Список екзопланет, відкритих у 2020 році: відмінності між версіями
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Версія за 08:57, 7 березня 2023
Ця стаття в процесі редагування певний час. Будь ласка, не редагуйте її, бо Ваші зміни можуть бути втрачені. Якщо ця сторінка не редагувалася кілька днів, будь ласка, приберіть цей шаблон. Це повідомлення призначене для уникнення конфліктів редагування. Останнє редагування зробив користувач Dmytro Tvardovskyi (внесок, журнали) о 08:57 UTC (630221 хвилину тому). |
Список екзопланет, відритих в 2020 році. Різні методи відмічені різними кольорами. Для екзопланет, відкритих методом зміни радіальних швидкостей, наведені мінімальні маси.
Умовні познрачення в таблиці:
- MП - маса планети у масах Юпітера (MJ)
- РП - радіус планети у радіусах Юпітера (RJ)
- МЗ - маса материнської зорі у масах Сонця (M☉)
- P - орбітальний період в добах
- a - велика піввість орбіти планети в а.о.
- ТП - температура поверхні планети або умовної поверхні для газових гігантів в кельвінах
- d - вістань від Землі до екзопланети у світлових роках.
У першій колонці в дужках навередна офіційна назва екзопланети за каталогом та власна назва в дужках (якщо є). Також, якщо замість власної офіційної є власна неофіційна назва планети, то наводиться неофіційна назва.
Таблиця
Назва (власна назва) | МП | РП | P | a | ТП | Метод відкриття | d | МЗ | ТЗ | Примітки |
---|---|---|---|---|---|---|---|---|---|---|
2MASS J1155-7919 b | 10 | 582 | imaging | 330 | [1] Very young Super-Jupiter on unusually wide orbit.[2] | |||||
HD 38677 b | 18.57±0.01 | 0.1462±0.0012 | 877 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[3] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 38677 c | 6.584+0.003 −0.002 |
0.0733+0.0006 −0.0007 |
1239 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[3] Found by Dispersed Matter Planet Project looking for hot ablating planets, 2:1 orbital resonance of unconfirmed transiting planet.[4] | ||
HD 38677 d | 2.882±0.001 | 0.0422+0.0004 −0.0003 |
1632 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[3] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 38677 e | 5.516+0.002 −0.004 |
0.0651±0.0005 | 1314 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[3] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 11231 b | 0.426+0.038 −0.052 |
5.2072+0.0002 −0.0055 |
0.0664±0.0005 | 1000 | radial vel. | 437.0495±13.04625 | 1.44±0.03 | 6500±100 | DMPP-2[3] Found by Dispersed Matter Planet Project looking for hot ablating planets. | |
HD 42936 Ab | 2.58+0.35 −0.58 |
6.6732+0.0011 −0.0003 |
0.0662±0.0013 | 854 | radial vel. | 159.4905±1.956938 | 0.87±0.05 | 5138±99 | DMPP-3[3] Found by Dispersed Matter Planet Project looking for hot ablating planets. | |
ja | 0.02753±0.00343 | 0.174±0.008 | 3.5951±0.0003 | 0.047+0.005 −0.007 |
1616+150 −80 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [5] |
ja | 0.04616±0.00595 | 0.3274+0.0152 −0.0125 |
15.624±0.001 | 0.13+0.01 −0.02 |
990+68 −29 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [5] |
ja | 0.03203+0.00774 −0.00761 |
0.3515±0.0116 | 35.747±0.005 | 0.22+0.02 −0.04 |
752+69 −37 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [5][6] |
Gliese 180 d | 7.56±1.07 | 106.341+0.261 −0.34 |
0.31+0.024 −0.029 |
radial vel. | 39.96±0.01 | 0.43 | 3371 | [7] | ||
Gliese 229 Ac | 0.025 | 122.005+0.364 −0.382 |
0.339+0.024 −0.029 |
radial vel. | 18.78±0.004 | 0.58 | 3564 | [8][9] | ||
Gliese 251 b | >0.013 | 14.238 | 0.0818 | 351 | radial vel. | 18.205±0.006 | 0.360±0.015 | 3451±51 | False positive in 2019, rediscovered in 2020[10][11] | |
Gliese 433 d | 0.019 | 36.052+0.045 −0.031 |
0.178+0.013 −0.015 |
radial vel. | 29.57±0.01 | 0.48 | 3600 | [12][13] | ||
Gliese 1061 b | 0.00431+0.00050 −0.00047 |
3.204±0.001 | 0.021±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [14] | ||
Gliese 1061 c | 0.00547±0.00072 | 6.689±0.005 | 0.035±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [15] | ||
Gliese 1061 d | 0.00516+0.00076 −0.00072 |
13.031+0.025 −0.032 |
0.054±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [16] | ||
Gliese 1252 b | 0.0042±0.0009 | 0.105±0.007 | 0.5182349+0.0000063 −0.0000050 |
0.00915±0.00015 | 1410+91 −125 |
transit | 66.49±0.06 | 0.381±0.019 | 3458+140 −133 |
[17] No atmosphere[18] |
Gliese 3082 b | 0.02759+0.011 −0.01334 |
11.949±0.022 | 0.079+0.006 −0.007 |
radial vel. | 54.2 | 0.47 | [19] | |||
HATS-47b | 0.369 | 1.117 | 3.9228 | 852.9 | transit | 984.01±6.20 | 0.674 | [20] | ||
HATS-48Ab | 0.243 | 0.800 | 3.1317 | 0.03769±0.00011 | 954.6 | transit | 865 | 0.7279 | 4546.0+23 −18 |
[20][21] |
HATS-49b | 0.353 | 0.765 | 4.1480 | 834.8 | transit | 1058.70±7.18 | 0.7133 | [20] | ||
HATS-72b | 0.1254 | 0.7224 | 7.3279 | 739.3 | transit | 416.37±1.70 | 0.7311 | [20] | ||
HD 80653 b | 0.0176±0.0014 | 0.1439±0.0063 | 0.719573±0.000021 | 0.0166±0.0003 | transit | 358.1197±2.641867 | 1.18±0.04 | [22] | ||
ja | 3.213±0.078 | 2.03+0.61 −0.49 |
0.9809761+0.000037 −0.000034 |
0.01782±0.00021 | 1411±15 | transit | 201.85818±0.2609251 | 0.781±0.027 | 4590±49 | an ultra-short-period Jupiter orbiting a bright (V=11.1 mag) K4-dwarf.[23][24][25][26] |
KELT-2019-BLG-1953 b | 0.59+0.71 −0.32 |
0.8+0.9 −0.6 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[27][28] | ||||
KELT-2019-BLG-1953 c | 0.28+0.35 −0.15 |
0.8+0.9 −0.7 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[29][28] | ||||
Kepler-1661(AB) b | 0.053±0.038 | 0.345±0.005 | 175.06±0.06 | 0.633±0.005 | 243 | transit | 1355.26±9.56 | 0.841±0.022 | 5100±100 | [30][31] |
ja | 0.0145±0.00176 | 0.124±0.008 | 1.4015±0.00018 | 0.02091±0.00024 | 816±160 | transit | 82.02833±0.07827753 | 0.62±0.03 | 3800±70 | [32] |
ja | 0.0125+0.0185 −0.0084 |
0.68+0.27 −0.22 |
microlensing | 27000±3500 | 0.12+0.14 −0.08 |
Milky way bulge[33] | ||||
TOI-132 b | 0.07048+0.00598 −0.00604 |
0.305±0.012 | 2.1097019+0.000012 −0.000011 |
0.026+0.002 −0.003 |
1395+52 −72 |
transit | 536.43±89.11 | 0.970±0.06 | 5397±46 | [34] |
TOI-257b | 0.134±0.023 | 0.626±0.013 | 18.38827±0.00072 | 0.1523±0.0017 | 1033±19 | transit | 251.37±0.065 | 1.38+0.056 −0.009 |
6075±90 | Host star also called HD 19916.[35][36][37] |
TOI-700 b | 0.00406+0.003 −0.00116 |
0.0901+0.00839 −0.00776 |
9.97701+0.00024 −0.00028 |
0.0637+0.0064 −0.006 |
transit | 101.5 | 0.416±0.01 | 3480±135 | [38] | |
TOI-700 c | 0.0249+0.0085 −0.0057 |
0.2346+0.0214 −0.0205 |
16.051998+0.000089 −0.000092 |
0.0925+0.0088 −0.0083 |
transit | 101.5 | 0.416±0.01 | 3480±135 | [38] | |
TOI-700 d | 0.00711+0.0022 −0.00164 |
0.1062±0.0098 | 37.426+0.0007 −0.001 |
0.163±0.015 | 295±55 | transit | 101.5 | 0.416±0.01 | 3480±135 | First "Earth sized" discovered by TESS[38][39] |
TOI-732 b | 0.098 | 0.119 | 0.7683881 | 0.012 | 892 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[40][41] |
TOI-732 c | 0.027 | 0.205 | 12.25 | 0.07673 | 323 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[40][41] |
TOI-813 b | 0.599±0.034 | 83.8911+0.0027 −0.0031 |
0.423+0.031 −0.037 |
610+28 −21 |
transit | 864.8192±5.156379 | 1.32±0.06 | 5907±150 | [42] | |
TOI-1338 b | 0.10382±0.0622 | 0.61±0.0169 | 95.2 | 0.4607 | 724 | transit | 1301 | First circumbinary planet discovered by TESS[43] | ||
HD 191939 b | 0.301 | 8.880411 | 0.089 | 778+58 −41 |
transit | 175 | 0.92 | 5400 | Host star also known as TOI-1339[44] | |
HD 191939 c | 0.287 | 28.58060 | 0.178 | 550±45 | transit | 175 | 0.92 | 5400 | Host star also known as TOI-1339[44] | |
HD 191939 d | 0.282 | 38.3561 | 0.216 | 499+12 −11 |
transit | 175 | 0.92 | 5400 | Host star also known as TOI-1339[44] | |
USco1621 b | 16 | 2880 | 2270 | imaging | 450 | 0.36 | 3460 | [45] | ||
USco1556 b | 15 | 3500 | 2240 | imaging | 459 | 0.33 | 3410 | [45] | ||
XO-7b | 0.709 | 1.373 | 2.8641424 | 0.04421 | 1743 | transit | 763 | 1.405 | 6250 | [46] |
LHS 1815 b | 0.0132±0.0047 | 0.0971±0.005 | 3.81433±0.00003 | 0.0404±0.0094 | 617±84 | transit | 97 | 0.502 | 3643±142 | [47][48] |
TOI-157 b | 1.18±0.13 | 1.29±0.02 | 2.0845435±0.0000023 | 0.03138+0.00025 −0.00020 |
1588+21 −20 |
transit | 1171 | 0.948+0.023 −0.018 |
5404+70 −67 |
[23] |
ja | 0.791+0.064 −0.06 |
1.086+0.081 −0.048 |
2.2554477±0.0000063 | 0.03524+0.00069 −0.00079 |
1715+22 −20 |
transit | 1345 | 1.147+0.069 −0.075 |
5880+54 −49 |
[23] |
TOI-849 b | 0.128±0.008 | 0.308+0.014 −0.011 |
0.7655240±0.0000027 | 0.01598±0.00013 | 1800 | transit | 735 | 0.929±0.023 | 5329±48 | Neptunian Desert planet[49] |
HD 95338 b | 0.124+0.019 −0.013 |
0.355+0.008 −0.007 |
55.086+0.018 −0.019 |
0.231+0.005 −0.009 |
402+6 −9 |
transit | 120 | 0.76+0.16 −0.1 |
5212+16 −11 |
[50] |
HD 332231 b | 0.251±0.017 | 0.867+0.027 −0.025 |
18.70173±0.00028 | 0.1436+0.0032 −0.0033 |
876±17 | transit | 262 | 1.127±0.077 | 6089+97 −96 |
TOI 1456[51][52] |
TOI-1130 b | 0.3256±0.009 | 4.066499±0.000046 | 0.04394+0.00035 −0.00038 |
876±17 | transit | 190 | 0.684+0.16 −0.17 |
4250±67 | [53][54] | |
TOI-1130 c | 0.974+0.043 −0.044 |
1.5+0.27 −0.22 |
8.350381±0.000033 | 0.07098+0.00056 −0.0006 |
637±12 | transit | 190 | 0.684+0.16 −0.17 |
4250±67 | [53][55] |
HD 79211 b | 0.0334±0.004 | 24.422±0.014 | 0.142±0.005 | 345 | radial vel. | 20.658±0.005 | 0.64±0.07 | 4005±51 | Orbiting primary star of binary ADS 7251[56][57] | |
WASP-150 b | 8.46+0.28 −0.2 |
1.07+0.024 −0.025 |
5.644207+0.00003 −0.000004 |
0.0694+0.0011 −0.0008 |
1460±11 | transit | 2422 | 1.394+0.07 −0.049 |
6218+49 −45 |
[58] |
WASP-176 b | 0.855+0.072 −0.069 |
1.505+0.05 −0.045 |
3.899052±0.00005 | 0.0535+0.001 −0.0019 |
1721+28 −21 |
transit | 1883 | 1.345+0.08 −0.13 |
5941+77 −79 |
[58] |
TOI-1235 b | 0.0217±0.00025 | 0.155±0.007 | 3.444729+0.000031 −0.000028 |
0.03845+0.00037 −0.0004 |
754±18 | transit | 129 | 0.640±0.016 | 3872±70 | one more suspected planet in system[59] |
OGLE-2017-BLG-0406 b | 0.41±0.05 | 3.5±0.3 | microlensing | 17000±1600 | 0.56±0.07 | 4848 | High fidelity microlensing event[60] | |||
TOI-421 b | 0.051+0.004 −0.003 |
0.461±0.012 | 16.06815+0.00034 −0.00035 |
0.1182+0.0026 −0.0027 |
696.6±12.2 | transit | 244.3±1.9 | 0.852+0.029 −0.021 |
5325+78 −58 |
Also in system a red dwarf star at 2200 a.u. separation[61] |
TOI-421 c | 0.0222±0.0022 | 0.243±0.017 | 5.19676+0.00049 −0.00048 |
0.0557+0.0012 −0.0013 |
1014.9+17.9 −17.6 |
transit | 244.3±1.9 | 0.852+0.029 −0.021 |
5325+78 −58 |
Also in system a red dwarf star at 2200 a.u. separation[61] |
HD108236 b | 0.1415±0.0087 | 3.79523+0.00047 −0.00044 |
0.0469±0.0017 | 1099+19 −18 |
transit | 211 | 0.97 | 5730±50 | [62] | |
HD108236 c | 0.1845+0.0089 −0.0081 |
6.2037+0.00064 −0.00052 |
0.0651±0.0024 | 932+17 −16 |
transit | 211 | 0.97 | 5730±50 | [62] | |
HD108236 d | 0.2423±0.0097 | 14.1756+0.001 −0.0011 |
0.1131±0.004 | 708+13 −12 |
transit | 211 | 0.97 | 5730±50 | [62] | |
HD108236 e | 0.279+0.012 −0.011 |
19.592±0.002 | 0.14±0.0052 | 636+12 −11 |
transit | 211 | 0.97 | 5730±50 | [62] | |
WASP-148 b | 0.291±0.025 | 0.722±0.055 | 8.80381±0.000043 | 0.22±0.063 | 940±80 | transit | 809±5 | 1.00±0.08 | 5460±130 | [63][64] |
WASP-148 c | 0.397+0.203 −0.044 |
34.515±0.029 | 0.359±0.086 | 590±50 | radial vel. | 809±5 | 1.00±0.08 | 5460±130 | [63][64] | |
NGTS-11 b | 0.37±0.14 | 0.823±0.035 | 35.4553±0.0002 | 0.201±0.002 | 440±40 | transit | 624±6 | 0.862±0.028 | 5050±80 | [65] |
HIP 67522 b | 0.25 | 0.894+0.048 −0.047 |
6.9596+0.000016 −0.000015 |
1174±21 | transit | 416±4 | 1.22±0.05 | 5675±75 | One more candidate planet around very young (age below 20 million years) star[66] | |
HD 63433 b | 0.017 | ±0.009 | 7.10801+0.00046 −0.00034 |
0.0710+0.0033 −0.0041 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | [67] | |
HD 63433 c | 0.023 | 0.238±0.01 | 20.5455±0.001 | 0.1531+0.0074 −0.0092 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | [67][68] | |
HD 164922 d | 0.013±0.003 | 12.458±0.003 | 0.103±0.003 | radial vel. | 72.1±0.9 | 0.874±0.012 | 5293±32 | [69] | ||
OGLE-2006-BLG-284 b | 0.45+0.14 −0.40 |
2.2±0.8 | microlensing | 13000±4900 | 0.35+0.3 −0.2 |
Binary host with 2.1 astronomical unit separation and uncertain, possibly unstable, planetary orbit.[70] | ||||
Wendelstein-1b | 0.59+0.17 −0.13 |
1.0314+0.00204 −0.021 |
2.663416±0.000001 | 0.0282±0.0009 | 1727+78 −90 |
transit | 1004±10 | 0.65±0.1 | 3984+152 −46 |
[71] |
Wendelstein-2b | 0.731+0.541 −0.311 |
1.1592±0.0061 | 1.7522239±0.0000008 | 0.0234±0.0015 | 1852+120 −140 |
transit | 1875±20 | 0.73±0.11 | 4288+133 −111 |
Extended gaseous envelope[71] |
Kepler-160d | 0.170+0.015 −0.012 |
378.417+0.028 −0.025 |
1.089+0.037 −0.073 |
244.8+2.1 −2.9 |
transit | 3140±60 | 0.88 | 5471+115 −37 |
Next expected transit in September 2020.[72] | |
K2-315b | 0.085±0.005 | 3.1443189±0.0000049 | 0.0234 | 460±5 | transit | 185±1 | 0.174±0.004 | 3300±30 | Also called the "Pi Earth" due its orbital period, or EPIC 249631677b[73] | |
TOI-1266 b | 0.2193+0.074 −0.066 |
10.894879+0.00007 −0.00007 |
0.0745+0.0046 −0.0069 |
410+21 −15 |
transit | 117.4±1.0 | 0.437±0.021 | 3563±77 | [74] | |
TOI-1266 c | 0.1492+0.077 −0.095 |
18.80152+0.00054 −0.00067 |
0.1037+0.0026 −0.0025 |
347.1+7.9 −8 |
transit | 117.4±1.0 | 0.437±0.021 | 3563±77 | [74] Possibly atmosphere of steam[75] | |
AU Microscopii b | 0.18 | 0.375 | 8.46321±0.00004 | 0.066 | transit | 32.3±0.3 | 0.31 | 3500±100 | [76][77][78] | |
TOI-1728 b | 0.084+0.017 −0.016 |
0.450±0.014 | 3.491510+0.000062 −0.000057 |
0.0391±0.0009 | 767±8 | transit | 198.2±0.5 | 0.646+0.023 −0.022 |
3980+31 −32 |
[79] |
BD-11 4672 c | 0.048±0.009 | 74.2+0.06 −0.08 |
0.30±0.01 | radial vel. | 88.63±0.11 | 0.651+0.031 −0.029 |
4550±110 | Habitable zone, highly eccentric orbit.[80] | ||
OGLE-2018-BLG-1269Lb | 0.69+0.44 −0.22 |
4383 | 4.61+1.70 −1.17 |
microlensing | 8300+3000 −2000 |
0.35+0.3 −0.2 |
Very high fidelity event[81] | |||
Lacaille 9352 b | 0.0132±0.0019 | 9.262±0.001 | 0.068±0.002 | 468 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | [82] | |
Lacaille 9352 c | 0.0234±0.0038 | 21.789+0.004 −0.005 |
0.120±0.004 | 352 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | [82] | |
HAT-P-58b | 0.372±0.03 | 1.332±0.043 | 4.0138379±0.0000024 | 0.04994±0.00044 | 1622±18 | transit | 1690±40 | 1.031±0.028 | 6078±48 | [83] |
HAT-P-59b | 1.540±0.067 | 1.123±0.013 | 4.1419771±0.0000012 | 0.05064±0.00037 | 1278±7 | transit | 871±4 | 1.008±0.022 | 5678±16 | [83] |
HAT-P-60b | 0.574±0.038 | 1.631±0.024 | 4.7947813±0.0000024 | 0.06277±0.00017 | 1772±12 | transit | 767±7 | 1.435±0.012 | 6212±26 | [83] |
HAT-P-61b | 1.057±0.07 | 0.899±0.027 | 1.90231289±0.00000077 | 0.03010±0.00034 | 1505±16 | transit | 1120±20 | 1.004±0.012 | 5587±45 | [83] |
HAT-P-62b | 0.761±0.088 | 1.073±0.029 | 2.6453235±0.0000039 | 0.03772±0.00024 | 1512±13 | transit | 1150±20 | 1.023±0.020 | 5629±48 | [83] |
HAT-P-63b | 0.614±0.024 | 1.119±0.033 | 3.377728±0.000013 | 0.04294±0.00035 | 1237±11 | transit | 1330±20 | 0.925±0.023 | 5400+55 −39 |
[83] |
HAT-P-64b | 0.58+0.18 −0.13 |
1.703±0.07 | 4.0072320±0.0000017 | 0.05387±0.00030 | 1766+22 −16 |
transit | 2135±20 | 1.298±0.021 | 6457+55 −36 |
[83] |
TOI-1899 b | 0.67±0.04 | 0.99±0.03 | 29.090312+0.000036 −0.000035 |
0.1587+0.067 −0.075 |
362±7 | transit | 419±1 | 0.627+0.026 −0.028 |
3841+54 −45 |
[84][85] |
HATS-37A b | 0.099±0.042 | 0.606±0.016 | 4.3315 | 0.1587+0.067 −0.075 |
1085+16 −12 |
transit | 695 | 0.843+0.017 −0.012 |
5247±50 | One more red dwarf in system[86] |
HATS-38 b | 0.074±0.011 | 0.614±0.0176 | 4.3750 | 0.1587+0.067 −0.075 |
1294±10 | transit | 1131 | 0.890+0.016 −0.012 |
5740±50 | [86] |
TYC 8998-760-1 c | 6±1 | 1.1+0.6 −0.3 |
320 | 1240+160 −170 |
imaging | 309.4±0.9 | 4783 | [87] | ||
HD 86226 c | 0.023±0.004 | 0.193±0.007 | 3.98442±0.00018 | 0.049±0.001 | 1311±28 | transit | 149 | 1.019+0.061 −0.066 |
5863±88 | [88] |
Gliese 2056 b | 0.444±0.053 | 69.971±0.061 | 0.283±0.0013 | radial vel. | 92.8 | 0.62±0.08 | habitable zone[89] | |||
Gliese 480 b | 0.042±0.005 | 9.567±0.005 | 0.068±0.001 | radial vel. | 46.4 | 0.45±0.02 | [89] | |||
Gliese 687 c | 0.050±0.013 | 728±12 | 1.165±0.023 | radial vel. | 14.83 | 0.40±0.02 | Second Neptune sized planet discovered in this system[89] | |||
HIP 107772 b | 0.049+0.014 −0.030 |
55.259+0.111 −0.311 |
0.243+0.022 −0.027 |
radial vel. | 77.1 | 0.63±0.08 | habitable zone[89] | |||
HIP 38594 b | 0.026+0.012 −0.014 |
60.711+0.426 −0.192 |
0.256+0.006 −0.007 |
radial vel. | 58.0 | 0.61±0.02 | habitable zone[89] | |||
HIP 38594 c | 0.135+0.077 −0.035 |
3525+541 −572 |
3.842+0.399 −0.441 |
radial vel. | 58.0 | 0.61±0.02 | [89] | |||
HIP 4845 b | 0.053+0.016 −0.028 |
34.151+0.17 −0.09 |
0.177+0.016 −0.020 |
radial vel. | 68.8 | 0.62±0.04 | [89] | |||
HIP 48714 b | 0.071+0.023 −0.020 |
17.819+0.004 −0.009 |
0.112±0.003 | radial vel. | 34.3 | 0.58±0.02 | [89] | |||
TOI 824 b | 0.058±0.006 | 0.261+0.018 −0.017 |
1.392978+0.000018 −0.000017 |
0.02177±0.00032 | 1253+38 −37 |
transit | 208 | 0.69+0.009 −0.007 |
4569±50 | Neptunian Desert planet,[90] likely stripped of hydrogen envelope[91] |
Proxima Centauri c | 0.0179±0.006 | 1928±20 | 1.489±0.049 | 39+16 −18 |
radial vel. | 4.244±0.001 | 0.1221±0.0022 | 3042±117 | [92][93] Second planet discovered orbiting nearest star to the Solar System | |
TOI-763 b | 0.031±0.002 | 0.203±0.010 | 5.6057±0.0013 | 0.0600±0.0006 | 1038±16 | transit | 311 | 0.917±0.028 | 5444±110 | [94] |
TOI-763 c | 0.029±0.003 | 0.235±0.011 | 12.2737+0.0053 −0.0077 |
0.1011±0.0010 | 800±12 | transit | 311 | 0.917±0.028 | 5444±110 | [94] |
TOI-763 d | 0.030±0.005 | 47.7991±2.7399 | 0.2504+0.0093 −0.0105 |
509±12 | radial vel. | 311 | 0.917±0.028 | 5444±110 | [94] | |
TOI-561 b | 0.0050±0.0011 | 0.127±0.006 | 0.446578±0.000017 | 0.01055±0.00008 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[95][96] | |
TOI-561 c | 0.017±0.003 | 0.257±0.009 | 10.779±0.004 | 0.08809±0.0007 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[95][96] | |
TOI-561 d | 0.038±0.004 | 0.226±0.011 | 25.62±0.04 | 0.1569±0.0012 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[95][96] | |
TOI-561 e | 0.050±0.007 | 0.238±0.010 | 77.23±0.39 | 0.3274+0.0028 −0.0027 |
transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[95] | |
TOI-1266 b | 0.042+0.035 −0.028 |
0.212+0.014 −0.011 |
10.894843+0.000067 −0.000066 |
0.0736+0.0016 −0.0017 |
413±20 | transit | 117.5±0.1 | 0.48±0.1 | 3570±100 | [97] |
TOI-1266 c | 0.007+0.006 −0.005 |
0.139+0.013 −0.012 |
18.80151+0.00067 −0.00069 |
0.1058+0.0023 −0.0024 |
344±16 | transit | 117.5±0.1 | 0.48±0.1 | 3570±100 | [97] |
Gl 414 A b | 0.029+0.010 −0.008 |
0.263+0.099 −0.081 |
50.817+0.031 −0.03 |
0.24±0.01 | 303.7±32.5 | radial vel. | 38.8 | 0.650±0.08 | 4120±109 | Planets orbiting primary star of binary system[98] |
Gl 414 A c | 0.177+0.033 −0.031 |
0.784+0.360 −0.238 |
748.3+1.3 −1.2 |
1.43±0.06 | 123.3±13.2 | radial vel. | 38.8 | 0.650±0.08 | 4120±109 | Planets orbiting primary star of binary system[98] |
TOI 837 b | <1.2 | 0.768+0.091 −0.072 |
8.3248762±0.0000157 | transit | 466.5±1.2 | 1.118±0.059 | 6047±162 | Belongs to open cluster IC 2602[99] | ||
TOI-776 b | 0.0147±0.0031 | 0.163±0.010 | 8.24664+0.00009 −0.00006 |
0.0652±0.0011 | 513±12 | transit | 88.6±0.1 | 0.544±0.028 | 3709±70 | [100] |
TOI-776 c | 0.0192±0.0047 | 0.184±0.012 | 15.6653+0.0008 −0.0007 |
0.1000±0.0017 | 415±10 | transit | 88.6±0.1 | 0.544±0.028 | 3709±70 | [100] |
MOA-2009-BLG-319Lb | 0.2077±0.0255 | 2.03±0.21 | microlensing | 22800±2300 | 0.514±0.063 | [101] | ||||
TOI-481 b | 1.53±0.03 | 0.99±0.01 | 10.33111±0.00002 | 0.097±0.001 | 1370±10 | transit | 587 | 1.14+0.02 −0.01 |
5735±72 | [102] |
TOI-892 b | 0.95±0.07 | 1.07±0.02 | 10.62656±0.00007 | 0.092±0.005 | 1397±40 | transit | 1120 | 1.28+0.03 −0.02 |
6261±80 | [102] |
GJ 3473 b | 0.0059±0.0009 | 0.113±0.004 | 1.1980035+0.0000018 −0.0000019 |
0.01589±0.00062 | 773+16 −15 |
transit | 89.29±0.13 | 0.360±0.016 | 3347±54 | Also called TOI-488 b[103] |
GJ 3473 c | 0.0233+0.0029 −0.0027 |
15.509±0.033 | 0.0876+0.0035 −0.0034 |
329.1+6.6 −6.4 |
radial vel. | 89.29±0.13 | 0.360±0.016 | 3347±54 | Also called TOI-488 c[103] | |
NGTS-12b | 0.208±0.022 | 1.048±0.032 | 7.532806±0.000048 | 0.0757±0.0014 | 1257±34 | transit | 1474±25 | 1.021+0.056 −0.049 |
5690±130 | [104] |
OGLE-2016-BLG-1928 | 0.001 | n/a | microlensing | 30000 | n/a | n/a | Rogue planet[105] | |||
LTT 9779 b | 0.092±0.003 | 0.421±0.021 | 0.792054±0.000014 | 0.01679±0.0014 | 2000 | transit | 262.8±1.0 | 1.02+0.02 −0.03 |
5499±50 | Neptune desert planet[106] |
TOI 540 b | 0.081±0.005 | 1.2391491±0.0000017 | 0.01223±0.00036 | 611±23 | transit | 45.67±0.29 | 0.159±0.014 | 3216±83 | [107] | |
HD 238090 b | 0.0217+0.0029 −0.0030 |
13.671+0.011 −0.010 |
0.0932±0.0011 | 469.6+2.3 −2.6 |
radial vel. | 49.68±0.03 | 0.578±0.021 | 3933±51 | Orbiting primary star in binary system Gliese 458[11] | |
TIC 237913194b | 1.942+0.092 −0.091 |
1.117+0.054 −0.047 |
15.168865±0.000018 | 0.1207±0.0037 | 974 | transit | 1009±6 | 1.026+0.057 −0.055 |
5788±80 | Very eccentric orbit[108] |
EPIC 201170410 b | 0.09341 | 6.7987 | 0.0349 | transit | 437+149 −130 |
0.287+0.101 −0.084 |
3648+172 −143 |
[109] | ||
EPIC 201757695 b | 0.08101 | 2.0478 | 0.0296 | transit | 1880±110 | 0.727+0.044 −0.053 |
4520+108 −54 |
[109] | ||
OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 |
1.27+0.45 −0.29 |
microlensing | 16000 | 0.08+0.08 −0.02 |
[110] | ||||
TOI-954 b | 0.174+0.018 −0.017 |
0.852+0.053 −0.062 |
3.6849729+0.0000027 −0.0000028 |
0.04963+0.00089 −0.00090 |
1526+123 −164 |
transit | 768.5±8.3 | 1.201+0.066 −0.064 |
5710+53 −49 |
[111] |
EPIC 246193072 b | 0.260+0.020 −0.022 |
0.774+0.026 −0.024 |
12.4551225±0.0000031 | 0.1016+0.0018 −0.0019 |
650+53 −70 |
transit | 760±9 | 0.912+0.048 −0.049 |
5282+40 −39 |
[111] |
WASP-186 b | 4.22±0.18 | 1.11±0.03 | 5.026799+0.000012 −0.000014 |
0.0600+0.0012 −0.0013 |
1348+23 −22 |
transit | 913±11 | 1.22+0.07 −0.08 |
6361+105 −82 |
Also called TOI-1494[112] |
WASP-187 b | 0.80±0.09 | 1.64±0.05 | 5.147878+0.000005 −0.000009 |
0.0653±0.0013 | 1726+31 −2 |
transit | 1224±21 | 1.54±0.09 | 6150+92 −85 |
Also called TOI-1493[112] |
TOI 122b | 0.028+0.029 −0.010 |
0.243±0.016 | 5.078030±0.000015 | 0.0392±0.0007 | 471 | transit | 202.9±0.7 | 0.312±0.007 | 3403±100 | [113] |
TOI 237b | 0.009+0.006 −0.003 |
0.128±0.011 | 5.436098±0.000039 | 0.0341±0.0010 | 388 | transit | 124.2±0.7 | 0.179±0.004 | 3212±100 | [113] |
HAT-P-68b | 0.724±0.043 | 1.072±0.012 | 2.29840551±0.00000052 | 0.02996+0.00043 −0.00012 |
1027.8±8.2 | transit | 662±3 | 0.6785+0.0299 −0.0079 |
4514±50 | [114] |
LP 714-47 b | 0.097±0.005 | 0.420±0.027 | 4.052037±0.000004 | 0.0417±0.0005 | 700+19 −24 |
transit | 171.8±0.4 | 0.59±0.02 | 3950±51 | Host star also known as G 160-62 or TOI 442, planet in Neptune desert[115] |
CFHTWIR-Oph 98 B | 7.8+0.7 −0.8 |
1.86±0.04 | 200 | 1800±40 | imaging | 447±13 | 0.015 | 2320±40 | Very young superjovian planet orbiting a brown dwarf known as 2MASS J16274422-2358521[116] | |
HD 190007 b | 0.052±0.005 | 11.72 | radial vel. | 41.47±0.03 | 0.77±0.02 | 4610±20 | [117] | |||
HD 216520 b | 0.032±0.003 | 35.45 | radial vel. | 63.77±0.03 | 0.82±0.04 | 5103±20 | [117] | |||
HD 216520 c | 0.030±0.005 | 154.43 | radial vel. | 63.77±0.03 | 0.82±0.04 | 5103±20 | [117] | |||
TOI-519 b | <14 | 0.75±0.21 | 1.2652328±0.0000005 | 0.012±0.004 | 760±54 | transit | 378±3 | 0.369+0.026 −0.097 |
3350+100 −200 |
Very faint 17-magnitude host star[118] |
TOI-260 b | 0.009+0.013 −0.009 |
0.157±0.027 | 13.478048±0.005188 | transit | 65.84±0.07 | Host star also called HIP 1532 and BD-10 47[119] | ||||
TOI-784 b | 0.031±0.004 | 0.171±0.015 | 2.797179±0.000158 | transit | 211±0.4 | Host star also called HD 307842[119] | ||||
TOI-836 b | 0.0143±0.0028 | 0.152±0.006 | 3.81673±0.00001 | 0.04220±0.00093 | 871±36 | transit | 89.72±0.09 | 0.678+0.049 −0.041 |
4552±154 | Host star also called HIP 73427 and CD-23 12010[119][120] |
TOI-836 c | 0.0302±0.0082 | 0.231±0.008 | 8.59545±0.00001 | 0.0750±0.0016 | 665±27 | transit | 89.72±0.09 | 0.678+0.049 −0.041 |
4552±154 | Host star also called HIP 73427 and CD-23 12010[119][120] |
EPIC 201085153 b | 0.214±0.089 | 0.25722±0.000039 | transit | 3945±386 | Extremely tight orbit[121] | |||||
EPIC 201085153 c | 0.125+0.179 −0.125 |
2.259797±0.0008 | transit | 3945±386 | [121] | |||||
EPIC 201427007 b | 0.134±0.018 | 0.72091±0.000067 | transit | 5633±111 | [121] | |||||
EPIC 201595106 b | 0.116±0.009 | 0.877214±0.000087 | transit | 762±9 | 5820±20 | Candidate since 2018[121] | ||||
EPIC 201650711 c | 0.036±0.007 | 5.544059±0.00016 | transit | 298.8±1.7 | 4310±92 | Ternary star system, and planet b unconfirmed[121] | ||||
EPIC 205152172 b | 0.107±0.018 | 0.980088±0.000026 | transit | 517±2 | 0.669±0.016 | 4202±242 | Candidate since 2016[121] | |||
K2-299c | 0.223±0.080 | 14.648966±0.000031 | transit | 1219±16 | 5724±72 | Also known as EPIC 206024342 p2[121] | ||||
K2-299d | 0.152±0.054 | 4.507464±0.0000077 | transit | 1219±16 | 5724±72 | Also known as EPIC 206024342 p3[121] | ||||
K2-301c | 0.152±0.018 | 5.2986±0.00035 | transit | 1491±45 | 4114±99 | Also known as EPIC 206042996 p2[121] | ||||
TOI-251b | 0.245±0.016 | 4.937770+0.000028 −0.000029 |
0.05741+0.00023 −0.00017 |
transit | 324.4±1.4 | 1.036+0.013 −0.009 |
5875+100 −190 |
[122] | ||
TOI-942b | 0.429±0.018 | 4.324190±0.00003 | 0.04796+0.00073 −0.00065 |
transit | 498±2 | 0.788+0.037 −0.031 |
4928+125 −85 |
[122][123] Host star TYC 5909-319-1 | ||
TOI-942c | 0.517+0.017 −0.016 |
10.156430+0.000069 −0.000079 |
0.0847+0.0012 −0.0011 |
transit | 498±2 | 0.788+0.037 −0.031 |
4928+125 −85 |
[122][123] Host star TYC 5909-319-1 | ||
K2-302c | 0.089±0.009 | 2.255438±0.000037 | transit | 359.3±3.5 | 3297±73 | Also known as EPIC 206215704 p2[121] | ||||
K2-302d | 0.098±0.009 | 2.909216±0.000032 | transit | 359.3±3.5 | 3297±73 | Also known as EPIC 206215704 p3[121] | ||||
EPIC 206298289 b | 0.078±0.009 | 0.434847±0.000022 | transit | 492±6 | 3875±157 | Candidate since 2016[121] | ||||
K2-85 b | 0.107±0.009 | 0.684559±0.000026 | transit | 317.8±1.2 | 4427±48 | Also known as EPIC 210707130 p1[121] | ||||
EPIC 210801536 b | 0.088±0.027 | 0.892592±0.00012 | transit | 5304±259 | Candidate since 2019, one more planet candidate in system[121] | |||||
EPIC 212624936 b | 0.517+0.098 −0.027 |
0.578657±0.000066 | transit | 5765±170 | [121] Host star TYC 5557-667-1 | |||||
EPIC 212624936 c | 0.214+0.098 −0.057 |
11.811437±0.00016 | transit | 5765±170 | [121] Host star TYC 5557-667-1 | |||||
K2-211c | 0.116±0.018 | 2.601404±0.000072 | transit | 895±14 | 0.882+0.019 −0.027 |
5360±51 | [121] | |||
EPIC 220440058 b | 0.125±0.036 | 0.626683±0.00005 | transit | 3682±217 | One more planet candidate in system[121] | |||||
EPIC 220492298 b | 0.085±0.018 | 0.762406±0.00014 | transit | 5620±31 | [121] | |||||
K2-282d | 0.232±0.027 | 27.248322±0.00047 | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | [121] | |||
EPIC 228836835 b | 0.089±0.027 | 0.728113±0.00004 | transit | 491±6 | 3782±152 | [121] | ||||
K2-106c | 0.188±0.018 | 13.334621±0.000068 | transit | 803±10 | 5613±39 | Candidate since 2017[121] | ||||
Kepler-1514c | 0.1049+0.0051 −0.0039 |
10.514181±0.000039 | 0.0997±0.0018 | 1066+16 −14 |
transit | 1240 | 1.196+0.065 −0.063 |
6145+99 −80 |
[124] | |
OGLE-2017-BLG-1049Lb | 5.53+3.62 −2.87 |
3.92+1.10 −1.32 |
microlensing | 18500+3600 −4500 |
0.55+0.36 −0.29 |
[125] | ||||
AU Microscopii c | <0.087 | 0.320±0.014 | 18.858991±0.000010 | 0.1101±0.0022 | 454±16 | transit | 31.7 | 0.50±0.03 | 3700±100 | [126] Precise radial velocities of giant stars |
HD 25723 b | 2.51 | 456.78 | 1.49 | radial vel. | 375 | 2.1±0.3 | Giant star host[127] | |||
HD 25723 c | 1.33 | 2369.84 | 4.35 | radial vel. | 375 | 2.1±0.3 | Giant star host[127] | |||
Chi Scorpii b | 4.32+0.15 −0.12 |
573.4±2.0 | 1.45±0.02 | radial vel. | 408 | 1.09±0.15 | 4157±11 | Giant star host[127] | ||
HD 60292 b | 6.5±1.0 | 495.4±3.0 | 1.5±0.1 | radial vel. | 1036±10 | 1.7±0.2 | 4348±28 | Giant star host[128] | ||
HD 112640 b | 5.0±1.0 | 613.2±5.8 | 1.7±0.1 | radial vel. | 1065±6 | 1.8±0.2 | 4155±15 | Giant star host[128] | ||
K2-111 c | 0.0356±0.0035 | 15.6785+0.0064 −0.0063 |
0.1166±0.0025 | radial vel. | 680±60 | 0.89±0.02 | 5730±50 | [129] | ||
K2-316b | 0.119 | 1.133 | 0.0147 | 841 | transit | 368 | EPIC 249384674b[130] | |||
K2-316c | 0.163 | 5.260 | 0.0582 | 423 | transit | 368 | EPIC 249384674c[130] | |||
K2-317b | 0.261 | 6.220 | 0.0542 | 432 | transit | 577 | EPIC 249557502b[130] | |||
K2-318b | 0.148 | 7.010 | 0.0911 | 456 | transit | 483 | EPIC 249826231b[130] | |||
K2-319b | 0.249 | 26.680 | 0.1516 | 641 | transit | 686 | EPIC 201663879b[130] | |||
K2-320b | 0.234 | 1.995 | 0.0142 | 698 | transit | 356 | EPIC 201796690b[130] | |||
K2-321b | 0.174 | 2.298 | 0.0410 | 701 | transit | 254 | EPIC 248480671b[130] | |||
K2-322b | 0.171 | 8.205 | 0.0594 | 635 | transit | 404 | EPIC 248558190b[130] | |||
K2-323b | 0.187 | 24.930 | 0.1275 | 318 | transit | 387 | EPIC 248616368b[130] | |||
K2-324b | 0.217 | 3.262 | 0.0331 | 707 | transit | 447 | EPIC 248639308b[130] | |||
K2-325b | 0.196 | 6.930 | 0.0419 | 423 | transit | 365 | EPIC 246074965b[130] | |||
K2-326b | 0.203 | 1.256 | 0.0198 | 1114 | transit | 928 | EPIC 246472939b[130] | |||
KMT-2016-BLG-2397b | 2.42 | 2.83 | microlensing | 16000 | 0.62+0.29 −0.30 |
Multiple solutions for planetary parameters[131] | ||||
KMT-2016-BLG-2364b | 3.93 | 2.63 | microlensing | 21000 | 0.50+0.40 −0.22 |
[131] | ||||
OGLE-2017-BLG-1375b | 10.33 | 2.97 | microlensing | 12000 | 0.77+0.27 −0.23 |
Multiple solutions for planetary parameters[131] | ||||
OGLE-2017-BLG-0604b | 0.51 | 4.06 | microlensing | 13000 | 0.70±0.28 | [131] | ||||
KMT-2018-BLG-0748Lb | 0.18+0.29 −0.10 |
0.62±0.09 | microlensing | 24000 | 0.0870+0.138 −0.047 |
[132] | ||||
KMT-2019-BLG-1339Lb | 12.2+16.1 −6.7 |
0.67+0.77 −0.55 |
microlensing | 23000±3000 | 0.27+0.366 −0.15 |
Multiple solutions for planetary parameters[133] | ||||
ja | 0.19 | microlensing | 12000 | Free-floating planet[134] | ||||||
OGLE-2019-BLG-0551 | 0.0242 | microlensing | Poorly characterized free-floating planet[135] | |||||||
TVLM 513-46546 b | 0.38±0.24 | 221±5 | 0.3±0.0036 | astrometry | 34.90±0.07 | 0.09 | 2500 | [136] | ||
CD Ceti b | 0.0124+0.0013 −0.0014 |
2.29070±0.00012 | 0.0185+0.0013 −0.0013 |
464±18 | radial vel. | 28.07 | 0.161±0.010 | 3130±51 | [137] | |
OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 |
1.27+0.45 −0.29 |
microlensing | 16000 | 0.08+0.08 −0.02 |
[138] | ||||
WD 1856+534 b | 13.8 | 0.93±0.09 | 1.4079405±0.0000011 | 0.0204±0.0012 | transit | 80.737±0.144 | 0.518±0.055 | 4710±60 | Orbiting a white dwarf star[139] | |
Kepler-1649c | 0.0038 | 0.095+0.014 −0.010 |
19.53527±0.00010 | 0.0649 | 234±20 | transit | 301.6±1.6 | 0.1977±0.0051 | 3240±61 | Habitable zone, Earth-like[140] |
Kepler-305e | 0.160 | 3.20538 | transit | 2900±90 | [141] | |||||
Kepler-385d | 0.233 | 56.4159 | transit | 4870±160 | [141] | |||||
Kepler-598c | 0.270 | 86.4945 | transit | 2260±40 | FPP=1.0%[141] | |||||
Kepler-647c | 0.357 | 29.6663 | transit | 3660±70 | [141] | |||||
Kepler-716c | 0.124 | 3.96999 | transit | 2110±30 | FPP=0.6%[141] | |||||
Kepler-783c | 0.208 | 7.05395 | transit | 1707±15 | [141] | |||||
Kepler-1001c | 0.140 | 9.18186 | transit | 3110±80 | [141] | |||||
Kepler-1085c | 0.291 | 56.7771 | transit | 4630±150 | [141] | |||||
Kepler-1662b | 0.223 | 0.790 | 134.4628 | transit | [142] Host star also known as KOI-1783[143] | |||||
Kepler-1663b | 0.294 | 17.6046 | transit | 1112±11 | Host star also known as KOI-252[141] | |||||
Kepler-1664b | 0.270 | 14.3868 | transit | Host star also known as KOI-349[141] | ||||||
Kepler-1665b | 0.253 | 11.9548 | transit | 1104±5 | Host star also known as KOI-650[141] | |||||
Kepler-1666b | 0.257 | 25.8476 | transit | 4680±190 | Host star also known as KOI-945[141] | |||||
Kepler-1666c | 0.257 | 25.8476 | transit | 4680±190 | Host star also known as KOI-945[141] | |||||
Kepler-1667b | 0.266 | 83.5781 | transit | 2080±20 | Host star also known as KOI-1311[141] | |||||
Kepler-1668b | 0.388 | 15.434 | transit | 4500±200 | Host star also known as KOI-1470[141] | |||||
Kepler-1669b | 0.248 | 9.51216 | transit | 1800±40 | Host star also known as KOI-1475[141] | |||||
Kepler-1670b | 0.299 | 20.4998 | transit | 7200±400 | Host star also known as KOI-1705[141] | |||||
Kepler-1671b | 0.118 | 4.16787 | transit | 1176±7 | Host star also known as KOI-1738[141] | |||||
Kepler-1672b | 0.265 | 150.878 | transit | 1189±14 | Host star also known as KOI-1822[141] | |||||
Kepler-1673b | 0.262 | 33.7888 | transit | 2420±20 | Host star also known as KOI-1863[141] | |||||
Kepler-1674b | 0.286 | 62.5611 | transit | 3400±100 | Host star also known as KOI-1892[141] | |||||
Kepler-1675b | 0.279 | 63.0382 | transit | 2163±19 | Host star also known as KOI-1928[141] | |||||
Kepler-1676b | 0.301 | 29.9221 | transit | Host star also known as KOI-1943[141] | ||||||
Kepler-1677b | 0.241 | 22.064 | transit | 2250±30 | Host star also known as KOI-1984, FPP=0.6%[141] | |||||
Kepler-1678b | 0.295 | 147.974 | transit | 2830±70 | Host star also known as KOI-2066, FPP=0.5%[141] | |||||
Kepler-1679b | 0.184 | 9.75376 | transit | 3040±100 | Host star also known as KOI-2106[141] | |||||
Kepler-1680b | 0.121 | 8.77424 | transit | 1020±5 | Host star also known as KOI-2120[141] | |||||
Kepler-1681b | 0.2227 | 69.8956 | transit | 2100±300 | Host star also known as KOI-2132[141] | |||||
Kepler-1682b | 0.257 | 14.8334 | transit | 3900±160 | Host star also known as KOI-2229[141] | |||||
Kepler-1683b | 0.167 | 15.0337 | transit | 2440±50 | Host star also known as KOI-2293[141] | |||||
Kepler-1684b | 0.256 | 47.7055 | transit | 2060±40 | Host star also known as KOI-2417[141] | |||||
Kepler-1685b | 0.230 | 20.4905 | transit | 3840±150 | Host star also known as KOI-2504[141] | |||||
Kepler-1686b | 0.127 | 9.30987 | transit | 2430±30 | Host star also known as KOI-2559[141] | |||||
Kepler-1687b | 0.147 | 5.77954 | transit | 1375±17 | Host star also known as KOI-2588[141] | |||||
Kepler-1688b | 0.112 | 5.62012 | transit | 1850±380 | Host star also known as KOI-2733[141] | |||||
Kepler-1689b | 0.084 | 8.483 | transit | 967±5 | Host star also known as KOI-2755[141] | |||||
Kepler-1690b | 0.250 | 234.636 | transit | 2340±30 | Host star also known as KOI-2757[141] | |||||
Kepler-1691b | 0.163 | 3.8482 | transit | 4290±110 | Host star also known as KOI-2802[141] | |||||
Kepler-1692b | 0.099 | 5.95966 | transit | 1960±20 | Host star also known as KOI-2849[141] | |||||
Kepler-1693b | 0.115 | 12.0999 | transit | 2530±50 | Host star also known as KOI-2871[141] | |||||
Kepler-1694b | 0.105 | 3.89526 | transit | 1698±16 | Host star also known as KOI-2878, FPP=0.6%[141] | |||||
Kepler-1695b | 0.099 | 4.7329 | transit | 2640±40 | Host star also known as KOI-3048, FPP=0.5%[141] | |||||
Kepler-1696b | 0.250 | 65.9409 | transit | 5100±200 | Host star also known as KOI-3361[141] | |||||
Kepler-1697b | 0.112 | 33.4969 | transit | 813±2 | Host star also known as KOI-3478[141] | |||||
Kepler-1698b | 0.095 | 1.2107 | transit | 729±3 | Host star also known as KOI-3864[141] | |||||
Kepler-1699b | 0.139 | 3.49082 | transit | Host star also known as KOI-3933[141] | ||||||
Kepler-1701b | 0.198 | 169.134 | transit | 1940±20 | Host star also known as KOI-4054,[141] potentially habitable exoplanet | |||||
Kepler-1702b | 0.143 | 18.5012 | transit | 2860±90 | Host star also known as KOI-4386[141] | |||||
HD 100939 b | 7.1±1.6 | 2574.9±86.1 | 3.73±0.08 | radial vel. | 400.4±1.9 | 1.04+0.07 −0.06 |
4769±55 | Red giant host star also known as HIP 56640[144][145] | ||
HD 136295 b | 1.79±0.16 | 926.4±12.8 | 2.02±0.02 | radial vel. | 269.0±1.3 | 1.28+0.11 −0.10 |
4891±50 | Red giant host star also known as HIP 75092[144] | ||
HD 170707 b | 1.96±0.09 | 453.9±2.0 | 1.26±0.01 | radial vel. | 307.6±1.2 | 1.30±0.08 | 4884±58 | Red giant host star also known as HIP 90988[144] | ||
HD 219553 b | 1.94±0.17 | 1481.6±61.7 | 2.84±0.08 | radial vel. | 332.9±1.7 | 1.39±0.09 | 4824±60 | Red giant host star also known as HIP 114933[144] | ||
Gliese 317 c | 2.13±0.19 | 6700 | radial vel. | 49.25±0.72 | 0.42±0.05 | 3510±50 | [146] |
Дивіться також
- Списки екзопланет
- Списки екзопланет за роком відкриття: до 2000, 2000-2009, 2010, 2011, 2012, 2013, 2014, 2015, 2016, 2017, 2018, 2019, 2020, 2021, 2022, 2023
Література
- ↑ exoplanet.eu Planet 2MASS J1155-7919 b
- ↑ www.sci-news.com Astronomers Discover Nearest-Known Newborn Gas Giant
- ↑ а б в г д е Haswell, Carole A. та ін. (2019). Dispersed Matter Planet Project discoveries of ablating planets orbiting nearby bright stars. Nature Astronomy. 4 (4): 408—418. arXiv:1912.10874. Bibcode:2020NatAs...4..408H. doi:10.1038/s41550-019-0973-y. S2CID 209444484.
- ↑ Jones, Mark H.; Haswell, Carole A.; Barnes, John R.; Staab, Daniel; Heller, René (2020). A possible transit of a disintegrating exoplanet in the nearby multiplanet system DMPP-1. The Astrophysical Journal. 895 (1): L17. arXiv:2005.07086. Bibcode:2020ApJ...895L..17J. doi:10.3847/2041-8213/ab8f2b. S2CID 218630238.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б в Hidalgo, D.; Pallé, E.; Alonso, R.; Gandolfi, D.; Fridlund, M.; Nowak, G.; Luque, R.; Hirano, T.; Justesen, A. B.; Cochran, W. D.; Barragán, O.; Spina, L.; Rodler, F.; Albrecht, S.; Anderson, D.; Amado, P.; Bryant, E.; Caballero, J. A.; Cabrera, J.; Csizmadia, Sz.; Dai, F.; De Leon, J.; Deeg, H. J.; Eigmuller, Ph.; Endl, M.; Erikson, A.; Esposito, M.; Figueira, P.; Georgieva, I. та ін. (2020), Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M⊕ super-Earth and two warm 14.7 and 10.2-M⊕ sub-Neptunes, Astronomy & Astrophysics, 636: A89, arXiv:2002.01755v1, Bibcode:2020A&A...636A..89H, doi:10.1051/0004-6361/201937080, S2CID 211032193
- ↑ exoplanet.eu Planet EPIC 249893012 d
- ↑ GJ 180 d
- ↑ GJ 229 A c
- ↑ Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. (2020). Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs. The Astrophysical Journal Supplement Series. 246 (1): 11. arXiv:2001.02577. Bibcode:2020ApJS..246...11F. doi:10.3847/1538-4365/ab5e7c. S2CID 210064560.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Barnes, J. R. та ін. (11 червня 2019). Frequency of planets orbiting M dwarfs in the Solar neighbourhood (англ.). arXiv:1906.04644 [astro-ph.EP].
- ↑ а б Stock, S. та ін. (2020), The CARMENES search for exoplanets around M dwarfs, Astronomy & Astrophysics, 643: A112, arXiv:2010.00474, Bibcode:2020A&A...643A.112S, doi:10.1051/0004-6361/202038820, S2CID 222090233
- ↑ www.sci-news.com Astronomers Discover Five New Planets around Nearby Red Dwarfs
- ↑ GJ 433 d
- ↑ GJ 1061 b
- ↑ GJ 1061 c
- ↑ GJ 1061 d
- ↑ GJ 1252 b
- ↑ Crossfield, Ian J. M.; Malik, Matej; Hill, Michelle L.; Kane, Stephen R.; Foley, Bradford; Polanski, Alex S.; Coria, David; Brande, Jonathan; Zhang, Yanzhe; Wienke, Katherine; Kreidberg, Laura; Cowan, Nicolas B.; Dragomir, Diana; Gorjian, Varoujan; Mikal-Evans, Thomas; Benneke, Björn; Christiansen, Jessie L.; Deming, Drake; Morales, Farisa Y. (2022), GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere, The Astrophysical Journal Letters, 937: L17, arXiv:2208.09479, doi:10.3847/2041-8213/ac886b, S2CID 251710304
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu Planet GJ 3082 b
- ↑ а б в г Hartman, J. D. та ін. (2020). HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs. The Astronomical Journal. 159 (4): 173. arXiv:2002.05776. Bibcode:2020AJ....159..173H. doi:10.3847/1538-3881/ab7821. S2CID 211126666.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu hats-48a b
- ↑ exoplanet.eu HD 80653 b
- ↑ а б в Nielsen, L. та ін. (2020). Three Short Period Jupiters from TESS. Astronomy & Astrophysics. 639: A76. arXiv:2003.05932. doi:10.1051/0004-6361/202037941. S2CID 212675311.
- ↑ exoplanet.eu HIP 65A b
- ↑ Wong, Ian та ін. (2020). Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission. The Astronomical Journal. 160 (4): 155. arXiv:2003.06407. Bibcode:2020AJ....160..155W. doi:10.3847/1538-3881/ababad. S2CID 212717799.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Iosup, Alexandru; Musaafir, Ahmed; Uta, Alexandru; Arnau Prat Pérez; Szárnyas, Gábor; Chafi, Hassan; Ilie Gabriel Tănase; Nai, Lifeng; Anderson, Michael; Capotă, Mihai; Sundaram, Narayanan; Boncz, Peter; Depner, Siegfried; Heldens, Stijn; Manhardt, Thomas; Hegeman, Tim; Wing Lung Ngai; Xia, Yinglong (2021), The Solar Neighborhood XLIX: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance, arXiv:2011.15028
- ↑ exoplanet.eu Planet KELT-2019-BLG-1953 b
- ↑ а б Han, Cheongho та ін. (2020). One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953. The Astronomical Journal. 160 (1): 17. arXiv:2002.05310. Bibcode:2020AJ....160...17H. doi:10.3847/1538-3881/ab91ac. S2CID 211096807.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu Planet KELT-2019-BLG-1953 c
- ↑ Kepler-1661 b
- ↑ Socia, Quentin J. та ін. (2020). Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary. The Astronomical Journal. 159 (3): 94. arXiv:2001.02840. Bibcode:2020AJ....159...94S. doi:10.3847/1538-3881/ab665b. S2CID 210116655.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu L 168-9 b
- ↑ Herrera-Martín, Antonio та ін. (2020). Ogle-2018-BLG-0677lb: A super earth near the galactic bulge. The Astronomical Journal. 159 (6): 256. arXiv:2003.02983. Bibcode:2020AJ....159..256H. doi:10.3847/1538-3881/ab893e. S2CID 212628627.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ TOI-132 b
- ↑ exoplanet.eu toi-257_b
- ↑ Addison, Brett C. та ін. (2021), TOI-257b (HD 19916b): A warm sub-saturn orbiting an evolved F-type star, Monthly Notices of the Royal Astronomical Society, 502 (3): 3704—3722, arXiv:2001.07345, doi:10.1093/mnras/staa3960
- ↑ Millholland, Sarah; Petigura, Erik; Batygin, Konstantin (2020), Tidal Inflation Reconciles Low-density Sub-Saturns with Core Accretion, The Astrophysical Journal, 897 (1): 7, arXiv:2005.11209, Bibcode:2020ApJ...897....7M, doi:10.3847/1538-4357/ab959c, S2CID 218863127
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б в Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet та ін. (2020). The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System. The Astronomical Journal. 160 (3): 116. arXiv:2001.00952. Bibcode:2020AJ....160..116G. doi:10.3847/1538-3881/aba4b2. S2CID 209862554.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Suissa, Gabrielle; Wolf, Eric T.; Ravi kumar Kopparapu; Villanueva, Geronimo L.; Fauchez, Thomas; Mandell, Avi M.; Arney, Giada; Gilbert, Emily A.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Lopez, Eric; Rodriguez, Joseph E.; Vanderburg, Andrew (2020). The First Habitable-zone Earth-sized Planet from TESS. III. Climate States and Characterization Prospects for TOI-700 D. The Astronomical Journal. 160 (3): 118. arXiv:2001.00955. Bibcode:2020AJ....160..118S. doi:10.3847/1538-3881/aba4b4. S2CID 209862275.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Cloutier, Ryan та ін. (2020). A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780. The Astronomical Journal. 160 (1): 3. arXiv:2003.01136. Bibcode:2020AJ....160....3C. doi:10.3847/1538-3881/ab91c2. S2CID 211817805.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Nowak, G. та ін. (2020). The CARMENES search for exoplanets around M dwarfs. Astronomy & Astrophysics. 642: A173. arXiv:2003.01140. doi:10.1051/0004-6361/202037867. S2CID 211818198.
- ↑ exoplanet.eu toi-813_b
- ↑ Kostov, Veselin B.; Orosz, Jerome A.; Feinstein, Adina D.; Welsh, William F.; Cukier, Wolf; Haghighipour, Nader; Quarles, Billy; Martin, David V.; Montet, Benjamin T.; Torres, Guillermo; Triaud, Amaury H. M. J.; Barclay, Thomas; Boyd, Patricia; Briceno, Cesar; Andrew Collier Cameron; Correia, Alexandre C. M.; Gilbert, Emily A.; Gill, Samuel; Gillon, Michael; Haqq-Misra, Jacob; Hellier, Coel; Dressing, Courtney; Fabrycky, Daniel C.; Furesz, Gabor; Jenkins, Jon; Kane, Stephen R.; Kopparapu, Ravi; Vedad Kunovac Hodzic; Latham, David W. та ін. (2020). TOI-1338: TESS' First Transiting Circumbinary Planet. The Astronomical Journal. 159 (6): 253. arXiv:2004.07783. Bibcode:2020AJ....159..253K. doi:10.3847/1538-3881/ab8a48. S2CID 215785933.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б в Badenas-Agusti, Mariona та ін. (2020). HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away. The Astronomical Journal. 160 (3): 113. arXiv:2002.03958. Bibcode:2020AJ....160..113B. doi:10.3847/1538-3881/aba0b5. S2CID 211069628.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Chinchilla, Patricia та ін. (2020). USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius. Astronomy & Astrophysics. 633: A152. arXiv:1912.04150. Bibcode:2020A&A...633A.152C. doi:10.1051/0004-6361/201936130. S2CID 208910589.
- ↑ Crouzet, Nicolas та ін. (2020). XO-7 b: A Transiting Hot Jupiter with a Massive Companion on a Wide Orbit. The Astronomical Journal. 159 (2): 44. arXiv:1912.02821. Bibcode:2020AJ....159...44C. doi:10.3847/1538-3881/ab5b12. S2CID 208857410.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Gan, Tianjun та ін. (2020). LHS 1815b: The First Thick-Disk Planet Detected by TESS. The Astronomical Journal. 159 (4): 160. arXiv:2003.04525. Bibcode:2020AJ....159..160G. doi:10.3847/1538-3881/ab775a. S2CID 212644667.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu LHS 1815 b
- ↑ Armstrong, David J. та ін. (2020). A remnant planetary core in the hot Neptunian desert. Nature. 583 (7814): 39—42. arXiv:2003.10314. Bibcode:2020Natur.583...39A. doi:10.1038/s41586-020-2421-7. PMID 32612222. S2CID 214612138.
- ↑ Díaz, Matías R. та ін. (2020). The Magellan/PFS Exoplanet Search: A 55-day period dense Neptune transiting the bright ($V=8.6$) star HD 95338. arXiv:2003.10319. doi:10.1093/mnras/staa1724. S2CID 214611611.
- ↑ Dalba, Paul A. та ін. (2020). The TESS-Keck Survey I: A Warm Sub-Saturn-Mass Planet and a Caution about Stray Light in TESS Cameras. The Astronomical Journal. 159 (5): 241. arXiv:2003.10451. Bibcode:2020AJ....159..241D. doi:10.3847/1538-3881/ab84e3. S2CID 214623340.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Sedaghati, Elyar; Sánchez-López, Alejando; Czesla, Stefan; López-Puertas, Manuel; Amado, Pedro; Palle, Enric; Molaverdikhani, Karan; Caballero, José; Nortmann, Lisa; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar (2022), Moderately misaligned orbit of the warm sub-Saturn HD 332231 B, Astronomy & Astrophysics, 659: A44, arXiv:2110.10282, doi:10.1051/0004-6361/202142471, S2CID 239049424
- ↑ а б Huang, Chelsea X. та ін. (2020). TESS Spots a Hot Jupiter with an Inner Transiting Neptune. The Astrophysical Journal. 892 (1): L7. arXiv:2003.10852. Bibcode:2020ApJ...892L...7H. doi:10.3847/2041-8213/ab7302. S2CID 214623301.
{{cite journal}}
: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ exoplanet.eu toi-1130 b
- ↑ exoplanet.eu toi-1130 c
- ↑ González-Álvarez, E.; Zapatero-Osorio, María Rosa; Caballero, J. A.; Sanz-Forcada, J.; Béjar, V. J. S.; González-Cuesta, L.; Dreizler, S.; Bauer, F. F.; Rodríguez, E.; Tal-Or, L.; Zechmeister, M.; Montes, D.; López-González, M. J.; Ribas, I.; Reiners, Ansgar; Quirrenbach, A.; Amado, P. J.; Anglada-Escudé, G.; Azzaro, M.; Cortés-Contreras, M.; Hatzes, A. P.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, Martin; Lafarga, M.; Morales, J. C.; Pallé, E.; Perger, M.; Schmitt, Jürgen H. M. M. (2020). The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B). Astronomy & Astrophysics. A93: 637. arXiv:2003.13052. Bibcode:2020A&A...637A..93G. doi:10.1051/0004-6361/201937050. S2CID 214714124.
- ↑ DiTomasso, Victoria та ін. (2022), Independent validation of the temperate Super-Earth HD79211 b using HARPS-N, arXiv:2210.12211
- ↑ а б Cooke, Benjamin F.; Pollacco, Don; Almleaky, Y.; Barkaoui, K.; Benkhaldoun, Z.; Blake, James A.; Bouchy, François; Boumis, Panos; Brown, D. J. A.; Bruni, Ivan; Burdanov, A.; Andrew Collier Cameron; Chote, Paul; Daassou, A.; D'ago, Giuseppe; Dalal, Shweta; Damasso, Mario; Delrez, L.; Doyle, A. P.; Ducrot, E.; Gillon, M.; Hébrard, G.; Hellier, C.; Henning, Thomas; Jehin, E.; Kiefer, Flavien; King, George W.; Liakos, Alexios; Lopez, Théo та ін. (2020). Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b. The Astronomical Journal. 159 (6): 255. arXiv:2004.06622. Bibcode:2020AJ....159..255C. doi:10.3847/1538-3881/ab88db. S2CID 215754471.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Cloutier, Ryan; Rodriguez, Joseph E.; Irwin, Jonathan; Charbonneau, David; Stassun, Keivan G.; Mortier, Annelies; Latham, David W.; Isaacson, Howard; Howard, Andrew W.; Udry, Stéphane; Wilson, Thomas G.; Watson, Christopher A.; Pinamonti, Matteo; Lienhard, Florian; Giacobbe, Paolo; Guerra, Pere; Collins, Karen A.; Beiryla, Allyson; Esquerdo, Gilbert A.; Matthews, Elisabeth; Crossfield, Ian J. M.; Winters, Jennifer G.; Nava, Chantanelle; Ment, Kristo; Lopez, Eric D.; Ricker, George; Vanderspek, Roland; Seager, Sara; Jenkins, Jon M. та ін. (2020). TOI-1235 b: A keystone super-Earth for testing radius valley emergence models around early M dwarfs. The Astronomical Journal. 160 (1): 22. arXiv:2004.06682. Bibcode:2020AJ....160...22C. doi:10.3847/1538-3881/ab9534. S2CID 215754432.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Hirao, Yuki; Bennett, David P.; Ryu, Yoon-Hyun; Koshimoto, Naoki; Udalski, Andrzej; Yee, Jennifer C.; Sumi, Takahiro; Bond, Ian A.; Shvartzvald, Yossi; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Donachie, Martin; Fukui, Akihiko; Itow, Yoshitaka; Kondo, Iona; Man Cheung Alex Li; Matsubara, Yutaka; Matsuo, Taro; Miyazaki, Shota; Muraki, Yasushi; Nagakane, Masayuki; Onishi, Kohji; Ranc, Clement; Rattenbury, Nicholas J.; Suematsu, Haruno; Shibai, Hiroshi; Sullivan, Denis J.; Suzuki, Daisuke та ін. (2020). OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet orbiting M-dwarf Host in the Inner Galactic Disk. The Astronomical Journal. 160 (2): 74. arXiv:2004.09067. doi:10.3847/1538-3881/ab9ac3. S2CID 215827466.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Carleo, Ilaria; Gandolfi, Davide; Barragán, Oscar; Livingston, John H.; Persson, Carina M.; Lam, Kristine W. F.; Vidotto, Aline; Lund, Michael B.; Carolina Villarreal D'Angelo; Collins, Karen A.; LucaFossati; Howard, Andrew W.; Kubyshkina, Daria; Brahm, Rafael; Oklopčić, Antonija; Mollière, Paul; Redfield, Seth; Luisa Maria Serrano; Dai, Fei; Fridlund, Malcolm; Borsa, Francesco; Korth, Judith; Esposito, Massimiliano; Díaz, Matías R.; Louise Dyregaard Nielsen; Hellier, Coel; Mathur, Savita; Deeg, Hans J.; Hatzes, Artie P. та ін. (2020). The Multiplanet System TOI-421. The Astronomical Journal. 160 (3): 114. arXiv:2004.10095. Bibcode:2020AJ....160..114C. doi:10.3847/1538-3881/aba124. S2CID 225478068.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б в г Daylan, Tansu; Pingle, Kartik; Wright, Jasmine; Guenther, Maximilian N.; Stassun, Keivan G.; Kane, Stephen R.; Vanderburg, Andrew; Jontof-Hutter, Daniel; Rodriguez, Joseph E.; Shporer, Avi; Huang, Chelsea; Mikal-Evans, Tom; Badenas-Agusti, Mariona; Collins, Karen A.; Rackham, Benjamin; Quinn, Sam; Cloutier, Ryan; Collins, Kevin I.; Guerra, Pere; Jensen, Eric L. N.; Kielkopf, John F.; Massey, Bob; Schwarz, Richard P.; Charbonneau, David; Lissauer, Jack J.; Irwin, Jonathan M.; Basturk, Ozgur; Fulton, Benjamin; Soubkiou, Abderahmane та ін. (2021). TESS Discovery of a Super-Earth and Three Sub-Neptunes Hosted by the Bright, Sun-like Star HD 108236. The Astronomical Journal. 161 (2): 85. arXiv:2004.11314. Bibcode:2021AJ....161...85D. doi:10.3847/1538-3881/abd73e. S2CID 216080635.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Hebrard, G.; Diaz, R. F.; Correia, A. C. M.; Collier Cameron, A.; Laskar, J.; Pollacco, D.; Almenara, J. -M.; Anderson, D. R.; Barros, S. C. C.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Boue, G.; Boumis, P.; Brown, D. J. A.; Dalal, S.; Deleuil, M.; Demangeon, O.; Doyle, A. P.; Haswell, C. A.; Hellier, C.; Osborn, H.; Kiefer, F.; Kolb, U. C.; Lam, K.; Lecavelier des Etangs, A.; Lopez, T.; Martin-Lagarde, M.; Maxted, P. та ін. (2020). Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets. Astronomy & Astrophysics. A32: 640. arXiv:2004.14645. Bibcode:2020A&A...640A..32H. doi:10.1051/0004-6361/202038296. S2CID 216867348.
- ↑ а б Maciejewski, G.; Fernández, M.; Sota, A.; Garcìa Segura, A.J. (2020), A Newtonian Model for the WASP-148 Exoplanetary System Enhanced with TESS and Ground-based Photometric Observations, Acta Astronomica, 70 (3): 203, arXiv:2012.02602, Bibcode:2020AcA....70..203M, doi:10.32023/0001-5237/70.3.3, S2CID 227305904
- ↑ Gill, Samuel; Wheatley, Peter J.; Cooke, Benjamin F.; Jordán, Andrés; Nielsen, Louise D.; Bayliss, Daniel; Anderson, David R.; Vines, Jose I.; Lendl, Monika; Acton, Jack S.; Armstrong, David J.; Bouchy, François; Brahm, Rafael; Bryant, Edward M.; Burleigh, Matthew R.; Casewell, Sarah L.; Eigmüller, Philipp; Espinoza, Néstor; Gillen, Edward; Goad, Michael R.; Grieves, Nolan; Günther, Maximilian N.; Henning, Thomas; Hobson, Melissa J.; Hogan, Aleisha; Jenkins, James S.; McCormac, James; Moyano, Maximiliano; Osborn, Hugh P. та ін. (2020). NGTS-11 b / TIC-54002556 b: A transiting warm Saturn recovered from a TESS single-transit event. arXiv:2005.00006. doi:10.3847/2041-8213/ab9eb9. S2CID 220845943.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Rizzuto, Aaron C.; Newton, Elisabeth R.; Mann, Andrew W.; Tofflemire, Benjamin M.; Vanderburg, Andrew; Kraus, Adam L.; Wood, Mackenna L.; Quinn, Samuel N.; Zhou, George; Pa Chia Thao; Law, Nicholas M.; Ziegler, Carl; Briceno, Cesar (2020). TESS Hunt for Young and Maturing Exoplanets (THYME) II: A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association. The Astronomical Journal. 160 (1): 33. arXiv:2005.00013. Bibcode:2020AJ....160...33R. doi:10.3847/1538-3881/ab94b7. S2CID 218470215.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Mann, Andrew W.; Johnson, Marshall C.; Vanderburg, Andrew; Kraus, Adam L.; Rizzuto, Aaron C.; Wood, Mackenna L.; Bush, Jonathan L.; Rockcliffe, Keighley; Newton, Elisabeth R.; Latham, David W.; Mamajek, Eric E.; Zhou, George; Quinn, Samuel N.; Pa Chia Thao; Benatti, Serena; Cosentino, Rosario; Desidera, Silvano; Harutyunyan, Avet; Lovis, Christophe; Mortier, Annelies; Pepe, Francesco A.; Poretti, Ennio; Wilson, Thomas G.; Kristiansen, Martti H.; Gagliano, Robert; Jacobs, Thomas; LaCourse, Daryll M.; Omohundro, Mark; Hans Martin Schwengeler та ін. (2020). TESS Hunt for Young and Maturing Exoplanets (THYME). III. A Two-planet System in the 400 Myr Ursa Major Group. The Astronomical Journal. 160 (4): 179. arXiv:2005.00047. Bibcode:2020AJ....160..179M. doi:10.3847/1538-3881/abae64. S2CID 218470494.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Dai, Fei та ін. (2020), The TESS-Keck Survey. III. A Stellar Obliquity Measurement of TOI-1726 C, The Astronomical Journal, 160 (4): 193, arXiv:2008.12397, Bibcode:2020AJ....160..193D, doi:10.3847/1538-3881/abb3bd, S2CID 221370690
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Benatti, S.; Damasso, M.; Desidera, S.; Marzari, F.; Biazzo, K.; Claudi, R.; Di Mauro, M. P.; Lanza, A. F.; Pinamonti, M.; Barbato, D.; Malavolta, L.; Poretti, E.; Sozzetti, A.; Affer, L.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Brogi, M.; Bruno, G.; Carleo, I.; Cosentino, R.; Covino, E.; Frustagli, G.; Giacobbe, P.; Gonzalez, M.; Gratton, R.; Harutyunyan, A.; Knapic, C.; Leto, G. та ін. (2020). The GAPS Programme at TNG -- XXIII. HD 164922 d: A close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion. Astronomy & Astrophysics. A50: 639. arXiv:2005.03368. Bibcode:2020A&A...639A..50B. doi:10.1051/0004-6361/202037939. S2CID 218538033.
- ↑ Bennett, David P.; Udalski, Andrzej; Bond, Ian A.; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Donachie, Martin; Fujii, Hirosane; Fukui, Akihiko; Hirao, Yuki; Itow, Yoshitaka; Kawasaki, Kohei; Kirikawa, Rintaro; Kondo, Iona; Koshimoto, Naoki; Man Cheung Alex Li; Matsubara, Yutaka; Miyazaki, Shota; Muraki, Yasushi; Ranc, Clément; Rattenbury, Nicholas J.; Satoh, Yuki; Shoji, Hikaru; Sumi, Takahiro; Suzuki, Daisuke; Tanaka, Yuzuru; Tristram, Paul J.; Yamawaki, Tsubasa; Yonehara, Atsunori та ін. (2020). A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System. The Astronomical Journal. 160 (2): 72. arXiv:2005.07199. Bibcode:2020AJ....160...72B. doi:10.3847/1538-3881/ab9cb9. S2CID 218665248.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Obermeier, C.; Steuer, J.; Kellermann, H.; Saglia, R. P.; Henning, Th.; Riffeser, A.; Hopp, U.; Stefansson, G.; Cañas, C.; Ninan, J.; Mahadevan, S.; Isaacson, H.; Howard, A. W.; Livingston, J.; Koppenhoefer, J.; Bender, R. (2020). Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2b. Astronomy & Astrophysics. 639: A130. arXiv:2005.13560. Bibcode:2020A&A...639A.130O. doi:10.1051/0004-6361/202037715. S2CID 218971735.
- ↑ Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve (2020). Transit least-squares survey. Astronomy & Astrophysics. 638: A10. arXiv:2006.02123. doi:10.1051/0004-6361/201936929. S2CID 219260293.
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Stefansson, Gudmundur; Kopparapu, Ravi; Lin, Andrea; Mahadevan, Suvrath; Cañas, Caleb; Kanodia, Shubham; Ninan, Joe; Cochran, William; Endl, Michael; Hebb, Leslie; Wisniewski, John; Gupta, Arvind; Everett, Mark; Bender, Chad; Diddams, Scott; Ford, Eric; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Levi, Eric; Maney, Marissa; Metcalf, Andrew; Monson, Andrew; Ramsey, Lawrence; Robertson, Paul; Roy, Arpita; Schwab, Christian; Terrien, Ryan; Wright, Jason (2020), A Mini-Neptune and a Venus-Zone Planet in the Radius Valley Orbiting the Nearby M2-dwarf TOI-1266: Validation with the Habitable-zone Planet Finder, arXiv:2006.11180
- ↑ Harman, C. E.; Ravi Kumar Kopparapu; Stefánsson, Guðmundur; Lin, Andrea S. J.; Mahadevan, Suvrath; Hedges, Christina; Batalha, Natasha E. (2021), A Snowball in Hell: The Potential Steam Atmosphere of TOI-1266c, arXiv:2109.10838
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ EXOPLANET CATALOG AU Microscopii b on exoplanets.nasa.gov
- ↑ Kanodia, Shubham; Cañas, Caleb I.; Stefansson, Gudmundur; Ninan, Joe P.; Hebb, Leslie; Lin, Andrea S. J.; Baran, Helen; Maney, Marissa; Terrien, Ryan C.; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Dong, Jiayin; Bender, Chad F.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Metcalf, Andrew J.; Monson, Andrew; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Wright, Jason T. (2020), TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host, The Astrophysical Journal, 899 (1): 29, arXiv:2006.14546, Bibcode:2020ApJ...899...29K, doi:10.3847/1538-4357/aba0a2, S2CID 220056014
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Barbato, D.; Pinamonti, M.; Sozzetti, A.; Biazzo, K.; Benatti, S.; Damasso, M.; Desidera, S.; Lanza, A. F.; Maldonado, J.; Mancini, L.; Scandariato, G.; Affer, L.; Andreuzzi, G.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Carleo, I.; Claudi, R.; Cosentino, R.; Covino, E.; Fiorenzano, A. F. M.; Giacobbe, P.; Harutyunyan, A.; Knapic, C.; Leto, G.; Lorenzi, V.; Maggio, A.; Malavolta, L.; Micela, G. та ін. (2020), The GAPS programme at TNG, Astronomy & Astrophysics, 641: A68, arXiv:2006.14393, doi:10.1051/0004-6361/202037954, S2CID 220055727
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б Jeffers, S. V.; Dreizler, S.; Barnes, J. R.; Haswell, C. A.; Nelson, R. P.; Rodríguez, E.; López-González, M. J.; Morales, N.; Luque, R. та ін. (2020), A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887, Science, 368 (6498): 1477—1481, arXiv:2006.16372, Bibcode:2020Sci...368.1477J, doi:10.1126/science.aaz0795, PMID 32587019, S2CID 220075207
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Cañas, Caleb I.; Stefansson, Gudmundur; Kanodia, Shubham; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Robertson, Paul; Bender, Chad F.; Ninan, Joe P.; Beard, Corey; Lubin, Jack; Gupta, Arvind F.; Everett, Mark E.; Monson, Andrew; Wilson, Robert F.; Lewis, Hannah M.; Brewer, Mary; Majewski, Steven R.; Hebb, Leslie; Dawson, Rebekah I.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Lin, Andrea S. J.; Metcalf, Andrew J.; Rajagopal, Jayadev; Ramsey, Lawrence W. та ін. (2020), A Warm Jupiter Transiting an M Dwarf: A TESS Single-transit Event Confirmed with the Habitable-zone Planet Finder, The Astronomical Journal, 160 (3): 147, arXiv:2007.07098, Bibcode:2020AJ....160..147C, doi:10.3847/1538-3881/abac67, S2CID 220514735
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ The unusual M-dwarf Warm Jupiter TOI-1899 b: Refinement of orbital and planetary parameters, 2023, arXiv:2301.10837
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Bohn, Alexander J.; Kenworthy, Matthew A.; Ginski, Christian; Rieder, Steven; Mamajek, Eric E.; Meshkat, Tiffany; Pecaut, Mark J.; Reggiani, Maddalena; De Boer, Jozua; Keller, Christoph U.; Snik, Frans; Southworth, John (2020), Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1, The Astrophysical Journal, 898 (1): L16, arXiv:2007.10991, Bibcode:2020ApJ...898L..16B, doi:10.3847/2041-8213/aba27e, S2CID 220686536
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Teske, Johanna; Díaz, Matías R.; Luque, Rafael; Močnik, Teo; Seidel, Julia V.; Otegi, Jon Fernández; Feng, Fabo; Jenkins, James S.; Pallè, Enric; Ségransan, Damien; Udry, Stèphane; Collins, Karen A.; Eastman, Jason D.; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Anderson, David. R.; Barclay, Thomas; Bouchy, François; Burt, Jennifer A.; Butler, R. Paul; Caldwell, Douglas A.; Collins, Kevin I.; Crane, Jeffrey D.; Dorn, Caroline; Flowers, Erin та ін. (2020), TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet, The Astronomical Journal, 160 (2): 96, arXiv:2007.13927, Bibcode:2020AJ....160...96T, doi:10.3847/1538-3881/ab9f95, S2CID 220830943
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ а б в г д е ж и Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R. (2020), Search for Nearby Earth Analogs .III. Detection of 10 New Planets, 3 Planet Candidates, and Confirmation of 3 Planets around 11 Nearby M Dwarfs, The Astrophysical Journal Supplement Series, 250 (2): 29, arXiv:2008.07998, Bibcode:2020ApJS..250...29F, doi:10.3847/1538-4365/abb139, S2CID 221150644
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Burt, Jennifer A. та ін. (2020), TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert, The Astronomical Journal, 160 (4): 153, arXiv:2008.11732, Bibcode:2020AJ....160..153B, doi:10.3847/1538-3881/abac0c, S2CID 221340866
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Is the hot, dense sub-Neptune TOI-824 b an exposed Neptune mantle? Spitzer detection of the hot day side and reanalysis of the interior composition, 2022, arXiv:2211.11793
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- ↑ Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo; Ogihara, Masahiro; Oppenheimer, Rebecca; o'Toole, S. J.; Shectman, Stephen A.; Wittenmyer, Robert A.; Wang, Sharon X.; Wright, D. J.; Xuan, Yifan (2022), 3D Selection of 167 Substellar Companions to Nearby Stars, The Astrophysical Journal Supplement Series, 262 (1): 21, arXiv:2208.12720, Bibcode:2022ApJS..262...21F, doi:10.3847/1538-4365/ac7e57, S2CID 251864022
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання) - ↑ Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Wang, Sharon Xuesong; Thompson, Ian B.; Díaz, Matías R.; Butler, R. Paul (2020), Search for Nearby Earth Analogs .III. Detection of 10 New Planets, 3 Planet Candidates, and Confirmation of 3 Planets around 11 Nearby M Dwarfs, The Astrophysical Journal Supplement Series, 250 (2): 29, arXiv:2008.07998, Bibcode:2020ApJS..250...29F, doi:10.3847/1538-4365/abb139, S2CID 221150644
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: Обслуговування CS1: Сторінки із непозначеним DOI з безкоштовним доступом (посилання)