List of exoplanets detected by microlensing

This article needs to be updated. Please help update this article to reflect recent events or newly available information. (August 2014)

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This is a list of exoplanets detected by gravitational microlensing. The phenomenon results in the background star's light being warped around a foreground object, causing a distorted image. If the foreground object is a star with an orbiting planet, we would observe an abnormally bright image. By comparing the luminosity and light distortion of the background star to theoretical models, we can estimate the planet's mass and the distance from its star.

The least massive planet detected by microlensing is KMT-2020-BLG-0414Lb, which has a mass about 1.9 times the mass of earth, or OGLE-2013-BLG-0341LBb, which has a mass about 2 times the mass of earth.[1][2] The widest separation between a planet and a star is OGLE-2008-BLG-092Lb, which is ~18 AU; the shortest separation is MOA-2015-BLG-337Lb, which is 0.24 AU. There are 7 known multi-planetary systems detected by microlensing, all of which have two planets.[3]

## List

[edit]

Yellow rows denote the members of multi-planet systems. Green rows denote the members of multi-star systems.

Planet | Mass (MJ)  | Projected separation (AU)  | Period (d)  | Eccentricity | Inclination (°)  | Year of discovery

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OGLE-2003-BLG-235Lb | 2.6 | 5.1 |  |  |  | 2004[4][5]
OGLE-2005-BLG-071Lb | 3.5 | 3.6 | ~ 3600 |  |  | 2005[6][7]
OGLE-2005-BLG-390Lb | 0.017 | 2.1 | 3500 |  |  | 2005[8]
OGLE-2005-BLG-169Lb | 0.04 | 2.8 | 3300 |  |  | 2006[9]
OGLE-2006-BLG-109Lb | 0.727 | 2.3 | 1790 |  | 64 | 2008[10]
OGLE-2006-BLG-109Lc | 0.271 | 4.5 | 4931 | 0.15 | 64 | 2008[10]
MOA-2007-BLG-192Lb | 0.01 | 0.66 |  |  |  | 2008[11]
MOA-2007-BLG-400Lb | 0.9 | 0.85 |  |  |  | 2008[12]
MOA-2008-BLG-310Lb | 0.23 | 1.25 |  |  |  | 2009[13]
OGLE-2007-BLG-368Lb | 0.0694 | 3.3 |  |  |  | 2009[14]
MOA-2009-BLG-319Lb | 0.157 | 2.0 |  |  |  | 2010[15]
MOA-2009-BLG-387Lb | 2.6 | 1.8 | 1970 |  |  | 2011[16]
MOA-2009-BLG-266Lb | 0.0327 | 3.2 | 2780 |  |  | 2011[17]
MOA-2011-BLG-293Lb | 2.4 | 1.0 |  |  |  | 2012[18]
MOA-bin-1Lb | 3.7 | 8.3 |  |  |  | 2012[19]
MOA-2010-BLG-477Lb | 1.5 | 2±1 |  |  |  | 2012[20]
OGLE-2012-BLG-0026Lb | 0.11 | 3.82 | ~3000 |  |  | 2012[21]
OGLE-2012-BLG-0026Lc | 0.68 | 4.63 | ~4000 |  |  | 2012[21]
MOA-2010-BLG-073Lb | 11 | 1.21 |  |  |  | 2012[22]
OGLE-2011-BLG-0251Lb | 0.53±0.21 | 2.72±0.75 or 1.5±0.5 |  |  |  | 2013[23]
OGLE-2012-BLG-0406Lb | 2.73±0.43 | 3.45±0.26 |  |  |  | 2013[24]
OGLE-2012-BLG-0358Lb | 1.9±0.2 | 0.87 |  |  |  | 2013[25]
MOA-2010-BLG-328Lb | 0.03 ± 0.0075 | 0.92 |  |  |  | 2013[26]
MOA-2011-BLG-322Lb | 11.6 | 4.3 |  |  |  | 2013[27]
MOA-2008-BLG-379Lb | 5±2.5 | 4±1.6 |  |  |  | 2013[28]
MOA-2011-BLG-262Lb[note 1] | ~0.053 or ~0.0015 | ~0.95 or ~0.13 |  |  |  | 2013[29]
MOA-2013-BLG-220Lb | 2.74 | 3.03 |  |  |  | 2014[30][31]
OGLE-2008-BLG-355Lb | 4.6 | 1.7 |  |  |  | 2014[32]
OGLE-2013-BLG-0341LBb | 0.00522 | 0.702 |  |  |  | 2014[2]
OGLE-2013-BLG-0102Lb | 13.6 | 0.8 |  |  |  | 2014[33]
OGLE-2008-BLG-092Lb | 0.137 | ~18 |  |  |  | 2014[34]
OGLE-2014-BLG-0124Lb | 0.51±0.16 | 3.1±0.5 | ~2400 |  |  | 2014[35]
OGLE-2011-BLG-0265Lb | 1.0 ± 0.3 | 2 |  |  |  | 2014[36]
OGLE-2012-BLG-0563Lb | 0.39 | 0.74 |  |  |  | 2015[37]
OGLE-2015-BLG-0966Lb | 0.066 | 2.7 |  |  |  | 2015[38]
MOA-2010-BLG-353Lb | 0.27 | 1.72 |  |  |  | 2015[39]
MOA-2013-BLG-605Lb | 0.0102 | 0.93 |  |  |  | 2015[40]
MOA-2011-BLG-028Lb | 0.09 | 4.14 |  |  |  | 2015[41]
OGLE-2015-BLG-0954Lb | 3.4 | 1.6 |  |  |  | 2016[42]
OGLE-2014-BLG-1760Lb | 0.56 | 1.75 |  |  |  | 2016[43]
OGLE-2012-BLG-0724Lb | 0.47 | 1.6 |  |  |  | 2016[44]
OGLE-2015-BLG-0051Lb | 0.72 | 0.73 |  |  |  | 2016[45]
OGLE-2012-BLG-0950Lb | 0.079 | 2.2 |  |  |  | 2016[46]
OGLE-2007-BLG-349L(AB)b | 0.25 | 2.59 | 2557 |  |  | 2016[47]
OGLE-2014-BLG-0676Lb | 3.68 | 4.53 |  |  |  | 2016[48]
OGLE-2016-BLG-1195Lb | 0.0312 | 2.62 |  |  |  | 2017[49][50]
MOA-2012-BLG-505Lb | 0.0211 | 0.9 |  |  |  | 2017[51]
MOA-2012-BLG-006Lb | 8.4 | 10.2 |  |  |  | 2017[52]
MOA-2016-BLG-227Lb | 2.8 | 1.39 |  |  |  | 2017[53]
OGLE-2013-BLG-0132Lb | 0.29 | 3.6 |  |  |  | 2017[54]
OGLE-2013-BLG-1721Lb | 0.64 | 2.6 |  |  |  | 2017[54]
OGLE-2016-BLG-0263Lb | 4.1 | 5.4 |  |  |  | 2017[55]
OGLE-2016-BLG-0613L(AB)b | 4.18 | 6.4 |  |  |  | 2017[56]
OGLE-2016-BLG-1190Lb | 13.38 | 2.17 | 1220 | 0.42 | 41.2 | 2017[57]
UKIRT-2017-BLG-001Lb | 1.28 | 4.18 |  |  |  | 2018[58]
TCP J05074264+2447555b | 0.0629  | 0.940  |  |  |  | 2018[59][60][61]
OGLE-2017-BLG-1522Lb | 0.75  | 0.59  |  |  |  | 2018[62]
OGLE-2017-BLG-1434Lb  | 0.014±0.0016 | 1.18±0.1 |  |  |  | 2018[63]
OGLE-2017-BLG-1140Lb  | 1.59  | 1.02  |  |  |  | 2018[64]
OGLE-2017-BLG-0482Lb  | 0.028  | 1.8  |  |  |  | 2018[65]
OGLE-2017-BLG-0373Lb  | 0.401  | 2.424  |  |  |  | 2018[66]
OGLE-2017-BLG-0173Lb  | 0.01029  | 3.913  |  |  |  | 2018[67]
OGLE-2014-BLG-1722Lb  | 0.174  | 1.5  |  |  |  | 2018[68]
OGLE-2014-BLG-1722Lc  | 0.263  | 1.7  |  |  |  | 2018[68]
OGLE-2013-BLG-1761Lb  | 2.7  | 1.8  |  |  |  | 2018[69]
OGLE-2011-BLG-0173Lb  | 0.19  | 8  |  |  |  | 2018[70]
MOA-2016-BLG-319Lb  | 0.62  | 0.95  |  |  |  | 2018[71]
MOA-2015-BLG-337Lb  | 0.106  | 0.24  |  |  |  | 2018[72]
MOA-2011-BLG-291Lb  | 0.057  | 0.69  |  |  |  | 2018[73]
MOA-2010-BLG-117Lb  | 0.54  | 2.42  |  |  |  | 2018[74]
KMT-2017-BLG-0165Lb  | 0.11  | 3.45  |  |  |  | 2018[75]
KMT-2016-BLG-2142Lb  | 15.49  | 0.83  |  |  |  | 2018[76]
KMT-2016-BLG-1820Lb  | 4.57  | 1.08  |  |  |  | 2018[76]
KMT-2016-BLG-1397Lb  | 7.0  | 5.1  |  |  |  | 2018[77]
KMT-2016-BLG-0212Lb  | 18  | 2.2  |  |  |  | 2018[78]
OGLE-2018-BLG-1011Lb  | 1.8  | 1.8  |  |  |  | 2019[79]
OGLE-2018-BLG-1011Lc  | 2.8  | 0.8  |  |  |  | 2019[79]
OGLE-2018-BLG-0740Lb  | 4.8  | 5.0  | 5480  | 0  |  | 2019[80]
OGLE-2018-BLG-0596Lb  | 0.04383  | 0.97  |  |  |  | 2019[81]
OGLE-2016-BLG-1067Lb  | 0.43  | 1.70  |  |  |  | 2019[82]
OGLE-2015-BLG-1670Lb  | 0.0563  | 2.62  |  |  |  | 2019[83]
OGLE-2015-BLG-1649Lb  | 2.54  | 2.07  |  |  |  | 2019[84]
OGLE-2013-BLG-0911Lb  | 9.51  | 0.39  |  |  |  | 2019[85]
MOA-bin-29Lb | 0.6 | 0.48 |  |  |  | 2019[86]
KMT-2018-BLG-1990Lb  | 0.605  | 1.083  |  |  |  | 2019[87]
KMT-2017-BLG-1146Lb  | 0.71  | 1.6  |  |  |  | 2019[88]
KMT-2017-BLG-1038Lb  | 2.0  | 1.8  |  |  |  | 2019[88]
KMT-2016-BLG-1836Lb  | 2.2  | 3.5  |  |  |  | 2019[89]
KMT-2016-BLG-1107Lb  | 3.283  | 0.342  |  |  |  | 2019[90]
OGLE-2018-BLG-1700Lb  | 4.40  | 2.8  |  |  |  | 2020[91]
OGLE-2018-BLG-1269Lb  | 0.67  | 4.51  |  |  |  | 2020[92]
OGLE-2018-BLG-0677Lb  | 0.0125  | 0.63  |  |  |  | 2020[93]
OGLE-2018-BLG-0532Lb  | 0.01960  | 1.064  |  |  |  | 2020[94]
OGLE-2017-BLG-1375Lb  | 11.28  | 3.04  |  |  |  | 2020[95]
OGLE-2017-BLG-1049Lb  | 5.53  | 3.92  |  |  |  | 2020[96]
OGLE-2017-BLG-0604Lb  | 0.51  | 4.06  |  |  |  | 2020[95]
OGLE-2017-BLG-0406Lb  | 0.41  | 3.5  |  |  |  | 2020[97]
OGLE-2016-BLG-1227Lb  | 0.79  | 3.4  |  |  |  | 2020[98]
OGLE-2015-BLG-1771Lb  | 0.433  | 0.85  |  |  |  | 2020[99]
OGLE-2012-BLG-0838Lb  | 0.167  | 4.43  |  |  |  | 2020[100]
OGLE-2006-BLG-284LAb  | 0.453  | 2.17  |  |  |  | 2020[101]
KMT-2019-BLG-1953Lb  | 0.64  |  |  |  |  | 2020[102]
KMT-2019-BLG-1339Lb  | 1.25  | 2.15  |  |  |  | 2020[103]
KMT-2019-BLG-0842Lb  | 0.03234  | 3.31  |  |  |  | 2020[104]
KMT-2018-BLG-1292Lb  | 4.42  | 6.03  |  |  |  | 2020[105]
KMT-2018-BLG-0748Lb  | 0.19  | 0.62  |  |  |  | 2020[106]
KMT-2018-BLG-0029Lb  | 0.0239  | 4.27  |  |  |  | 2020[107]
KMT-2016-BLG-2397Lb  | 2.63  | 3.64  |  |  |  | 2020[95]
KMT-2016-BLG-2364Lb  | 3.93  | 2.63  |  |  |  | 2020[95]
OGLE-2019-BLG-1053Lb  | 0.00780  | 3.4  |  |  |  | 2021[108]
OGLE-2019-BLG-0960Lb  | 0.0079  | 1.90  |  |  |  | 2021[109]
OGLE-2019-BLG-0954Lb  | 14.2  | 2.65  |  |  |  | 2021[110]
OGLE-2019-BLG-0304Lb  | 0.510  | 1.23  |  |  |  | 2021[111]
OGLE-2019-BLG-0299Lb  | 6.220  | 2.80  |  |  |  | 2021[112]
OGLE-2017-BLG-1099Lb  | 3.02  | 2.73  |  |  |  | 2021[112]
OGLE-2018-BLG-1428Lb  | 0.77  | 3.30  |  |  |  | 2021[113]
OGLE-2018-BLG-1185Lb  | 0.0264  | 1.54  |  |  |  | 2021[114]
OGLE-2018-BLG-0962Lb  | 1.34  | 3.59  |  |  |  | 2021[115]
OGLE-2018-BLG-0567Lb  | 0.32  | 2.72  |  |  |  | 2021[115]
KMT-2017-BLG-2509Lb  | 2.09  | 2.14  |  |  |  | 2021[112]
KMT-2018-BLG-1976Lb  | 2.22  | 3.54  |  |  |  | 2021[110]
KMT-2018-BLG-1996Lb  | 1.09  | 4.27  |  |  |  | 2021[110]
KMT-2021-BLG-0322Lb  | 6.40  |  |  |  |  | 2021[116]
KMT-2020-BLG-0414Lb  | 0.00588  | 2.07  |  |  |  | 2021[117][1]
KMT-2020-BLG-0414Lc  | 27  | 22.3  |  |  |  | 2021[117][1]
KMT-2019-BLG-1715Lb  | 2.56  | 3.32  |  |  |  | 2021[118]
KMT-2019-BLG-0371Lb | 7.7 | 0.79 |  |  |  | 2021[119]
KMT-2018-BLG-1743Lb  | 0.245  | 1.449  |  |  |  | 2021[120]
KMT-2018-BLG-1025Lb  | 0.019064  | 1.305  |  |  |  | 2021[121]
KMT-2016-BLG-2605Lb  | 0.7710  | 0.681  |  |  |  | 2021[122]
OGLE-2019-BLG-1470L(AB)c  | 2.2  | 3.2  |  |  |  | 2022[123]
OGLE-2019-BLG-1492Lb  | 0.117  | 2.7  |  |  |  | 2022[124]
OGLE-2018-BLG-0977Lb  | 0.0201  | 2.0  |  |  |  | 2022[124]
OGLE-2018-BLG-0516Lb  | 0.0632  | 2.2  |  |  |  | 2022[124]
OGLE-2018-BLG-0506Lb  | 0.0513  | 3.0  |  |  |  | 2022[124]
OGLE-2019-BLG-0468Lb  | 3.43  | 3.29  |  |  |  | 2022[125]
OGLE-2019-BLG-0468Lc  | 10.22  | 2.77  |  |  |  | 2022[125]
OGLE-2019-BLG-0362Lb  | 3.26  | 2.18  |  |  |  | 2022[126]
OGLE-2018-BLG-1647Lb  | 0.970  | 1.36  |  |  |  | 2022[127]
OGLE-2018-BLG-1367Lb  | 0.950  | 1.21  |  |  |  | 2022[127]
OGLE-2018-BLG-1126Lb  | 0.056  | 3.23  |  |  |  | 2022[127]
OGLE-2018-BLG-1119Lb | 0.910  | 4.06  |  |  |  | 2022[128]
OGLE-2018-BLG-0298Lb  | 0.14  | 2.86  |  |  |  | 2022[128]
OGLE-2018-BLG-0383Lb  | 0.0201  | 1.8  |  |  |  | 2022[129]
OGLE-2017-BLG-1691Lb  | 0.046  | 2.41  |  |  |  | 2022[130]
OGLE-2018-BLG-0799Lb | 0.26  | 1.28  |  |  |  | 2022[131]
OGLE-2018-BLG-0932Lb  | 0.890  | 1.75  |  |  |  | 2022[127]
OGLE-2018-BLG-1212Lb  | 0.20  | 1.68  |  |  |  | 2022[127]
OGLE-2016-BLG-1093Lb  | 0.71  | 2.13  |  |  |  | 2022[132]
OGLE-2014-BLG-0319Lb  | 0.57  | 3.49  |  |  |  | 2022[133]
MOA-2020-BLG-135Lb  | 0.0356  | 1.11  |  |  |  | 2022[134]
MOA-2019-BLG-008Lb  | 18  |  |  |  |  | 2022[135]
KMT-2019-BLG-0253Lb  | 0.0488  | 1.1  |  |  |  | 2022[124]
KMT-2021-BLG-2294Lb  | 0.070  | 1.15  |  |  |  | 2022[136]
KMT-2021-BLG-1898Lb  | 0.730  | 1.9  |  |  |  | 2022[137]
KMT-2021-BLG-1689Lb  | 0.14  | 2.5  |  |  |  | 2022[138]
KMT-2021-BLG-0119Lb  | 5.52  | 2.92  |  |  |  | 2022[136]
KMT-2021-BLG-0192Lb  | 0.11  | 1.62  |  |  |  | 2022[136]
KMT-2021-BLG-0171Lb  | 0.0352  | 3.5  |  |  |  | 2022[138]
KMT-2021-BLG-1303Lb  | 0.38  | 2.89  |  |  |  | 2022[130]
KMT-2021-BLG-0320Lb  | 0.10  | 1.54  |  |  |  | 2022[130]
KMT-2021-BLG-1554Lb  | 0.12  | 0.72  |  |  |  | 2022[130]
KMT-2021-BLG-1391Lb  | 0.0143  | 2.29  |  |  |  | 2022[139]
KMT-2021-BLG-1372Lb  | 0.1928  | 2.37  |  |  |  | 2022[139]
KMT-2021-BLG-1253Lb  | 0.05994  | 1.52  |  |  |  | 2022[139]
KMT-2019-BLG-0953Lb  | 0.0289  | 3.1  |  |  |  | 2022[124]
KMT-2021-BLG-0748Lb  | 0.45  | 2.43  |  |  |  | 2022[139]
KMT-2021-BLG-1077Lb  | 0.22  | 1.26  |  |  |  | 2022[140]
KMT-2021-BLG-1077Lc  | 0.25  | 0.930  |  |  |  | 2022[140]
KMT-2021-BLG-0912Lb  | 0.00884  | 3.14  |  |  |  | 2022[141]
KMT-2021-BLG-0240Lb  | 0.21  | 2.8  |  |  |  | 2022[142]
KMT-2021-BLG-2974Lb  | 0.28  | 2.0  |  |  |  | 2022[143]
KMT-2019-BLG-1552Lb  | 4.05  | 2.6  |  |  |  | 2022[143]
KMT-2019-BLG-1042Lb  | 0.19  | 1.7  |  |  |  | 2022[143]
KMT-2018-BLG-1988Lb  | 0.0175  | 3.09  |  |  |  | 2022[144]
KMT-2019-BLG-0414Lb  | 4.57  | 1.16  |  |  |  | 2022[145]
KMT-2017-BLG-0673Lb  | 3.67  | 2.34  |  |  |  | 2022[145]
KMT-2018-BLG-0087Lb  | 0.23  | 0.870  |  |  |  | 2022[128]
KMT-2018-BLG-0030Lb  | 1.45  | 4.39  |  |  |  | 2022[128]
KMT-2018-BLG-0247Lb  | 2.11  | 2.46  |  |  |  | 2022[128]
KMT-2018-BLG-2602Lb  | 1.15  | 3.81  |  |  |  | 2022[128]
OGLE-2019-BLG-1180Lb  | 1.747  | 5.19  |  |  |  | 2023[146]
OGLE-2019-BLG-0679Lb  | 3.34  | 6.99  |  |  |  | 2023[147]
OGLE-2019-BLG-0249Lb  | 7.12  | 1.84  |  |  |  | 2023[147]
OGLE-2017-BLG-1806Lb  | 0.0166  | 1.75  |  |  |  | 2023[148]
MOA-2022-BLG-249Lb  | 0.0152  | 1.63  |  |  |  | 2023[149]
MOA-2020-BLG-208Lb  | 0.14  | 2.74  |  |  |  | 2023[150]
KMT-2022-BLG-1013Lb  | 0.31  | 1.38  |  |  |  | 2023[151]
KMT-2022-BLG-0440Lb  | 0.0485  | 1.9  |  |  |  | 2023[152]
KMT-2022-BLG-0371Lb  | 0.26  | 3.02  |  |  |  | 2023[151]
KMT-2021-BLG-2478Lb  | 0.900  | 1.85  |  |  |  | 2023[153]
KMT-2021-BLG-2010Lb  | 1.07  | 1.79  |  |  |  | 2023[154]
KMT-2021-BLG-1770Lb  | 21  | 0.900  |  |  |  | 2023[155]
KMT-2021-BLG-1547Lb  | 1.47  | 4.5  |  |  |  | 2023[156]
KMT-2021-BLG-1150Lb  | 0.880  | 4.5  |  |  |  | 2023[157]
KMT-2021-BLG-1105Lb  | 1.30  | 3.54  |  |  |  | 2023[153]
KMT-2021-BLG-0909Lb  | 1.26  | 1.75  |  |  |  | 2023[153]
KMT-2021-BLG-0712Lb  | 0.1202  | 2.22  |  |  |  | 2023[153]
KMT-2019-BLG-2783Lb  | 1.16  | 1.85  |  |  |  | 2023[147]
KMT-2019-BLG-1806Lb  | 0.0147  | 3.02  |  |  |  | 2023[148]
KMT-2019-BLG-1367Lb  | 0.0128  | 1.70  |  |  |  | 2023[148]
KMT-2019-BLG-1216Lb  | 0.0940  | 2.44  |  |  |  | 2023[147]
KMT-2019-BLG-0335Lb  | 21  | 1.64  |  |  |  | 2023[158]
KMT-2019-BLG-0298Lb  | 1.81  | 5.67  |  |  |  | 2023[147]
KMT-2019-BLG-0297Lb  | 19  | 0.960  |  |  |  | 2023[158]
KMT-2018-BLG-0885Lb  | 29  | 1.07  |  |  |  | 2023[158]
KMT-2017-BLG-1194Lb  | 0.0111  | 1.78  |  |  |  | 2023[148]
KMT-2017-BLG-1003Lb  | 0.01633  | 1.38  |  |  |  | 2023[148]
KMT-2017-BLG-0428Lb  | 0.0176  | 1.81  |  |  |  | 2023[148]
KMT-2016-BLG-1105Lb  | 0.00730  | 2.44  |  |  |  | 2023[148]
K2-2016-BLG-0005Lb | 1.10  | 4.16  | 4700  |  |  | 2023[159]
OGLE-2017-BLG-1275Lb  | 5.90  | 2.09  |  |  |  | 2024[160]
OGLE-2017-BLG-1237Lb  | 3.80  | 2.53  |  |  |  | 2024[160]
OGLE-2017-BLG-0640Lb  | 1.62  | 1.14  |  |  |  | 2024[160]

### Candidate rogue planets

[edit]

A number of candidate rogue planets have been detected by microlensing.

Planet  | Mass | Year of discovery

|
|

MOA-2011-BLG-274L | 0.8±0.3 MJ | 2014[161]
OGLE-2016-BLG-1540L | ~35 M🜨 | 2017[162]
OGLE-2012-BLG-1323L | ~2.3 M🜨 | 2018[163]
OGLE-2017-BLG-0560L | ~1.9 MJ | 2018[163]
OGLE-2019-BLG-0551L | ~7.7 M🜨 | 2020[164]
KMT-2019-BLG-2073L | ~59 M🜨 | 2020[165]
OGLE-2016-BLG-1928L | ~0.3 M🜨 | 2020[166]
KMT-2017-BLG-2820L | ~8.2 M🜨 | 2020[167]

### Unconfirmed detections

[edit]

Some microlensing events, such as MACHO-98-BLG-35 and PA-99-N2, suggest the possible presence of a planetary companion to the lensing star, but this is unconfirmed. Since microlensing relies on a one-time chance alignment, it is likely not possible to confirm these detections.

In some cases, a planetary interpretation for a microlensing event was proposed, but has been disproven. MACHO-1997-BLG-41 was initially interpreted as a binary star system orbited by a circumbinary planet, but a different model with two stars and no planet was later found to be a better fit to the data. Similarly, OGLE-2013-BLG-0723L was initially interpreted as a binary system of a star and a brown dwarf, with a low-mass planet orbiting the brown dwarf, but a model where the system consists of two low-mass stars with no planet was found to be a better fit to the data.[168]

## See also

[edit]

* Lists of exoplanets
* Method of exoplanet detection using microlensing

## Notes

[edit]

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 ME exomoon or a red dwarf with 18 ME planet.

## References

[edit]

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155. ^ Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D.; Gould, Andrew; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok (2023-10-01). "Brown dwarf companions in binaries detected in the 2021 season high-cadence microlensing surveys". Astronomy and Astrophysics. 678: A190. arXiv:2307.04921. Bibcode:2023A&A...678A.190H. doi:10.1051/0004-6361/202347014. ISSN 0004-6361.
156. ^ Han, Cheongho; Zang, Weicheng; Jung, Youn Kil; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D.; Gould, Andrew; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; Yee, Jennifer C.; Cha, Sang-Mok; Kim, Doeon (2023-10-01). "KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity". Astronomy and Astrophysics. 678: A101. arXiv:2309.01280. Bibcode:2023A&A...678A.101H. doi:10.1051/0004-6361/202347366. ISSN 0004-6361.
157. ^ Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Chung, Sun-Ju; Albrow, Michael D.; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Doeon (2023-07-01). "KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal". Astronomy and Astrophysics. 675: A36. arXiv:2305.15628. Bibcode:2023A&A...675A..36H. doi:10.1051/0004-6361/202346596. ISSN 0004-6361.
158. ^ a b c Han, Cheongho; Kil Jung, Youn; Kim, Doeon; Gould, Andrew; Bozza, Valerio; Bond, Ian A.; Chung, Sun-Ju; Albrow, Michael D.; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; Zang, Weicheng; Cha, Sang-Mok (2023-07-01). "Probable brown dwarf companions detected in binary microlensing events during the 2018-2020 seasons of the KMTNet survey". Astronomy and Astrophysics. 675: A71. arXiv:2305.06605. Bibcode:2023A&A...675A..71H. doi:10.1051/0004-6361/202245455. ISSN 0004-6361.
159. ^ Specht, D.; Poleski, R.; Penny, M. T.; Kerins, E.; McDonald, I.; Lee, Chung-Uk; Udalski, A.; Bond, I. A.; Shvartzvald, Y.; Zang, Weicheng; Street, R. A.; Hogg, D. W.; Gaudi, B. S.; Barclay, T.; Barentsen, G. (2023-04-01). "Kepler K2 Campaign 9 - II. First space-based discovery of an exoplanet using microlensing". Monthly Notices of the Royal Astronomical Society. 520 (4): 6350–6366\. arXiv:2203.16959. Bibcode:2023MNRAS.520.6350S. doi:10.1093/mnras/stad212. ISSN 0035-8711.6350-6366&rft.date=2023-04-01&rft_id=info:arxiv/2203.16959&rft.issn=0035-8711&rft_id=info:doi/10.1093/mnras/stad212&rft_id=info:bibcode/2023MNRAS.520.6350S&rft.aulast=Specht&rft.aufirst=D.&rft.au=Poleski,+R.&rft.au=Penny,+M.+T.&rft.au=Kerins,+E.&rft.au=McDonald,+I.&rft.au=Lee,+Chung-Uk&rft.au=Udalski,+A.&rft.au=Bond,+I.+A.&rft.au=Shvartzvald,+Y.&rft.au=Zang,+Weicheng&rft.au=Street,+R.+A.&rft.au=Hogg,+D.+W.&rft.au=Gaudi,+B.+S.&rft.au=Barclay,+T.&rft.au=Barentsen,+G.&rft_id=https://doi.org/10.1093%2Fmnras%2Fstad212&rfr_id=info:sid/en.wikipedia.org:List+of+exoplanets+detected+by+microlensing" class="Z3988">
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161. ^ 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.
162. ^ Mróz, Przemek; et al. (2018). "A Neptune-mass Free-floating Planet Candidate Discovered by Microlensing Surveys". The Astronomical Journal. 155 (3): 121. arXiv:1712.01042. Bibcode:2018AJ....155..121M. doi:10.3847/1538-3881/aaaae9. S2CID 118894684.
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## External links

[edit]

* "Exoplanets detected by microlensing". Extrasolar Planets Encyclopaedia. 1995. Retrieved 2011-01-20.
* "Exoplanets Data Explorer". Retrieved 2011-01-20.

* v
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Exoplanets

* Planet
* Definition
* IAU
* Planetary science

Main topics|

* Exoplanet
* Exoplanet orbital and physical parameters
* Methods of detecting exoplanets
* Planetary system
* Planet-hosting stars

Sizes
and
types|

| Terrestrial|

* Carbon planet
* Coreless planet
* Desert planet
* Dwarf planet
* Hycean planet
* Ice planet
* Iron planet (Super-Mercury)
* Lava planet
* Ocean world
* Mega-Earth
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|

Gaseous|

* Eccentric Jupiter
* Mini-Neptune (Gas dwarf)
* Helium planet
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* Hot Neptune
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* Super-Jupiter
* Super-Neptune
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* Ultra-hot Neptune

Other types|

* Blanet
* Brown dwarf
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* Circumtriple planet
* Disrupted planet
* Double planet
* Ecumenopolis
* Eyeball planet
* Giant planet
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Formation
and
evolution|

* Accretion
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* Cosmic dust
* Debris disk
* Detached object
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Systems|

* Exocomet
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* Tidally detached
* Rogue planet
* Orbits
* Retrograde
* Trojan
* Mean-motion resonances
* Titius–Bode law

Host stars|

* A
* B
* Binary star
* Brown dwarfs
* F/Yellow-white dwarfs
* G/Yellow dwarfs
* Herbig Ae/Be
* K/Orange dwarfs
* M/Red dwarfs
* Pulsar
* Red giant
* Subdwarf B
* Subgiant
* T Tauri
* White dwarfs
* Yellow giants

Detection|

* Astrometry
* Direct imaging
* list
* Microlensing
* list
* Polarimetry
* Timing
* list
* Radial velocity
* list
* Transit method
* list
* Transit-timing variation

Habitability|

* Astrobiology
* Astrooceanography
* Circumstellar habitable zone
* Earth analog
* Extraterrestrial liquid water
* Galactic habitable zone
* Habitability of binary star systems
* Habitability of F-type main-sequence star systems
* Habitability of K-type main-sequence star systems
* Habitability of natural satellites
* Habitability of neutron star systems
* Habitability of red dwarf systems
* Habitability of yellow dwarf systems
* Habitable zone for complex life
* List of potentially habitable exoplanets
* Tholin
* Superhabitable planet

Catalogues|

* Nearby Habitable Systems
* Exoplanet Data Explorer
* Extrasolar Planets Encyclopaedia
* NASA Exoplanet Archive
* NASA Star and Exoplanet Database
* Open Exoplanet Catalogue

Lists|

* Exoplanetary systems
* Host stars
* Multiplanetary systems
* Stars with proto-planetary discs

* Exoplanets
* Discoveries
* Extremes
* Firsts
* Nearest
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* Terrestrial candidates
* Kepler
* 1–500
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* 1501–2000
* K2
* Potentially habitable
* Proper names

* Discovered exoplanets by year
* before 2000
* 2000–2009
* 2010
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* 2012
* 2013
* 2014
* 2015
* 2016
* 2017
* 2018
* 2019
* 2020
* 2021
* 2022
* 2023
* 2024
* 2025

Other|

* Carl Sagan Institute
* Exoplanet naming convention
* Exoplanet phase curves
* Exoplanetary Circumstellar Environments and Disk Explorer
* Extragalactic planet
* Extrasolar planets in fiction
* Geodynamics of terrestrial exoplanets
* Neptunian desert
* Nexus for Exoplanet System Science
* Planets in globular clusters
* Small planet radius gap
* Sudarsky's gas giant classification

* Discoveries of exoplanets
* Search projects

*[v]: View this template
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