2020년 발견된 외계 행성 목록
List of exoplanets discovered in 20202020년에 발견된 외계 행성 목록은 2020년에 처음 관측된 확인된 외계 행성의 목록입니다.
오직 방사 속도에 의해서만 감지되는 외계 행성의 경우, 질량에 대한 목록에 있는 값은 하한입니다. 자세한 내용은 최소 질량을 참조하십시오.
이름. | 질량()MJ | 반지름()RJ | 기간(일) | 반장축(AU) | 온도 (K) | 발견방법 | 거리(ly) | 주성질량()M☉ | 호스트 별 온도 (K) | 언급 |
---|---|---|---|---|---|---|---|---|---|---|
2MASS J1155-7919 b | 10 | 582 | 영상화 | 330 | [1] 아주 젊은 슈퍼주피터가 비정상적으로 넓은 궤도를 돌고 있습니다.[2] | |||||
AU 마이크로스코피 b | 0.054±0.015 | 0.371±0.016 | 8.463000±0.000002 | 0.0645±0.0013 | 593±21 | 환승의 | 31.718±0.015 | 0.50±0.03 | 3700±100 | [3][4][5][6] |
AU 마이크로스코픽 | 0.007 < AU Mic c < 0.079 | 0.295±0.014 | 18.859019±0.000016 | 0.1101±0.0022 | 454±16 | 환승의 | 31.718±0.015 | 0.50±0.03 | 3700±100 | [6] 거대 항성의 정확한 반지름 속도 |
BD-11 4672 c | 0.04837+0.00935 −0.00884 | 74.2+0.06 −0.08 | 0.30±0.01 | 방사형 벨 | 88.63±0.11 | 0.651+0.031 −0.029 | 4550±110 | 거주 가능 영역, 매우 편심된 궤도.[7] | ||
CD 고래자리 | 0.0124+0.0013 −0.0014 | 2.29070±0.00012 | 0.0185+0.0013 −0.0013 | 464±18 | 방사형 벨 | 28.07 | 0.161±0.010 | 3130±51 | [8] | |
CFHTWIR-Oph 98 b | 7.8+0.7 −0.8 | 1.86±0.04 | 8,040,000±470,000 | 200 | 1800±40 | 영상화 | 447±13 | 0.015±0.0008 | 2320±40 | 2MASS J16274422-2358521로[9] 알려진 갈색왜성 주위를 돌고 있는 아주 젊은 슈퍼조비안 행성 |
치 스콜피비브 | 4.32+0.15 −0.12 | 578.38+2.01 −2.09 | 1.45+0.02 −0.02 | 방사형 벨 | 378.3+16 −15 | 1.22+0.13 −0.14 | 4157+11 −10 | 거성 호스트[10][11] | ||
CoRoT-30b | 2.90±0.22 | 1.009±0.076 | 9.06005±0.00024 | 0.0844±0.0012 | 환승의 | 3130+220 −130 | 0.98+0.03 −0.05 | 5650±100 | [12] | |
CoRoT-31b | 0.84±0.34 | 1.46±0.30 | 4.62941±0.00075 | 0.0586±0.0034 | 환승의 | 7140±2300 | 1.25+0.22 −0.21 | 5700±120 | [12] | |
EPIC 201085153 b | 0.214±0.089 | 0.25722±0.000039 | 환승의 | 3945±386 | 극도로 촘촘한 궤도[13][citation needed] | |||||
EPIC 201085153 c | 0.125+0.179 −0.125 | 2.259797±0.0008 | 환승의 | 3945±386 | [13][citation 필요] | |||||
EPIC 201170410 b | 0.00362 | 0.09341+0.0246 −0.0229 | 6.7987±0.0001 | 0.0349+0.0027 −0.0022 | 환승의 | 437+149 −130 | 0.287+0.101 −0.084 | 3648+172 −143 | [14][15] | |
EPIC 201650711 c | 0.036±0.007 | 5.544059±0.00016 | 환승의 | 298.8±1.7 | 4310±92 | 3원성계, 행성 미확정[13][citation needed] | ||||
EPIC 201757695 b | 0.00217 | 0.08101+0.0052 −0.0057 | 2.0478±0.0001 | 0.0296±0.0005 | 환승의 | 1880±110 | 0.727+0.044 −0.053 | 4520+108 −54 | [14][16][17] | |
EPIC 205152172 b | 0.107±0.018 | 0.980088±0.000026 | 환승의 | 517±2 | 0.669±0.016 | 4202±242 | 2016년[13][citation needed] 이후의 후보자 | |||
EPIC 206298289 b | 0.078±0.009 | 0.434847±0.000022 | 환승의 | 492±6 | 3875±157 | 2016년[13][citation needed] 이후의 후보자 | ||||
EPIC 210801536 b | 0.088±0.027 | 0.892592±0.00012 | 환승의 | 5304±259 | 2019년 이후 후보, 시스템[13][citation needed] 내 행성 후보 1명 추가 | |||||
EPIC 220440058 b | 0.125±0.036 | 0.626683±0.00005 | 환승의 | 3682± | 행성[13][citation needed] 후보 하나가 더 있습니다 | |||||
EPIC 249893012 b | 0.02753±0.00343 | 0.174±0.008 | 3.5951±0.0003 | 0.047+0.005 −0.007 | 1616+150 −80 | 환승의 | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18] |
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 | 환승의 | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18] |
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 | 환승의 | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18][19] |
GJ 1061 b | 0.00431+0.00050 −0.00047 | 0.098 | 3.204±0.001 | 0.021±0.001 | 방사형 벨 | 11.98±0.003 | 0.12±0.01 | 2953±98 | 지구보다[20][21][22] 더 큰 잠재적인 암석 세계 | |
GJ 1061c | 0.00547±0.00072 | 0.105 | 6.689±0.005 | 0.035±0.001 | 방사형 벨 | 11.98±0.003 | 0.12±0.01 | 2953±98 | 지구보다[23][21][24] 더 큰 잠재적인 암석 세계 | |
GJ 1061 d | 0.00516+0.00076 −0.00072 | 0.104 | 13.031+0.025 −0.032 | 0.054±0.001 | 방사형 벨 | 11.98±0.003 | 0.12±0.01 | 2953±98 | 지구보다[25][21][26] 더 큰 잠재적인 암석 세계 | |
GJ 1252b | 0.0042±0.0009 | 0.105±0.007 | 0.5182349+0.0000063 −0.0000050 | 0.00915±0.00015 | 1410+91 −125 | 환승의 | 66.49±0.06 | 0.381±0.019 | 3458+140 −133 | [27] 지구보다[28][29] 더 큰, 대기가 없는 뜨거운 암석 행성 |
GJ 2056 b | 0.0510±0.011 | 0.372 | 69.971±0.061 | 0.283±0.0013 | 방사형 벨 | 92.8 | 0.62±0.08 | 인간이 거주할 수 있는 지역에[30][31] 있는 해왕성 같은 얼음 거인 | ||
GJ 3082 b | 0.02759+0.011 −0.01334 | 0.249 | 11.949±0.022 | 0.079+0.006 −0.007 | 방사형 벨 | 54.2 | 0.47 | 해왕성 같은 얼음 거인.[32][33][34] | ||
GJ 3473 b | 0.0059±0.0009 | 0.113+0.0045 −0.0044 | 1.1980035+0.0000018 −0.0000019 | 0.01589±0.00062 | 773+16 −15 | 환승의 | 89.29±0.13 | 0.360±0.016 | 3347±54 | TOI-488 b라고도[35] 불리는, 지구보다 더 큰 잠재적인 암석 세계 |
GJ 3473c | 0.0233+0.0029 −0.0027 | 0.235 | 15.509±0.033 | 0.0876+0.0035 −0.0034 | 329.1+6.6 −6.4 | 방사형 벨 | 89.29±0.13 | 0.360±0.016 | 3347±54 | TOI-488 c라고도[35][36][37] 불리는 해왕성 같은 얼음 거인 |
GJ 9689b | 0.0304±0.00444 | 0.274 | 18.27+0.01 −0.01 | 0.1139±0.0039 | 413.88-492.19 | 방사형 벨 | 100 | 0.59±0.06 | 3836±69 | 해왕성 같은 얼음 거인.[38][39] |
Gliese 180 d | 0.0236+0.00837 −0.00733 | 0.237 | 106.341+0.261 −0.34 | 0.31+0.024 −0.029 | 방사형 벨 | 39.96±0.01 | 0.43 | 3371 | 해왕성 같은 얼음 거인.[40][33] | |
Gliese 229 Ac | 0.0250+0.00752 −0.00733 | 0.256 | 122.005+0.364 −0.382 | 0.339+0.024 −0.029 | 방사형 벨 | 18.78±0.004 | 0.58 | 3564 | 해왕성 같은 얼음 거인.[41][42][43] | |
Gliese 251 b | 0.0126+0.00126 −0.00126 | 0.163 | 14.238+0.002 −0.002 | 0.0818+0.0011 −0.0012 | 351+1.4 −1.3 | 방사형 벨 | 18.205±0.006 | 0.360±0.015 | 3451±51 | 지구보다 더 큰, 잠재적인 바위 세상. |
Gliese 317 c | 1.664+0.118 −0.166 | 1.2 | 6718.777+375.180 −282.469 | 방사형 벨 | 49.25±0.72 | 0.42±0.05 | 3510±50 | 가스 거인[30][47] | ||
Gliese 414 Ab | 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 | 방사형 벨 | 38.8 | 0.650±0.08 | 4120±109 | 쌍성계의 주성 주위를 도는 행성들. Gl 414A는 HD 97101 및 HIP 546으로도 알려져 있습니다.[48] |
Gliese 414 Ac | 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 | 방사형 벨 | 38.8 | 0.650±0.08 | 4120±109 | 쌍성계의 주성 주위를 도는 행성들. Gl 414A는 HD 97101 및 HIP 546으로도 알려져 있습니다.[48] |
Gliese 433 d | 0.01643±0.00290 | 0.191 | 36.052+0.045 −0.031 | 0.178+0.013 −0.015 | 방사형 벨 | 29.57±0.01 | 0.48 | 3600 | 해왕성 같은 얼음 거인.[49][50][51] | |
Gliese 480 b | 0.042±0.005 | 0.33 | 9.567±0.005 | 0.068±0.001 | 방사형 벨 | 46.4 | 0.45±0.02 | 해왕성 같은 얼음 거인.[52][53][33] | ||
Gliese 687 c | 0.0503±0.013 | 0.369 | 727.562±12.198 | 1.165±0.023 | 방사형 벨 | 14.83 | 0.40±0.02 | 이 시스템에서 발견된 두 번째 해왕성 같은 얼음 거인. | ||
HAT-P-58b | 0.372±0.03 | 1.332±0.043 | 4.0138379±0.0000024 | 0.04994±0.00044 | 1622±18 | 환승의 | 1690±40 | 1.031±0.028 | 6078±48 | [55] |
HAT-P-59b | 1.540±0.067 | 1.123±0.013 | 4.1419771±0.0000012 | 0.05064±0.00037 | 1278±7 | 환승의 | 871±4 | 1.008±0.022 | 5678±16 | [55] |
HAT-P-60b | 0.574±0.038 | 1.631±0.024 | 4.7947813±0.0000024 | 0.06277±0.00017 | 1772±12 | 환승의 | 767±7 | 1.435±0.012 | 6212±26 | [55] |
HAT-P-61b | 1.057±0.07 | 0.899±0.027 | 1.90231289±0.00000077 | 0.03010±0.00034 | 1505±16 | 환승의 | 1120±20 | 1.004±0.012 | 5587±45 | [55] |
HAT-P-62b | 0.761±0.088 | 1.073±0.029 | 2.6453235±0.0000039 | 0.03772±0.00024 | 1512±13 | 환승의 | 1150±20 | 1.023±0.020 | 5629±48 | [55] |
HAT-P-63b | 0.614±0.024 | 1.119±0.033 | 3.377728±0.000013 | 0.04294±0.00035 | 1237±11 | 환승의 | 1330±20 | 0.925±0.023 | 5400+55 −39 | [55] |
HAT-P-64b | 0.58+0.18 −0.13 | 1.703±0.07 | 4.0072320±0.0000017 | 0.05387±0.00030 | 1766+22 −16 | 환승의 | 2135±20 | 1.298±0.021 | 6457+55 −36 | [55] |
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 | 환승의 | 662±3 | 0.6785+0.0299 −0.0079 | 4514±50 | [56] |
HATS-37Ab | 0.099±0.042 | 0.606±0.016 | 4.3315 | 0.1587+0.067 −0.075 | 1085+16 −12 | 환승의 | 695 | 0.843+0.017 −0.012 | 5247±50 | 적색왜성 하나[57] 더 |
HATS-38b | 0.074±0.011 | 0.614±0.0176 | 4.3750 | 0.1587+0.067 −0.075 | 1294±10 | 환승의 | 1131 | 0.890+0.016 −0.012 | 5740±50 | [57] |
HATS-47b | 0.369 | 1.117 | 3.9228 | 852.9 | 환승의 | 984.01±6.20 | 0.674 | [58] | ||
HATS-48Ab | 0.243 | 0.800 | 3.1317 | 0.03769±0.00011 | 954.6 | 환승의 | 865 | 0.7279 | 4546.0+23 −18 | [58][59] |
HATS-49b | 0.353 | 0.765 | 4.1480 | 834.8 | 환승의 | 1058.70±7.18 | 0.7133 | [58] | ||
HATS-72b | 0.1254 | 0.7224 | 7.3279 | 739.3 | 환승의 | 416.37±1.70 | 0.7311 | [58] | ||
HD 11231 b | 0.426+0.038 −0.052 | 5.2072+0.0002 −0.0055 | 0.0664±0.0005 | 1000 | 방사형 벨 | 437.0495±13.04625 | 1.44±0.03 | 6500±100 | DMPP-2[60] 열선화 행성을 찾는 분산 물질 행성 프로젝트에 의해 발견되었습니다. | |
HD 25723 b | 2.51 | 456.78 | 1.49 | 방사형 벨 | 375 | 2.1±0.3 | 거성 호스트[10] | |||
HD 25723 c | 1.33 | 2369.84 | 4.35 | 방사형 벨 | 375 | 2.1±0.3 | 거성 호스트[10] | |||
HD 38677 b | 18.57±0.01 | 0.1462±0.0012 | 877 | 방사형 벨 | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[60] 열선화 행성을 찾는 분산형 물질 행성 프로젝트에서 발견되었습니다. | ||
HD 38677 c | 6.584+0.003 −0.002 | 0.0733+0.0006 −0.0007 | 1239 | 방사형 벨 | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[60] 열선화 행성을 찾는 분산 물질 행성 프로젝트에 의해 발견된, 확인되지 않은 통과 행성의 2:1 궤도 공명.[61] | ||
HD 38677 d | 2.882±0.001 | 0.0422+0.0004 −0.0003 | 1632 | 방사형 벨 | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[60] 열선화 행성을 찾는 분산형 물질 행성 프로젝트에서 발견되었습니다. | ||
HD 38677 e | 5.516+0.002 −0.004 | 0.0651±0.0005 | 1314 | 방사형 벨 | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[60] 열선화 행성을 찾는 분산형 물질 행성 프로젝트에서 발견되었습니다. | ||
HD 42936 Ab | 2.58+0.35 −0.58 | 6.6732+0.0011 −0.0003 | 0.0662±0.0013 | 854 | 방사형 벨 | 159.4905±1.956938 | 0.87±0.05 | 5138±99 | DMPP-3[60] 열선화 행성을 찾는 분산 물질 행성 프로젝트에 의해 발견되었습니다. | |
HD 60292 b | 6.5±1.0 | 495.4±3.0 | 1.5±0.1 | 방사형 벨 | 1036±10 | 1.7±0.2 | 4348±28 | 거성 호스트[62] | ||
HD 63433 b | 0.017 | ±0.009 | 7.10801+0.00046 −0.00034 | 0.0710+0.0033 −0.0041 | 환승의 | 73.08±0.07 | 0.99±0.03 | 5640±74 | [63] | |
HD 63433 c | 0.0489 | 0.238±0.01 | 20.5455±0.001 | 0.1531+0.0074 −0.0092 | 환승의 | 73.08±0.07 | 0.99±0.03 | 5640±74 | [63][64][65] | |
HD 79211 b | 0.0334±0.004 | 24.422±0.014 | 0.142±0.005 | 345 | 방사형 벨 | 20.658±0.005 | 0.64±0.07 | 4005±51 | 쌍성 ADS 7251[66][67] 주위를 도는 주성 | |
HD 80653 b | 0.0176±0.0014 | 0.1439±0.0063 | 0.719573±0.000021 | 0.0166±0.0003 | 환승의 | 358.1197±2.641867 | 1.18±0.04 | [68] | ||
HD 86226 c | 0.023±0.004 | 0.193±0.007 | 3.98442±0.00018 | 0.049±0.001 | 1311±28 | 환승의 | 149 | 1.019+0.061 −0.066 | 5863±88 | [69] |
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 | 환승의 | 120 | 0.76+0.16 −0.1 | 5212+16 −11 | [70] |
HD108236 b | 0.1415±0.0087 | 3.79523+0.00047 −0.00044 | 0.0469±0.0017 | 1099+19 −18 | 환승의 | 211 | 0.97 | 5730±50 | [71] | |
HD108236 c | 0.1845+0.0089 −0.0081 | 6.2037+0.00064 −0.00052 | 0.0651±0.0024 | 932+17 −16 | 환승의 | 211 | 0.97 | 5730±50 | [71] | |
HD108236 d | 0.2423±0.0097 | 14.1756+0.001 −0.0011 | 0.1131±0.004 | 708+13 −12 | 환승의 | 211 | 0.97 | 5730±50 | [71] | |
HD108236 e | 0.279+0.012 −0.011 | 19.592±0.002 | 0.14±0.0052 | 636+12 −11 | 환승의 | 211 | 0.97 | 5730±50 | [71] | |
HD 100939 b | 7.1±1.6 | 2574.9±86.1 | 3.73±0.08 | 방사형 벨 | 400.4±1.9 | 1.04+0.07 −0.06 | 4769±55 | HIP 56640으로도[72][73] 알려진 적색 거성 호스트 항성 | ||
HD 112640 b | 5.0±1.0 | 613.2±5.8 | 1.7±0.1 | 방사형 벨 | 1065±6 | 1.8±0.2 | 4155±15 | 거성 호스트[62] | ||
HD 136295 b | 1.79±0.16 | 926.4±12.8 | 2.02±0.02 | 방사형 벨 | 269.0±1.3 | 1.28+0.11 −0.10 | 4891±50 | HIP 75092라고도[72] 알려진 적색 거성 | ||
HD 164922 d | 0.013±0.003 | 12.458±0.003 | 0.103±0.003 | 방사형 벨 | 72.1±0.9 | 0.874±0.012 | 5293±32 | [74] | ||
HD 170707 b | 1.96±0.09 | 453.9±2.0 | 1.26±0.01 | 방사형 벨 | 307.6±1.2 | 1.30±0.08 | 4884±58 | HIP 90988로도[72] 알려진 적색 거성 호스트 스타 | ||
HD 190007 b | 0.052±0.005 | 11.72 | 방사형 벨 | 41.47±0.03 | 0.77±0.02 | 4610±20 | [75] | |||
HD 191939 b | 0.03147±0.022 | 0.304±0.0067 | 8.880326 | 0.0804+0.0025 −0.0023 | 880±20 | 환승의 | 175 | 0.81±0.04 | 5348±100 | 호스트성은 TOI-1339로도[76][77][78] 알려져 있습니다. |
HD 191939 c | 0.02518±0.0031 | 0.285±0.0067 | 28.57974 | 0.1752+0.0055 −0.0050 | 600±13 | 환승의 | 175 | 0.81±0.04 | 5348±100 | 호스트성은 TOI-1339로도[76][77][78] 알려져 있습니다. |
HD 191939 d | 0.00881±0.0019 | 2.943±0.0062 | 38.35304 | 0.2132+0.0065 −0.0061 | 540±11 | 환승의 | 175 | 0.81±0.04 | 5348±100 | 호스트성은 TOI-1339로도[76][77][78] 알려져 있습니다. |
HD 216520 b | 0.032±0.003 | 35.45 | 방사형 벨 | 63.77±0.03 | 0.82±0.04 | 5103±20 | [75] | |||
HD 216520 c | 0.030±0.005 | 154.43 | 방사형 벨 | 63.77±0.03 | 0.82±0.04 | 5103±20 | [75] | |||
HD 219553 b | 1.94±0.17 | 1481.6±61.7 | 2.84±0.08 | 방사형 벨 | 332.9±1.7 | 1.39±0.09 | 4824±60 | HIP 114933으로도[72] 알려진 적색 거성 호스트 항성 | ||
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 | 방사형 벨 | 49.68±0.03 | 0.578±0.021 | 3933±51 | 쌍성계 글리제 458[45] 주위를 도는 주성 | |
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 | 환승의 | 262 | 1.127±0.077 | 6089+97 −96 | TOI 1456[79][80] |
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 | 환승의 | 201.85818±0.2609251 | 0.781±0.027 | 4590±49 | K4 왜성 주위를 도는 초단주기 [81][82][83][84]목성 |
HIP 38594 b | 0.026+0.012 −0.014 | 60.711+0.426 −0.192 | 0.256+0.006 −0.007 | 방사형 벨 | 58.0 | 0.61±0.02 | 거주할 수 있는 지역[53] | |||
HIP 38594 c | 0.135+0.077 −0.035 | 3525+541 −572 | 3.842+0.399 −0.441 | 방사형 벨 | 58.0 | 0.61±0.02 | [53] | |||
HIP4845b | 0.053+0.016 −0.028 | 34.151+0.17 −0.09 | 0.177+0.016 −0.020 | 방사형 벨 | 68.8 | 0.62±0.04 | [53] | |||
HIP 48714 b | 0.071+0.023 −0.020 | 17.819+0.004 −0.009 | 0.112±0.003 | 방사형 벨 | 34.3 | 0.58±0.02 | [53] | |||
HIP 67522 b | 0.25 | 0.894+0.048 −0.047 | 6.9596+0.000016 −0.000015 | 1174±21 | 환승의 | 416±4 | 1.22±0.05 | 5675±75 | 아주 어린(2천만 년 미만의 나이) 항성[85] 주위에 후보 행성 하나 더 | |
HIP 107772 b | 0.049+0.014 −0.030 | 55.259+0.111 −0.311 | 0.243+0.022 −0.027 | 방사형 벨 | 77.1 | 0.63±0.08 | 거주할 수 있는 지역[53] | |||
K2-85b | 0.107±0.009 | 0.684559±0.000026 | 환승의 | 317.8±1.2 | 4427±48 | EPIC 210707130 p1이라고도[13] 함 | ||||
K2-106c | 0.188±0.018 | 13.334621±0.000068 | 환승의 | 803±10 | 5613±39 | 2017년[13] 이후의 후보 | ||||
K2-111c | 0.0356±0.0035 | 15.6785+0.0064 −0.0063 | 0.1166±0.0025 | 방사형 벨 | 680±60 | 0.89±0.02 | 5730±50 | [86] | ||
K2-211c | 0.116±0.018 | 2.601404±0.000072 | 환승의 | 895±14 | 0.882+0.019 −0.027 | 5360±51 | [13] | |||
K2-282d | 0.232±0.027 | 27.248322±0.00047 | 환승의 | 1638.22±25.34 | 0.94±0.04 | 5499±109 | [13] | |||
K2-299c | 0.223±0.080 | 14.648966±0.000031 | 환승의 | 1219±16 | 5724±72 | EPIC 206024342 p2라고도[13] 함 | ||||
K2-299d | 0.152±0.054 | 4.507464±0.0000077 | 환승의 | 1219±16 | 5724±72 | EPIC 206024342 p3라고도[13] 함 | ||||
K2-301c | 0.152±0.018 | 5.2986±0.00035 | 환승의 | 1491±45 | 4114±99 | EPIC 206042996 p2라고도[13] 함 | ||||
K2-302c | 0.089±0.009 | 2.255438±0.000037 | 환승의 | 359.3±3.5 | 3297±73 | EPIC 206215704 p2라고도[13] 함 | ||||
K2-302d | 0.098±0.009 | 2.909216±0.000032 | 환승의 | 359.3±3.5 | 3297±73 | EPIC 206215704 p3라고도[13] 함 | ||||
K2-315b | 0.085±0.005 | 3.1443189±0.0000049 | 0.0234 | 460±5 | 환승의 | 185±1 | 0.174±0.004 | 3300±30 | 궤도 주기 때문에 "Pi Earth" 또는 EPIC 249631677b라고도[87] 불립니다. | |
K2-316b | 0.119 | 1.133 | 0.0147 | 841 | 환승의 | 368 | EPIC 249384674b[88] | |||
K2-316c | 0.163 | 5.260 | 0.0582 | 423 | 환승의 | 368 | EPIC 249384674c[88] | |||
K2-317b | 0.261 | 6.220 | 0.0542 | 432 | 환승의 | 577 | EPIC 249557502b[88] | |||
K2-318b | 0.148 | 7.010 | 0.0911 | 456 | 환승의 | 483 | EPIC 249826231b[88] | |||
K2-319b | 0.249 | 26.680 | 0.1516 | 641 | 환승의 | 686 | EPIC 201663879b[88] | |||
K2-320b | 0.234 | 1.995 | 0.0142 | 698 | 환승의 | 356 | EPIC 201796690b[88] | |||
K2-321b | 0.174 | 2.298 | 0.0410 | 701 | 환승의 | 254 | EPIC 248480671b[88] | |||
K2-322b | 0.171 | 8.205 | 0.0594 | 635 | 환승의 | 404 | EPIC 248558190b[88] | |||
K2-323b | 0.187 | 24.930 | 0.1275 | 318 | 환승의 | 387 | EPIC 248616368b[88] | |||
K2-324b | 0.217 | 3.262 | 0.0331 | 707 | 환승의 | 447 | EPIC 248639308b[88] | |||
K2-325b | 0.196 | 6.930 | 0.0419 | 423 | 환승의 | 365 | EPIC 246074965b[88] | |||
K2-326b | 0.203 | 1.256 | 0.0198 | 1114 | 환승의 | 928 | EPIC 246472939b[88] | |||
K2-329b | 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 | 환승의 | 760±9 | 0.912+0.048 −0.049 | 5282+40 −39 | EPIC 246193072 b라고도[89] 함 |
KELT-2019-BLG-1953 b | 0.59+0.71 −0.32 | 0.8+0.9 −0.6 | 마이크로렌즈 | 23000+3600 −4300 | 0.31+0.37 −0.17 | [90][91] | ||||
KELT-2019-BLG-1953 c | 0.28+0.35 −0.15 | 0.8+0.9 −0.7 | 마이크로렌즈 | 23000+3600 −4300 | 0.31+0.37 −0.17 | [92][91] | ||||
케플러-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 | 환승의 | 3140±60 | 0.88 | 5471+115 −37 | 다음은 2020년 9월에 운송 예정입니다.[93] | |
케플러-385d | 0.233 | 56.4159 | 환승의 | 4870±160 | [94] | |||||
케플러-305e | 0.160 | 3.20538 | 환승의 | 2900±90 | [94] | |||||
케플러-598c | 0.270 | 86.4945 | 환승의 | 2260±40 | FPP=1.0% | |||||
케플러-647c | 0.357 | 29.6663 | 환승의 | 3660±70 | [94] | |||||
케플러-716c | 0.124 | 3.96999 | 환승의 | 2110±30 | FPP=0.6% | |||||
케플러-783c | 0.208 | 7.05395 | 환승의 | 1707±15 | [94] | |||||
케플러-1001c | 0.140 | 9.18186 | 환승의 | 3110±80 | [94] | |||||
케플러-1085c | 0.291 | 56.7771 | 환승의 | 4630±150 | [94] | |||||
케플러-1514c | 0.1049+0.0051 −0.0039 | 10.514181±0.000039 | 0.0997±0.0018 | 1066+16 −14 | 환승의 | 1240 | 1.196+0.065 −0.063 | 6145+99 −80 | [95] | |
케플러-1661(AB) b | 0.053±0.038 | 0.345±0.005 | 175.06±0.06 | 0.633±0.005 | 243 | 환승의 | 1355.26±9.56 | 0.841±0.022 | 5100±100 | [96][97] |
케플러-1649c | 0.0038 | 0.095+0.014 −0.010 | 19.53527±0.00010 | 0.0649 | 234±20 | 환승의 | 301.6±1.6 | 0.1977±0.0051 | 3240±61 | 거주 가능 지역, 지구와[98] 같은 |
케플러-1662b | 0.223 | 0.790 | 134.4628 | 환승의 | [99] 주성은 KOI-1783으로도[100] 알려져 있습니다. | |||||
케플러-1663b | 0.294 | 17.6046 | 환승의 | 1112±11 | 주성은 KOI-252로도[94] 알려져 있습니다. | |||||
케플러-1664b | 0.270 | 14.3868 | 환승의 | 주성은 KOI-349로도[94] 알려져 있습니다. | ||||||
케플러-1665b | 0.253 | 11.9548 | 환승의 | 1104±5 | 주성은 KOI-650으로도[94] 알려져 있습니다. | |||||
케플러-1666b | 0.257 | 25.8476 | 환승의 | 4680±190 | 주성은 KOI-945로도[94] 알려져 있습니다. | |||||
케플러-1666c | 0.257 | 25.8476 | 환승의 | 4680±190 | 주성은 KOI-945로도[94] 알려져 있습니다. | |||||
케플러-1667b | 0.266 | 83.5781 | 환승의 | 2080±20 | 주성은 KOI-1311이라고도[94] 합니다. | |||||
케플러-1668b | 0.388 | 15.434 | 환승의 | 4500±200 | 주성은 KOI-1470으로도[94] 알려져 있습니다. | |||||
케플러-1669b | 0.248 | 9.51216 | 환승의 | 1800±40 | 주성은 KOI-1475로도[94] 알려져 있습니다. | |||||
케플러-1670b | 0.299 | 20.4998 | 환승의 | 7200±400 | 주성은 KOI-1705로도[94] 알려져 있습니다. | |||||
케플러-1671b | 0.118 | 4.16787 | 환승의 | 1176±7 | 주성은 KOI-1738로도[94] 알려져 있습니다. | |||||
케플러-1672b | 0.265 | 150.878 | 환승의 | 1189±14 | 주성은 KOI-1822로도[94] 알려져 있습니다. | |||||
케플러-1673b | 0.262 | 33.7888 | 환승의 | 2420±20 | 주성은 KOI-1863으로도[94] 알려져 있습니다. | |||||
케플러-1674b | 0.286 | 62.5611 | 환승의 | 3400±100 | 주성은 KOI-1892로도[94] 알려져 있습니다. | |||||
케플러-1675b | 0.279 | 63.0382 | 환승의 | 2163±19 | 호스트 스타 KOI-1928[94] | |||||
케플러-1676b | 0.301 | 29.9221 | 환승의 | 호스트 스타 KOI-1943[94] | ||||||
케플러-1677b | 0.241 | 22.064 | 환승의 | 2250±30 | 호스트 스타 KOI-1984, FPP=0.6% | |||||
케플러-1678b | 0.295 | 147.974 | 환승의 | 2830±70 | 호스트 스타 KOI-2066, FPP=0.5% | |||||
케플러-1679b | 0.184 | 9.75376 | 환승의 | 3040±100 | 주성은 KOI-2106이라고도[94] 합니다. | |||||
케플러-1680b | 0.121 | 8.77424 | 환승의 | 1020±5 | 호스트 스타 KOI-2120[94] | |||||
케플러-1681b | 0.2227 | 69.8956 | 환승의 | 2100±300 | 주성은 KOI-2132로도[94] 알려져 있습니다. | |||||
케플러-1682b | 0.257 | 14.8334 | 환승의 | 3900±160 | 주성은 KOI-2229라고도[94] 합니다. | |||||
케플러-1683b | 0.167 | 15.0337 | 환승의 | 2440±50 | 주성은 KOI-2293이라고도[94] 합니다. | |||||
케플러-1684b | 0.256 | 47.7055 | 환승의 | 2060±40 | 주성은 KOI-2417이라고도[94] 합니다. | |||||
케플러-1685b | 0.230 | 20.4905 | 환승의 | 3840±150 | 주성은 KOI-2504로도[94] 알려져 있습니다. | |||||
케플러-1686b | 0.127 | 9.30987 | 환승의 | 2430±30 | 주성은 KOI-2559로도[94] 알려져 있습니다. | |||||
케플러-1687b | 0.147 | 5.77954 | 환승의 | 1375±17 | 주성은 KOI-2588이라고도[94] 합니다. | |||||
케플러-1688b | 0.112 | 5.62012 | 환승의 | 1850±380 | 주성은 KOI-2733이라고도[94] 합니다. | |||||
케플러-1689b | 0.084 | 8.483 | 환승의 | 967±5 | 주성은 KOI-2755라고도[94] 합니다. | |||||
케플러-1690b | 0.250 | 234.636 | 환승의 | 2340±30 | 주성은 KOI-2757이라고도[94] 합니다. | |||||
케플러-1691b | 0.163 | 3.8482 | 환승의 | 4290±110 | 주성은 KOI-2802로도[94] 알려져 있습니다. | |||||
케플러-1692b | 0.099 | 5.95966 | 환승의 | 1960±20 | 주성은 KOI-2849라고도[94] 합니다. | |||||
케플러-1693b | 0.115 | 12.0999 | 환승의 | 2530±50 | 주성은 KOI-2871이라고도[94] 합니다. | |||||
케플러-1694b | 0.105 | 3.89526 | 환승의 | 1698±16 | 호스트 스타 KOI-2878, FPP=0.6% | |||||
케플러-1695b | 0.099 | 4.7329 | 환승의 | 2640±40 | 호스트 스타 KOI-3048, FPP=0.5% | |||||
케플러-1696b | 0.250 | 65.9409 | 환승의 | 5100±200 | 주성은 KOI-3361이라고도[94] 합니다. | |||||
케플러-1697b | 0.112 | 33.4969 | 환승의 | 813±2 | 주성은 KOI-3478이라고도[94] 합니다. | |||||
케플러-1698b | 0.095 | 1.2107 | 환승의 | 729±3 | 주성은 KOI-3864로도[94] 알려져 있습니다. | |||||
케플러-1699b | 0.139 | 3.49082 | 환승의 | 주성은 KOI-3933이라고도[94] 합니다. | ||||||
케플러-1701b | 0.198 | 169.134 | 환승의 | 1940±20 | 주성 KOI-4054, [94]외계 행성 거주 가능성 | |||||
케플러-1702b | 0.143 | 18.5012 | 환승의 | 2860±90 | 주성은 KOI-4386이라고도[94] 합니다. | |||||
KMT-2016-BLG-2397b | 2.42 | 2.83 | 마이크로렌즈 | 16000 | 0.62+0.29 −0.30 | 행성 매개변수에[101] 대한 여러 솔루션 | ||||
KMT-2016-BLG-2364b | 3.93 | 2.63 | 마이크로렌즈 | 21000 | 0.50+0.40 −0.22 | [101] | ||||
KMT-2018-BLG-0748Lb | 0.18+0.29 −0.10 | 0.62±0.09 | 마이크로렌즈 | 24000 | 0.0870+0.138 −0.047 | [102] | ||||
KMT-2019-BLG-1339Lb | 12.2+16.1 −6.7 | 0.67+0.77 −0.55 | 마이크로렌즈 | 23000±3000 | 0.27+0.366 −0.15 | 행성 매개변수에[103] 대한 여러 솔루션 | ||||
KMT-2019-BLG-2073 | 0.19 | 마이크로렌즈 | 12000 | 자유롭게 떠다니는 행성[104] | ||||||
L 168-9b | 0.0145±0.00176 | 0.124±0.008 | 1.4015±0.00018 | 0.02091±0.00024 | 816±160 | 환승의 | 82.02833±0.07827753 | 0.62±0.03 | 3800±70 | [105] |
라카유 9352b | 0.0132±0.0019 | 0.168 | 9.262±0.001 | 0.068±0.002 | 468 | 방사형 벨 | 10.721±0.002 | 0.468±0.012 | 3688±86 | GJ 887b라고도[106][107] 알려진 지구보다 더 큰 잠재적인 암석 세계 |
라카유 9352c | 0.0234±0.0038 | 0.238 | 21.789+0.004 −0.005 | 0.120±0.004 | 352 | 방사형 벨 | 10.721±0.002 | 0.468±0.012 | 3688±86 | 지구보다 더 큰 잠재적인 거주 가능성, GJ 887c로도[106][108] 알려져 있습니다. |
LHS 1815 b | 0.0132±0.0047 | 0.0971±0.005 | 3.81433±0.00003 | 0.0404±0.0094 | 617±84 | 환승의 | 97 | 0.502 | 3643±142 | [109][110] |
LP 714-47 b | 0.097±0.005 | 0.420±0.027 | 4.052037±0.000004 | 0.0417±0.0005 | 700+19 −24 | 환승의 | 171.8±0.4 | 0.59±0.02 | 3950±51 | G 160-62 또는 TOI 442로도 알려진 호스트성, 해왕성 사막의[111] 행성 |
LTT 9779 b | 0.092±0.003 | 0.421±0.021 | 0.792054±0.000014 | 0.01679±0.0014 | 2000 | 환승의 | 262.8±1.0 | 1.02+0.02 −0.03 | 5499±50 | 해왕성 사막 행성[112] |
MOA-2009-BLG-319Lb | 0.2077±0.0255 | 2.03±0.21 | 마이크로렌즈 | 22800±2300 | 0.514±0.063 | [113] | ||||
NGTS-11b | 0.37±0.14 | 0.823±0.035 | 35.4553±0.0002 | 0.201±0.002 | 440±40 | 환승의 | 624±6 | 0.862±0.028 | 5050±80 | [114] |
NGTS-12b | 0.208±0.022 | 1.048±0.032 | 7.532806±0.000048 | 0.0757±0.0014 | 1257±34 | 환승의 | 1474±25 | 1.021+0.056 −0.049 | 5690±130 | [115] |
OGLE-2006-BLG-284 b | 0.45+0.14 −0.40 | 2.2±0.8 | 마이크로렌즈 | 13000±4900 | 0.35+0.3 −0.2 | 2.1 천문단위 분리와 불확실하고 불안정한 행성 궤도를 가진 쌍성 호스트.[116] | ||||
OGLE-2016-BLG-1928 | 0.001 | n/a | 마이크로렌즈 | 30000 | n/a | n/a | 불량 행성[117] | |||
OGLE-2017-BLG-0406 b | 0.41±0.05 | 3.5±0.3 | 마이크로렌즈 | 17000± | 0.56±0.07 | 4848 | 고충실도 마이크로렌즈 이벤트[118] | |||
OGLE-2017-BLG-0604b | 0.51 | 4.06 | 마이크로렌즈 | 13000 | 0.70±0.28 | [101] | ||||
OGLE-2017-BLG-1049Lb | 5.53+3.62 −2.87 | 3.92+1.10 −1.32 | 마이크로렌즈 | 18500+3600 −4500 | 0.55+0.36 −0.29 | [119] | ||||
OGLE-2017-BLG-1375b | 10.33 | 2.97 | 마이크로렌즈 | 12000 | 0.77+0.27 −0.23 | 행성 매개변수에[101] 대한 여러 솔루션 | ||||
OGLE-2018-BLG-0677Lb | 0.0125+0.0185 −0.0084 | 0.68+0.27 −0.22 | 마이크로렌즈 | 27000±3500 | 0.12+0.14 −0.08 | 은하 팽대부[120] | ||||
OGLE-2018-BLG-1269Lb | 0.69+0.44 −0.22 | 4383 | 4.61+1.70 −1.17 | 마이크로렌즈 | 8300+3000 −2000 | 0.35+0.3 −0.2 | 매우 높은 충실도 이벤트[121] | |||
OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 | 1.27+0.45 −0.29 | 마이크로렌즈 | 16000 | 0.08+0.08 −0.02 | [122][123] | ||||
OGLE-2019-BLG-0551 | 0.0242 | 마이크로렌즈 | 특성이 좋지 않은 자유 부유 행성[124] | |||||||
센타우루스자리 프록시마 c | 0.0179±0.006 | 1928±20 | 1.489±0.049 | 39+16 −18 | 방사형 벨 | 4.244±0.001 | 0.1221±0.0022 | 3042±117 | [125][126] 태양계에서 가장 가까운 별 주위를 도는 두 번째 행성 발견 | |
TIC 237913194b | 1.942+0.092 −0.091 | 1.117+0.054 −0.047 | 15.168865±0.000018 | 0.1207±0.0037 | 974 | 환승의 | 1009±6 | 1.026+0.057 −0.055 | 5788±80 | 매우 편심한[127] 궤도 |
TOI 122b | 0.028+0.029 −0.010 | 0.243±0.016 | 5.078030±0.000015 | 0.0392±0.0007 | 471 | 환승의 | 202.9±0.7 | 0.312±0.007 | 3403±100 | [128] |
TOI-132b | 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 | 환승의 | 536.43±89.11 | 0.970±0.06 | 5397±46 | [129] |
TOI-157b | 1.18±0.13 | 1.29±0.02 | 2.0845435±0.0000023 | 0.03138+0.00025 −0.00020 | 1588+21 −20 | 환승의 | 1171 | 0.948+0.023 −0.018 | 5404+70 −67 | [81] |
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 | 환승의 | 1345 | 1.147+0.069 −0.075 | 5880+54 −49 | [81] |
TOI 237b | 0.009+0.006 −0.003 | 0.128±0.011 | 5.436098±0.000039 | 0.0341±0.0010 | 388 | 환승의 | 124.2±0.7 | 0.179±0.004 | 3212±100 | [128] |
TOI-251b | 0.245±0.016 | 4.937770+0.000028 −0.000029 | 0.05741+0.00023 −0.00017 | 환승의 | 324.4±1.4 | 1.036+0.013 −0.009 | 5875+100 −190 | [130] | ||
TOI-257b | 0.134±0.023 | 0.626±0.013 | 18.38827±0.00072 | 0.1523±0.0017 | 1033±19 | 환승의 | 251.37±0.065 | 1.38+0.056 −0.009 | 6075±90 | 호스트 스타는 HD 19916이라고도 불립니다.[131][132][133] |
TOI-260b | 0.009+0.013 −0.009 | 0.157±0.027 | 13.478048±0.005188 | 환승의 | 65.84±0.07 | HIP 1532, BD-1047이라고도[134] 불리는 호스트 스타 | ||||
TOI-421b | 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 | 환승의 | 244.3±1.9 | 0.852+0.029 −0.021 | 5325+78 −58 | 또한 2200 a.u. 떨어져[135] 있는 적색 왜성 |
TOI-421c | 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 | 환승의 | 244.3±1.9 | 0.852+0.029 −0.021 | 5325+78 −58 | 또한 2200 a.u. 떨어져[135] 있는 적색 왜성 |
TOI-481b | 1.53±0.03 | 0.99±0.01 | 10.33111±0.00002 | 0.097±0.001 | 1370±10 | 환승의 | 587 | 1.14+0.02 −0.01 | 5735±72 | [136] |
TOI-519b | <14 | 0.75±0.21 | 1.2652328±0.0000005 | 0.012±0.004 | 760±54 | 환승의 | 378±3 | 0.369+0.026 −0.097 | 3350+100 −200 | 매우 희미한 17등급의 호스트성[137] |
TOI 540 b | 0.081±0.005 | 1.2391491±0.0000017 | 0.01223±0.00036 | 611±23 | 환승의 | 45.67±0.29 | 0.159±0.014 | 3216±83 | [138] | |
TOI-561b | 0.0050±0.0011 | 0.127±0.006 | 0.446578±0.000017 | 0.01055±0.00008 | 환승의 | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 | [139][140] | |
TOI-561c | 0.017±0.003 | 0.257±0.009 | 10.779±0.004 | 0.08809±0.0007 | 환승의 | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 | [139][140] | |
TOI-561d | 0.038±0.004 | 0.226±0.011 | 25.62±0.04 | 0.1569±0.0012 | 환승의 | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 | [139][140] | |
TOI-561e | 0.050±0.007 | 0.238±0.010 | 77.23±0.39 | 0.3274+0.0028 −0.0027 | 환승의 | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 | [139] | |
TOI-700b | 0.00406+0.003 −0.00116 | 0.0901+0.00839 −0.00776 | 9.97701+0.00024 −0.00028 | 0.0637+0.0064 −0.006 | 환승의 | 101.5 | 0.416±0.01 | 3480±135 | [141] | |
TOI-700c | 0.0249+0.0085 −0.0057 | 0.2346+0.0214 −0.0205 | 16.051998+0.000089 −0.000092 | 0.0925+0.0088 −0.0083 | 환승의 | 101.5 | 0.416±0.01 | 3480±135 | [141] | |
TOI-700d | 0.00711+0.0022 −0.00164 | 0.1062±0.0098 | 37.426+0.0007 −0.001 | 0.163±0.015 | 295±55 | 환승의 | 101.5 | 0.416±0.01 | 3480±135 | TESS에[141][142] 의해 최초로 발견된 "지구 크기" |
TOI-732b | 0.098 | 0.119 | 0.7683881 | 0.012 | 892 | 환승의 | 72 | 0.379 | 3360 | 쌍성 LDS 3977[143][144] 주위를 도는 주성 |
TOI-732c | 0.027 | 0.205 | 12.25 | 0.07673 | 323 | 환승의 | 72 | 0.379 | 3360 | 쌍성 LDS 3977[143][144] 주위를 도는 주성 |
TOI-763b | 0.031±0.002 | 0.203±0.010 | 5.6057±0.0013 | 0.0600±0.0006 | 1038±16 | 환승의 | 311 | 0.917±0.028 | 5444±110 | [145] |
TOI-763c | 0.029±0.003 | 0.235±0.011 | 12.2737+0.0053 −0.0077 | 0.1011±0.0010 | 800±12 | 환승의 | 311 | 0.917±0.028 | 5444±110 | [145] |
TOI-763d | 0.030±0.005 | 47.7991±2.7399 | 0.2504+0.0093 −0.0105 | 509±12 | 방사형 벨 | 311 | 0.917±0.028 | 5444±110 | [145] | |
TOI-776b | 0.0147±0.0031 | 0.163±0.010 | 8.24664+0.00009 −0.00006 | 0.0652±0.0011 | 513±12 | 환승의 | 88.6±0.1 | 0.544±0.028 | 3709±70 | [146] |
TOI-776c | 0.0192±0.0047 | 0.184±0.012 | 15.6653+0.0008 −0.0007 | 0.1000±0.0017 | 415±10 | 환승의 | 88.6±0.1 | 0.544±0.028 | 3709±70 | [146] |
TOI-784b | 0.031±0.004 | 0.171±0.015 | 2.797179±0.000158 | 환승의 | 211±0.4 | HD 307842라고도[134] 불리는 항성 | ||||
TOI-813b | 0.599±0.034 | 83.8911+0.0027 −0.0031 | 0.423+0.031 −0.037 | 610+28 −21 | 환승의 | 864.8192±5.156379 | 1.32±0.06 | 5907±150 | [147] | |
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 | 환승의 | 208 | 0.69+0.009 −0.007 | 4569±50 | 넵투니아 사막 행성,[148] 수소 외피가[149] 벗겨졌을 가능성 |
TOI-892b | 0.95±0.07 | 1.07±0.02 | 10.62656±0.00007 | 0.092±0.005 | 1397±40 | 환승의 | 1120 | 1.28+0.03 −0.02 | 6261±80 | [136] |
TOI-836b | 0.0143±0.0028 | 0.152±0.006 | 3.81673±0.00001 | 0.04220±0.00093 | 871±36 | 환승의 | 89.72±0.09 | 0.678+0.049 −0.041 | 4552±154 | HIP 73427, CD-23 12010이라고도 불리는[134][150] 호스트 스타 |
TOI-836c | 0.0302±0.0082 | 0.231±0.008 | 8.59545±0.00001 | 0.0750±0.0016 | 665±27 | 환승의 | 89.72±0.09 | 0.678+0.049 −0.041 | 4552±154 | HIP 73427, CD-23 12010이라고도 불리는[134][150] 호스트 스타 |
TOI 837 b | <1.2 | 0.768+0.091 −0.072 | 8.3248762±0.0000157 | 환승의 | 466.5±1.2 | 1.118±0.059 | 6047±162 | 오픈 클러스터 IC 2602에[151] 속해 있습니다. | ||
TOI-849b | 0.128±0.008 | 0.308+0.014 −0.011 | 0.7655240±0.0000027 | 0.01598±0.00013 | 1800 | 환승의 | 735 | 0.929±0.023 | 5329±48 | 넵투니아 사막 행성[152] |
TOI-942b | 0.429±0.018 | 4.324190±0.00003 | 0.04796+0.00073 −0.00065 | 환승의 | 498±2 | 0.788+0.037 −0.031 | 4928+125 −85 | [130][153] 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 | 환승의 | 498±2 | 0.788+0.037 −0.031 | 4928+125 −85 | [130][153] Host star TYC 5909-319-1 | ||
TOI-954b | 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 | 환승의 | 768.5±8.3 | 1.201+0.066 −0.064 | 5710+53 −49 | [89] |
TOI-1130b | 0.3256±0.009 | 4.066499±0.000046 | 0.04394+0.00035 −0.00038 | 876±17 | 환승의 | 190 | 0.684+0.16 −0.17 | 4250±67 | [154][155] | |
TOI-1130c | 0.974+0.043 −0.044 | 1.5+0.27 −0.22 | 8.350381±0.000033 | 0.07098+0.00056 −0.0006 | 637±12 | 환승의 | 190 | 0.684+0.16 −0.17 | 4250±67 | [154][156] |
TOI-1235b | 0.0217±0.00025 | 0.155±0.007 | 3.444729+0.000031 −0.000028 | 0.03845+0.00037 −0.0004 | 754±18 | 환승의 | 129 | 0.640±0.016 | 3872±70 | 지구상에[157] 또 하나의 의심스러운 행성. |
TOI-1266b | 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 | 환승의 | 117.5±0.1 | 0.48±0.1 | 3570±100 | [158][159] |
TOI-1266c | 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 | 환승의 | 117.5±0.1 | 0.48±0.1 | 3570±100 | [158] 증기의[160][159] 분위기일 가능성 |
TOI-1338b | 0.10382±0.0622 | 0.61±0.0169 | 95.2 | 0.4607 | 724 | 환승의 | 1301 | TESS에[161] 의해 최초로 발견된 반원형 행성 | ||
TOI-1728b | 0.084+0.017 −0.016 | 0.450±0.014 | 3.491510+0.000062 −0.000057 | 0.0391±0.0009 | 767±8 | 환승의 | 198.2±0.5 | 0.646+0.023 −0.022 | 3980+31 −32 | [162] |
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 | 환승의 | 419±1 | 0.627+0.026 −0.028 | 3841+54 −45 | [163][164] |
TVLM 513-46546 b | 0.38±0.24 | 221±5 | 0.3±0.0036 | 측도법 | 34.90±0.07 | 0.09 | 2500 | [165] | ||
TYC 8998-760-1 c | 6±1 | 1.1+0.6 −0.3 | 320 | 1240+160 −170 | 영상화 | 309.4±0.9 | 4783 | [166] | ||
USco1621 b | 16 | 2880 | 2270 | 영상화 | 450 | 0.36 | 3460 | [167] | ||
USco1556 b | 15 | 3500 | 2240 | 영상화 | 459 | 0.33 | 3410 | [167] | ||
XO-7b | 0.709 | 1.373 | 2.8641424 | 0.04421 | 1743 | 환승의 | 763 | 1.405 | 6250 | [168] |
WASP-148b | 0.291±0.025 | 0.722±0.055 | 8.80381±0.000043 | 0.22±0.063 | 940±80 | 환승의 | 809±5 | 1.00±0.08 | 5460±130 | [169][170] |
WASP-148c | 0.397+0.203 −0.044 | 34.515±0.029 | 0.359±0.086 | 590±50 | 방사형 벨 | 809±5 | 1.00±0.08 | 5460±130 | [169][170] | |
WASP-150b | 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 | 환승의 | 2422 | 1.394+0.07 −0.049 | 6218+49 −45 | [171] |
WASP-176b | 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 | 환승의 | 1883 | 1.345+0.08 −0.13 | 5941+77 −79 | [171] |
WASP-186b | 4.22±0.18 | 1.11±0.03 | 5.026799+0.000012 −0.000014 | 0.0600+0.0012 −0.0013 | 1348+23 −22 | 환승의 | 913±11 | 1.22+0.07 −0.08 | 6361+105 −82 | TOI-1494라고도[172] 함 |
WASP-187b | 0.80±0.09 | 1.64±0.05 | 5.147878+0.000005 −0.000009 | 0.0653±0.0013 | 1726+31 −2 | 환승의 | 1224±21 | 1.54±0.09 | 6150+92 −85 | TOI-1493이라고도[172] 함 |
웬델슈타인-1b | 0.59+0.17 −0.13 | 1.0314+0.00204 −0.021 | 2.663416±0.000001 | 0.0282±0.0009 | 1727+78 −90 | 환승의 | 1004±10 | 0.65±0.1 | 3984+152 −46 | [173] |
웬델슈타인-2b | 0.731+0.541 −0.311 | 1.1592±0.0061 | 1.7522239±0.0000008 | 0.0234±0.0015 | 1852+120 −140 | 환승의 | 1875±20 | 0.73±0.11 | 4288+133 −111 | 확장기체외피[173] |
WD 1856+534 b | 13.8 | 0.93±0.09 | 1.4079405±0.0000011 | 0.0204±0.0012 | 환승의 | 80.737±0.144 | 0.518±0.055 | 4710±60 | 백색 왜성[174] 주위를 도는 것 |
외계 행성 목록
- 직접 촬영한 외계 행성 목록
- 외계 행성의 극값 목록
- 외계 행성 최초의 목록
- 케플러 우주망원경에 의해 발견된 외계 행성 목록
- 케플러의 K2 임무 수행 중 관측된 외계 행성 목록
- 액체 상태의 물에 대한 외계인 후보 목록
- 가장 뜨거운 외계 행성 목록
- 다중 행성계 목록
- 가장 가까운 외계 행성 목록
- 지구에서 가장 가까운 외계 행성 후보 목록
- 외계 행성 목록
- 외계 행성의 고유 명칭 목록
- 가장 작은 외계 행성 목록
- 외계행성 목록
외계 행성 목록
- 2000년 이전에 발견된 외계 행성 목록 (31)
- 2000년에서 2009년 사이에 발견된 외계 행성 목록
- 2010년 발견된 외계 행성 목록 (109)
- 2011년 발견된 외계 행성 목록 (179)
- 2012년 발견된 외계 행성 목록 (149)
- 2013년 발견된 외계 행성 목록 (151)
- 2014년 발견된 외계 행성 목록 (878)
- 2015년 발견된 외계 행성 목록 (151)
- 2016년 발견된 외계 행성 목록 (1513년)
- 2017년 발견된 외계 행성 목록 (158)
- 2018년 발견된 외계 행성 목록 (306)
- 2019년 발견된 외계 행성 목록 (172개)
- 2020년 발견된 외계 행성 목록 (258)
- 2021년 발견된 외계 행성 목록 (248)
- 2022년 발견된 외계 행성 목록 (315)
- 2023년 발견된 외계 행성 목록 (126)
참고문헌
- ^ exoplanet.eu 플래닛2MASS J1155-7919 b
- ^ www.sci-news.com 천문학자들이 가장 가까운 곳에 알려진 신생 가스 거인을 발견했습니다.
- ^ Plavchan, Peter; Barclay, Thomas; Gagné, Jonathan; et al. (2020). "A planet within the debris disk around the pre-main-sequence star AU Microscopii". Nature. 582 (7813): 497–500. arXiv:2006.13248. Bibcode:2020Natur.582..497P. doi:10.1038/s41586-020-2400-z. PMC 7323865. PMID 32581383. S2CID 220042005.
- ^ 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 (2021), "The Youngest Planet to Have a Spin-Orbit Alignment Measurement AU Mic B", The Astronomical Journal, 162 (4): 137, arXiv:2006.13675, Bibcode:2021AJ....162..137A, doi:10.3847/1538-3881/ac1685, S2CID 220041674
{{citation}}
: CS1 메인트: 플래그 없는 무료 DOI(링크) - ^ 태양계외 행성 카탈로그 AU 마이크로스코피 b exoplanets.nasa.gov
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