Exoplanet Catalog직접 촬영법으로 발견된 외계행성
| 행성 | 모항성 | 연도 | 거리(광년) | 공전 주기(일) | 반지름(지구 = 1) |
|---|---|---|---|---|---|
| HIP 54515 b | HIP 54515 | 2026 | 270.1 | 33,000.00 | 12.20 |
| KOINTREAU-1 b | XEST 17-036 | 2026 | 517.3 | – | 12.40 |
| KOINTREAU-3 b | ISO-Oph 96 | 2026 | 458.5 | – | 13.10 |
| KOINTREAU-4 b | 2MASS J16262785-2625152 | 2026 | 474.3 | – | 12.20 |
| WISPIT 2 c | WISPIT 2 | 2026 | 440.0 | – | 17.93 |
| bet Pic d | bet Pic | 2026 | 64.4 | 33,200.00 | 14.12 |
| CWISEP J193518.59-154620.3 b | CWISEP J193518.59-154620.3 | 2025 | 47.1 | – | 12.20 |
| HD 135344 A b | HD 135344 A | 2025 | 461.8 | – | 16.25 |
| HD 143811 AB b | HD 143811 A | 2025 | 445.6 | 117,000.00 | 15.69 |
| TWA 7 b | TWA 7 | 2025 | 110.9 | – | 12.70 |
| V2376 Ori b | V2376 Ori | 2025 | – | – | 87.21 |
| WISPIT 1 b | WISPIT 1 | 2025 | 750.2 | – | 12.40 |
| WISPIT 1 c | WISPIT 1 | 2025 | 750.2 | – | 12.80 |
| WISPIT 2 b | WISPIT 2 | 2025 | 440.0 | – | 17.93 |
| 2MASS J03590986+2009361 b | 2MASS J03590986+2009361 | 2024 | 383.0 | – | 12.20 |
| 2MASS J11011926-7732383 b | 2MASS J11011926-7732383 | 2024 | – | – | 11.90 |
| 2MASS J11550485-7919108 b | 2MASS J11550485-7919108 | 2024 | 329.0 | – | 12.10 |
| 2MASS J21252752-8138278 b | 2MASS J21252752-8138278 | 2024 | 111.3 | – | 12.40 |
| G 196-3 b | G 196-3 | 2024 | 71.1 | – | 12.00 |
| GJ 900 b | GJ 900 A | 2024 | 67.9 | – | 12.40 |
| HIP 39017 b | HIP 39017 | 2024 | 216.3 | 31,000.00 | 12.00 |
| HIP 77900 b | HIP 77900 | 2024 | 492.0 | – | 12.10 |
| ITG 15 b | ITG 15 A | 2024 | 444.8 | – | 12.10 |
| UCAC3 113-933 b | UCAC3 113-933 | 2024 | 171.5 | – | 12.10 |
| UCAC4 328-061594 b | UCAC4 328-061594 | 2024 | 130.2 | – | 12.10 |
| AF Lep b | AF Lep | 2023 | 87.6 | 8,905.00 | 13.00 |
| HD 169142 b | HD 169142 | 2023 | 370.5 | – | 13.10 |
| HIP 81208 C b | HIP 81208 C | 2023 | 481.2 | 104,100.00 | 12.30 |
| HIP 99770 b | HIP 99770 | 2023 | 130.7 | 18,600.00 | 12.20 |
| MWC 758 c | MWC 758 | 2023 | 520.3 | – | – |
| PZ Tel b | PZ Tel | 2023 | 153.5 | 44,000.00 | 11.90 |
| WISE J033605.05-014350.4 b | WISE J033605.05-014350.4 | 2023 | – | 2,560.00 | 12.60 |
| AB Aur b | AB Aur | 2022 | 528.8 | – | 12.50 |
| HD 206893 c | HD 206893 | 2022 | 132.9 | 2,290.00 | 16.37 |
| HIP 21152 b | HIP 21152 | 2022 | 141.6 | 22,000.00 | 12.00 |
| mu2 Sco b | mu2 Sco | 2022 | – | – | 12.30 |
| 2M0437 b | 2MASS J04372171+2651014 | 2021 | 419.1 | – | 13.00 |
| BD+60 1417 b | BD+60 1417 | 2021 | 146.6 | – | 14.68 |
| COCONUTS-2 b | COCONUTS-2 A | 2021 | 35.5 | 402,000,000.00 | 12.58 |
| HD 206893 b | HD 206893 | 2021 | 132.9 | 11,100.00 | 14.01 |
| b Cen AB b | b Cen A | 2021 | 319.9 | 1,790,000.00 | 12.40 |
| CFHTWIR-Oph 98 b | CFHTWIR-Oph 98 A | 2020 | – | 8,040,000.00 | 20.85 |
| TYC 8998-760-1 b | TYC 8998-760-1 | 2020 | 308.6 | – | 21.18 |
| TYC 8998-760-1 c | TYC 8998-760-1 | 2020 | 308.6 | – | 12.33 |
| HIP 79098 AB b | HIP 79098 AB | 2019 | 475.5 | – | 12.10 |
| PDS 70 c | PDS 70 | 2019 | 368.8 | – | 22.19 |
| USco1556 b | USco1556 A | 2019 | 458.7 | – | 12.30 |
| USco1621 b | USco1621 A | 2019 | 449.8 | – | 12.20 |
| 2MASS J0249-0557 c | 2MASS J0249-0557 A | 2018 | 215.5 | – | 17.37 |
| 2MASS J22501512+2325342 b | 2MASS J22501512+2325342 | 2018 | 186.7 | – | 11.90 |
| PDS 70 b | PDS 70 | 2018 | 368.8 | 43,500.00 | 21.97 |
| HD 284149 AB b | HD 284149 A | 2017 | 384.2 | – | 12.00 |
| HIP 65426 b | HIP 65426 | 2017 | 355.1 | – | 16.81 |
| Luhman 16 b | Luhman 16 A | 2017 | – | 9,697.00 | 11.90 |
| 2MASS J22362452+4751425 b | 2MASS J22362452+4751425 | 2016 | 226.9 | – | 12.30 |
| HR 2562 b | HR 2562 | 2016 | 110.9 | – | 12.44 |
| 2MASS J02192210-3925225 b | 2MASS J02192210-3925225 | 2015 | 130.8 | – | 16.14 |
| 51 Eri b | 51 Eri | 2015 | 97.1 | 9,100.00 | – |
| LkCa 15 b | LkCa 15 | 2015 | 515.8 | – | – |
| LkCa 15 c | LkCa 15 | 2015 | 515.8 | – | – |
| VHS J125601.92-125723.9 b | VHS J125601.92-125723.9 | 2015 | 41.4 | 5,800,000.00 | 13.67 |
| GU Psc b | GU Psc | 2014 | 155.1 | – | 14.18 |
| HD 100546 b | HD 100546 | 2014 | 357.7 | – | 77.34 |
| 2MASS J01033563-5515561 AB b | 2MASS J01033563-5515561 A | 2013 | 153.9 | – | 12.30 |
| 2MASS J01225093-2439505 b | 2MASS J01225093-2439505 | 2013 | 110.3 | – | 11.21 |
| GJ 504 b | GJ 504 | 2013 | 57.2 | – | 12.11 |
| HD 106906 b | HD 106906 | 2013 | 336.0 | – | 12.40 |
| HD 95086 b | HD 95086 | 2013 | 281.2 | – | 12.90 |
| ROXs 12 b | ROXs 12 | 2013 | 445.7 | – | 12.20 |
| ROXs 42 B b | ROXs 42 B | 2013 | 468.3 | – | 12.50 |
| WISEP J121756.91+162640.2 A b | WISEP J121756.91+162640.2 A | 2012 | 32.9 | – | 10.47 |
| kap And b | kap And | 2012 | 163.1 | – | 15.92 |
| CFBDSIR J145829+101343 b | CFBDSIR J145829+101343 | 2011 | 75.3 | 10,037.50 | 12.40 |
| WD 0806-661 b | WD 0806-661 | 2011 | 62.8 | – | 12.11 |
| 2MASS J04414489+2301513 b | 2MASS J04414489+2301513 | 2010 | 392.8 | – | 12.60 |
| GSC 06214-00210 b | GSC 06214-00210 | 2010 | 353.9 | – | 20.18 |
| HIP 78530 b | HIP 78530 | 2010 | 446.0 | – | 12.00 |
| HR 8799 e | HR 8799 | 2010 | 134.5 | 20,815.60 | 13.11 |
| Ross 458 c | Ross 458 | 2010 | 37.5 | – | 14.01 |
| SR 12 AB c | SR 12 AB | 2010 | 366.3 | – | 12.30 |
| 1RXS J160929.1-210524 b | 1RXS J160929.1-210524 | 2008 | 453.8 | – | 18.65 |
| FU Tau b | FU Tau | 2008 | 435.4 | – | 12.20 |
| HR 8799 b | HR 8799 | 2008 | 134.5 | 170,000.00 | 13.00 |
| HR 8799 c | HR 8799 | 2008 | 134.5 | 69,000.00 | 13.00 |
| HR 8799 d | HR 8799 | 2008 | 134.5 | 37,000.00 | 13.00 |
| USco CTIO 108 b | USco CTIO 108 | 2008 | 469.7 | – | 12.30 |
| bet Pic b | bet Pic | 2008 | 64.4 | 8,682.00 | 18.49 |
| CT Cha b | CT Cha | 2007 | 622.0 | – | 24.66 |
| CHXR 73 b | CHXR 73 | 2006 | 620.9 | – | 12.30 |
| HD 203030 b | HD 203030 | 2006 | 128.0 | – | 14.46 |
| HN Peg b | HN Peg | 2006 | 59.1 | – | 11.78 |
| LP 261-75 b | LP 261-75 A | 2006 | 110.7 | – | 12.10 |
| Oph 11 b | Oph 11 | 2006 | 444.1 | 7,300,000.00 | 12.30 |
| AB Pic b | AB Pic | 2005 | 163.2 | – | 12.30 |
| 2MASS J12073346-3932539 b | 2MASS J12073346-3932539 | 2004 | 209.7 | – | 15.69 |
| DH Tau b | DH Tau | 2004 | 439.8 | – | 30.26 |
| GQ Lup b | GQ Lup | 2004 | 493.0 | – | 33.60 |
값은 아카이브의 종합 매개변수로 여러 논문 값을 결합했을 수 있으며, 질량은 최소 질량(M·sin i)일 수 있습니다. “–”는 아카이브에 값이 없음을 뜻합니다.
이 페이지에 대해
직접 촬영법 방법으로 발견된 확인된 외계행성은 97개입니다.