最近類地太陽系外行星列表
外观
最近類地太陽系外行星列表中包含距離地球50光年內的類地(岩石)太陽系外行星系統。
他們主要可能由矽酸鹽岩石和(或)金屬所構成。類地行星在太陽系中是最接近太陽的內行星。
大多數列表中的行星的陸地成分尚未有科學共識,表中僅列出可能的陸地成分。
2012年9月,天文學家宣布[1][2] 發現兩個行星環繞格利澤163[3],其中一顆格利澤163c,質量約地球的6.9倍,比地球還熱,被認為位於適居帶中[1][2]。
名稱 | 圖片(想像圖) | 質量(M⊕) | 半徑(R⊕) | 密度 | 表面重力 (g) | 表面溫度 | 半長軸 (AU) | 離心率 | 地球相似指數 | 適居性 | 參考 | 主星 | 與太陽的距離(ly) |
比鄰星b | ≥1.27 | ~1.1 | 234 K | 0.05 | <0.35 | 位於適居帶中 | [4] | 比鄰星 | 4.22 | ||||
比邻星c | 7 | 39 K -234.2 °C |
1.489 | 0.04 | 比鄰星 | 4.22 | |||||||
半人馬座α Bb | ≥1.1 | 1200 K | 0.04 | 半人馬座α B | 4.23 | ||||||||
巴納德星b | ≥3.23 | 105 K -168.15 °C |
0.404 | 0.32 | [5] | 巴納德星 | 5.958 | ||||||
羅斯128b | ≥1.35 | ~1.1 | 羅斯128 | 10.89 | |||||||||
魯坦b | ≥2.89 | ≥1.35 | 259 K -14 °C |
0.091 | 0.10 | 魯坦星 | 12.20 | ||||||
沃夫1061b | ≥1.36 | ≥1.44 | 沃夫1061 | 13.8 | |||||||||
沃夫1061c | ≥4.3 | ≥1.64 | [6] | 沃夫1061 | 13.8 | ||||||||
沃夫1061d | ≥5.21 | ≥2.04 | 沃夫1061 | 13.8 | |||||||||
葛利斯876d[7] | 6.8 | 157 – 377 °C[8] |
0.021 | 0.21 | 估計表面溫度: 157-377°C[8] | [9] | 葛利斯876 | 15 | |||||
格利泽682b | ≥2 | [10] [11] [6] |
格利泽682 | 16 | |||||||||
葛利斯832c | ≥5.4 | 295 K 22 °C |
0.162 | 0.03 | [12][13] | 葛利斯832 | 16.16 | ||||||
天园增三b | ≥2.7 | 660 K 387 °C[14] |
0.1207 | 0 | [15] | 天园增三 | 19.71 | ||||||
天园增三c | ≥2.4 | 508 K 235 °C[14] |
0.2036 | 0 | [15] | 天园增三 | 19.71 | ||||||
天园增三d | ≥4.8 | 388 K 115 °C[14] |
0.3499 | 0 | [15] | 天园增三 | 19.71 | ||||||
葛利斯581e | ≥1.7 | 0.029 | 0 | 表面溫度過高,可能沒有大氣層存在 | [16] | 葛利斯581 | 20 | ||||||
葛利斯581c [17] | ≥5.6 | 0.072 | 0 | 公轉軌道可能位於適居帶外側[18] | [19] | 葛利斯581 | 20 | ||||||
葛利斯581d [20] | ≥5.6 | 2.34[21] | 1.27[21] | 233 K[21] | 0,218 | 0 | 0.69[21] | 可能是一顆海洋行星[21]位於適居帶中[22] | [23] | 葛利斯581 | 20 | ||
HD 219134 b | 4.5 | 1.6 | 700 K 427 °C |
[24] | HD 219134 | 21 | |||||||
葛利斯667Cc[25][26] | 5.24 | 1.99 | 1.32 | 302 K | 0.13 | 0.34 | 0.82 | 位於適居帶中 | [21] | 葛利斯667C | 22 | ||
室女座61b[27] | ≥5.1 | 0.050 | 0.12 | 公轉軌道太過接近恆星 | [28] | 室女座61 | 28 | ||||||
HD 85512 b[29] | ≥3.6 | 1.74[21] | 1.33[21] | 351 K[21] | 0.26 | 0.11 | 0.76[21] | 曾被認為是最適合人類居住的行星[21][30]直到發現葛利斯667Cc為止 | [30] | HD 85512 | 36 | ||
GJ 180 b | ≥2.3 | 312 K 39 °C |
[10][12] | 葛利斯180 | 38 | ||||||||
TRAPPIST-1b | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1c | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1d | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1e | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1f | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1g | [31] | TRAPPIST-1 | 39.5 | ||||||||||
TRAPPIST-1h | [31] | TRAPPIST-1 | 39.5 | ||||||||||
巨蟹座55e | 8.6 | 0.016 | 0.17 | 公轉軌道太過接近恆星 | [32] | 巨蟹座55 | 40 | ||||||
HD 40307 b[33] | ≥4.2 | 0.047 | 0.2 | 公轉軌道太過接近恆星 | [34] | HD 40307 | 42 | ||||||
HD 40307 c[33] | ≥6.8 | 0.081 | 0.06 | 公轉軌道太過接近恆星 | [34] | HD 40307 | 42 | ||||||
HD 40307 d [35] | ≥9.2 | 0.134 | 0.07 | 公轉軌道太過接近恆星 | [36] | HD 40307 | 42 | ||||||
HD 40307 e | ≥3.5 | 0.1886 | 0.15 | [37] | HD 40307 | 42 | |||||||
HD 40307 f | ≥5.2 | 385 K | 0.247 | 0.02 | [37] | HD 40307 | 42 | ||||||
HD 40307 g | ≥7.1 | 284 K[38] | 0.600 | 0.29 | [37] | HD 40307 | 42 |
參見
[编辑]參考資料
[编辑]- ^ 1.0 1.1 Méndez, Abel. A Hot Potential Habitable Exoplanet around Gliese 163. University of Puerto Rico at Arecibo (Planetary Habitability Laboratory). August 29, 2012 [September 20, 2012]. (原始内容存档于2019-10-21).
- ^ 2.0 2.1 Nola Taylor Redd. Newfound Alien Planet a Top Contender to Host Life. Space.com. September 20, 2012 [September 20, 2012]. (原始内容存档于2019-12-26).
- ^ Staff. LHS 188 -- High proper-motion Star. Centre de données astronomiques de Strasbourg(Strasbourg astronomical Data Center). September 20, 2012 [September 20, 2012]. (原始内容存档于2016-03-26).
- ^ Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; Berdiñas, Zaira M.; Butler, R. Paul; Coleman, Gavin A. L.; de la Cueva, Ignacio; Dreizler, Stefan; Endl, Michael; Giesers, Benjamin; Jeffers, Sandra V.; Jenkins, James S.; Jones, Hugh R. A.; Kiraga, Marcin; Kürster, Martin; López-González, Marίa J.; Marvin, Christopher J.; Morales, Nicolás; Morin, Julien; Nelson, Richard P.; Ortiz, José L.; Ofir, Aviv; Paardekooper, Sijme-Jan; Reiners, Ansgar; Rodríguez, Eloy; Rodrίguez-López, Cristina; Sarmiento, Luis F.; Strachan, John P.; Tsapras, Yiannis; Tuomi, Mikko; Zechmeister, Mathias. A terrestrial planet candidate in a temperate orbit around Proxima Centauri. Nature. 25 August 2016, 536 (7617): 437–440 [2016-08-25]. ISSN 0028-0836. doi:10.1038/nature19106. (原始内容存档于2017-01-06) (英语).
- ^ 存档副本 (PDF). [2018-11-16]. (原始内容存档 (PDF)于2019-03-26).
- ^ 6.0 6.1 存档副本. [2016-08-25]. (原始内容存档于2018-09-30).
- ^ Fogg, M. J.; Nelson, R. P. Oligarchic and giant impact growth of terrestrial planets in the presence of gas giant planet migration. Astronomy and Astrophysics. 2005, 441 (2): 791–806 [2012-10-19]. Bibcode:2005A&A...441..791F. arXiv:astro-ph/0507180 . doi:10.1051/0004-6361:20053453. (原始内容存档于2021-02-25).
- ^ 8.0 8.1 Rivera, E. et al. (2005). "A ~7.5 M⊕ Planet Orbiting the Nearby Star, GJ 876". The Astrophysical Journal 634 (1): 625–640
- ^ Eugenio J. Rivera, Gregory Laughlin, R. Paul Butler, Steven S. Vogt, Nader Haghighipour, Stefano Meschiari (2010). \"The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration\".
- ^ 10.0 10.1 引用错误:没有为名为
arxiv.org
的参考文献提供内容 - ^ 存档副本. [2018-11-16]. (原始内容存档于2016-03-04).
- ^ 12.0 12.1 HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo. [3 October 2015]. (原始内容存档于2018-09-30).
- ^ A Nearby Super-Earth with the Right Temperature but Extreme Seasons - Planetary Habitability Laboratory @ UPR Arecibo. [3 October 2015]. (原始内容存档于2019-05-13).
- ^ 14.0 14.1 14.2 引用错误:没有为名为
aaa534
的参考文献提供内容 - ^ 15.0 15.1 15.2 引用错误:没有为名为
epe_HD_20794
的参考文献提供内容 - ^ Vogt, S. S.; et al. (2010). \"The Lick-Carnegie Exoplanet Survey: A 3.1 M_Earth Planet in the Habitable Zone of the Nearby M3V Star Gliese 581
- ^ Valencia; Sasselov, Dimitar D.; O'Connell, Richard J.; et al. Radius and Structure Models of the First Super-Earth Planet. The Astrophysical Journal. 2006, 656 (1): 545–551. Bibcode:2007ApJ...656..545V. arXiv:astro-ph/0610122 . doi:10.1086/509800.
- ^ von Bloh et al. (2007). "The Habitability of Super-Earths in Gliese 581". Astronomy and Astrophysics 476 (3): 1365–1371.
- ^ Vogt, S. S.; et al. (2010). \"The Lick-Carnegie Exoplanet Survey: A 3.1 M_Earth Planet in the Habitable Zone of the Nearby M3V Star Gliese 581\".
- ^ von Bloh, W.; Bounama, C.; Cuntz, M.; Franck, S. The Habitability of Super-Earths in Gliese 581. Astronomy & Astrophysics. 2007, 476 (3): 1365–1371. Bibcode:2007A&A...476.1365V. arXiv:0705.3758 . doi:10.1051/0004-6361:20077939.
- ^ 21.00 21.01 21.02 21.03 21.04 21.05 21.06 21.07 21.08 21.09 21.10 The Habitable Exoplanets Catalog (页面存档备份,存于互联网档案馆). The values are just the best estimates and are subject to change.
- ^ M. Mayor, X. Bonfils, T. Forveille, X. Delfosse, S. Udry, J.-L. Bertaux, H. Beust, F. Bouchy, C. Lovis, F. Pepe, C. Perrier, D. Queloz, N. C. Santos (2009). "The HARPS search for southern extra-solar planets,XVIII. An Earth-mass planet in the GJ 581 planetary system".
- ^ Vogt, S. S.; et al. (2010). \"The Lick-Carnegie Exoplanet Survey: A 3.1 M⊕ Planet in the Habitable Zone of the Nearby M3V Star Gliese 581
- ^ 存档副本. [2017-11-17]. (原始内容存档于2015-07-31).
- ^ Bonfils; Delfosse; Udry; Forveille; Mayor; Perrier; Bouchy; Gillon; Lovis. The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample. 2011. arXiv:1111.5019 [astro-ph.EP].
- ^ A Potential Habitable Exoplanet in a Nearby Triple Star System. [2012-10-19]. (原始内容存档于2021-02-25).
- ^ Vogt, Steven; Wittenmyer; Paul Butler; Simon O'Toole; Henry; Rivera; Stefano Meschiari; Gregory Laughlin; Tinney. A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis. 2009. arXiv:0912.2599v1 [astro-ph.EP].
- ^ Vogt, Steven (2009). \"A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis
- ^ Kaltenegger, L; Udry, S; Pepe, F. A Habitable Planet around HD 85512? 1108: 3561. 2011. Bibcode:2011arXiv1108.3561K. arXiv:1108.3561 .
- ^ 30.0 30.1 Kaltenegger, L.; Udry, S.; Pepe, F. (2011). A Habitable Planet around HD 85512?
- ^ 31.0 31.1 31.2 31.3 31.4 31.5 31.6 Gillon, M; Triaud, AH; Demory, BO; Jehin, E; Agol, E; Deck, KM; Lederer, SM; de Wit, J; Burdanov, A; Ingalls, JG; Bolmont, E; Leconte, J; Raymond, SN; Selsis, F; Turbet, M; Barkaoui, K; Burgasser, A; Burleigh, MR; Carey, SJ; Chaushev, A; Copperwheat, CM; Delrez, L; Fernandes, CS; Holdsworth, DL; Kotze, EJ; Van Grootel, V; Almleaky, Y; Benkhaldoun, Z; Magain, P; Queloz, D. Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1 (PDF). Nature: 456–460. [2017-11-17]. Bibcode:2017Natur.542..456G. PMC 5330437 . PMID 28230125. arXiv:1703.01424 . doi:10.1038/nature21360. (原始内容存档 (PDF)于2017-02-23).
- ^ Rebekah et al.; Fabrycky (2010-05-21). \"Radial velocity planets de-aliased. A new, short period for Super-Earth 55 Cnc e\". The Astrophysical Journal 722: 937–953
- ^ 33.0 33.1 M. Mayor, S. Udry, C. Lovis, F. Pepe, D. Queloz, W. Benz, J.-L. Bertaux, F. Bouchy, C. Mordasini, D. Segransan. The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses). Astronomy and Astrophysics. 2009, 493 (2): 639–644. Bibcode:2009A&A...493..639M. arXiv:0806.4587 . doi:10.1051/0004-6361:200810451.
- ^ 34.0 34.1 M. Mayor, S. Udry, C. Lovis, F. Pepe, D. Queloz, W. Benz, J.-L. Bertaux, F. Bouchy, C. Mordasini, D. Segransan (2009). \"The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)\". Astronomy and Astrophysics 493 (2): 639–644
- ^ Barnes, R., Jackson, B., Raymond, S., West, A., Greenberg, R. The HD 40307 Planetary System: Super-Earths or Mini-Neptunes?. The Astrophysical Journal. 2009, 695 (2): 1006. Bibcode:2009ApJ...695.1006B. arXiv:0901.1698 . doi:10.1088/0004-637X/695/2/1006.
- ^ M. Mayor, S. Udry, C. Lovis, F. Pepe, D. Queloz, W. Benz, J.-L. Bertaux, F. Bouchy, C. Mordasini, D. Segransan (2009). \"The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)\". Astronomy and Astrophysics 493 (2): 639–644.
- ^ 37.0 37.1 37.2 引用错误:没有为名为
tuomi12
的参考文献提供内容 - ^ HEC: Data of Potential Habitable Worlds. University of Puerto Rico at Arecibo (Planetary Habitability Laboratory). November 12, 2012 [2016-08-25]. (原始内容存档于2018-09-30).