List of exoplanets discovered in 2024
Appearance
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 | 2.599 | 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 | 4.696 | 0.0437±0.0016 | 553±24 | transit | ||||
TOI-663 d | <0.0164 | 0.171±0.0116 | 7.103 | 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 | 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]
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
Lists of exoplanets by year of discovery[edit]
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (378)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (178)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (150)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (306)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (253)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (298)
- List of exoplanets discovered in 2024 (132)
Notes[edit]
- ^ a b c Distance calculated from parallax
- ^ The radius is the same as that of the Earth, with an uncertainty of 10%
- ^ 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
- ^ Since the density is only a lower limit, the radius is an upper limit.
- ^ 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. - ^ 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.
- ^ a b c Assuming albedos of 0.3 and 0 respectively.
- ^ a b It is not known which of the stars the planet orbits.
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