List of exoplanets detected by microlensing

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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 M. 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 [1] 0.01 0.66 2008
MOA-2007-BLG-400Lb [2] 0.9 0.85 2008
MOA-2011-BLG-293Lb 2.4 1.0 2012
MOA-2008-BLG-310Lb [3] 0.23 1.25 2009
MOA-2009-BLG-387Lb [4] 2.6 1.8 1970 2011
MOA-2009-BLG-319b [5] 0.157 2.0 2010
OGLE-2005-BLG-390Lb [6] 0.017 2.1 3500 2005
OGLE-2006-BLG-109Lb [7] 0.727 2.3 1790 64 2008
OGLE-2005-BLG-169Lb [8] 0.04 2.8 3300 2005
MOA-2009-BLG-266Lb [9] 0.0327 3.2 2780 2010
OGLE-2007-BLG-368Lb [10] 0.0694 3.3 2008
OGLE-2005-BLG-071Lb [11] 3.5 3.6 ~ 3600 2005
OGLE-2006-BLG-109Lc [7] 0.271 4.5 4931 0.15 64 2008
OGLE-2003-BLG-235Lb [12] 2.6 5.1 2004
MOA-bin-1 b 3.7 8.3 2012
OGLE-2012-BLG-0026Lb [13] 0.11 3.82 ~3000 2012
OGLE-2012-BLG-0026Lc [13] 0.68 4.63 ~4000 2012
MOA-2010-BLG477L b[14] 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 [15] 2013
MOA-2008-BLG-379b 5±2.5 4±1.6 2013
MOA-2011-BLG-262 or MOA-2011-BLG-262 b[16] ~3.2 or 0.055 [note 1] Free-floating or ~1 2013
MOA-2011-BLG-274 b[17] 0.8 40 2014
OGLE-2014-BLG-0124Lb[18] 0.51±0.16 3.1±0.5 ~2400 2014
OGLE-2013-BLG-0102Lb[19] 13.6 0.8 2014
OGLE-2008-BLG-092Lb[20] 0.137 2014
OGLE-2013-BLG-0341Lb[21] 0.00522291791209 0.702 2014
OGL-2008-BLG-355Lb[22] 4.6 2014
MOA-2013-BLG-220Lb[23] 0.188780165497278 0.7 2014
OGLE-2011-BLG-0265Lb[24] 1.0 ± 0.3 2 2014

See also


  1. ^ The nature of the observed system is unclear. It is either a rogue planet with about 3.2 MJ masses and a 0.5 M exomoon or a red dwarf with 18 M planet.


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  22. ^ 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.
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