List of exoplanets detected by microlensing

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 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 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 [1]0.010.662008
MOA-2007-BLG-400Lb [2]0.90.852008
MOA-2011-BLG-293Lb2.41.02012
MOA-2008-BLG-310Lb [3]0.231.252009
MOA-2009-BLG-387Lb [4]2.61.819702011
MOA-2009-BLG-319b [5]0.1572.02010
OGLE-2005-BLG-390Lb [6]0.0172.135002005
OGLE-2006-BLG-109Lb [7]0.7272.31790642008
OGLE-2005-BLG-169Lb [8]0.042.833002005
MOA-2009-BLG-266Lb [9]0.03273.227802010
OGLE-2007-BLG-368Lb [10]0.06943.32008
OGLE-2005-BLG-071Lb [11]3.53.6~ 36002005
OGLE-2006-BLG-109Lc [7]0.2714.549310.15642008
OGLE-2003-BLG-235Lb/MOA-2003-BLG-53Lb [12]2.65.12004
MOA-bin-1 b3.78.32012
OGLE-2012-BLG-0026Lb [13]0.113.82~30002012
OGLE-2012-BLG-0026Lc [13]0.684.63~40002012
MOA-2010-BLG-477L b[14]1.52±12012
OGLE-2011-BLG-0251b0.53±0.212.72±0.75 or 1.5±0.52012/2013
OGLE-2012-BLG-0406Lb2.73±0.433.45±0.262013
OGLE-2012-BLG-0358Lb1.9±0.20.872013
MOA-2008-BLG-379b5±2.54±1.62013
MOA-2010-BLG-328Lb0.03 ± 0.00750.92 [15]2013
MOA-2008-BLG-379b5±2.54±1.62013
MOA-2011-BLG-262L or MOA-2011-BLG-262L b[16]~3.2 or 0.055 [note 1]Free-floating or ~12013
MOA-2011-BLG-274 b[17]0.8402014
OGLE-2014-BLG-0124Lb[18]0.51±0.163.1±0.5~24002014
OGLE-2013-BLG-0102Lb[19]13.60.82014
OGLE-2008-BLG-092Lb[20]0.1372014
OGLE-2013-BLG-0341Lb[21]0.005222917912090.7022014
OGL-2008-BLG-355Lb[22]4.62014
MOA-2013-BLG-220Lb[23]0.1887801654972780.72014
OGLE-2011-BLG-0265Lb[24]1.0 ± 0.322014
MOA-bin-29 b0.6[25] 0.48[26] 2019[27]
KMT-2019-BLG-2073Free-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

  • List of exoplanets

Notes

  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.

References

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  25. "Eyes on Exoplanets-MOA-bin-29 b".
  26. "Eyes on Exoplanets-MOA-bin-29 b".
  27. "Eyes on Exoplanets-MOA-bin-29 b".
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