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| | ] || 5±2.5 || 4±1.6 || || || || 2013 | | ] || 5±2.5 || 4±1.6 || || || || 2013 | ||
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| | ] || 0.03 ± 0.0075 || 0.92 <ref>{{cite journal |
| ] || 0.03 ± 0.0075 || 0.92 <ref>{{cite journal|title=MOA-2010-BLG-328Lb: A Sub-Neptune Orbiting very Late M Dwarf?|first1=K.|last1=Furusawa|first2=A.|last2=Udalski|first3=T.|last3=Sumi|first4=D. P.|last4=Bennett|first5=I. A.|last5=Bond|first6=A.|last6=Gould|first7=U. G.|last7=Jørgensen|first8=C.|last8=Snodgrass|first9=D. Dominis|last9=Prester|first10=M. D.|last10=Albrow|first11=F.|last11=Abe|first12=C. S.|last12=Botzler|first13=P.|last13=Chote|first14=M.|last14=Freeman|first15=A.|last15=Fukui|first16=P.|last16=Harris|first17=Y.|last17=Itow|first18=C. H.|last18=Ling|first19=K.|last19=Masuda|first20=Y.|last20=Matsubara|first21=N.|last21=Miyake|first22=Y.|last22=Muraki|first23=K.|last23=Ohnishi|first24=N. J.|last24=Rattenbury|first25=To|last25=Saito|first26=D. J.|last26=Sullivan|first27=D.|last27=Suzuki|first28=W. L.|last28=Sweatman|first29=P. J.|last29=Tristram|first30=K.|last30=Wada|first31=P. C. M.|last31=Yock|first32=The MOA|last32=Collaboration|first33=M. K.|last33=Szymański|first34=I.|last34=Soszyński|first35=M.|last35=Kubiak|first36=R.|last36=Poleski|first37=K.|last37=Ulaczyk|first38=G.|last38=Pietrzyński|first39=Ł|last39=Wyrzykowski|first40=The OGLE|last40=Collaboration|first41=J.-Y.|last41=Choi|first42=G. W.|last42=Christie|first43=D. L.|last43=DePoy|first44=Subo|last44=Dong|first45=J.|last45=Drummond|first46=B. S.|last46=Gaudi|first47=C.|last47=Han|last48=L.-W. Hung|first49=K.-H.|last49=Hwang|first50=C.-U.|last50=Lee|first51=J.|last51=McCormick|first52=D.|last52=Moorhouse|first53=T.|last53=Natusch|first54=M.|last54=Nola|first55=E.|last55=Ofek|first56=R. W.|last56=Pogge|last57=I.-G. Shin|first58=J.|last58=Skowron|first59=G.|last59=Thornley|first60=J. C.|last60=Yee|first61=The μFUN|last61=Collaboration|first62=K. A.|last62=Alsubai|first63=V.|last63=Bozza|first64=P.|last64=Browne|first65=M. J.|last65=Burgdorf|first66=S. Calchi|last66=Novati|first67=P.|last67=Dodds|first68=M.|last68=Dominik|first69=F.|last69=Finet|first70=T.|last70=Gerner|first71=S.|last71=Hardis|first72=K.|last72=Harpsøe|first73=T. C.|last73=Hinse|last74=M. Hundertmark|first75=N.|last75=Kains|first76=E.|last76=Kerins|first77=C.|last77=Liebig|first78=L.|last78=Mancini|first79=M.|last79=Mathiasen|first80=M. T.|last80=Penny|first81=S.|last81=Proft|first82=S.|last82=Rahvar|last83=D. Ricci|first84=G.|last84=Scarpetta|first85=S.|last85=Schäfer|first86=F.|last86=Schönebeck|first87=J.|last87=Southworth|first88=J.|last88=Surdej|first89=J.|last89=Wambsganss|first90=The MiNDSTEp|last90=Consortium|first91=R. A.|last91=Street|first92=D. M.|last92=Bramich|first93=I. A.|last93=Steele|first94=Y.|last94=Tsapras|first95=The RoboNet|last95=Collaboration|first96=K.|last96=Horne|last97=J. Donatowicz|first98=K. C.|last98=Sahu|first99=E.|last99=Bachelet|first100=V.|last100=Batista|first101=T. G.|last101=Beatty|first102=J.-P.|last102=Beaulieu|first103=C. S.|last103=Bennett|first104=C.|last104=Black|first105=|last105=R. Bowens-Rubin|first106=S.|last106=Brillant|first107=J. A. R.|last107=Caldwell|first108=A.|last108=Cassan|first109=A. A.|last109=Cole|first110=E.|last110=Corrales|first111=C.|last111=Coutures|first112=|last112=S. Dieters|first113=P.|last113=Fouqué|first114=J.|last114=Greenhill|first115=C. B.|last115=Henderson|first116=D.|last116=Kubas|first117=J.-B.|last117=Marquette|first118=R.|last118=Martin|first119=J. W.|last119=Menzies|first120=|last120=B. Shappee|first121=A.|last121=Williams|first122=D.|last122=Wouters|first123=J. van|last123=Saders|first124=R.|last124=Zellem|first125=M.|last125=Zub|first126=The PLANET|last126=Collaboration|date=23 April 2018|journal=The Astrophysical Journal|volume=779|issue=2|pages=91|doi=10.1088/0004-637X/779/2/91|arxiv=1309.7714|bibcode=2013ApJ...779...91F|displayauthors=29}}</ref> || || || || 2013 | ||
| |- | |- | ||
| | ] || 5±2.5 || 4±1.6 || || || || 2013 | | ] || 5±2.5 || 4±1.6 || || || || 2013 | ||
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| == External links == | == External links == | ||
| * {{cite web |url=http://exoplanet.eu/catalog-microlensing.php |title=Exoplanets detected by microlensing | |
* {{cite web |url=http://exoplanet.eu/catalog-microlensing.php |title=Exoplanets detected by microlensing |encyclopedia=] |accessdate=2011-01-20}} | ||
| * {{cite web |url=http://exoplanets.org/table/ |title=Exoplanets Data Explorer |accessdate=2011-01-20}} | * {{cite web |url=http://exoplanets.org/table/ |title=Exoplanets Data Explorer |accessdate=2011-01-20}} | ||
Revision as of 21:07, 2 December 2019
 | This article needs to be updated. Please help update this article to reflect recent events or newly available information. (August 2014) |
This is the list of 19 extrasolar planets detected by microlensing, sorted by projected separations. To find planets using that method, the background star is temporarily magnified by a foreground star because of the gravity that bends light. If the foreground star has a planet, the light from background star would be slightly brighter than the star with no planet. Studying the brightness difference of background star between the foreground star with planets and foreground star with no planets, then mass can be estimated. The projected separation can be determined from how much the light bended.
The most massive planet detected by microlensing is MOA-bin-1b, which masses 3.7 MJ; the least massive is MOA-2007-BLG-192Lb, which masses 0.01 MJ or 3.3 ME. The widest separation between a planet and a star is MOA-bin-1b, which is 8.3 AU; the shortest separation is MOA-2007-BLG-192Lb, which is 0.66 AU.
There are 2 members of the multi-planet systems.
Yellow rows denote the members of the multi-planet system
| Planet | Mass (MJ) | Projected separation (AU) | Period (d) | Eccentricity | Inclination (°) | Year of discovery |
|---|---|---|---|---|---|---|
| MOA-2007-BLG-192Lb | 0.01 | 0.66 | 2008 | |||
| MOA-2007-BLG-400Lb | 0.9 | 0.85 | 2008 | |||
| MOA-2011-BLG-293Lb | 2.4 | 1.0 | 2012 | |||
| MOA-2008-BLG-310Lb | 0.23 | 1.25 | 2009 | |||
| MOA-2009-BLG-387Lb | 2.6 | 1.8 | 1970 | 2011 | ||
| MOA-2009-BLG-319b | 0.157 | 2.0 | 2010 | |||
| OGLE-2005-BLG-390Lb | 0.017 | 2.1 | 3500 | 2005 | ||
| OGLE-2006-BLG-109Lb | 0.727 | 2.3 | 1790 | 64 | 2008 | |
| OGLE-2005-BLG-169Lb | 0.04 | 2.8 | 3300 | 2005 | ||
| MOA-2009-BLG-266Lb | 0.0327 | 3.2 | 2780 | 2010 | ||
| OGLE-2007-BLG-368Lb | 0.0694 | 3.3 | 2008 | |||
| OGLE-2005-BLG-071Lb | 3.5 | 3.6 | ~ 3600 | 2005 | ||
| OGLE-2006-BLG-109Lc | 0.271 | 4.5 | 4931 | 0.15 | 64 | 2008 |
| OGLE-2003-BLG-235Lb | 2.6 | 5.1 | 2004 | |||
| MOA-bin-1 b | 3.7 | 8.3 | 2012 | |||
| OGLE-2012-BLG-0026Lb | 0.11 | 3.82 | ~3000 | 2012 | ||
| OGLE-2012-BLG-0026Lc | 0.68 | 4.63 | ~4000 | 2012 | ||
| MOA-2010-BLG477L b | 1.5 | 2±1 | 2012 | |||
| OGLE-2011-BLG-0251b | 0.53±0.21 | 2.72±0.75 or 1.5±0.5 | 2012/2013 | |||
| OGLE-2012-BLG-0406Lb | 2.73±0.43 | 3.45±0.26 | 2013 | |||
| OGLE-2012-BLG-0358Lb | 1.9±0.2 | 0.87 | 2013 | |||
| MOA-2008-BLG-379b | 5±2.5 | 4±1.6 | 2013 | |||
| MOA-2010-BLG-328Lb | 0.03 ± 0.0075 | 0.92 | 2013 | |||
| MOA-2008-BLG-379b | 5±2.5 | 4±1.6 | 2013 | |||
| MOA-2011-BLG-262 or MOA-2011-BLG-262 b | ~3.2 or 0.055 | Free-floating or ~1 | 2013 | |||
| MOA-2011-BLG-274 b | 0.8 | 40 | 2014 | |||
| OGLE-2014-BLG-0124Lb | 0.51±0.16 | 3.1±0.5 | ~2400 | 2014 | ||
| OGLE-2013-BLG-0102Lb | 13.6 | 0.8 | 2014 | |||
| OGLE-2008-BLG-092Lb | 0.137 | 2014 | ||||
| OGLE-2013-BLG-0341Lb | 0.00522291791209 | 0.702 | 2014 | |||
| OGL-2008-BLG-355Lb | 4.6 | 2014 | ||||
| MOA-2013-BLG-220Lb | 0.188780165497278 | 0.7 | 2014 | |||
| OGLE-2011-BLG-0265Lb | 1.0 ± 0.3 | 2 | 2014 |
See also
Notes
- The nature of the observed system is unclear. It is either a rogue planet with about 3.2 MJ masses and a 0.5 ME exomoon or a red dwarf with 18 ME planet.
References
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- Skowron, J.; Shin, I. -G.; Udalski, A.; Han, C.; Sumi, T.; Shvartzvald, Y.; Gould, A.; Dominis-Prester, D.; Street, R. A.; Jørgensen, U. G.; Bennett, D. P.; Bozza, V.; Szymański, M. K.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Poleski, R.; Kozłowski, S.; Pietrukowicz, P.; Ulaczyk, K.; Wyrzykowski, Ł.; Abe, F.; Bhattacharya, A.; Bond, I. A.; Botzler, C. S.; Freeman, M.; Fukui, A.; Fukunaga, D.; Itow, Y.; et al. (2014). "OGLE-2011-BLG-0265Lb: A Jovian Microlensing Planet Orbiting an M Dwarf". The Astrophysical Journal. 804 (1): 33. arXiv:1410.8252. Bibcode:2015ApJ...804...33S. doi:10.1088/0004-637X/804/1/33.
External links
- "Exoplanets detected by microlensing". Retrieved 2011-01-20.
{{cite web}}: Unknown parameter|encyclopedia=ignored (help) - "Exoplanets Data Explorer". Retrieved 2011-01-20.
