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List of exoplanets discovered in 2024

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This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
2MASS J05581644-4501559 b 6–12 1043 imaging 94.5 0.259±0.02[1] 3218±158[1] [2]
BD-10 47 b 0.0133±0.005 0.1529±0.0007 13.476 0.0943±0.0016 493±12 transit 65.89 0.616±0.032 4026±14 Also known as TOI-260 b[3]
BD-14 3065 b 12.11+0.95
−0.91 		1.926±0.094 4.3 0.0646±0.0026 1957±28 transit 1847.4[4][a] 1.4±0.06 6985±90 Located in a triple star system. It orbits the primary component of the system (BD-14 3065 A), a subgiant star. Also known as TOI-4987 b[5]
CI Tauri c 3.6±0.3 25.2±1.8 0.17 radial vel. 522.6±1.3 0.9±0.02 4250±50 Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.[6][7]
Gaia20eae b 6 0.062 disc thermal instability 9226+3130
−2021[8] 		1.15 4330±300[8] First object detected by this method[9]
Gliese 12 b 0.002769+0.00123
−0.0008 		0.0892±0.0089[b] 12.7 0.066±0.002 315±5 transit 39.65 0.241±0.006 3253±55 [10]
Gliese 238 b 0.05049±0.0012 1.74 0.02123+0.00016
−0.00017 		758+16
−15 		transit 49.6 0.419±0.01 3485±140 Mars-sized exoplanet, one of the smallest exoplanets currently known[11]
Gliese 341 b 0.00227±0.00044 0.0821±0.045 7.577 540 transit 33.9 0.506 3745 Also known as TOI-741 b[12]
Gliese 900 b 10.5 500,000,000[13] 12,000 imaging 68[13] 1.08 (combined) 3976[14] Located in a three-star system.[15] It has the longest orbital time of any exoplanet so far at 1.4 million years.[16]
Gliese 1289 b 0.01655+0.002958
−0.003052 		111.74 0.27±0.01 150 radial vel. 28.88 0.21±0.02 3296±30 Another planet candidate around Gliese 3378 (a similar red dwarf) was reported.[17]
HD 21520 b 0.02486+0.01007
−0.00944 		0.2409±0.008 25.13 0.1726±0.0071 637+13
−12 		transit 258 1.09±0.07 5871±62 [18]
HD 48948 b 0.0154±0.000661 7.34013±0.00040 0.0652±0.0005 957±11 radial vel. 54.915±0.0228 0.686+0.020
−0.013 		4593±60 [19]
HD 48948 c 0.0229±0.00220 37.920+0.026
−0.024 		0.1951±0.0016 553±6 radial vel. [19]
HD 48948 d 0.0333±0.00315 150.95+0.45
−0.41 		0.4894±0.0042 349±4 radial vel. [19]
HD 63433 d 0.09573±0.0141 4.21 0.0503±0.0027 1040±40 transit 71.7 0.99±0.03 5688±28 Hot Earth-sized exoplanet[20]
HD 73344 b 0.00939+0.00787
−0.00599 		0.2573+0.0073
−0.0064 		15.6 0.131 911±7 transit 114.7 1.2±0.02 6220±64 The temperature can be as high as 1,066 K if the planet is tidally locked. Another planet in the system (HD 77344 c) is suspected. It has a minimum mass of 116.3 ME and an orbital period of 66 days.[21]
HD 77946 b 0.02637±0.00415 0.24133+0.00767
−0.0071 		6.527 0.072±0.0012 1248+40
−38 		transit 322.7±1 1.17±0.06 6046.0±50.0 Also known as TOI-1778 b[22]
HD 104067 c 0.0415 13.8992+0.0047
−0.0037 		0.1058±0.0013 radial vel. 66.34±0.03 0.82±0.03 4952±100 [23]
HD 134606 e 0.00726+0.00113
−0.0011 		4.32 0.0527±0.0012 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[24]
HD 134606 f 0.01737+0.00232
−0.00229 		26.915 0.1784±0.004 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[24]
HD 148193 Ab 0.0894±0.0135 0.7476±0.017 20.38 0.1577 transit 626±3 1.261±0.183 6351±119 The host star is orbited by two red dwarfs 157 and 1950 AU away.[25]
HD 278878 b 0.6963±0.0242 0.9225±0.0571 8.71 0.08258 transit 520.8±4.9 0.989±0.126 5597±147 [26]
HIP 39017 b 23.6+9.1
−7.4 		0.87 30681+18627.8
−9496.5 		22.1+8.0
−4.9 		imaging 214.9±0.3 1.52+0.28
−0.26 		7201+142
−112[27] 		May be a brown dwarf. Estimates of the mass vary from 13.8 MJ to 30+31
−12 MJ.[28]
HS Piscium b 1.44+0.56
−0.44 		3.986 0.0435±0.0017 radial vel. 122.79+0.12
−0.14 		0.69±0.07 4203±116 [29]
KMT-2016-BLG-2321Lb 3.58±1.22 3.58±0.81 microlensing 11,670±3980 0.73±0.28 [30]
KMT-2020-BLG-0157Lb 10.71+6.17
−5.61 		11.54+1.61
−2.25 		microlensing 21,744+3032
−4238 		0.58+0.33
−0.30 		[31]
KMT-2022-BLG-0732Lb 1.12±0.65 4.11+0.74
−1.14 		microlensing 21,712+3879
−6000 		0.54±0.31 [31]
KMT-2022-BLG-1787Lb 6.64+4.98
−3.64 		6.3+0.75
−1.08 		microlensing 24,613+2901
−4038 		0.42+0.32
−0.23 		[31]
KMT-2022-BLG-1852Lb 4.98+5.42
−2.94 		5.03+0.72
−0.92 		microlensing 20,440+2934
−3749 		0.32+0.34
−0.19 		[31]
KMT-2023-BLG-0416Lb 6.15+3.03
−3.2 		3.73+0.56
−0.8 		microlensing 20,640+3100
−4400 		0.61+0.3
−0.32 		The mass of the planet can be as low as 0.042+0.021
−0.022 MJ.[32]
KMT-2023-BLG-0469Lb 0.124+0.092
−0.067 		2.37±0.9 microlensing 23,050+3260
−3910 		0.47±0.36 [33]
KMT-2023-BLG-0735Lb 0.12±0.07 2.75±1 microlensing 20,830+3910
−3260 		0.61±0.34 [33]
KMT-2023-BLG-1454Lb 0.63+0.71
−0.34 		1.18+0.17
−0.18 		microlensing 23,540+3460
−3590 		0.17+0.19
−0.09 		Estimates of the planet's mass varies between 0.3+0.34
−0.16 MJ and 0.77+0.87
−0.42 MJ[32]
KMT-2023-BLG-1642Lb 1.08+1.53
−0.58 		1.41+0.22
−0.27 		microlensing 22,750+3550
−4370 		0.17+0.24
−0.09 		[32]
KMT-2023-BLG-1866Lb 0.00828+0.00132
−0.00214 		2.63+0.37
−0.34 		microlensing 20,240+2840
−1100 		0.51+0.08
−0.13 		Super-Earth planet detected by microlensing.[34]
KMT-2023-BLG-2669 0.02517 microlensing Candidate rogue planet. Might have a mass ranging from sub-Neptune to Saturn-mass, depending on its distance.[35]
LHS 1678 d 0.00289+0.00208
−0.00107 		0.08752±0.0062 4.965 0.04+0.0018
−0.0017 		transit 65 0.345±0.014 3490±50 [36]
M62H b 2.83 <0.683 [c][d] 0.133 0.004908 timing 21,500[37] 1.4 Pulsar planet located in the globular cluster Messier 62.[38] Second shortest orbit of any exoplanet after PSR J1719-1438 b.[39]
MOA-2016-BLG-526Lb 6.93±0.75 2.07±0.35 microlensing 22,490 0.4 [30]
MOA-2022-BLG-563Lb 0.4+0.31
−0.25 		2.25±0.25 microlensing 21,290+3650
−5220 		0.48+0.36
−0.3 		[33]
OGLE-2016-BLG-1598Lb 5.91±1.74 2.5±0.88 microlensing 19,270±5670 0.55±0.32 [30]
NGTS-26 b 0.29+0.07
−0.06 		1.33+0.06
−0.05 		4.52 0.0490+0.0038
−0.0032 		1331+85
−72 		transit 3610±100 0.96+0.04
−0.03 		5550±100 Highly inflated planet (density = 0.153 g/cm3)[40]
NGTS-27 b 0.593+0.095
−0.072 		1.396+0.038
−0.035 		3.37 0.0446+0.0026
−0.0036 		1783+104
−88 		transit 3185±55 1.07±0.06 5700±80 [40]
NGTS-29 b 0.393 0.857 69.33 0.347 414 transit 487±1 1.034±0.032 5730±80 [41]
NGTS-30 b 0.96 0.93 98.3 0.408 390 transit 762.5 0.94 5455 Also known as TOI-4862 b[42]
OGLE-2016-BLG-1800Lb 2.59±1.46 1.88±0.51 microlensing 21,100±3360 0.41±0.22 [30]
OGLE-2017-BLG-0640Lb 1.62+1.64
−0.94 		1.14±0.38 microlensing 21,600+3550
−4730 		0.32+0.32
−0.18 		[43]
OGLE-2017-BLG-1237Lb 3.8+2.49
−1.99 		2.53+0.5
−0.64 		microlensing 19,660+3060
−4990 		0.46+0.3
−0.24 		[43]
OGLE-2017-BLG-1275Lb 5.9±2.2 1.19±0.36 microlensing 25,070±2930 0.63±0.23 Another solution suggests a larger semi-major axis, of 2.09±0.63 AU.[43]
OGLE-2023-BLG-0836Lb 4.36+2.35
−2.2 		3.7+1
−1.2 		microlensing 16,690+4430
−5250 		[e] The planet is located in a binary star system, and is likely to be orbiting both stars in the system.[44]
S1429 b 1.8±0.2 77.51±0.2 0.384±0.4 683±9 radial vel. 2836±26 1.26±0.04 6000±40 Located in the open cluster Messier 67.[45]
SPECULOOS-3 b 0.08716 0.719 0.00733 553 transit 57.9 0.1 2800 Ultra-short period planet[46]
Teegarden's Star d 0.00258±0.00053 26.13 0.0791 ±0.0027 159±3 radial vel. 12.5 0.097±0.01 3034±45 Orbits beyond the habitable zone of its star. Another planet in the system is suspected.[47]
TIC 4672985 b 12.74±1.01 1.026+0.065
−0.067 		69.05 0.33±0.019 517.2+11.3
−11.2 		transit 823.4[48][a] 1.01±0.03 5757+72
−65 		[49]
TIC 139270665 b 0.463 0.645 23.624 0.163 700 transit 618 1.035+0.052
−0.062 		5844+84
−82 		[50][51]
TIC 139270665 c 4.89+0.66
−0.37 		1010+780
−220 		2+0.93
−0.31 		200+18
−35 		radial vel. [51]
TIC 393818343 b 4.34±0.15 1.087+0.023
−0.021 		16.25 0.129±0.002 805.5+9.6
−9.4 		transit 306.3±1.1 1.082+0.055
−0.056 		5756+57
−66 		Highly eccentric orbit (e=0.6058)[52]
Also known as TOI-6883 b[53]
TOI-128 b 0.198 4.94 0.054 1345 transit 0.85 6086 [54]
TOI-201 b 0.42+0.05
−0.03 		1.008+0.012
−0.015 		52.978 0.3+0.02
−0.03 		759+37
−26 		transit 373 1.316±0.027 6394±75 [55]
TOI-238 c 0.0211±0.0035 0.1945±0.0161 8.466 0.0749±0.0013 696±15 transit 261.328±0.312 0.79±0.022 5059±89 [56]
TOI-261 b 0.271 3.36 0.035 1722 transit 0.50 5890 [54]
TOI-286 b 0.01425±0.00245 0.1267±0.0089 4.512 0.0503±0.001 979±31 transit 193 0.832±0.049 5152±12 There are three available models to explain the disagreement between the radial velocity and transit measurements.[f][3]
TOI-286 c 0.01171±0.00698 0.1677±0.0107 39.36 0.213±0.004 475±15 transit 193 0.832±0.049 5152±12 [3]
TOI-329 b 0.1271 5.71 0.064 transit 927.1 0.98 5560 Radius of the host star is significantly larger compared to mass (1.61 R☉)[57]
TOI-406 b 0.175 13.18 0.086 344 transit 0.48 3349 [54]
TOI-480 b 0.0654 6.866 transit 177.8 1.2 6,212 [58]
TOI-603 b 0.1495±0.0431 0.7075±0.018 16.18 0.1281 transit 671.3±5.15 1.072±0.136 5901±130 [59]
TOI-654 b 0.211 1.53 0.021 749 transit 0.53 3433 [54]
TOI-663 b 0.0140±0.00204 0.203±0.00892 2.5989020+0.0000032
−0.0000030 		0.0295±0.0011 674±30 transit 209.490±0.587 0.514±0.012 3681±70 [60]
TOI-663 c 0.0115±0.00305 0.202±0.00892 4.6955507+0.0000095
−0.0000094 		0.0437±0.0016 553±24 transit
TOI-663 d <0.0164 0.171±0.0116 7.1027268+0.0000297
−0.0000279 		0.0576+0.0021
−0.0022 		482±21 transit
TOI-782 b <0.06 0.244±0.008 8.024 0.0578±0.0018 398±6–435±6[g] transit 170.2±0.2 0.397±0.01 3370+29
−32 		[61]
TOI-815 b 0.0239±0.0047 0.2622±0.0044 11.197 0.0903+0.0018
−0.0019 		686+13
−14 		transit 193.76±0.15 0.776±0.036 4869±77 The host star is part of a binary star system with a red dwarf companion[62]
TOI-815 c 0.0739±0.00755 0.2337+0.0089
−0.008 		34.976 0.193±0.004 469±9 transit
TOI-880 b 0.248 2.57 0.034 1163 transit 0.81 4935 [54]
TOI-907 b 0.858 4.58 0.055 1847 transit 1.07 6272 [54]
TOI-1135 b 0.062+0.033
−0.031 		0.805±0.02 5.13±0.27 0.082±0.003 1198.9±21.3 transit 371.4±0.5 1.125±0.032 6122±25 [63]
TOI-1173 Ab 0.08213±0.00598 0.723±0.015 7.064 0.0702±0.0012 863.9±9.8 transit 430.85[64][a] 0.911+0.028
−0.03 		5350±340 Low-density planet located in a wide binary system.[65]
TOI-1199 b 0.239±0.02 0.938±0.025 3.671 0.04988±0.0009 1486±20 transit 805±2.6 1.23±0.07 5710±40 [66]
TOI-1224 b 0.1877+0.0084
−0.0081 		4.178 0.0355+0.0017
−0.0034 		541+26
−14 		transit 121.5 0.4±0.01 3326±66 Located in the MELANGE-5 association, which is 200 Myr old. The host star may be binary.[67]
TOI-1224 c 0.2573±0.0087 17.945 transit
TOI-1273 b 0.222±0.015 0.99±0.2 4.631 0.0549±0.001 1211±15 transit 574±1.3 1.06±0.06 5690±40 [66]
TOI-1294 b 0.1957±0.016 0.8199±0.0277 3.915 0.0489 transit 1052±7 1.02±0.13 5714±126 [68]
TOI-1294 c 0.467±0.053 160.1±2.5 0.581 radial vel. 1052±7 1.02±0.13 5714±126 [69]
TOI-1347 b 0.0349±0.0038 0.161±0.009 0.847 1400±40 transit 480.8±2 0.913±0.033 5464±100 Ultra-short period planet[70]
TOI-1347 c 0.0088±0.0072 0.143±0.009 4.842 1000±25 transit [70]
TOI-1386 b 0.148+0.019
−0.018 		0.54+0.018
−0.016 		25.838 0.1732+0.0027
−0.0033 		676.4+10
−8.3 		transit 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[71]
TOI-1386 c 0.309±0.038 227.6+4.6
−4 		0.739+0.015
−0.016 		327.4+5.3
−4.6 		radial vel. 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[71]
TOI-1410 b 0.262 1.22 0.020 1396 transit 0.72 4635 [54]
TOI-1448 b <0.0613 0.245±0.006 8.112 0.0567±0.0015 389±5–426±6[g] transit 240±0.3 0.372±0.009 3412+28
−32 		[61]
TOI-1450 Ab 0.00396±0.0004 0.1±0.004 2.04 722±35 transit 73.2±0.1 0.48±0.24 3437±86 Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement.[72]
TOI-1450 Ac 0.0048±0.0006 5.07 533±26 radial vel. Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab.[72]
TOI-1683 b 0.236 3.06 0.037 929 transit 0.69 4402 [54]
TOI-1751 b 0.0538±0.0101 0.2489±0.0259 37.468 0.2115±0.0024 820 transit 370.3±0.3 1.15±0.17 6116±22 The host star is metal-poor ([Fe/H] = –0.40 dex).[73]
TOI-1798 b 0.126 0.44 0.011 2122 transit 0.86 5165 [54]
TOI-1806 b 0.304 15.15 0.088 337 transit 0.39 3272 [54]
TOI-1824 b 0.0582±0.01 0.2346±0.0133 22.8 0.149±0.003 577±19 transit 192.3 0.85±0.05 5180±110 High-density planet, situated in the small group of "superdense sub-Neptunes". TOI-1824 has also a red dwarf companion star named TIC 142387022.[74]
TOI-1828 b 0.1841±0.012 0.769±0.017 9.09 0.0859 transit 1208±8 1.04±0.13 5809±127 [75]
TOI-1855 b 1.133±0.096 1.65+0.37
−0.62 		1.364 0.02398+0.00037
−0.00036 		1700±20 transit + radial vel. 576.3±4.6 0.987+0.058
−0.045 		5359+89
−83 		[76]
TOI-2107 b 0.83±0.11 1.211±0.035 2.454 0.0315+0.0006
−0.00067 		1397±20 transit + radial vel. 767.4+6.2
−5.9 		0.961+0.049
−0.054 		5627+94
−93 		[76]
TOI-2120 b <0.02139 0.1893±0.0056 5.8 0.0377±0.0013 351±6–384±6[g] transit 104.9 0.211±0.005 3131±30 [61]
TOI-2266 b 0.1374±0.008 2.326 0.02±0.002 550±47 transit 168.6±0.2 0.23±0.02 3240±160 [77]
TOI-2368 b 0.65±0.18 0.967+0.06
−0.03 		5.175 0.05649±0.001 1000+44
−30 		transit 685±3.9 0.897+0.048
−0.049 		5360+230
−170 		[76]
TOI-2373 b 9.3±0.2 0.93±0.02 13.337 0.112±0.001 860±10 transit 1617±33 1.041+0.032
−0.028 		5651±180 [78]
TOI-2374 b 0.1782+0.011
−0.0134 		0.6075±0.0268 4.314 0.0471 <885±22 transit 439±3 0.75±0.01 4802±97 [79]
TOI-2416 b 3+0.1
−0.09 		0.88±0.02 8.275 0.0831±0.0007 1080±10 transit 1767±261 1.118+0.029
−0.027 		5808±80 [78]
TOI-2524 b 0.64±0.04 1+0.02
−0.03 		7.186 0.073±0.0007 1100±20 transit 1399±36 1.007+0.032
−0.029 		5831±80 [78]
TOI-2529 b 2.34±0.2 1.03±0.05 64.5949±0.0003 0.327±0.02 636±15.7 transit 965.8+14
−13.7 		1.11+0.02
−0.02 		5802+60
−52 		[49]
TOI-3071 b 0.2146±0.011 0.6388+0.0509
−0.0455 		1.267 0.0249 <2155±40 transit 1582±29 1.29±0.02 6177±62 [79]
TOI-3321 b 0.554±0.076 1.39+0.07
−0.06 		3.652 0.047±0.001 1616±30 transit 928+10.8
−10.4 		1.041+0.084
−0.068 		5850±140 [76]
TOI-3353 b 0.238 4.67 0.060 1264 transit 1.33 6365 [54]
TOI-3894 b 0.85±0.15 1.36±0.05 4.335 0.0543±0.0014 1519±22 transit 1343+12.7
−12.4 		1.138+0.089
−0.075 		6000±110 [76]
TOI-3919 b 3.88±0.023 1.1±0.05 7.433 0.0795±0.0016 1200±15 transit 1973+28.7
−28.4 		1.208+0.067
−0.07 		6100±110 [76]
TOI-4153 b 1.15±0.38 1.438±0.045 4.617 0.06311+0.00084
−0.00096 		1670+30
−40 		transit 1366±11.4 1.572+0.064
−0.071 		6860+150
−180 		[76]
TOI-4336 Ab 0.017+0.013
−0.007 		0.1891 16.337 0.0872+0.0013
−0.0014 		308±9 transit 73.15 0.331±0.015 3298+75
−73 		Located in a triple hierarchical stellar system.[80]
TOI-4438 b 0.017±0.0035 0.2248±0.0116 7.44 0.0534±0.009 400±50 transit 98 0.368±0.021 3422±81 [81]
TOI-4443 b 0.153 1.85 0.030 1639 transit 1.05 5834 [54]
TOI-4495 b 0.324 5.18 0.062 1383 transit 1.17 6156 [54]
TOI-4527 b 0.0812 0.40 0.008 1363 transit 0.48 3702 [54]
TOI-4602 b 0.227 3.98 0.051 1380 transit 1.12 6012 [54]
TOI-4633 c 0.15+0.087
−0.075 		0.285+0.018
−0.017 		271.94 0.847±0.061 290 transit 310.4±0.78 1.05±0.06 or 1.1±0.06[h] 5600±50 or 5800±50 [h] Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.[82]
TOI-5076 b 0.0503±0.00629 0.285±0.00892 23.445±0.001 615±20 transit 270.057±0.326 0.80±0.07 5070±143 [83]
TOI-5082 b 0.227 4.24 0.051 1165 transit 1.00 5670 [54]
TOI-5232 b 2.34±0.16 1.14+0.05
−0.045 		4.097 0.0599±0.001 1772+40
−45 		transit 1985+28
−27 		1.389+0.068
−0.075 		6500+180
−190 		[76]
TOI-5301 b 3.65±0.4 1.18+0.08
−0.07 		5.859 0.0726+0.0013
−0.0024 		1655±40 transit 1914+59
−55 		1.483+0.081
−0.14 		6240±160 [76]
TOI-5388 b 0.169 2.59 0.024 601 transit 0.29 3495 [54]
TOI-5720 b 0.0041+0.0029
−0.0015 		0.0972±0.0062 1.434 0.0183±0.0003 708±19 transit 116.9±0.1 0.383±0.019 3325±75 [84]
TOI-6008 b 0.00346+0.0023
−0.0011 		0.0919±0.0045 0.858 0.0108±0.0002 707±19 transit 75.05±0.03 0.23±0.011 3075±75 Ultra-short period planet[84]
TOI-6086 b 0.00346+0.00362
−0.00176 		0.1053±0.0062 1.389 0.0154±0.0002 634±16 transit 102.6 0.254±0.013 3200±75 [84]
V808 Aurigae b [ru] 6.8±0.7 4109±362 timing 698±13 0.9±0.1 The planet's host star is a polar. The mass value for the planet is only a minimum mass.[85]
VHS J183135.58-551355.9 6.5±1.5 1.42+0.04
−0.03 		1085±60 imaging 180.6±17.9 Free-floating planet[86]
Wolf 327 b 0.00796±0.00145 0.1106±0.0054 0.573 0.01 996±22 transit 92.9 0.405±0.019 3542±70 Ultra-short period planet[87]

Specific exoplanet lists[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery[edit]


Notes[edit]

  1. ^ a b c Distance calculated from parallax
  2. ^ The radius is the same as that of the Earth, with an uncertainty of 10%
  3. ^ Radius calculated with mass and lower limit in density in the equation d=(1.89813*10^(30)*m)/((4/3)*π*r3), where d is density (in g/cm3), m is the mass (in MJ and r is the radius (in centimeters). Should be divided by 7.1492×109 to convert from centimeters to RJ
  4. ^ Since the density is only a lower limit, the radius is an upper limit.
  5. ^ The planet is located in a two-star system, with masses of 0.78+0.38
    −0.36     M☉     and 0.56+0.3
    −0.28     M☉    . There is a large chance that it is orbiting both stars in the system, so the "host star mass" would be 0.78+0.38
    −0.36     M☉     + 0.56+0.3
    −0.28     M☉    . However, there is a small chance that is orbiting only one of the stars in the system.
  6. ^ The transit observations of TOI-286 indicate periodic transit signals of 4.5 abd 39.4 days. While this, radial velocity measurements with ESPRESSO do not immediately show evidence for periodic signals at either periods.
  7. ^ a b c Assuming albedos of 0.3 and 0 respectively.
  8. ^ a b It is not known which of the stars the planet orbits.


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