2020年發現的系外行星列表
维基媒体列表条目
僅由徑向速度發現的太陽系外行星，下列表格記載的質量為其下限。
| 名稱 | 質量（MJ） | 半徑（RJ） | 軌道周期（天） | 半長軸（AU） | 溫度（K）[3] | 發現方式 | 距離（ly） | 主星質量（M☉） | 主星溫度（K） | 注釋 |
|---|---|---|---|---|---|---|---|---|---|---|
| 2MASS J1155-7919 b | 10 | 582 | 影像 | 330 | [4]年輕的超級木星，軌道寬廣[5] | |||||
| HD 38677 b | 18.57+0.01 − |
0.1462+0.0012 − |
877 | 徑向速度 | 202.2169+3.261564 − |
1.21+0.03 − |
6196+29 − |
由DMPP（Dispersed Matter Planet Project）發現[6] | ||
| HD 38677 c | 6.584+0.003 −0.002 |
0.0733+0.0006 −0.0007 |
1239 | 徑向速度 | 202.2169+3.261564 − |
1.21+0.03 − |
6196+29 − |
由DMPP發現[6]，與另一顆未確認行有2:1的軌道共振[7] | ||
| HD 38677 d | 2.882+0.001 − |
0.0422+0.0004 −0.0003 |
1632 | 徑向速度 | 202.2169+3.261564 − |
1.21+0.03 − |
6196+29 − |
由DMPP發現[6] | ||
| HD 38677 e | 5.516+0.002 −0.004 |
0.0651+0.0005 − |
1314 | 徑向速度 | 202.2169+3.261564 − |
1.21+0.03 − |
6196+29 − |
由DMPP發現[6] | ||
| HD 11231 b | 0.426+0.038 −0.052 |
5.2072+0.0002 −0.0055 |
0.0664+0.0005 − |
1000 | 徑向速度 | 437.0495+13.04625 − |
1.44+0.03 − |
6500+100 − |
由DMPP發現[6] | |
| HD 42936 Ab | 2.58+0.35 −0.58 |
6.6732+0.0011 −0.0003 |
0.0662+0.0013 − |
854 | 徑向速度 | 159.4905+1.956938 − |
0.87+0.05 − |
5138+99 − |
由DMPP發現[6] | |
| EPIC 249893012 b | 0.02753+0.00343 − |
0.174+0.008 − |
3.5951+0.0003 − |
0.047+0.005 −0.007 |
1616+150 −80 |
凌日 | 1059.03+13.69857 − |
1.05+0.05 − |
5430+85 − |
[8] |
| EPIC 249893012 c | 0.04616+0.00595 − |
0.3274+0.0152 −0.0125 |
15.624+0.001 − |
0.13+0.01 −0.02 |
990+68 −29 |
凌日 | 1059.03+13.69857 − |
1.05+0.05 − |
5430+85 − |
[8] |
| EPIC 249893012 d | 0.03203+0.00774 −0.00761 |
0.3515+0.0116 − |
35.747+0.005 − |
0.22+0.02 −0.04 |
752+69 −37 |
凌日 | 1059.03+13.69857 − |
1.05+0.05 − |
5430+85 − |
[8][9] |
| G 9-40 b | 0.1807 | 5.746007 | 0.0385 | 456 | 凌日 | 91.1 | 0.290 | 3348 | [10] | |
| Gliese 180 d | 7.56+1.07 − |
106.341+0.261 −0.34 |
0.31+0.024 −0.029 |
徑向速度 | 39.96+0.01 − |
0.43 | 3371 | [11] | ||
| Gliese 229 Ac | 0.025 | 122.005+0.364 −0.382 |
0.339+0.024 −0.029 |
徑向速度 | 18.78+0.004 − |
0.58 | 3564 | [12][13] | ||
| Gliese 251 b | >0.013 | 14.238 | 0.0818 | 351 | 徑向速度 | 18.205+0.006 − |
0.360+0.015 − |
3451+51 − |
2019年被否認，2020年被重新確認[14][15] | |
| Gliese 433 d | 0.019 | 36.052+0.045 −0.031 |
0.178+0.013 −0.015 |
徑向速度 | 29.57+0.01 − |
0.48 | 3600 | [16][17] | ||
| Gliese 1061 b | 0.00431+0.00050 −0.00047 |
3.204+0.001 − |
0.021+0.001 − |
徑向速度 | 11.98+0.003 − |
0.12+0.01 − |
2953+98 − |
[18] | ||
| Gliese 1061 c | 0.00547+0.00072 − |
6.689+0.005 − |
0.035+0.001 − |
徑向速度 | 11.98+0.003 − |
0.12+0.01 − |
2953+98 − |
[19] | ||
| Gliese 1061 d | 0.00516+0.00076 −0.00072 |
13.031+0.025 −0.032 |
0.054+0.001 − |
徑向速度 | 11.98+0.003 − |
0.12+0.01 − |
2953+98 − |
[20] | ||
| Gliese 1252 b | 0.00658+0.00176 − |
0.1064+0.0066 − |
0.5182349+0.0000063 −0.0000050 |
0.00916+0.00076 − |
1089+69 − |
凌日 | 66.49+0.06 − |
0.381+0.019 − |
3458+140 −133 |
[21] |
| GJ 3082 b | 0.02759+0.011 −0.01334 |
11.949+0.022 − |
0.079+0.006 −0.007 |
徑向速度 | 54.2 | 0.47 | [22] | |||
| HATS-47b | 0.369 | 1.117 | 3.9228 | 852.9 | 凌日 | 984.01+6.20 − |
0.674 | [23] | ||
| HATS-48Ab | 0.243 | 0.800 | 3.1317 | 0.03769+0.00011 − |
954.6 | 凌日 | 865 | 0.7279 | 4546.0+23 −18 |
[23][24] |
| HATS-49b | 0.353 | 0.765 | 4.1480 | 834.8 | 凌日 | 1058.70+7.18 − |
0.7133 | [23] | ||
| HATS-72b | 0.1254 | 0.7224 | 7.3279 | 739.3 | 凌日 | 416.37+1.70 − |
0.7311 | [23] | ||
| HD 80653 b | 0.0176+0.0014 − |
0.1439+0.0063 − |
0.719573+0.000021 − |
0.0166+0.0003 − |
凌日 | 358.1197+2.641867 − |
1.18+0.04 − |
[25] | ||
| HIP 65 Ab | 3.213+0.078 − |
2.03+0.61 −0.49 |
0.9809761+0.000037 −0.000034 |
0.01782+0.00021 − |
1411+15 − |
凌日 | 201.85818+0.2609251 − |
0.781+0.027 − |
4590+49 − |
周期很短，圍繞明亮的K4型星（V=11.1 mag）運動[26][27][28] |
| KELT-2019-BLG-1953 b | 0.59+0.71 −0.32 |
0.8+0.9 −0.6 |
微重力透鏡 | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[29][30] | ||||
| KELT-2019-BLG-1953 c | 0.28+0.35 −0.15 |
0.8+0.9 −0.7 |
微重力透鏡 | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[31][30] | ||||
| 克卜勒-1661(AB) b | 0.053+0.038 − |
0.345+0.005 − |
175.06+0.06 − |
0.633+0.005 − |
243 | 凌日 | 1355.26+9.56 − |
0.841+0.022 − |
5100+100 − |
[32][33] |
| L 168-9b | 0.0145+0.00176 − |
0.124+0.008 − |
1.4015+0.00018 − |
0.02091+0.00024 − |
816+160 − |
凌日 | 82.02833+0.07827753 − |
0.62+0.03 − |
3800+70 − |
[34] |
| OGLE-2018-BLG-0677Lb | 0.0125+0.0185 −0.0084 |
0.68+0.27 −0.22 |
微重力透鏡 | 27000+3500 − |
0.12+0.14 −0.08 |
在銀河系核球[35] | ||||
| 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 |
凌日 | 536.43+89.11 − |
0.970+0.06 − |
5397+46 − |
[36] |
| TOI-257 b | 0.134+0.023 − |
0.626+0.013 − |
18.38827+0.00072 − |
0.1523+0.0017 − |
1033+19 − |
凌日 | 251.37+0.065 − |
1.38+0.056 −0.009 |
6075+90 − |
主星又名HD 19916[37][38][39] |
| 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 |
凌日 | 101.5 | 0.416+0.01 − |
3480+135 − |
[40] | |
| 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 |
凌日 | 101.5 | 0.416+0.01 − |
3480+135 − |
[40] | |
| 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 − |
凌日 | 101.5 | 0.416+0.01 − |
3480+135 − |
TESS發現的第一個地球大小的系外行星[40][41] |
| TOI-732 b | 0.098 | 0.119 | 0.7683881 | 0.012 | 892 | 凌日 | 72 | 0.379 | 3360 | 圍繞雙星系統LDS 3977的主星運動[42][43] |
| TOI-732 c | 0.027 | 0.205 | 12.25 | 0.07673 | 323 | 凌日 | 72 | 0.379 | 3360 | 圍繞雙星系統LDS 3977的主星運動[42][43] |
| TOI-813 b | 0.599+0.034 − |
83.8911+0.0027 −0.0031 |
0.423+0.031 −0.037 |
610+28 −21 |
凌日 | 864.8192+5.156379 − |
1.32+0.06 − |
5907+150 − |
[44] | |
| TOI-1338 b | 0.1038 | 0.611 | 95.2 | 0.4607 | 724 | 凌日 | 1301 | TESS發現的第一個環聯星運轉行星[45][46] | ||
| HD 191939 b | 0.301 | 8.880411 | 0.089 | 778+58 −41 |
凌日 | 175 | 0.92 | 5400 | 主星又名TOI-1339[47] | |
| HD 191939 c | 0.287 | 28.58060 | 0.178 | 550+45 − |
凌日 | 175 | 0.92 | 5400 | 主星又名TOI-1339[47] | |
| HD 191939 d | 0.282 | 38.3561 | 0.216 | 499+12 −11 |
凌日 | 175 | 0.92 | 5400 | 主星又名TOI-1339[47] | |
| USco1621 b | 16 | 2880 | 2270 | 影像 | 450 | 0.36 | 3460 | [48] | ||
| USco1556 b | 15 | 3500 | 2240 | 影像 | 459 | 0.33 | 3410 | [48] | ||
| XO-7b | 0.709 | 1.373 | 2.8641424 | 0.04421 | 1743 | 凌日 | 763 | 1.405 | 6250 | [49] |
| LHS 1815 b | 0.0132+0.0047 − |
0.0971+0.005 − |
3.81433+0.00003 − |
0.0404+0.0094 − |
617+84 − |
凌日 | 97 | 0.502 | 3643+142 − |
[50][51] |
| TOI-157 b | 1.18+0.13 − |
1.29+0.02 − |
2.0845435+0.0000023 − |
0.03138+0.00025 −0.00020 |
1588+21 −20 |
凌日 | 1171 | 0.948+0.023 −0.018 |
5404+70 −67 |
[26] |
| TOI-169 b | 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 |
凌日 | 1345 | 1.147+0.069 −0.075 |
5880+54 −49 |
[26] |
| TOI-849 b | 0.128+0.008 − |
0.308+0.014 −0.011 |
0.7655240+0.0000027 − |
0.01598+0.00013 − |
1800 | 凌日 | 735 | 0.929+0.023 − |
5329+48 − |
海王星沙漠行星[52] |
| 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 |
凌日 | 120 | 0.76+0.16 −0.1 |
5212+16 −11 |
[53] |
| HD 332231 b | 0.244+0.021 − |
0.867+0.027 −0.025 |
18.71204+0.00043 − |
0.1436+0.0032 −0.0033 |
876+17 − |
凌日 | 262 | 1.127+0.077 − |
6089+97 −96 |
TOI 1456[54] |
| TOI-1130 b | 0.3256+0.009 − |
4.066499+0.000046 − |
0.04394+0.00035 −0.00038 |
876+17 − |
凌日 | 190 | 0.684+0.16 −0.17 |
4250+67 − |
[55][56] | |
| 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 − |
凌日 | 190 | 0.684+0.16 −0.17 |
4250+67 − |
[55][57] |
| HD 79211 b | 0.032+0.005 − |
24.45+0.02 − |
0.141+0.005 − |
345 | 徑向速度 | 20.658+0.005 − |
0.64+0.07 − |
4005+51 − |
圍繞雙星系統 ADS 7251的主星運動[58] | |
| 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 − |
凌日 | 2422 | 1.394+0.07 −0.049 |
6218+49 −45 |
[59] |
| 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 |
凌日 | 1883 | 1.345+0.08 −0.13 |
5941+77 −79 |
[59] |
| 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 − |
凌日 | 129 | 0.640+0.016 − |
3872+70 − |
該系統中可能還有多於一個的行星[60] |
| OGLE-2017-BLG-0406 b | 0.41+0.05 − |
3.5+0.3 − |
微重力透鏡 | 17000+1600 − |
0.56+0.07 − |
4848 | 有高精度微重力透鏡事件[61] | |||
| 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 − |
凌日 | 244.3+1.9 − |
0.852+0.029 −0.021 |
5325+78 −58 |
星系中有一顆紅矮星，距離主星2200天文單位[62] |
| 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 |
凌日 | 244.3+1.9 − |
0.852+0.029 −0.021 |
5325+78 −58 |
星系中有一顆紅矮星，距離主星2200天文單位[62] |
| HD108236 b | 0.1415+0.0087 − |
3.79523+0.00047 −0.00044 |
0.0469+0.0017 − |
1099+19 −18 |
凌日 | 211 | 0.97 | 5730+50 − |
[63] | |
| HD108236 c | 0.1845+0.0089 −0.0081 |
6.2037+0.00064 −0.00052 |
0.0651+0.0024 − |
932+17 −16 |
凌日 | 211 | 0.97 | 5730+50 − |
[63] | |
| HD108236 d | 0.2423+0.0097 − |
14.1756+0.001 −0.0011 |
0.1131+0.004 − |
708+13 −12 |
凌日 | 211 | 0.97 | 5730+50 − |
[63] | |
| HD108236 e | 0.279+0.012 −0.011 |
19.592+0.002 − |
0.14+0.0052 − |
636+12 −11 |
凌日 | 211 | 0.97 | 5730+50 − |
[63] | |
| WASP-148 b | 0.291+0.025 − |
0.722+0.055 − |
8.80381+0.000043 − |
0.22+0.063 − |
940+80 − |
凌日 | 809+5 − |
1.00+0.08 − |
5460+130 − |
[64][65] |
| WASP-148 c | 0.397+0.203 −0.044 |
34.515+0.029 − |
0.359+0.086 − |
590+50 − |
徑向速度 | 809+5 − |
1.00+0.08 − |
5460+130 − |
[64][65] | |
| NGTS-11 b | 0.37+0.14 − |
0.823+0.035 − |
35.4553+0.0002 − |
0.201+0.002 − |
440+40 − |
凌日 | 624+6 − |
0.862+0.028 − |
5050+80 − |
[66] |
| HIP 67522 b | 0.25 | 0.894+0.048 −0.047 |
6.9596+0.000016 −0.000015 |
1174+21 − |
凌日 | 416+4 − |
1.22+0.05 − |
5675+75 − |
可能是行星。非常年輕，形成不超過2000萬年[67] | |
| HD 63433 b | 0.017 | +0.009 − |
7.10801+0.00046 −0.00034 |
0.0710+0.0033 −0.0041 |
凌日 | 73.08+0.07 − |
0.99+0.03 − |
5640+74 − |
[68] | |
| HD 63433 c | 0.023 | 0.238+0.01 − |
20.5455+0.001 − |
0.1531+0.0074 −0.0092 |
凌日 | 73.08+0.07 − |
0.99+0.03 − |
5640+74 − |
[68][69] | |
| HD 164922 d | 0.013+0.003 − |
12.458+0.003 − |
0.103+0.003 − |
徑向速度 | 72.1+0.9 − |
0.874+0.012 − |
5293+32 − |
[70] | ||
| OGLE-2006-BLG-284 b | 0.45+0.14 −0.40 |
2.2+0.8 − |
微重力透鏡 | 13000+4900 − |
0.35+0.3 −0.2 |
軌道不確定[71] | ||||
| 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 |
凌日 | 1004+10 − |
0.65+0.1 − |
3984+152 −46 |
[72] |
| Wendelstein-2b | 0.731+0.541 −0.311 |
1.1592+0.0061 − |
1.7522239+0.0000008 − |
0.0234+0.0015 − |
1852+120 −140 |
凌日 | 1875+20 − |
0.73+0.11 − |
4288+133 −111 |
有氣體包層[72] |
| 克卜勒-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 |
凌日 | 3140+60 − |
0.88 | 5471+115 −37 |
[73] | |
| K2-315b | 0.085+0.005 − |
3.1443189+0.0000049 − |
0.0234 | 460+5 − |
凌日 | 185+1 − |
0.174+0.004 − |
3300+30 − |
因其軌道周期長度，又名Pi Eeath或EPIC 249631677b[74] | |
| TOI-1266 b | 0.2193+0.074 −0.066 |
10.894879+0.00007 −0.00007 |
0.0745+0.0046 −0.0069 |
410+21 −15 |
凌日 | 117.4+1.0 − |
0.437+0.021 − |
3563+77 − |
[75] | |
| 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 |
凌日 | 117.4+1.0 − |
0.437+0.021 − |
3563+77 − |
[75] | |
| AU Microscopii b | 0.18 | 0.375 | 8.46321+0.00004 − |
0.066 | 凌日 | 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 − |
凌日 | 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 − |
徑向速度 | 88.63+0.11 − |
0.651+0.031 −0.029 |
4550+110 − |
處在宜居帶內，軌道高度偏心[80] | ||
| OGLE-2018-BLG-1269Lb | 0.69+0.44 −0.22 |
4383 | 4.61+1.70 −1.17 |
微重力透鏡 | 8300+3000 −2000 |
0.35+0.3 −0.2 |
[81] | |||
| Lacaille 9352 b | 0.0132+0.0019 − |
9.262+0.001 − |
0.068+0.002 − |
468 | 徑向速度 | 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 | 徑向速度 | 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 − |
凌日 | 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 − |
凌日 | 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 − |
凌日 | 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 − |
凌日 | 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 − |
凌日 | 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 − |
凌日 | 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 |
凌日 | 2135+20 − |
1.298+0.021 − |
6457+55 −36 |
[83] |
| TOI-1899 b | 0.66+0.07 − |
1.37+0.05 −0.06 |
29.02+0.36 −0.23 |
0.1587+0.067 −0.075 |
362+7 − |
凌日 | 419+1 − |
0.627+0.026 −0.028 |
3841+54 −45 |
[84] |
| HATS-37A b | 0.099+0.042 − |
0.606+0.016 − |
4.3315 | 0.1587+0.067 −0.075 |
1085+16 −12 |
凌日 | 695 | 0.843+0.017 −0.012 |
5247+50 − |
星系中還有一個紅矮星[85] |
| HATS-38 b | 0.074+0.011 − |
0.614+0.0176 − |
4.3750 | 0.1587+0.067 −0.075 |
1294+10 − |
凌日 | 1131 | 0.890+0.016 −0.012 |
5740+50 − |
[85] |
| TYC 8998-760-1 c | 6+1 − |
1.1+0.6 −0.3 |
320 | 1240+160 −170 |
影像 | 309.4+0.9 − |
4783 | [86] | ||
| HD 86226 c | 0.023+0.004 − |
0.193+0.007 − |
3.98442+0.00018 − |
0.049+0.001 − |
1311+28 − |
凌日 | 149 | 1.019+0.061 −0.066 |
5863+88 − |
[87] |
| Gliese 2056 b | 0.444+0.053 − |
69.971+0.061 − |
0.283+0.0013 − |
徑向速度 | 92.8 | 0.62+0.08 − |
處於宜居帶內[88] | |||
| Gliese 480 b | 0.042+0.005 − |
9.567+0.005 − |
0.068+0.001 − |
徑向速度 | 46.4 | 0.45+0.02 − |
[88] | |||
| Gliese 687 c | 0.050+0.013 − |
728+12 − |
1.165+0.023 − |
徑向速度 | 14.83 | 0.40+0.02 − |
該系統中發現的第二個海王星大小行星[88] | |||
| HIP 107772 b | 0.049+0.014 −0.030 |
55.259+0.111 −0.311 |
0.243+0.022 −0.027 |
徑向速度 | 77.1 | 0.63+0.08 − |
處於宜居帶內[88] | |||
| HIP 38594 b | 0.026+0.012 −0.014 |
60.711+0.426 −0.192 |
0.256+0.006 −0.007 |
徑向速度 | 58.0 | 0.61+0.02 − |
處於宜居帶內[88] | |||
| HIP 38594 c | 0.135+0.077 −0.035 |
3525+541 −572 |
3.842+0.399 −0.441 |
徑向速度 | 58.0 | 0.61+0.02 − |
[88] | |||
| HIP 4845 b | 0.053+0.016 −0.028 |
34.151+0.17 −0.09 |
0.177+0.016 −0.020 |
徑向速度 | 68.8 | 0.62+0.04 − |
[88] | |||
| HIP 48714 b | 0.071+0.023 −0.020 |
17.819+0.004 −0.009 |
0.112+0.003 − |
徑向速度 | 34.3 | 0.58+0.02 − |
[88] | |||
| 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 |
凌日 | 208 | 0.69+0.009 −0.007 |
4569+50 − |
海王星沙漠行星[89] |
| Proxima Centauri c | 0.0179+0.006 − |
1928+20 − |
1.489+0.049 − |
39+16 −18 |
徑向速度 | 4.244+0.001 − |
0.1221+0.0022 − |
3042+117 − |
已知軌道第二近的行星[90][91] | |
| TOI-763 b | 0.031+0.002 − |
0.203+0.010 − |
5.6057+0.0013 − |
0.0600+0.0006 − |
1038+16 − |
凌日 | 311 | 0.917+0.028 − |
5444+110 − |
[92] |
| TOI-763 c | 0.029+0.003 − |
0.235+0.011 − |
12.2737+0.0053 −0.0077 |
0.1011+0.0010 − |
800+12 − |
凌日 | 311 | 0.917+0.028 − |
5444+110 − |
[92] |
| TOI-763 d | 0.030+0.005 − |
47.7991+2.7399 − |
0.2504+0.0093 −0.0105 |
509+12 − |
徑向速度 | 311 | 0.917+0.028 − |
5444+110 − |
[92] | |
| TOI-561 b | 0.0050+0.0011 − |
0.127+0.006 − |
0.446578+0.000017 − |
0.01055+0.00008 − |
凌日 | 279.2+1.6 − |
0.785+0.018 − |
5455+65 −47 |
[93][94] | |
| TOI-561 c | 0.017+0.003 − |
0.257+0.009 − |
10.779+0.004 − |
0.08809+0.0007 − |
凌日 | 279.2+1.6 − |
0.785+0.018 − |
5455+65 −47 |
[93][94] | |
| TOI-561 d | 0.038+0.004 − |
0.226+0.011 − |
25.62+0.04 − |
0.1569+0.0012 − |
凌日 | 279.2+1.6 − |
0.785+0.018 − |
5455+65 −47 |
[93][94] | |
| TOI-561 e | 0.050+0.007 − |
0.238+0.010 − |
77.23+0.39 − |
0.3274+0.0028 −0.0027 |
凌日 | 279.2+1.6 − |
0.785+0.018 − |
5455+65 −47 |
[93] | |
| 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 − |
凌日 | 117.5+0.1 − |
0.48+0.1 − |
3570+100 − |
[95] |
| 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 − |
凌日 | 117.5+0.1 − |
0.48+0.1 − |
3570+100 − |
[95] |
| 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 − |
徑向速度 | 38.8 | 0.650+0.08 − |
4120+109 − |
行星圍繞雙星系統的主星運動[96] |
| 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 − |
徑向速度 | 38.8 | 0.650+0.08 − |
4120+109 − |
行星圍繞雙星系統的主星運動[96] |
| TOI 837 b | <1.2 | 0.768+0.091 −0.072 |
8.3248762+0.0000157 − |
凌日 | 466.5+1.2 − |
1.118+0.059 − |
6047+162 − |
位於疏散星團 IC 2602[97] | ||
| TOI-776 b | 0.0147+0.0031 − |
0.163+0.010 − |
8.24664+0.00009 −0.00006 |
0.0652+0.0011 − |
513+12 − |
凌日 | 88.6+0.1 − |
0.544+0.028 − |
3709+70 − |
[98] |
| TOI-776 c | 0.0192+0.0047 − |
0.184+0.012 − |
15.6653+0.0008 −0.0007 |
0.1000+0.0017 − |
415+10 − |
凌日 | 88.6+0.1 − |
0.544+0.028 − |
3709+70 − |
[98] |
| MOA-2009-BLG-319Lb | 0.2077+0.0255 − |
2.03+0.21 − |
微重力透鏡 | 22800+2300 − |
0.514+0.063 − |
[99] | ||||
| TOI-481 b | 1.53+0.03 − |
0.99+0.01 − |
10.33111+0.00002 − |
0.097+0.001 − |
1370+10 − |
凌日 | 587 | 1.14+0.02 −0.01 |
5735+72 − |
[100] |
| TOI-892 b | 0.95+0.07 − |
1.07+0.02 − |
10.62656+0.00007 − |
0.092+0.005 − |
1397+40 − |
凌日 | 1120 | 1.28+0.03 −0.02 |
6261+80 − |
[100] |
| GJ 3473 b | 0.0059+0.0009 − |
0.113+0.004 − |
1.1980035+0.0000018 −0.0000019 |
0.01589+0.00062 − |
773+16 −15 |
凌日 | 89.29+0.13 − |
0.360+0.016 − |
3347+54 − |
又稱TOI-488 b[101] |
| 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 |
徑向速度 | 89.29+0.13 − |
0.360+0.016 − |
3347+54 − |
又稱TOI-488 c[101] | |
| NGTS-12b | 0.208+0.022 − |
1.048+0.032 − |
7.532806+0.000048 − |
0.0757+0.0014 − |
1257+34 − |
凌日 | 1474+25 − |
1.021+0.056 −0.049 |
5690+130 − |
[102] |
| OGLE-2016-BLG-1928 | 0.001 | n/a | 微重力透鏡 | 30000 | n/a | n/a | 星際行星[103] | |||
| LTT 9779 | 0.092+0.003 − |
0.421+0.021 − |
0.792054+0.000014 − |
0.01679+0.0014 − |
2000 | 凌日 | 262.8+1.0 − |
1.02+0.02 −0.03 |
5499+50 − |
海王星沙漠 行星[104] |
| TOI-540 b | 0.081+0.005 − |
1.2391491+0.0000017 − |
0.01223+0.00036 − |
611+23 − |
凌日 | 45.67+0.29 − |
0.159+0.014 − |
3216+83 − |
[105] | |
| 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 |
徑向速度 | 49.68+0.03 − |
0.578+0.021 − |
3933+51 − |
在格利澤458雙星系統中繞主星轉動[15] | |
| TIC 237913194b | 1.942+0.092 −0.091 |
1.117+0.054 −0.047 |
15.168865+0.000018 − |
0.1207+0.0037 − |
974 | 凌日 | 1009+6 − |
1.026+0.057 −0.055 |
5788+80 − |
軌道十分偏心[106] |
| EPIC 201170410 b | 0.09341 | 6.7987 | 0.0349 | 凌日 | 437+149 −130 |
0.287+0.101 −0.084 |
3648+172 −143 |
[107] | ||
| EPIC 201757695 b | 0.08101 | 2.0478 | 0.0296 | 凌日 | 1880+110 − |
0.727+0.044 −0.053 |
4520+108 −54 |
[107] | ||
| OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 |
1.27+0.45 −0.29 |
微重力透鏡 | 16000 | 0.08+0.08 −0.02 |
[108] | ||||
| 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 |
凌日 | 768.5+8.3 − |
1.201+0.066 −0.064 |
5710+53 −49 |
[109] |
| 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 |
凌日 | 760+9 − |
0.912+0.048 −0.049 |
5282+40 −39 |
[109] |
| 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 |
凌日 | 913+11 − |
1.22+0.07 −0.08 |
6361+105 −82 |
又稱TOI-1494[110] |
| WASP-187 b | 0.80+0.09 − |
1.64+0.05 − |
5.147878+0.000005 −0.000009 |
0.0653+0.0013 − |
1726+31 −2 |
凌日 | 1224+21 − |
1.54+0.09 − |
6150+92 −85 |
又稱TOI-1493[110] |
| TOI 122b | 0.028+0.029 −0.010 |
0.243+0.016 − |
5.078030+0.000015 − |
0.0392+0.0007 − |
471 | 凌日 | 202.9+0.7 − |
0.312+0.007 − |
3403+100 − |
[111] |
| TOI 237b | 0.009+0.006 −0.003 |
0.128+0.011 − |
5.436098+0.000039 − |
0.0341+0.0010 − |
388 | 凌日 | 124.2+0.7 − |
0.179+0.004 − |
3212+100 − |
[111] |
| 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 − |
凌日 | 662+3 − |
0.6785+0.0299 −0.0079 |
4514+50 − |
[112] |
| LP 714-47 b | 0.097+0.005 − |
0.420+0.027 − |
4.052037+0.000004 − |
0.0417+0.0005 − |
700+19 −24 |
凌日 | 171.8+0.4 − |
0.59+0.02 − |
3950+51 − |
主星又名G 160-62或TOI 442。海王星沙漠行星[113] |
| CFHTWIR-Oph 98 B | 7.8+0.7 −0.8 |
1.86+0.04 − |
200 | 1800+40 − |
影像 | 447+13 − |
0.015 | 2320+40 − |
年輕的超級木星，圍繞棕矮星運動。又名2MASS J16274422-2358521[114] | |
| HD 190007 b | 0.052+0.005 − |
11.72 | 徑向速度 | 41.47+0.03 − |
0.77+0.02 − |
4610+20 − |
[115] | |||
| HD 216520 b | 0.032+0.003 − |
35.45 | 徑向速度 | 63.77+0.03 − |
0.82+0.04 − |
5103+20 − |
[115] | |||
| HD 216520 c | 0.030+0.005 − |
154.43 | 徑向速度 | 63.77+0.03 − |
0.82+0.04 − |
5103+20 − |
[115] | |||
| TOI-519 b | <14 | 0.75+0.21 − |
1.2652328+0.0000005 − |
0.012+0.004 − |
760+54 − |
凌日 | 378+3 − |
0.369+0.026 −0.097 |
3350+100 −200 |
主星很暗，絕對星等為17[116] |
| TOI-260 b | 0.009+0.013 −0.009 |
0.157+0.027 − |
13.478048+0.005188 − |
凌日 | 65.84+0.07 − |
主星又稱HIP 1532或BD-10 47[117] | ||||
| TOI-784 b | 0.031+0.004 − |
0.171+0.015 − |
2.797179+0.000158 − |
凌日 | 211+0.4 − |
主星又稱HD 307842[117] | ||||
| TOI-836 b | 0.047+0.011 − |
0.224+0.029 − |
8.592004+0.002328 − |
凌日 | 89.73+0.10 − |
主星又稱HIP 73427或CD-23 12010[117] | ||||
| TOI-836 c | 0.018+0.004 − |
0.162+0.024 − |
3.816514+0.000757 − |
凌日 | 89.73+0.10 − |
主星又稱HIP 73427或CD-23 12010[117] | ||||
| EPIC 201085153 b | 0.214+0.089 − |
0.25722+0.000039 − |
凌日 | 3945+386 − |
軌道短[118] | |||||
| EPIC 201085153 c | 0.125+0.179 −0.125 |
2.259797+0.0008 − |
凌日 | 3945+386 − |
[118] | |||||
| EPIC 201427007 b | 0.134+0.018 − |
0.72091+0.000067 − |
凌日 | 5633+111 − |
[118] | |||||
| EPIC 201595106 b | 0.116+0.009 − |
0.877214+0.000087 − |
凌日 | 762+9 − |
5820+20 − |
2018年成為行星候選[118] | ||||
| EPIC 201650711 c | 0.036+0.007 − |
5.544059+0.00016 − |
凌日 | 298.8+1.7 − |
4310+92 − |
位於三元恆星系，行星b為確認[118] | ||||
| EPIC 205152172 b | 0.107+0.018 − |
0.980088+0.000026 − |
凌日 | 517+2 − |
0.669+0.016 − |
4202+242 − |
2016年成為行星候選[118] | |||
| K2-299c | 0.223+0.080 − |
14.648966+0.000031 − |
凌日 | 1219+16 − |
5724+72 − |
又名EPIC 206024342 p2[118] | ||||
| K2-299d | 0.152+0.054 − |
4.507464+0.0000077 − |
凌日 | 1219+16 − |
5724+72 − |
又名EPIC 206024342 p3[118] | ||||
| K2-301c | 0.152+0.018 − |
5.2986+0.00035 − |
凌日 | 1491+45 − |
4114+99 − |
又名EPIC 206042996 p2[118] | ||||
| TOI-251b | 0.245+0.016 − |
4.937770+0.000028 −0.000029 |
0.05741+0.00023 −0.00017 |
凌日 | 324.4+1.4 − |
1.036+0.013 −0.009 |
5875+100 −190 |
[119] | ||
| TOI-942b | 0.429+0.018 − |
4.324190+0.00003 − |
0.04796+0.00073 −0.00065 |
凌日 | 498+2 − |
0.788+0.037 −0.031 |
4928+125 −85 |
[119][120]主星為 TYC 5909-319-1 | ||
| TOI-942c | 0.517+0.017 −0.016 |
10.156430+0.000069 −0.000079 |
0.0847+0.0012 −0.0011 |
凌日 | 498+2 − |
0.788+0.037 −0.031 |
4928+125 −85 |
[119][120]主星為 TYC 5909-319-1 | ||
| K2-302c | 0.089+0.009 − |
2.255438+0.000037 − |
凌日 | 359.3+3.5 − |
3297+73 − |
又名EPIC 206215704 p2[118] | ||||
| K2-302d | 0.098+0.009 − |
2.909216+0.000032 − |
凌日 | 359.3+3.5 − |
3297+73 − |
又名EPIC 206215704 p3[118] | ||||
| EPIC 206298289 b | 0.078+0.009 − |
0.434847+0.000022 − |
凌日 | 492+6 − |
3875+157 − |
2016年成為行星候選[118] | ||||
| K2-85 b | 0.107+0.009 − |
0.684559+0.000026 − |
凌日 | 317.8+1.2 − |
4427+48 − |
又名EPIC 210707130 p1[118] | ||||
| EPIC 210801536 b | 0.088+0.027 − |
0.892592+0.00012 − |
凌日 | 5304+259 − |
2019年成為行星候選。該星系裡可能還有一個行星[118] | |||||
| EPIC 212624936 b | 0.517+0.098 −0.027 |
0.578657+0.000066 − |
凌日 | 5765+170 − |
[118]主星為 TYC 5557-667-1 | |||||
| EPIC 212624936 c | 0.214+0.098 −0.057 |
11.811437+0.00016 − |
凌日 | 5765+170 − |
[118]主星為 TYC 5557-667-1 | |||||
| K2-211c | 0.116+0.018 − |
2.601404+0.000072 − |
凌日 | 895+14 − |
0.882+0.019 −0.027 |
5360+51 − |
[118] | |||
| EPIC 220440058 b | 0.125+0.036 − |
0.626683+0.00005 − |
凌日 | 3682+217 − |
該星系裡可能還有一個行星[118] | |||||
| EPIC 220492298 b | 0.085+0.018 − |
0.762406+0.00014 − |
凌日 | 5620+31 − |
[118] | |||||
| K2-282d | 0.232+0.027 − |
27.248322+0.00047 − |
凌日 | 1638.22+25.34 − |
0.94+0.04 − |
5499+109 − |
[118] | |||
| EPIC 228836835 b | 0.089+0.027 − |
0.728113+0.00004 − |
凌日 | 491+6 − |
3782+152 − |
[118] | ||||
| K2-106c | 0.188+0.018 − |
13.334621+0.000068 − |
凌日 | 803+10 − |
5613+39 − |
2017年成為行星候選[118] | ||||
| 克卜勒-1514c | 0.1049+0.0051 −0.0039 |
10.514181+0.000039 − |
0.0997+0.0018 − |
1066+16 −14 |
凌日 | 1240 | 1.196+0.065 −0.063 |
6145+99 −80 |
[121] | |
| OGLE-2017-BLG-1049Lb | 5.53+3.62 −2.87 |
3.92+1.10 −1.32 |
微重力透鏡 | 18500+3600 −4500 |
0.55+0.36 −0.29 |
[122] | ||||
| AU Microscopii c | <0.087 | 0.320+0.014 − |
18.858991+0.000010 − |
0.1101+0.0022 − |
454+16 − |
凌日 | 31.7 | 0.50+0.03 − |
3700+100 − |
[123] |
| HD 25723 b | 2.51 | 456.78 | 1.49 | 徑向速度 | 375 | 2.1+0.3 − |
主星為巨星[124] | |||
| HD 25723 c | 1.33 | 2369.84 | 4.35 | 徑向速度 | 375 | 2.1+0.3 − |
主星為巨星[124] | |||
| Chi Scorpii b | 4.32+0.15 −0.12 |
573.4+2.0 − |
1.45+0.02 − |
徑向速度 | 408 | 1.09+0.15 − |
4157+11 − |
主星為巨星[124] | ||
| HD 60292 b | 6.5+1.0 − |
495.4+3.0 − |
1.5+0.1 − |
徑向速度 | 1036+10 − |
1.7+0.2 − |
4348+28 − |
主星為巨星[125] | ||
| HD 112640 b | 5.0+1.0 − |
613.2+5.8 − |
1.7+0.1 − |
徑向速度 | 1065+6 − |
1.8+0.2 − |
4155+15 − |
主星為巨星[125] | ||
| K2-111 c | 0.0356+0.0035 − |
15.6785+0.0064 −0.0063 |
0.1166+0.0025 − |
徑向速度 | 680+60 − |
0.89+0.02 − |
5730+50 − |
[126] | ||
| K2-316b | 0.119 | 1.133 | 0.0147 | 841 | 凌日 | 368 | EPIC 249384674b[127] | |||
| K2-316c | 0.163 | 5.260 | 0.0582 | 423 | 凌日 | 368 | EPIC 249384674c[127] | |||
| K2-317b | 0.261 | 6.220 | 0.0542 | 432 | 凌日 | 577 | EPIC 249557502b[127] | |||
| K2-318b | 0.148 | 7.010 | 0.0911 | 456 | 凌日 | 483 | EPIC 249826231b[127] | |||
| K2-319b | 0.249 | 26.680 | 0.1516 | 641 | 凌日 | 686 | EPIC 201663879b[127] | |||
| K2-320b | 0.234 | 1.995 | 0.0142 | 698 | 凌日 | 356 | EPIC 201796690b[127] | |||
| K2-321b | 0.174 | 2.298 | 0.0410 | 701 | 凌日 | 254 | EPIC 248480671b[127] | |||
| K2-322b | 0.171 | 8.205 | 0.0594 | 635 | 凌日 | 404 | EPIC 248558190b[127] | |||
| K2-323b | 0.187 | 24.930 | 0.1275 | 318 | 凌日 | 387 | EPIC 248616368b[127] | |||
| K2-324b | 0.217 | 3.262 | 0.0331 | 707 | 凌日 | 447 | EPIC 248639308b[127] | |||
| K2-325b | 0.196 | 6.930 | 0.0419 | 423 | 凌日 | 365 | EPIC 246074965b[127] | |||
| K2-326b | 0.203 | 1.256 | 0.0198 | 1114 | 凌日 | 928 | EPIC 246472939b[127] | |||
| KMT-2016-BLG-2397b | 2.42 | 2.83 | 微重力透鏡 | 16000 | 0.62+0.29 −0.30 |
這個行星有多種可能的情況[128] | ||||
| KMT-2016-BLG-2364b | 3.93 | 2.63 | 微重力透鏡 | 21000 | 0.50+0.40 −0.22 |
[128] | ||||
| OGLE-2017-BLG-1375b | 10.33 | 2.97 | 微重力透鏡 | 12000 | 0.77+0.27 −0.23 |
這個行星有多種可能的情況[128] | ||||
| OGLE-2017-BLG-0604b | 0.51 | 4.06 | 微重力透鏡 | 13000 | 0.70+0.28 − |
[128] | ||||
| KMT-2018-BLG-0748Lb | 0.18+0.29 −0.10 |
0.62+0.09 − |
微重力透鏡 | 24000 | 0.0870+0.138 −0.047 |
[129] | ||||
| KMT-2019-BLG-1339Lb | 12.2+16.1 −6.7 |
0.67+0.77 −0.55 |
微重力透鏡 | 23000+3000 − |
0.27+0.366 −0.15 |
這個行星有多種可能的情況[130] | ||||
| KMT-2019-BLG-2073 | 0.19 | 微重力透鏡 | 12000 | [131] | ||||||
| OGLE-2019-BLG-0551 | 0.0242 | 微重力透鏡 | [132] | |||||||
| TVLM 513-46546 b | 0.38+0.24 − |
221+5 − |
0.3+0.0036 − |
天體測量 | 34.90+0.07 − |
0.09 | 2500 | [133] | ||
| CD Ceti | 0.0124+0.0013 −0.0014 |
2.29070+0.00012 − |
0.0185+0.0013 −0.0013 |
464+18 − |
徑向速度 | 28.07 | 0.161+0.010 − |
3130+51 − |
[134] | |
| OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 |
1.27+0.45 −0.29 |
微重力透鏡 | 16000 | 0.08+0.08 −0.02 |
[135] | ||||
| WD 1856+534 b | 13.8 | 0.93+0.09 − |
1.4079405+0.0000011 − |
0.0204+0.0012 − |
凌日 | 80.737+0.144 − |
0.518+0.055 − |
4710+60 − |
圍繞白矮星運動[136] | |
| 克卜勒-1649c | 0.0038 | 0.095+0.014 −0.010 |
19.53527+0.00010 − |
0.0649 | 234+20 − |
凌日 | 301.6+1.6 − |
0.1977+0.0051 − |
3240+61 − |
處於宜居帶內，行星像地球[137] |
| Kepler-305e | 0.160 | 3.20538 | 凌日 | 2900+90 − |
[138] | |||||
| Kepler-385d | 0.233 | 56.4159 | 凌日 | 4870+160 − |
[138] | |||||
| Kepler-598c | 0.270 | 86.4945 | 凌日 | 2260+40 − |
FPP=1.0%[138] | |||||
| Kepler-647c | 0.357 | 29.6663 | 凌日 | 3660+70 − |
[138] | |||||
| Kepler-716c | 0.124 | 3.96999 | 凌日 | 2110+30 − |
FPP=0.6%[138] | |||||
| Kepler-783c | 0.208 | 7.05395 | 凌日 | 1707+15 − |
[138] | |||||
| Kepler-1001c | 0.140 | 9.18186 | 凌日 | 3110+80 − |
[138] | |||||
| Kepler-1085c | 0.291 | 56.7771 | 凌日 | 4630+150 − |
[138] | |||||
| 克卜勒-1662b | 0.223 | 0.790 | 134.4628 | 凌日 | [139]主星又名KOI-1783[140] | |||||
| 克卜勒-1663b | 0.294 | 17.6046 | 凌日 | 1112+11 − |
主星又名KOI-252[138] | |||||
| 克卜勒-1664b | 0.270 | 14.3868 | 凌日 | 主星又名KOI-349[138] | ||||||
| 克卜勒-1665b | 0.253 | 11.9548 | 凌日 | 1104+5 − |
主星又名KOI-650[138] | |||||
| Kepler-1666b | 0.257 | 25.8476 | 凌日 | 4680+190 − |
主星又名KOI-945[138] | |||||
| Kepler-1666c | 0.257 | 25.8476 | 凌日 | 4680+190 − |
主星又名KOI-945[138] | |||||
| 克卜勒-1667b | 0.266 | 83.5781 | 凌日 | 2080+20 − |
主星又名KOI-1311[138] | |||||
| 克卜勒-1668b | 0.388 | 15.434 | 凌日 | 4500+200 − |
主星又名KOI-1470[138] | |||||
| 克卜勒-1669b | 0.248 | 9.51216 | 凌日 | 1800+40 − |
主星又名KOI-1475[138] | |||||
| 克卜勒-1670b | 0.299 | 20.4998 | 凌日 | 7200+400 − |
主星又名KOI-1705[138] | |||||
| 克卜勒-1671b | 0.118 | 4.16787 | 凌日 | 1176+7 − |
主星又名KOI-1738[138] | |||||
| 克卜勒-1672b | 0.265 | 150.878 | 凌日 | 1189+14 − |
主星又名KOI-1822[138] | |||||
| 克卜勒-1673b | 0.262 | 33.7888 | 凌日 | 2420+20 − |
主星又名KOI-1863[138] | |||||
| 克卜勒-1674b | 0.286 | 62.5611 | 凌日 | 3400+100 − |
主星又名KOI-1892[138] | |||||
| 克卜勒-1675b | 0.279 | 63.0382 | 凌日 | 2163+19 − |
主星又名KOI-1928[138] | |||||
| 克卜勒-1676b | 0.301 | 29.9221 | 凌日 | 主星又名KOI-1943[138] | ||||||
| 克卜勒-1677b | 0.241 | 22.064 | 凌日 | 2250+30 − |
主星又名KOI-1984， FPP=0.6%[138] | |||||
| 克卜勒-1678b | 0.295 | 147.974 | 凌日 | 2830+70 − |
主星又名KOI-2066， FPP=0.5%[138] | |||||
| 克卜勒-1679b | 0.184 | 9.75376 | 凌日 | 3040+100 − |
主星又名KOI-2106[138] | |||||
| 克卜勒-1680b | 0.121 | 8.77424 | 凌日 | 1020+5 − |
主星又名KOI-2120[138] | |||||
| 克卜勒-1681b | 0.2227 | 69.8956 | 凌日 | 2100+300 − |
主星又名KOI-2132[138] | |||||
| 克卜勒-1682b | 0.257 | 14.8334 | 凌日 | 3900+160 − |
主星又名KOI-2229[138] | |||||
| 克卜勒-1683b | 0.167 | 15.0337 | 凌日 | 2440+50 − |
主星又名KOI-2293[138] | |||||
| 克卜勒-1684b | 0.256 | 47.7055 | 凌日 | 2060+40 − |
主星又名KOI-2417[138] | |||||
| 克卜勒-1685b | 0.230 | 20.4905 | 凌日 | 3840+150 − |
主星又名KOI-2504[138] | |||||
| 克卜勒-1686b | 0.127 | 9.30987 | 凌日 | 2430+30 − |
主星又名KOI-2559[138] | |||||
| 克卜勒-1687b | 0.147 | 5.77954 | 凌日 | 1375+17 − |
主星又名KOI-2588[138] | |||||
| 克卜勒-1688b | 0.112 | 5.62012 | 凌日 | 1850+380 − |
主星又名KOI-2733[138] | |||||
| 克卜勒-1689b | 0.084 | 8.483 | 凌日 | 967+5 − |
主星又名KOI-2755[138] | |||||
| 克卜勒-1690b | 0.250 | 234.636 | 凌日 | 2340+30 − |
主星又名KOI-2757[138] | |||||
| 克卜勒-1691b | 0.163 | 3.8482 | 凌日 | 4290+110 − |
主星又名KOI-2802[138] | |||||
| 克卜勒-1692b | 0.099 | 5.95966 | 凌日 | 1960+20 − |
主星又名KOI-2849[138] | |||||
| 克卜勒-1693b | 0.115 | 12.0999 | 凌日 | 2530+50 − |
主星又名KOI-2871[138] | |||||
| 克卜勒-1694b | 0.105 | 3.89526 | 凌日 | 1698+16 − |
主星又名KOI-2878， FPP=0.6%[138] | |||||
| 克卜勒-1695b | 0.099 | 4.7329 | 凌日 | 2640+40 − |
主星又名KOI-3048， FPP=0.5%[138] | |||||
| 克卜勒-1696b | 0.250 | 65.9409 | 凌日 | 5100+200 − |
主星又名KOI-3361[138] | |||||
| 克卜勒-1697b | 0.112 | 33.4969 | 凌日 | 813+2 − |
主星又名KOI-3478[138] | |||||
| 克卜勒-1698b | 0.095 | 1.2107 | 凌日 | 729+3 − |
主星又名KOI-3864[138] | |||||
| 克卜勒-1699b | 0.139 | 3.49082 | 凌日 | 主星又名KOI-3933[138] | ||||||
| Kepler-1701b | 0.198 | 169.134 | 凌日 | 1940+20 − |
主星又名KOI-4054，[138] 可能宜居的系外行星 | |||||
| 克卜勒-1702b | 0.143 | 18.5012 | 凌日 | 2860+90 − |
主星又名KOI-4386[138] |
參考
- ^ NASA Exoplanet Archive. [20 December 2019]. （原始內容存檔於2021-03-22）.
- ^ Extrasolar Planet's Catalogue (sic). Kyoto University. [20 December 2019]. （原始內容存檔於2022-04-06）.
- ^ The Extrasolar Planets Encyclopaedia. [2015-11-09]. （原始內容存檔於2012-07-05）.
- ^ exoplanet.eu Planet 2MASS J1155-7919 b. [2021-08-24]. （原始內容存檔於2021-11-28）.
- ^ www.sci-news.com Astronomers Discover Nearest-Known Newborn Gas Giant. [2021-08-24]. （原始內容存檔於2020-03-03）.
- ^ 6.0 6.1 6.2 6.3 6.4 6.5 Haswell, Carole A.; et al. Dispersed Matter Planet Project discoveries of ablating planets orbiting nearby bright stars. Nature Astronomy. 2019, 4 (4): 408–418. Bibcode:2020NatAs...4..408H. S2CID 209444484. arXiv:1912.10874
. doi:10.1038/s41550-019-0973-y.
- ^ Jones, Mark H.; Haswell, Carole A.; Barnes, John R.; Staab, Daniel; Heller, René. A possible transit of a disintegrating exoplanet in the nearby multiplanet system DMPP-1. The Astrophysical Journal. 2020, 895 (1): L17. Bibcode:2020ApJ...895L..17J. S2CID 218630238. arXiv:2005.07086 . doi:10.3847/2041-8213/ab8f2b.
- ^ 8.0 8.1 8.2 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.; et al, 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, 2020, 636: A89, Bibcode:2020A&A...636A..89H, S2CID 211032193, arXiv:2002.01755v1 , doi:10.1051/0004-6361/201937080
- ^ exoplanet.eu Planet EPIC 249893012 d. [2021-08-24]. （原始內容存檔於2021-07-27）.
- ^ G 9-40 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 180 d. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 229 A c. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ 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. 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. 2020, 246 (1): 11. Bibcode:2020ApJS..246...11F. S2CID 210064560. arXiv:2001.02577 . doi:10.3847/1538-4365/ab5e7c.
- ^ Barnes, J. R.; et al. Frequency of planets orbiting M dwarfs in the Solar neighbourhood. 2019-06-11. arXiv:1906.04644 （英語）.
- ^ 15.0 15.1 The CARMENES search for exoplanets around M dwarfs Three temperate-to-warm super-Earths, 2020, arXiv:2010.00474
- ^ www.sci-news.com Astronomers Discover Five New Planets around Nearby Red Dwarfs. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 433 d. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 1061 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 1061 c. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ GJ 1061 d. [2021-08-24]. （原始內容存檔於2020-10-14）.
- ^ GJ 1252 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ exoplanet.eu Planet GJ 3082 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ 23.0 23.1 23.2 23.3 Hartman, J. D.; et al. HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs. The Astronomical Journal. 2020, 159 (4): 173. Bibcode:2020AJ....159..173H. S2CID 211126666. arXiv:2002.05776 . doi:10.3847/1538-3881/ab7821.
- ^ exoplanet.eu hats-48a b. [2021-08-24]. （原始內容存檔於2022-03-18）.
- ^ exoplanet.eu HD 80653 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ 26.0 26.1 26.2 Nielsen, L.; et al. Three Short Period Jupiters from TESS. Astronomy & Astrophysics. 2020, 639: A76. S2CID 212675311. arXiv:2003.05932 . doi:10.1051/0004-6361/202037941.
- ^ exoplanet.eu HIP 65A b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ Wong, Ian; et al. Systematic Phase Curve Study of Known Transiting Systems from Year 1 of the TESS Mission. 2020. arXiv:2003.06407 [astro-ph.EP].
- ^ exoplanet.eu Planet KELT-2019-BLG-1953 b. [2021-08-24]. （原始內容存檔於2020-02-17）.
- ^ 30.0 30.1 Han, Cheongho; et al. One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953. The Astronomical Journal. 2020, 160 (1): 17. Bibcode:2020AJ....160...17H. S2CID 211096807. arXiv:2002.05310 . doi:10.3847/1538-3881/ab91ac.
- ^ exoplanet.eu Planet KELT-2019-BLG-1953 c. [2021-08-24]. （原始內容存檔於2020-02-17）.
- ^ Kepler-1661 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ Socia, Quentin J.; et al. Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary. The Astronomical Journal. 2020, 159 (3): 94. Bibcode:2020AJ....159...94S. S2CID 210116655. arXiv:2001.02840 . doi:10.3847/1538-3881/ab665b.
- ^ exoplanet.eu L 168-9 b. [2021-08-24]. （原始內容存檔於2021-07-27）.
- ^ Herrera-Martín, Antonio; et al. Ogle-2018-BLG-0677lb: A super earth near the galactic bulge. The Astronomical Journal. 2020, 159 (6): 256. Bibcode:2020AJ....159..256H. S2CID 212628627. arXiv:2003.02983 . doi:10.3847/1538-3881/ab893e.
- ^ TOI-132 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ exoplanet.eu toi-257_b. [2021-08-24]. （原始內容存檔於2021-07-27）.
- ^ TOI-257b (HD 19916b): A Warm sub-Saturn on a Moderately Eccentric Orbit Around an Evolved F-type Star, 2020, arXiv:2001.07345
- ^ TIDAL INFLATION RECONCILES LOW-DENSITY SUB-SATURNS WITH CORE ACCRETION, 2020, arXiv:2005.11209
- ^ 40.0 40.1 40.2 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; et al. The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 System. 2020. arXiv:2001.00952 [astro-ph.EP].
- ^ 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. The First Habitable Zone Earth-sized Planet from TESS. III: Climate States and Characterization Prospects for TOI-700 D. 2020. arXiv:2001.00955 [astro-ph.EP].
- ^ 42.0 42.1 Cloutier, Ryan; et al. A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780. The Astronomical Journal. 2020, 160 (1): 3. Bibcode:2020AJ....160....3C. S2CID 211817805. arXiv:2003.01136 . doi:10.3847/1538-3881/ab91c2.
- ^ 43.0 43.1 Nowak, G.; et al. The CARMENES search for exoplanets around M dwarfs. Two planets on the opposite sides of the radius gap transiting the nearby M dwarf LP 729-54. 2020. arXiv:2003.01140 [astro-ph.EP].
- ^ exoplanet.eu toi-813_b. [2021-08-24]. （原始內容存檔於2021-07-19）.
- ^ 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.; et al. TOI-1338: TESS' First Transiting Circumbinary Planet. The Astronomical Journal. 2020, 159 (6): 253. Bibcode:2020AJ....159..253K. S2CID 215785933. arXiv:2004.07783 . doi:10.3847/1538-3881/ab8a48.
- ^ Exoplanet-catalog - Exoplanet TOI-1338 b. [2021-08-24]. （原始內容存檔於2021-08-08）.
- ^ 47.0 47.1 47.2 Badenas-Agusti, Mariona; et al. HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away. 2020. arXiv:2002.03958 [astro-ph.EP].
- ^ 48.0 48.1 Chinchilla, Patricia; et al. USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius. Astronomy & Astrophysics. 2020, 633: A152. Bibcode:2020A&A...633A.152C. S2CID 208910589. arXiv:1912.04150 . doi:10.1051/0004-6361/201936130.
- ^ Crouzet, Nicolas; et al. XO-7 b: A Transiting Hot Jupiter with a Massive Companion on a Wide Orbit. The Astronomical Journal. 2020, 159 (2): 44. Bibcode:2020AJ....159...44C. S2CID 208857410. arXiv:1912.02821 . doi:10.3847/1538-3881/ab5b12.
- ^ Gan, Tianjun; et al. LHS 1815b: The First Thick-Disk Planet Detected by TESS. The Astronomical Journal. 2020, 159 (4): 160. Bibcode:2020AJ....159..160G. S2CID 212644667. arXiv:2003.04525 . doi:10.3847/1538-3881/ab775a.
- ^ exoplanet.eu LHS 1815 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ Armstrong, David J.; et al. A remnant planetary core in the hot Neptunian desert. Nature. 2020, 583 (7814): 39–42. Bibcode:2020Natur.583...39A. PMID 32612222. S2CID 214612138. arXiv:2003.10314 . doi:10.1038/s41586-020-2421-7.
- ^ Díaz, Matías R.; et al. The Magellan/PFS Exoplanet Search: A 55-day period dense Neptune transiting the bright ($V=8.6$) star HD 95338. 2020. S2CID 214611611. arXiv:2003.10319 . doi:10.1093/mnras/staa1724.
- ^ Dalba, Paul A.; et al. The TESS-Keck Survey I: A Warm Sub-Saturn-Mass Planet and a Caution about Stray Light in TESS Cameras. The Astronomical Journal. 2020, 159 (5): 241. Bibcode:2020AJ....159..241D. S2CID 214623340. arXiv:2003.10451 . doi:10.3847/1538-3881/ab84e3.
- ^ 55.0 55.1 Huang, Chelsea X.; et al. TESS Spots a Hot Jupiter with an Inner Transiting Neptune. The Astrophysical Journal. 2020, 892 (1): L7. Bibcode:2020ApJ...892L...7H. S2CID 214623301. arXiv:2003.10852 . doi:10.3847/2041-8213/ab7302.
- ^ exoplanet.eu toi-1130 b. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ exoplanet.eu toi-1130 c. [2021-08-24]. （原始內容存檔於2021-07-26）.
- ^ González-Álvarez, E.; Zapatero Osorio, M. R.; 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, A.; Quirrenbach, A.; Amado, P. J.; Anglada-Escudé, G.; Azzaro, M.; Cortés-Contreras, M.; Hatzes, A. P.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; Morales, J. C.; Pallé, E.; Perger, M.; Schmitt, J. H. M. M. The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B). Astronomy & Astrophysics. 2020, A93: 637. Bibcode:2020A&A...637A..93G. S2CID 214714124. arXiv:2003.13052 . doi:10.1051/0004-6361/201937050.
- ^ 59.0 59.1 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; et al. Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b. The Astronomical Journal. 2020, 159 (6): 255. Bibcode:2020AJ....159..255C. S2CID 215754471. arXiv:2004.06622 . doi:10.3847/1538-3881/ab88db.
- ^ 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.; et al. TOI-1235 b: A keystone super-Earth for testing radius valley emergence models around early M dwarfs. The Astronomical Journal. 2020, 160 (1): 22. Bibcode:2020AJ....160...22C. S2CID 215754432. arXiv:2004.06682 . doi:10.3847/1538-3881/ab9534.
- ^ 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; et al. OGLE-2017-BLG-0406: ${\it Spitzer}$ Microlens Parallax Reveals Saturn-mass Planet orbiting M-dwarf Host in the Inner Galactic Disk. 2020. S2CID 215827466. arXiv:2004.09067 . doi:10.3847/1538-3881/ab9ac3.
- ^ 62.0 62.1 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.; et al. The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary. 2020. arXiv:2004.10095 [astro-ph.EP].
- ^ 63.0 63.1 63.2 63.3 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; et al. TESS discovery of a super-Earth and three sub-Neptunes hosted by the bright, Sun-like star HD 108236. 2020. arXiv:2004.11314 [astro-ph.EP].
- ^ 64.0 64.1 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.; et al. Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets. Astronomy & Astrophysics. 2020, A32: 640. Bibcode:2020A&A...640A..32H. S2CID 216867348. arXiv:2004.14645 . doi:10.1051/0004-6361/202038296.
- ^ 65.0 65.1 A Newtonian model for the WASP-148 exoplanetary system enhanced with TESS and ground-based photometric observations, 2020, arXiv:2012.02602
- ^ 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.; et al. NGTS-11 b / TIC-54002556 b: A transiting warm Saturn recovered from a TESS single-transit event. 2020. S2CID 220845943. arXiv:2005.00006 . doi:10.3847/2041-8213/ab9eb9.
- ^ 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. TESS Hunt for Young and Maturing Exoplanets (THYME) II: A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association. The Astronomical Journal. 2020, 160 (1): 33. Bibcode:2020AJ....160...33R. S2CID 218470215. arXiv:2005.00013 . doi:10.3847/1538-3881/ab94b7.
- ^ 68.0 68.1 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; et al. TESS Hunt for Young and Maturing Exoplanets (THYME) III: A two-planet system in the 400 Myr Ursa Major Group. 2020. arXiv:2005.00047 [astro-ph.EP].
- ^ The TESS-Keck Survey III: A Stellar Obliquity Measurement of TOI-1726 c, 2020, arXiv:2008.12397
- ^ 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.; et al. 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. 2020, A50: 639. Bibcode:2020A&A...639A..50B. S2CID 218538033. arXiv:2005.03368 . doi:10.1051/0004-6361/202037939.
- ^ 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; et al. A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System. The Astronomical Journal. 2020, 160 (2): 72. Bibcode:2020AJ....160...72B. S2CID 218665248. arXiv:2005.07199 . doi:10.3847/1538-3881/ab9cb9.
- ^ 72.0 72.1 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. Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2b. Astronomy & Astrophysics. 2020, 639: A130. Bibcode:2020A&A...639A.130O. S2CID 218971735. arXiv:2005.13560 . doi:10.1051/0004-6361/202037715.
- ^ Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve. Transit least-squares survey. Astronomy & Astrophysics. 2020, 638: A10. S2CID 219260293. arXiv:2006.02123 . doi:10.1051/0004-6361/201936929.
- ^ Niraula, Prajwal; Julien de Wit; Rackham, Benjamin V.; Ducrot, Elsa; Burdanov, Artem; Crossfield, Ian J. M.; Valerie Van Grootel; Murray, Catriona; Garcia, Lionel J.; Alonso, Roi; Beard, Corey; Yilen Gomez Maqueo Chew; Delrez, Laetitia; Demory, Brice-Olivier; Fulton, Benjamin J.; Gillon, Michael; Gunther, Maximilian N.; Howard, Andrew W.; Issacson, Howard; Jehin, Emmanuel; Pedersen, Peter P.; Pozuelos, Francisco J.; Queloz, Didier; Rebolo-Lopez, Rafael; Sairam, Lalitha; Sebastian, Daniel; Thompson, Samantha; Triaud, Amaury H. M. J. $π$ Earth: A 3.14-day Earth-sized Planet from $\textit{K2}$'s Kitchen Served Warm by the SPECULOOS Team. 2020. arXiv:2006.07308 [astro-ph.EP].
- ^ 75.0 75.1 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, 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, 2020, arXiv:2006.11180
- ^ Plavchan, Peter; Barclay, Thomas; Gagné, Jonathan; et al. A planet within the debris disk around the pre-main-sequence star AU Microscopii. Nature. 2020, 582 (7813): 497–500. Bibcode:2020Natur.582..497P. PMID 32581383. S2CID 220042005. arXiv:2006.13248 . doi:10.1038/s41586-020-2400-z.
- ^ Addison, Brett C.; Horner, Jonathan; Wittenmyer, Robert A.; Plavchan, Peter; Wright, Duncan J.; Nicholson, Belinda A.; Marshall, Jonathan P.; Clark, Jake T.; Kane, Stephen R.; Hirano, Teruyuki; Kielkopf, John; Shporer, Avi; Tinney, C. G.; Zhang, Hui; Ballard, Sarah; Bedding, Timothy; Bowler, Brendan P.; Mengel, Matthew W.; Okumura, Jack; Gaidos, Eric, The Youngest Planet to Have a Spin-Orbit Alignment Measurement AU Mic b, 2020, arXiv:2006.13675
- ^ EXOPLANET CATALOG AU Microscopii b on exoplanets.nasa.gov. [2021-08-24]. （原始內容存檔於2021-06-14）.
- ^ 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., TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host, The Astrophysical Journal, 2020, 899 (1): 29, Bibcode:2020ApJ...899...29K, S2CID 220056014, arXiv:2006.14546 , doi:10.3847/1538-4357/aba0a2
- ^ 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.; et al, The GAPS Programme at TNG XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone, 2020, arXiv:2006.14393
- ^ Youn Kil Jung; Gould, Andrew; Udalski, Andrzej; Sumi, Takahiro; Yee, Jennifer C.; Han, Cheongho; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Zhu, Wei; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Mróz, Przemek; Szymański, Michał K.; Skowron, Jan; Poleski, Radek; Soszyński, Igor; Pietrukowicz, Paweł; et al, OGLE-2018-BLG-1269Lb: A Jovian Planet With A Bright, I = 16 Host, 2020, arXiv:2006.15774
- ^ 82.0 82.1 Jeffers, S. V.; Dreizler, S.; Barnes, J. R.; Haswell, C. A.; Nelson, R. P.; Rodríguez, E.; López-González, M. J.; Morales, N.; Luque, R.; Zechmeister, M.; Vogt, S. S.; Jenkins, J. S.; Palle, E.; Berdi Ñas, Z. M.; Coleman, G. A. L.; Díaz, M. R.; Ribas, I.; Jones, H. R. A.; Butler, R. P.; Tinney, C. G.; Bailey, J.; Carter, B. D.; o'Toole, S.; Wittenmyer, R. A.; Crane, J. D.; Feng, F.; Shectman, S. A.; Teske, J.; Reiners, A.; et al, A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887, Science, 2020, 368 (6498): 1477–1481, Bibcode:2020Sci...368.1477J, PMID 32587019, S2CID 220075207, arXiv:2006.16372 , doi:10.1126/science.aaz0795
- ^ 83.0 83.1 83.2 83.3 83.4 83.5 83.6 Bakos, G. Á.; Hartman, J. D.; Bhatti, W.; Csubry, Z.; Penev, K.; Bieryla, A.; Latham, D. W.; Quinn, S.; Buchhave, L. A.; Kovács, G.; Torres, G.; Noyes, R. W.; Falco, E.; Béky, B.; Szklenár, T.; Esquerdo, G. A.; Howard, A. W.; Isaacson, H.; Marcy, G.; Sato, B.; Boisse, I.; Santerne, A.; Hébrard, G.; Rabus, M.; Harbeck, D.; McCully, C.; Everett, M. E.; Horch, E. P.; Hirsch, L.; et al, HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars, 2020, arXiv:2007.05528
- ^ 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.; et al, A warm Jupiter transiting an M dwarf: A TESS single transit event confirmed with the Habitable-zone Planet Finder, 2020, arXiv:2007.07098
- ^ 85.0 85.1 Jordán, A.; Bakos, G. Á.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Hartman, J. D.; Henning, Th.; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V.; de Val-Borro, M.; Zhou, G.; Butler, R. P.; Teske, J.; Crane, J.; Shectman, S.; Tan, T. G.; Thompson, I.; Wallace, J. J.; Lázár, J.; Papp, I.; Sári, P., HATS-37Ab AND HATS-38b: TWO TRANSITING HOT NEPTUNES IN THE DESERT, 2020, arXiv:2007.07135
- ^ 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, Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1, The Astrophysical Journal, 2020, 898 (1): L16, Bibcode:2020ApJ...898L..16B, S2CID 220686536, arXiv:2007.10991 , doi:10.3847/2041-8213/aba27e
- ^ 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; et al, TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet, The Astronomical Journal, 2020, 160 (2): 96, Bibcode:2020AJ....160...96T, S2CID 220830943, arXiv:2007.13927 , doi:10.3847/1538-3881/ab9f95
- ^ 88.0 88.1 88.2 88.3 88.4 88.5 88.6 88.7 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., Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs, 2020, arXiv:2008.07998
- ^ TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert, 2020, arXiv:2008.11732
- ^ Damasso, Mario; et al. A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU. Science Advances. 15 January 2020, 6 (3). eaax7467. Bibcode:2020SciA....6.7467D. PMC 6962037 . PMID 31998838. doi:10.1126/sciadv.aax7467.
- ^ Kervella, Pierre; et al. Orbital inclination and mass of the exoplanet candidate Proxima c. Astronomy & Astrophysics. 29 March 2020, 635: L14. Bibcode:2020A&A...635L..14K. ISSN 0004-6361. S2CID 214713486. arXiv:2003.13106 . doi:10.1051/0004-6361/202037551.
- ^ 92.0 92.1 92.2 The TOI-763 system: sub-Neptunes orbiting a Sun-like star, 2020, arXiv:2008.12535
- ^ 93.0 93.1 93.2 93.3 An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561, 2020, arXiv:2009.02332
- ^ 94.0 94.1 94.2 The TESS-Keck Survey II: Masses of Three Sub-Neptunes Transiting the Galactic Thick-Disk Star TOI-561, 2020, arXiv:2009.03071
- ^ 95.0 95.1 A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266, 2020, arXiv:2009.04317
- ^ 96.0 96.1 Two Planets Straddling the Habitable Zone of The Nearby K dwarf Gl 414A, 2020, arXiv:2009.06503
- ^ Cluster Difference Imaging Photometric Survey. II.TOI837: A Young Validated Planet in IC2602, 2020, arXiv:2009.07845
- ^ 98.0 98.1 A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776, 2020, arXiv:2009.08338
- ^ MOA-2009-BLG-319Lb: A Sub-Saturn Planet Inside the Predicted Mass Desert, 2020, arXiv:2009.08461
- ^ 100.0 100.1 TOI-481 b & TOI-892 b: Two long period hot Jupiters from the Transiting Exoplanet Survey Satellite, 2020, arXiv:2009.08881
- ^ 101.0 101.1 Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488), 2020, arXiv:2009.10432
- ^ NGTS-12b: A sub-Saturn mass transiting exoplanet in a 7.53 day orbit, 2020, arXiv:2009.10620
- ^ A terrestrial-mass rogue planet candidate detected in the shortest-timescale microlensing event, 2020, arXiv:2009.12377
- ^ An Ultra-Hot Neptune in the Neptune desert, 2020, arXiv:2009.12832
- ^ TOI 540 b: A Planet Smaller than Earth Orbiting a Nearby Rapidly Rotating Low-mass Star, 2020, arXiv:2009.13623
- ^ A Highly Eccentric Warm Jupiter Orbiting TIC 237913194, 2020, arXiv:2010.03570
- ^ 107.0 107.1 TFAW survey. I. Wavelet-based denoising of K2 light curves. Discovery and validation of two new Earth-sized planets in K2 campaign 1, arXiv, 2020, arXiv:2009.09285
- ^ OGLE-2018-BLG-0799Lb: a Sub-Saturn-Mass Planet Orbiting a Very Low Mass Dwarf, 2020, arXiv:2010.08732
- ^ 109.0 109.1 TOI-954 b and EPIC 246193072 b: Short-Period Saturn-Mass Planets that Test Whether Irradiation Leads to Inflation, 2020, arXiv:2010.14436
- ^ 110.0 110.1 WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS, 2020, arXiv:2010.15205
- ^ 111.0 111.1 TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by TESS, 2020, arXiv:2010.15905
- ^ HAT-P-68b: A TRANSITING HOT JUPITER AROUND A K5 DWARF STAR, 2020, arXiv:2010.16026
- ^ The CARMENES search for exoplanets around M dwarfs LP 714-47 b (TOI 442.01): Populating the Neptune desert, 2020, arXiv:2011.01716
- ^ A wide planetary-mass companion to a young low-mass brown dwarf in Ophiuchus, arXiv:2011.08871
- ^ 115.0 115.1 115.2 A collage of small planets from the Lick Carnegie Exoplanet Survey :Exploring the super-Earth and sub-Neptune mass regime, 2020, arXiv:2011.08867
- ^ TOI-519 b: a short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis, 2020, arXiv:2011.11458
- ^ 117.0 117.1 117.2 117.3 The Magellan-TESS Survey I: Survey Description and Mid-Survey Results, 2020, arXiv:2011.11560
- ^ 118.00 118.01 118.02 118.03 118.04 118.05 118.06 118.07 118.08 118.09 118.10 118.11 118.12 118.13 118.14 118.15 118.16 118.17 118.18 118.19 118.20 118.21 ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, 2020, arXiv:2011.11698
- ^ 119.0 119.1 119.2 Two young planetary systems around field stars with ages between 20 − 320 Myr from TESS, 2020, arXiv:2011.13349
- ^ 120.0 120.1 The GAPS Programme at TNG XXVIII A pair of hot-Neptunes orbiting the young star TOI-942, 2020, arXiv:2011.13795
- ^ Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. I. Confirmation of an Eccentric, Cool Jupiter With an Interior Earth-sized Planet Orbiting Kepler-1514, 2020, arXiv:2012.04676
- ^ OGLE-2017-BLG-1049: Another microlensing event with a giant planet, 2020, arXiv:2012.11080
- ^ New constraints on the planetary system around the young active star AU Mic Two transiting warm Neptunes near mean-motion resonance, 2020, arXiv:2012.13238
- ^ 124.0 124.1 124.2 Precise radial velocities of giant stars XIV. Evidence of planetary companions around HD 25723, 17 Sco, 3 Cnc, and 44 UMa. [2021-08-24]. （原始內容存檔於2021-10-09）.
- ^ 125.0 125.1 A SEARCH FOR EXOPLANETS AROUND NORTHERN CIRCUMPOLAR STARS VI. DETECTION OF PLANETARY COMPANIONS ORBITING THE GIANTS HD 60292 AND HD 112640 (PDF). [2021-08-24]. （原始內容 (PDF)存檔於2022-04-29）.
- ^ K2-111: an old system with two planets in near-resonance, 2020, arXiv:2010.01993
- ^ 127.00 127.01 127.02 127.03 127.04 127.05 127.06 127.07 127.08 127.09 127.10 127.11 Castro González, A.; Díez Alonso, E.; Menéndez Blanco, J.; et al. Planetary candidates transiting cool dwarf stars from Campaigns 12 to 15 of K2. 2020. arXiv:2007.12744v2 [astro-ph.EP].
- ^ 128.0 128.1 128.2 128.3 Four Microlensing Planets with Faint-source Stars Identified in the 2016 and 2017 Season Data, 2020, arXiv:2008.09258
- ^ KMT-2018-BLG-0748Lb: Sub-Saturn Microlensing Planet Orbiting an Ultracool Host, 2020, arXiv:2007.05204
- ^ KMT-2019-BLG-1339L: AN M DWARF WITH A GIANT PLANET OR A COMPANION NEAR THE PLANET/BROWN DWARF BOUNDARY, 2020, arXiv:2003.02375
- ^ KMT-2019-BLG-2073: Fourth Free-Floating-Planet Candidate with θE < 10 µas, 2020, arXiv:2007.06870
- ^ A free-floating or wide-orbit planet in the microlensing event OGLE-2019-BLG-0551, 2020, arXiv:2003.01126
- ^ Curiel, Salvador; Ortiz-León, Gisela N.; Mioduszewski, Amy J.; Torres, Rosa M. An Astrometric Planetary Companion Candidate to the M9 Dwarf TVLM 513–46546. The Astronomical Journal. 2020, 160 (3): 97. Bibcode:2020AJ....160...97C. S2CID 220961489. arXiv:2008.01595 . doi:10.3847/1538-3881/ab9e6e.
- ^ The CARMENES search for exoplanets around M dwarfs Measuring precise radial velocities in the near infrared: the example of the super-Earth CD Cet b, 2020, arXiv:2006.01684
- ^ OGLE-2018-BLG-0799Lb: a Sub-Saturn-Mass Planet Orbiting a Very Low Mass Dwarf, 2020, arXiv:2010.08732
- ^ Vanderburg, Andrew; Rappaport, Saul A.; Xu, Siyi; Crossfield, Ian J. M.; Becker, Juliette C.; Gary, Bruce; et al. A giant planet candidate transiting a white dwarf. Nature. September 2020, 585 (7825): 363–367. Bibcode:2020arXiv200907282V. PMID 32939071. S2CID 221738865. arXiv:2009.07282 . doi:10.1038/s41586-020-2713-y.
- ^ A Habitable-Zone Earth-Sized Planet Rescued from False Positive Status, 2020, arXiv:2004.06725
- ^ 138.00 138.01 138.02 138.03 138.04 138.05 138.06 138.07 138.08 138.09 138.10 138.11 138.12 138.13 138.14 138.15 138.16 138.17 138.18 138.19 138.20 138.21 138.22 138.23 138.24 138.25 138.26 138.27 138.28 138.29 138.30 138.31 138.32 138.33 138.34 138.35 138.36 138.37 138.38 138.39 138.40 138.41 138.42 138.43 138.44 138.45 138.46 138.47 Exoplanet Validation with Machine Learning: 50 new validated Kepler planets, 2020, arXiv:2008.10516
- ^ Vissapragada, Shreyas; Jontof-Hutter, Daniel; Shporer, Avi; Knutson, Heather A.; Liu, Leo; Thorngren, Daniel; Lee, Eve J.; Chachan, Yayaati; Mawet, Dimitri; Millar-Blanchaer, Maxwell A.; Nilsson, Ricky. Diffuser-Assisted Infrared Transit Photometry for Four Dynamically Interacting \textit{Kepler} Systems. The Astronomical Journal. 2020-02-13, 159 (3): 108. ISSN 1538-3881. doi:10.3847/1538-3881/ab65c8.
- ^ Exoplanet Archive. exoplanetarchive.ipac.caltech.edu. [2021-01-29]. （原始內容存檔於2020-10-31）.
