S. (2014). "Bayesian search for low-mass planets around nearby M dwarfs. Estimates for occurrence rate based on global detectability statistics". Monthly Notices of the Royal Astronomical Society. 441 (2): 1545–1569. arXiv:1403.0430. Bibcode:2014MNRAS.441.1545T. doi:10.1093/mnras/stu358.
  7. ^ Overbye, Dennis (November 4, 2013). "Far-Off Planets Like the Earth Dot the Galaxy". New York Times. Retrieved November 5, 2013.
  8. ^ Petigura, Eric A.; Howard, Andrew W.; Marcy, Geoffrey W. (October 31, 2013). "Prevalence of Earth-size planets orbiting Sun-like stars". Proceedings of the National Academy of Sciences of the United States of America. 110 (48): 19273–19278. arXiv:1311.6806. Bibcode:2013PNAS..11019273P. doi:10.1073/pnas.1319909110. PMC 3845182. PMID 24191033.
  9. Khan, Amina (November 4, 2013). "Milky Way may host billions of Earth-size planets". Los Angeles Times. Retrieved November 5, 2013.
  10. ^ Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; et al. (2016). "A terrestrial planet candidate in a temperate orbit around Proxima Centauri" (PDF). Nature. 536 (7617): 437–440. arXiv:1609.03449. Bibcode:2016Natur.536..437A. doi:10.1038/nature19106. PMID 27558064. S2CID 4451513.
  11. Billings, Lee. "Miniature Space Telescope Could Boost the Hunt for "Earth Proxima"". Scientific American.
  12. "The Search for Earth Proxima". The Atlantic.
  13. ^ Kossakowski, Diana; Kürster, Martin; Trifonov, Trifon; Henning, Thomas; Kemmer, Jonas; et al. (2023-02-10). "The CARMENES search for exoplanets around M dwarfs - Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star". Astronomy & Astrophysics. 670 (February 2023). A84. arXiv:2301.02477v2. doi:10.1051/0004-6361/202245322.
  14. Tognetti, Laurence (2023-02-03). "Astronomers discover potential habitable exoplanet only 31 light-years from Earth". Space.com.
  15. Nielbock, Marcus (2023-02-03). "A nearby potentially habitable Earth-mass exoplanet". Max Planck Institute for Astronomy. Retrieved 2024-10-07.
  16. Wall, Mike (12 April 2019). "Possible 2nd Planet Spotted Around Proxima Centauri". Space.com. Retrieved 22 July 2020.
  17. ^ "HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo". Archived from the original on 2012-06-01. Retrieved 2013-01-26.
  18. Fogg, M. J.; Nelson, R. P. (2005). "Oligarchic and giant impact growth of terrestrial planets in the presence of gas giant planet migration". Astronomy and Astrophysics. 441 (2): 791–806. arXiv:astro-ph/0507180. Bibcode:2005A&A...441..791F. doi:10.1051/0004-6361:20053453. S2CID 15248175.
  19. Rivera, E.; et al. (2005). "A ~7.5 M🜨 Planet Orbiting the Nearby Star, GJ 876". The Astrophysical Journal. 634 (1): 625–640. arXiv:astro-ph/0510508. Bibcode:2005ApJ...634..625R. doi:10.1086/491669. S2CID 14122053.
  20. Eugenio J. Rivera, Gregory Laughlin, R. Paul Butler, Steven S. Vogt, Nader Haghighipour, Stefano Meschiari (2010). "The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration".
  21. http://www.hpcf.upr.edu/~abel/phl/tuomi/hec_orbit_GJ_682_b.png
  22. ^ "HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo". Archived from the original on 1 June 2012. Retrieved 3 October 2015.
  23. "A Nearby Super-Earth with the Right Temperature but Extreme Seasons - Planetary Habitability Laboratory @ UPR Arecibo". Archived from the original on 13 May 2019. Retrieved 3 October 2015.
  24. ^ Vogt, S. S. (2010). "The Lick-Carnegie Exoplanet Survey: A 3.1 M_Earth Planet in the Habitable Zone of the Nearby M3V Star Gliese 581". The Astrophysical Journal. 723 (1): 954–965. arXiv:1009.5733. Bibcode:2010ApJ...723..954V. doi:10.1088/0004-637x/723/1/954. S2CID 3163906.
  25. Valencia; Sasselov, Dimitar D.; O'Connell, Richard J. (2007). "Radius and Structure Models of the First Super-Earth Planet". The Astrophysical Journal. 656 (1): 545–551. arXiv:astro-ph/0610122. Bibcode:2007ApJ...656..545V. doi:10.1086/509800. S2CID 17656317.
  26. von Bloh, W.; Bounama, C.; Cuntz, M.; Franck, S. (2007). "The Habitability of Super-Earths in Gliese 581". Astronomy & Astrophysics. 476 (3): 1365–1371. arXiv:0705.3758. Bibcode:2007A&A...476.1365V. doi:10.1051/0004-6361:20077939. S2CID 14475537.
  27. ^ The Habitable Exoplanets Catalog. The values are just the best estimates and are subject to change.
  28. "Astronomers find star with three super-Earths".
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