Berikut adalah daftar eksoplanet yang kemungkinan layak huni. Daftar dibawah sebagian besar didasari oleh perkiraan kelayakhunian oleh Katalog Eksoplanet Layak Huni (Habitable Exoplanets Catalog, HEC), dan data dari Arsip Eksoplanet NASA. HEC dikelola oleh Laboratorium Kelayakhunian Planet di Universitas Puerto Rico di Arecibo. Terdapat juga daftar spekulatif yang sedang dikembangkan, mengenai planet super laik huni.

Kelayakhunian pemukaan planet dianggap membutuhkan sebuah orbit pada jarak yang tepat dari bintang induknya agar dapat mempertahankan air cair di permukaan. Selain itu, aspek-aspek geofisik dan geodinamis lainnya, kepadatan atmosfer, jenis radiasi dan intensitasnya, beserta lingkungan plasma bintang induknya juga memengaruhi kelayakhunian planet.^[1]

Daftar

Dibawah adalah daftar eksoplanet didalam zona layak huni dibawah 10 massa Bumi dan lebih kecil daripada 2.5 radius Bumi, sehingga memiliki kemungkinan merupakan planet kebumian. Perlu diketahui bahwa dimasukkannya suatu planet pada daftar dibawah tidak menjadi kelayakhunian, dan terkhususnya planet-planet yang lebih besar, kemungkinan kecil memiliki komposisi terestrial.^[2] Bumi juga dimasukkan sebagai perbandingan.

Jumlah massa dan radius yang diawali dengan "~" belum pernah diukur, namun diperkirakan dengan hubungan massa-radius.

Referensi

1. ↑ Lammer, H.; Bredehöft, J. H.; Coustenis, A.; Khodachenko, M. L.; et al. (2009). "What makes a planet habitable?" (PDF). The Astronomy and Astrophysics Review. 17 (2): 181–249. Bibcode:2009A&ARv..17..181L. doi:10.1007/s00159-009-0019-z. S2CID 123220355. Diarsipkan dari asli (PDF) tanggal 2016-06-02. Diakses tanggal 2016-05-03.
2. ↑ Chen, Jingjing; Kipping, David (2017). "Probabilistic Forecasting of the Masses and Radii of Other Worlds". The Astrophysical Journal. 834 (1): 17. arXiv:1603.08614. Bibcode:2017ApJ...834...17C. doi:10.3847/1538-4357/834/1/17. S2CID 119114880.
3. ↑
4. ↑ "NASA Venus Fact Sheet". nssdc.gsfc.nasa.gov/. Diakses tanggal 2023-04-30.
5. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30
6. ↑
7. ↑ Damasso, M.; et al. (2022), "A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514", Astronomy & Astrophysics, 666: A187, arXiv:2204.06376, doi:10.1051/0004-6361/202243522, S2CID 248157318
8. ↑
9. ↑ LePage, Andrew (22 May 2017). "Habitable Planet Reality Check: Is GJ 625b a Super-Earth or a Super-Venus?". drewexmachina.com. Diakses tanggal 15 September 2022.
10. ↑ "GJ 625". hzgallery.org. Diakses tanggal 15 September 2022.
11. ↑
12. 1 2
13. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System (dalam bahasa Inggris). Diakses tanggal 2024-01-30.
14. ↑ Díaz, Rodrigo F.; et al. (2016). "The HARPS search for southern extra-solar planets". Astronomy & Astrophysics. 585: A134. arXiv:1510.06446. Bibcode:2016A&A...585A.134D. doi:10.1051/0004-6361/201526729. S2CID 118531921.
15. ↑ "Confirmed Planet Overview Page: K2-9b". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
16. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Diakses tanggal 2021-01-29.
17. ↑ https://science.nasa.gov/exoplanet-catalog/k2-288-b-b/
18. ↑ "Confirmed Planet Overview Page: Kepler-22 b". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
19. ↑ "Confirmed Planet Overview Page: Kepler-62e". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
20. ↑ "Confirmed Planet Overview Page: Kepler-62f". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
21. ↑ "Confirmed Planet Overview Page: Kepler-296e". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
22. ↑ Barclay, Thomas; Quintana, Elisa V; Adams, Fred C; Ciardi, David R; Huber, Daniel; Foreman-Mackey, Daniel; Montet, Benjamin T; Caldwell, Douglas (2015). "The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis". The Astrophysical Journal. 809 (1): 7. arXiv:1505.01845. Bibcode:2015ApJ...809....7B. doi:10.1088/0004-637X/809/1/7. S2CID 37742564.
23. ↑ "Confirmed Planet Overview Page: Kepler-296 f". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
24. ↑ "Confirmed Planet Overview Page: Kepler-452 b". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Diakses tanggal 4 June 2016.
25. ↑ "Targets of Note: Kepler-452 b". NASA Exoplanet Archive. Diakses tanggal 15 September 2022.
26. ↑ Mullally, Fergal; Thompson, Susan E.; Coughlin, Jeffrey L.; Burke, Christopher J.; Rowe, Jason F. (2018). "Kepler's Earth-like Planets Should Not be Confirmed without Independent Detection: The Case of Kepler-452b". The Astronomical Journal. 155 (5): 210. arXiv:1803.11307. Bibcode:2018AJ....155..210M. doi:10.3847/1538-3881/aabae3. S2CID 55481591.
27. ↑ Burke, Christopher J.; Mullally, F.; Thompson, Susan E.; Coughlin, Jeffrey L.; Rowe, Jason F. (2019). "Re-evaluating Small Long-period Confirmed Planets from Kepler". The Astronomical Journal. 157 (4): 143. arXiv:1901.00506. Bibcode:2019AJ....157..143B. doi:10.3847/1538-3881/aafb79. S2CID 119047713.
28. ↑ "Exoplanet-catalog-Exoplanet exploration-Kepler-1606b".
29. ↑ "Earth-Size, Habitable Zone Planet Found Hidden in Early NASA Kepler Data". Exoplanet Exploration: Planets Beyond our Solar System. Diakses tanggal 2021-01-02.
30. ↑ "Exoplanet catalog-Exoplanet exploration-Kepler-1701b".
31. ↑ "Comparison of the L 98-59 exoplanet system with the inner Solar System". www.eso.org (dalam bahasa Inggris). Diakses tanggal 2021-08-09.
32. ↑ Cadieux, Charles; Plotnykov, Mykhaylo; et al. (2024). "New Mass and Radius Constraints on the LHS 1140 Planets -- LHS 1140 b is Either a Temperate Mini-Neptune or a Water World". The Astrophysical Journal Letters. 960 (1): L3. arXiv:2310.15490. Bibcode:2024ApJ...960L...3C. doi:10.3847/2041-8213/ad1691.
33. ↑ Delrez, L.; Murray, C. A.; et al. (September 2022). "Two temperate super-Earths transiting a nearby late-type M dwarf". Astronomy & Astrophysics. 667: A59. arXiv:2209.02831. Bibcode:2022A&A...667A..59D. doi:10.1051/0004-6361/202244041. S2CID 252110654.
34. ↑
35. ↑
36. ↑ Wenz, John (15 November 2017). "A potentially habitable planet has been discovered just 11 light-years away". Astronomy. Diarsipkan dari asli tanggal 21 February 2018. Diakses tanggal 19 November 2017.
37. ↑ Harakawa, Hiroki; et al. (2022). "A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508". Publications of the Astronomical Society of Japan. 74 (4): 904–922. arXiv:2205.11986. Bibcode:2022PASJ...74..904H. doi:10.1093/pasj/psac044.
38. 1 2
39. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Diakses tanggal 2021-12-05.
40. ↑ Dransfield, Georgina; Timmermans, Mathilde; Triaud, Amaury H. M. J.; Dévora-Pajares, Martín; Aganze, Christian; Barkaoui, Khalid; Burgasser, Adam J.; Collins, Karen A.; Cointepas, Marion; Ducrot, Elsa; Günther, Maximilian N.; Howell, Steve B.; Murray, Catriona A.; Niraula, Prajwal; Rackham, Benjamin V. (2023-10-28). "A 1.55 R$_{\oplus}$ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole". Monthly Notices of the Royal Astronomical Society. 527 (1): 35–52. arXiv:2305.06206. doi:10.1093/mnras/stad1439. ISSN 0035-8711. Pemeliharaan CS1: DOI bebas tanpa ditandai (link)
41. ↑ https://science.nasa.gov/exoplanet-catalog/toi-715-b/
42. ↑ Schanche, N.; et al. (2022). "TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf". Astronomy & Astrophysics. 657: A45. arXiv:2111.01749. Bibcode:2022A&A...657A..45S. doi:10.1051/0004-6361/202142280. S2CID 240419956.
43. 1 2 3 4
44. 1 2 3 4
45. ↑ Kossakowski, D.; Kürster, M.; et al. (January 2023). "The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star". Astronomy & Astrophysics. 670: A84. arXiv:2301.02477. Bibcode:2023A&A...670A..84K. doi:10.1051/0004-6361/202245322.