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This is the list of 20 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 4 members of multi-planet systems.
List
Yellow rows denote the members of multi-planet systems.
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/MOA-2003-BLG-53Lb | 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-BLG-477L 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-262L or MOA-2011-BLG-262L 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 | |||
MOA-bin-29 b | 0.6 | 0.48 | 2019 | |||
KMT-2019-BLG-2073 | Free-floating | N/A | N/A | N/A | 2020 | |
OGLE-2019-BLG-0551 | 0.0242 | Free-floating | N/A | N/A | N/A | 2020 |
KMT-2019-BLG-0371b | 7.7 | 0.79 | 2021 |
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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- MOA 2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light
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- Bennett, D. P.; Batista, V.; Bond, I. A.; Bennett, C. S.; Suzuki, D.; Beaulieu, J.-P.; Udalski, A.; Donatowicz, J.; Abe, F.; Botzler, C. S.; Freeman, M.; Fukunaga, D.; Fukui, A.; Itow, Y.; Koshimoto, N.; Ling, C. H.; Masuda, K.; Matsubara, Y.; Muraki, Y.; Namba, S.; Ohnishi, K.; Rattenbury, N. J.; Saito, To; Sullivan, D. J.; Sumi, T.; Sweatman, W. L.; Tristram, P. J.; Tsurumi, N.; Wada, K.; et al. (7 April 2014). "A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge". The Astrophysical Journal. 785 (2): 155. arXiv:1312.3951. Bibcode:2014ApJ...785..155B. doi:10.1088/0004-637X/785/2/155. S2CID 118327512.
- Freeman, M.; Philpott, L. C.; Abe, F.; Albrow, M. D.; Bennett, D. P.; Bond, I. A.; Botzler, C. S.; Bray, J. C.; Cherrie, J. M.; Christie, G. W.; Dionnet, Z.; Gould, A.; Han, C.; Heyrovsky, D.; McCormick, J. M.; Moorhouse, D. M.; Muraki, Y.; Natusch, T.; Rattenbury, N. J.; Skowron, J.; Sumi, T.; Suzuki, D.; Tan, T. -G.; Tristram, P. J.; Yock, P. C. M. (2014). "Can the masses of isolated planetary-mass gravitational lenses be measured by terrestrial parallax?". The Astrophysical Journal. 799 (2): 181. arXiv:1412.1546. Bibcode:2015ApJ...799..181F. doi:10.1088/0004-637X/799/2/181. S2CID 118415208.
- Udalski, A.; Yee, J. C.; Gould, A.; Carey, S.; Zhu, W.; Skowron, J.; Kozłowski, S.; Poleski, R.; Pietrukowicz, P.; Pietrzyński, G.; Szymański, M. K.; Mróz, P.; Soszyński, I.; Ulaczyk, K.; Wyrzykowski, Ł.; Han, C.; Calchi Novati, S.; Pogge, R. W. (2014). "Spitzer as Microlens Parallax Satellite: Mass Measurement for the OGLE-2014-BLG-0124L Planet and its Host Star". The Astrophysical Journal. 799 (2): 237. arXiv:1410.4219. Bibcode:2015ApJ...799..237U. doi:10.1088/0004-637X/799/2/237. S2CID 30683835.
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- Poleski, Radosław; et al. (13 October 2014). "Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet". The Astrophysical Journal. 795 (1): 42. arXiv:1408.6223. Bibcode:2014ApJ...795...42P. doi:10.1088/0004-637X/795/1/42. S2CID 118678130.
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- Koshimoto, N.; et al. (20 June 2014). "OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND A LATE-TYPE STAR". The Astrophysical Journal. 788 (2): 128. arXiv:1403.7005. Bibcode:2014ApJ...788..128K. doi:10.1088/0004-637X/788/2/128. S2CID 119194503.
- Yee, J. C.; Han, C.; Gould, A.; Skowron, J.; Bond, I. A.; Udalski, A.; Hundertmark, M.; Monard, L. A. G.; Porritt, I.; Nelson, P.; Bozza, V.; Albrow, M. D.; Choi, J. -Y.; Christie, G. W.; DePoy, D. L.; Gaudi, B. S.; Hwang, K. -H.; Jung, Y. K.; Lee, C. -U.; McCormick, J.; Natusch, T.; Ngan, H.; Park, H.; Pogge, R. W.; Shin, I. -G.; Tan, T. -G.; Abe, F.; Bennett, D. P.; Botzler, C. S.; et al. (2014). "MOA-2013-BLG-220Lb: Massive Planetary Companion to Galactic-Disk Host". The Astrophysical Journal. 790 (1): 14. arXiv:1403.2134. Bibcode:2014ApJ...790...14Y. doi:10.1088/0004-637X/790/1/14. S2CID 118711190.
- 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. S2CID 45737293.
- ^ "Eyes on Exoplanets-MOA-bin-29 b".
External links
- "Exoplanets detected by microlensing". The Extrasolar Planets Encyclopaedia. Retrieved 2011-01-20.
- "Exoplanets Data Explorer". Retrieved 2011-01-20.