最近類地太陽系外行星列表

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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

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
Artist's impression of the planet orbiting Proxima Centauri.jpg
≥1.27~1.1234 K0.05<0.35位於適居帶中[4]比鄰星4.22
半人馬座α Bb
Artist’s impression of the planet around Alpha Centauri B (Annotated).jpg
≥1.11200 K0.04公轉軌道太過接近恆星
半人馬座α B
4.23
巴納德星b
Artist’s impression of the surface of a super-Earth orbiting Barnard’s Star.jpg
≥3.23105 K
-168.15 °C
0.4040.32[5]巴納德星5.958
羅斯128b
Artist's impression of the planet Ross 128 b.jpg
≥1.35~1.1羅斯12810.89
魯坦星b≥2.89≥1.35259 K
-14 °C
0.0910.10魯坦星12.20
沃夫1061b≥1.36≥1.44沃夫106113.8
沃夫1061c
Planets Under a Red Sun.jpg
≥4.3≥1.64[6]沃夫106113.8
沃夫1061d≥5.21≥2.04沃夫106113.8

葛利斯876d[7]
Artist’s view of an exoplanet inspired by the discovery of Gliese 876 d.jpg
6.8157

377 °C[8]
0.0210.21估計表面溫度: 157-377°C[9][10]葛利斯87615
格利泽682b≥2
[11]
[12]
[6]
格利泽68216
葛利斯832c
Artist’s impression of a cloud-covered planet inspired by the data of Gliese 832 c.png
≥5.4295 K
22 °C
0.1620.03
[13][14]
葛利斯83216.16
天园增三b≥2.7660 K
387 °C[15]
0.12070[16]天园增三19.71
天园增三c≥2.4508 K
235 °C[15]
0.20360[16]天园增三19.71
天园增三d≥4.8388 K
115 °C[15]
0.34990[16]天园增三19.71
葛利斯581e
Planet Gliese 581 e.png
≥1.70.0290表面溫度過高,可能沒有大氣層存在[17]葛利斯58120

葛利斯581c [18]
Planetary System in Gliese 581 (artist's impression).jpg
≥5.60.0720公轉軌道可能位於適居帶外側[19][20]葛利斯58120

葛利斯581d [21]
Planet Gliese 581 d.png
≥5.62.34[22]1.27[22]233 K[22]0,21800.69[22]可能是一顆海洋行星[22]位於適居帶中[23][24]葛利斯58120
HD 219134 b
PIA19833-RockyExoplanet-HD219134b-ArtistConcept-20150730.jpg
4.51.6700 K
427 °C
[25]HD 21913421

葛利斯667Cc[26][27]
Gliese 667 Cc sunset.jpg
5.241.991.32302 K0.130.340.82位於適居帶中[22]葛利斯667C22

室女座61b[28]
Artist concept 61vir b.png
≥5.10.0500.12公轉軌道太過接近恆星[29]室女座6128

HD 85512 b[30]
HD 85512 b (Artists's impression).jpg
≥3.61.74[22]1.33[22]351 K[22]0.260.110.76[22]曾被認為是最適合人類居住的行星[22][31]直到發現葛利斯667Cc為止[31]HD 8551236
GJ 180 b≥2.3312 K
39 °C

[11][13]
葛利斯18038
TRAPPIST-1b
TRAPPIST-1b Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1c
TRAPPIST-1c Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1d
TRAPPIST-1d Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1e
TRAPPIST-1e Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1f
TRAPPIST-1f Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1g
TRAPPIST-1g Artist's Impression.png
[32]TRAPPIST-139.5
TRAPPIST-1h
TRAPPIST-1h Artist's Impression.png
[32]TRAPPIST-139.5
巨蟹座55e
Newneptune nasa big.jpg
8.60.0160.17公轉軌道太過接近恆星[33]巨蟹座5540

HD 40307 b[34]
≥4.20.0470.2公轉軌道太過接近恆星[35]HD 4030742

HD 40307 c[34]
≥6.80.0810.06公轉軌道太過接近恆星[35]HD 4030742

HD 40307 d [36]
A Trio of Super-Earths (artist's impression).jpg
≥9.20.1340.07公轉軌道太過接近恆星[37]HD 4030742
HD 40307 e≥3.50.18860.15[38]HD 4030742
HD 40307 f≥5.2385 K0.2470.02[38]HD 4030742
HD 40307 g≥7.1284 K[39]0.6000.29[38]HD 4030742


參見


  • 臨近恆星列表

  • 確定存在的太陽系外行星列表

  • 不確定存在的太陽系外行星列表

  • 位於適居帶的太陽系外行星列表

  • 類太陽恆星

  • 恆星際旅行


參考資料




  1. ^ 1.01.1 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]. 


  2. ^ 2.02.1 Nola Taylor Redd. Newfound Alien Planet a Top Contender to Host Life. Space.com. September 20, 2012 [September 20, 2012]. 


  3. ^ Staff. LHS 188 -- High proper-motion Star. Centre de données astronomiques de Strasbourg(Strasbourg astronomical Data Center). September 20, 2012 [September 20, 2012]. 


  4. ^ 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. ISSN 0028-0836. doi:10.1038/nature19106 (英语). 


  5. ^ https://www.eso.org/public/archives/releases/sciencepapers/eso1837/eso1837a.pdf


  6. ^ 6.06.1 http://phl.upr.edu/projects/habitable-exoplanets-catalog/data


  7. ^ 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. Bibcode:2005A&A...441..791F. arXiv:astro-ph/0507180. doi:10.1051/0004-6361:20053453. 


  8. ^ Rivera, E. et al. (2005). "A ~7.5 M⊕ Planet Orbiting the Nearby Star, GJ 876". The Astrophysical Journal 634 (1): 625–640


  9. ^ Rivera, E. et al. (2005). "A ~7.5 M⊕ Planet Orbiting the Nearby Star, GJ 876". The Astrophysical Journal 634 (1): 625–640


  10. ^ 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".


  11. ^ 11.011.1 引用错误:没有为名为arxiv.org的参考文献提供内容


  12. ^ http://www.hpcf.upr.edu/~abel/phl/tuomi/hec_orbit_GJ_682_b.png


  13. ^ 13.013.1 HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo. [3 October 2015]. 


  14. ^ A Nearby Super-Earth with the Right Temperature but Extreme Seasons - Planetary Habitability Laboratory @ UPR Arecibo. [3 October 2015]. 


  15. ^ 15.015.115.2 引用错误:没有为名为aaa534的参考文献提供内容


  16. ^ 16.016.116.2 引用错误:没有为名为epe_HD_20794的参考文献提供内容


  17. ^ 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


  18. ^ Valencia; Sasselov, Dimitar D.; O'Connell, Richard J.; 等. 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.  引文格式1维护:显式使用等标签 (link)


  19. ^ von Bloh et al. (2007). "The Habitability of Super-Earths in Gliese 581". Astronomy and Astrophysics 476 (3): 1365–1371.


  20. ^ 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".


  21. ^ 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. 


  22. ^ 22.0022.0122.0222.0322.0422.0522.0622.0722.0822.0922.10 The Habitable Exoplanets Catalog. The values are just the best estimates and are subject to change.


  23. ^ 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".


  24. ^ 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


  25. ^ http://phys.org/news/2015-07-astronomers-star-super-earths.html


  26. ^ 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]. 


  27. ^ A Potential Habitable Exoplanet in a Nearby Triple Star System


  28. ^ 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].  引文使用过时参数version (帮助)


  29. ^ Vogt, Steven (2009). "A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis


  30. ^ Kaltenegger, L; Udry, S; Pepe, F. A Habitable Planet around HD 85512? 1108: 3561. 2011. Bibcode:2011arXiv1108.3561K. arXiv:1108.3561. 


  31. ^ 31.031.1 Kaltenegger, L.; Udry, S.; Pepe, F. (2011). A Habitable Planet around HD 85512?


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  33. ^ 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


  34. ^ 34.034.1 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. 


  35. ^ 35.035.1 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


  36. ^ 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. 


  37. ^ 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.


  38. ^ 38.038.138.2 引用错误:没有为名为tuomi12的参考文献提供内容


  39. ^ HEC: Data of Potential Habitable Worlds. University of Puerto Rico at Arecibo (Planetary Habitability Laboratory). November 12, 2012. 


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