List Of Potentially Habitable Exoplanets

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Template:Life in the Universe The following list includes potentially habitable exoplanets. It is mostly based on estimates of habitability by the Habitable Worlds Catalog (HWC), and data from the NASA Exoplanet Archive. The HWC is maintained by the Planetary Habitability Laboratory at the University of Puerto Rico at Arecibo.[1]

Surface planetary habitability is thought to require an orbit at the right distance from the host star for liquid surface water to be present, in addition to various geophysical and geodynamical aspects, atmospheric density, radiation type and intensity, and the host star's plasma environment.[2]

Main list

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by expanding it with reliably sourced entries.

This is a list of confirmed exoplanets within the circumstellar habitable zone that are either under 10 Earth masses or smaller than 2.5 Earth radii and thus have a chance of being rocky.[1][3] Note that inclusion on this list does not guarantee habitability, and in particular the larger planets are less likely to have a rocky composition and more likely to be mini-Neptunes.[4] Earth is included for both comparison and reference, while Venus and Mars are included for reference only.

Note that mass and radius values prefixed with "~" have not been measured, but are predicted from a mass–radius relationship.

Object Star Star type Mass (M⊕) Radius (R⊕) Density (g/cm3) Flux (F⊕) Teq (K) Period (days) Distance (ly) Refs/notes
Earth
(reported for reference)		 Sun Template:StarG 1.00 1.00 5.514 1.00 255 365.25 0 Only planet confirmed to support life
Venus
(reported for reference)		 Sun Template:StarG 0.815 0.950 5.243 1.911 244.261 224.70 0.0000042 [5]
Mars
(reported for reference)		 Sun Template:StarG 0.107 0.533 3.934 0.431 209.8 686.98 0.0000058–0.000042 [6]
55 Cancri Bc 55 Cancri B Template:StarM ≥5.3 — — 0.3 200 33.7 40.9 [7]
Gliese 12 b Gliese 12 Template:StarM 0.71 or 0.95[8][9] 0.904+0.037
−0.034[9] 		5.3 or 7.1 1.6±0.2 315 12.7 39.7 Near inner edge of HZ, might resemble Venus[10]
Gliese 163 c Gliese 163 Template:StarM ≥6.80 — — 1.25 277 25.6 49 [1]
Gliese 180 d Gliese 180 Template:StarM ≥7.56 — — 0.26 — 106.3 39 [1]
Gliese 251 c Gliese 251 Template:StarM ≥3.84 — — — — 53.6 18.2 [11]
Gliese 357 d Gliese 357 Template:StarM ≥6.10 — — 0.38 200 55.7 31
Gliese 433 d Gliese 433 Template:StarM ≥5.22 — — 1.06 — 36.1 29.6 [1]
Gliese 514 b Gliese 514 Template:StarM ≥5.20 — — 0.28+0.51
−0.166		 202 140.4 25 Highly eccentric[12]
Gliese 555 b Gliese 555 Template:StarM ≥5.46 — — 0.5 214[13] 36.2 20.4 [14]
Gliese 625 b Gliese 625 Template:StarM ≥2.82 — — — 14.628 21.1 Likely too hot[15][16][17]
Gliese 667 Cc Gliese 667 C Template:StarM ≥3.81 ~1.54 — 0.88 277 28.1 23.62 [18][1]
GJ 1002 b GJ 1002 Template:StarM ≥1.08 ~1.03 — 0.67 231 10.3 15.8 [19]
GJ 1002 c GJ 1002 Template:StarM ≥1.36 1.1 — 0.26 182 21.2 15.8 [19][20]
GJ 1061 c GJ 1061 Template:StarM 1.81+0.13
−0.11[21]		 ~1.18 — 1.45 275 6.7 12 [22]
GJ 1061 d GJ 1061 Template:StarM 1.67+0.17
−0.16[21]		 ~1.16 — 0.69 218 13.0 12 [23]
GJ 3293 d GJ 3293 Template:StarM ≥7.60 — — 0.59 223 48.1 66 [1]
GJ 3998 d GJ 3998 Template:StarM ≥6.07 — — — 41.8 58 [24]
HD 20794 d HD 20794 Template:StarG ≥5.82 — — — — 647.6 19.7 Highly eccentric orbit[25][26]
HD 216520 c HD 216520 Template:StarK ≥9.44 — — 1.28 — 154.4 64 [1]
HIP 38594 b HIP 38594 Template:StarM ≥8.10 — — 1.34 — 60.7 58 [1]
K2-72e K2-72 Template:StarM ~2.21 1.29 — 1.30 261 24.2 217 [27]
K2-155d K2-155 Template:StarK 4.27 1.64 — — 289 40.6 290
K2-288Bb K2-288 B Template:StarM 4.27 1.91 — 0.44 207 31.4 214 [28]
K2-332b K2-332 Template:StarM — 2.20 — 1.17 — 17.7 402 [1]
Kepler-22b Kepler-22 Template:StarG ~9.1 or ~35 2.38 — 1.10 261 289.9 635 [1][29]
Kepler-62e Kepler-62 Template:StarK 4.5+14.2
−2.6		 1.61 — 1.15 264 122.4 981 [1][30]
Kepler-62f Kepler-62 Template:StarK 2.8±0.4 1.41 — 0.41 204 267.3 981 [1][31]
Kepler-155c Kepler-155 Template:StarM — 2.24 — 1.05 — 52.7 957 [1]
Kepler-174d Kepler-174 Template:StarK — 2.19 — 0.59 206 247.4 1,254 [1]
Kepler-186f Kepler-186 Template:StarM 1.44+2.33
−1.12		 1.17 — 0.29 188 129.9 579 [1]
Kepler-283c Kepler-283 Template:StarK — 1.82 — 0.89 248 92.7 1,526 [1]
Kepler-296e Kepler-296 Template:StarK 2.96 1.52 — 1.41 276 34.1 737 [1][32][33]
Kepler-296f Kepler-296 Template:StarK — 1.80 — 0.44 225 63.3 737 [1][34]
Kepler-440b Kepler-440 Template:StarK — 1.91 — 1.44 273 101.1 981 [1]
Kepler-442b Kepler-442 Template:StarK 2.36+5.9
−1.3		 1.35 — 0.70 233 112.3 1,193 [1]
Kepler-443b Kepler-443 Template:StarK — 2.35 — 0.89 247 177.7 2,615 [1]
Kepler-705b Kepler-705 Template:StarM — 2.11 — 0.77 243 56.1 903
Kepler-725 c Kepler-725 Template:StarG 9.7 — — — 207.5 2,526
Kepler-1229b Kepler-1229 Template:StarM 2.540 1.40 — 0.32 213 86.8 865 [1]
Kepler-1410b Kepler-1410 Template:StarK — 1.78 — 1.07 274 60.9 1196
Kepler-1455b Kepler-1455 Template:StarK — 2.10 — 1.30 49.3 1280 [35]
Kepler-1540b Kepler-1540 Template:StarK — 2.49 — 0.78 250 125.4 799
Kepler-1544 b Kepler-1544 Template:StarK — 1.78 — 0.84 248 168.8 1092 [1]
Kepler-1606b Kepler-1606 Template:StarG — 2.07 — 1.64 277 196.4 2710 [36]
Kepler-1649c Kepler-1649 Template:StarM 1.20 1.06 — 0.75 237 19.5 301 [37]
Kepler-1652b Kepler-1652 Template:StarM — 1.60 — 0.84 244 38.1 822
Kepler-1653 b Kepler-1653 Template:StarK — 2.17 — 1.04 258 140.3 2461 [1]
Kepler-1701b Kepler-1701 Template:StarK — 2.22 — 1.42 275 169.1 1904 [1][38]
LHS 1140 b LHS 1140 Template:StarM 5.60 1.73 5.9±0.3 0.43 226 24.7 49 Likely an ocean world with an atmosphere[39]
LP 890-9 c LP 890-9 Template:StarM — 1.37 — 0.91 272 8.46 105 [40]
Luyten b Luyten's Star Template:StarM ≥2.89 ~1.35 — 1.06 258 18.65 12.3 [41]
Proxima Centauri b Proxima Centauri Template:StarM ≥1.07[42]: 16  1.17±0.23 — 0.70 228 11.186 4.25 Affected by stellar flare, possibly affected by high radiation flux[43]
Ross 128 b Ross 128 Template:StarM ≥1.40 ~1.80 — 1.48 280 9.87 11.0 [44]
Ross 508 b Ross 508 Template:StarM ≥4.00 — — 1.32 — 10.8 37 [45]
Struve 2398 Bc Struve 2398 Template:StarM ≥3.4 — — 37.9 11.5 [46]
Teegarden's Star b Teegarden's Star Template:StarM ≥1.05 ~1.02 — 1.15 264 4.91 12.5 [47][48]
Teegarden's Star c Teegarden's Star Template:StarM ≥1.11 ~1.04 — 0.37 199 11.4 12.5 [47]
L 98-59 f L 98-59 Template:StarM ≥2.97 — — >1 289 23.07 34.6 [49][50]
TOI-700 d TOI-700 Template:StarM ~1.72 1.14 — 0.87 246 37.4 101
TOI-700 e TOI-700 Template:StarM 0.82 0.95 — 1.27[51] 273 27.8 101 [52]
TOI-715 b TOI-715 Template:StarM 3.02 1.55 — 0.67 234 19.29 137 [53][54]
TOI-2094 Ab TOI-2094 Template:StarM 1.90 — 0.98 18.8 164 [55]
TOI-2257 b TOI-2257 Template:StarM 5.712+4.288
−2.311 		2.20 — 0.57+1.68
−0.31		 256+61
−17 		35.2 188 Highly eccentric[1][56]
TOI-2285 b TOI-2285 Template:StarM 4.1 1.75 — — 284 27 137 Likely too hot[57][58][59]
TOI-7166 b TOI-7166 Template:StarM 2.01 — 1.07 249 12.9 115 [60]
TRAPPIST-1e TRAPPIST-1 Template:StarM 0.69 0.92 5.65 0.65 230 6.1 41 Confirmed to be rocky. Possibly has an atmosphere.[61][62][63]
TRAPPIST-1f TRAPPIST-1 Template:StarM 1.04 1.04 3.3 ± 0.9 0.37 200 9.2 41 Confirmed to be rocky[61][62]
TRAPPIST-1g TRAPPIST-1 Template:StarM 1.32 1.13 4.186 0.25 182 12.4 41 Confirmed to be rocky[61][62]
Wolf 1069 b Wolf 1069 Template:StarM ≥1.26 ~1.08 — 0.65 250 15.6 31.2 [64]
Wolf 1061c Wolf 1061 Template:StarM ≥3.41 ~1.60 — 1.30 271 17.9 13.8 [1]

Current candidates

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by expanding it with reliably sourced entries.

This is a list of notable exoplanets within the circumstellar habitable zone that are either under 10 Earth masses or smaller than 2.5 Earth radii and have not yet been confirmed. Earth is included for both comparison and reference, while Venus and Mars are included for reference only.

Object Star Star type Mass (M⊕) Radius (R⊕) Density (g/cm3) Flux (F⊕) Teq (K) Period (days) Distance (ly) Refs/notes
Earth
(reported for reference)		 Sun Template:StarG 1.00 1.00 5.514 1.00 255 365.25 0 Only planet confirmed to support life
Venus
(reported for reference)		 Sun Template:StarG 0.815 0.950 5.243 1.911 244.261 224.70 0.0000042 [5]
Mars
(reported for reference)		 Sun Template:StarG 0.107 0.533 3.934 0.431 209.8 686.98 0.0000058–0.000042 [6]
Gliese 180 c Gliese 180 Template:StarM ≥6.40 — — 0.78 239 24.3 39 [1][65]
HD 40307 g HD 40307 Template:StarK ≥7.09 — — 0.67 226 197.8 42 [1][66]
HD 137010 b HD 137010 Template:StarK 1.06 — 0.29 355 146 [67]
Kepler-452b Kepler-452 Template:StarG ~5 1.63 — 1.11 261 384.8 1799 [1][68][69][70][71]
KOI-4878.01 KOI-4878 Template:StarF ~1.9+1.1
−0.5		 1.05 — 1.04+1.1
−0.34		 257 449.0 1,075 [72][73]
KOI-5715.01 KOI-5715 Template:StarK — 1.93 260 190 2,964 [74]
Lacaille 9352 d Lacaille 9352 Template:StarM ≥8.3 — — 50.7 10.7 [75]
LTT 1445 Ad LTT 1445A Template:StarM ≥2.72 — — — 24.3 22.4 [76]
Tau Ceti f Tau Ceti Template:StarG ≥3.93 — — 0.27 190 642 11.9 Has been only in HZ for less than 1 Gya[77][78][79]
TOI-715.02 TOI-715 Template:StarM 1.066±0.092 0.48+0.12
−0.17		 25.6 137 [53]
WD 1054–226 b WD 1054–226 DAZ ~1 — — 1.04 118 [80] The surface temperature might be high enough for habitability[81]

Previous candidates

Some habitable exoplanets detected by radial velocity were considered as stellar artifacts by some studies. These include Gliese 581 d and g,[82][83][84] Gliese 667 Ce and f,[18][85] Gliese 682 b and c,[65] Kapteyn b,[86][87] Gliese 229 Ac,[88] HD 85512 b and Gliese 832 c.[89]

Several other planets, such as Gliese 180 b, also appear to be examples of planets once considered potentially habitable but later found to be interior to the habitable zone.[1] Similarly, Tau Ceti e[lower-alpha 1], HD 85512 b and Kepler-69c were thought to be likely habitable,[91] but with improved models of the circumstellar habitable zone, PHL does not consider it potentially habitable.[1] Kepler-438b was also initially considered potentially habitable; however, it was later found to be a subject of powerful flares that can strip a planet of its atmosphere, so it is now considered non-habitable.[1]

K2-3d and K2-18b were originally considered potentially habitable, and the latter remains listed in the HWC,[1] but recent studies have shown them to be gaseous sub-Neptune rather than being the Hycean planet and thus unlikely to be habitable.[92][93][94][95][96][97]

Kepler-1638b was thought to be a possibly habitable planet with a radius smaller than 2 R🜨 after the validation. However based on the later measurement of host star parallax by Gaia, the radius of the planet was revised upward to 3.226+0.201
−0.315 R🜨, meaning it is more likely an ice giant like Neptune with poor prospect for habitability.[98][99]

KOI-1686.01 was also considered a potentially habitable exoplanet after its detection in 2011, until proven a false positive by NASA in 2015.[100] Several other KOIs, like Kepler-577b and Kepler-1649b, were considered potentially habitable prior to confirmation, but with new data are no longer considered habitable.

TRAPPIST-1 d was considered to be potentially habitable until JWST/NIRSpec data found little evidence for an atmosphere with Earth-like surface pressure, highly likely ruling out habitability.[101]

See also

Notes

  1. ↑ The existence of Tau Ceti e is dubious, see[90]

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 1.15 1.16 1.17 1.18 1.19 1.20 1.21 1.22 1.23 1.24 1.25 1.26 1.27 1.28 1.29 1.30 1.31 1.32 1.33 1.34 "The Habitable Worlds Catalog". University of Puerto Rico at Arecibo. https://phl.upr.edu/hwc. 
  2. ↑ Lammer, H. et al. (2009). "What makes a planet habitable?". The Astronomy and Astrophysics Review 17 (2): 181–249. doi:10.1007/s00159-009-0019-z. Bibcode: 2009A&ARv..17..181L. http://veilnebula.jorgejohnson.me/uploads/3/5/8/7/3587678/lammer_et_al_2009_astron_astro_rev-4.pdf. Retrieved 2016-05-03. 
  3. ↑ Méndez, A.; González-Espada, W. (2016). Searching for Habitable Worlds: An Introduction. IOP Concise Physics. Morgan & Claypool Publishers. p. 1. ISBN 978-1-68174-401-8. https://books.google.com/books?id=bD9iDwAAQBAJ&pg=PP1. Retrieved 28 November 2019. 
  4. ↑ Chen, Jingjing; Kipping, David (2017). "Probabilistic Forecasting of the Masses and Radii of Other Worlds". The Astrophysical Journal 834 (1): 17. doi:10.3847/1538-4357/834/1/17. Bibcode: 2017ApJ...834...17C. 
  5. ↑ 5.0 5.1 "NASA Venus Fact Sheet". https://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.html. 
  6. ↑ 6.0 6.1 "NASA Mars Fact Sheet". https://nssdc.gsfc.nasa.gov/planetary/factsheet/marsfact.html. 
  7. ↑ Moutou, C.; Petit, P.; Charpentier, P.; Cristofari, P.; Baruteau, C.; Thébault, P.; Arnold, L.; Artigau, E. et al. (2025-10-13). "YARARA: Significant improvement in RV precision through post-processing of spectral time series". Astronomy & Astrophysics 653: A43. doi:10.1051/0004-6361/202140986. Bibcode: 2021A&A...653A..43C. 
  8. ↑ Brady, Madison; Bean, Jacob; Basant, Ritvik; Brown, Nina; Das, Tanya; Nixon, Matthew; Luque, Rafael; Piaulet-Ghorayeb, Caroline et al. (2025-06-25). "THE CHEMICAL COMPOSITION OF τ CETI AND POSSIBLE EFFECTS ON TERRESTRIAL PLANETS". The Astrophysical Journal 803 (2): 90. doi:10.1088/0004-637X/803/2/90. Bibcode: 2015ApJ...803...90P. 
  9. ↑ 9.0 9.1 Turner, Daisy A. et al. (2025). "The mass of the exo-Venus Gliese 12 b, as revealed by HARPS-N, ESPRESSO, and CARMENES". Monthly Notices of the Royal Astronomical Society 545 (1). doi:10.1093/mnras/staf1703. Bibcode: 2026MNRAS.545f1703T. 
  10. ↑ Dholakia, Shishir; Palethorpe, Larissa; Venner, Alexander; Mortier, Annelies; Wilson, Thomas G.; Huang, Chelsea X.; Rice, Ken; Van Eylen, Vincent et al. (2024-05-21), "Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS", Monthly Notices of the Royal Astronomical Society 531 (1): 1276, doi:10.1093/mnras/stae1152, Bibcode: 2024MNRAS.531.1276D 
  11. ↑ Beard, Corey et al. (October 2025). "Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging". The Astronomical Journal 170 (5): 279. doi:10.3847/1538-3881/ae0e20. Bibcode: 2025AJ....170..279B. 
  12. ↑ Damasso, M. et al. (2022). "A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514". Astronomy & Astrophysics 666: A187. doi:10.1051/0004-6361/202243522. 
  13. ↑ "HN Lib b". http://www.exoplanetkyoto.org/exohtml/HN_Lib_b.html. 
  14. ↑ Ribas, I. et al. (February 2023). "The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)". Astronomy & Astrophysics 670: A139. doi:10.1051/0004-6361/202244879. Bibcode: 2023A&A...670A.139R. 
  15. ↑ Suárez Mascareño, A. et al. (2017). "HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625". Astronomy and Astrophysics 605: A92. doi:10.1051/0004-6361/201730957. Bibcode: 2017A&A...605A..92S. https://www.aanda.org/articles/aa/full_html/2017/09/aa30957-17/aa30957-17.html. 
  16. ↑ LePage, Andrew (22 May 2017). "Habitable Planet Reality Check: Is GJ 625b a Super-Earth or a Super-Venus?". https://www.drewexmachina.com/2017/05/22/habitable-planet-reality-check-is-gj-625b-a-super-earth-or-a-super-venus/. 
  17. ↑ "GJ 625". http://hzgallery.org/3972_2.png. 
  18. ↑ 18.0 18.1 Feroz, F.; Hobson, M. P. (2014). "Bayesian analysis of radial velocity data of GJ667C with correlated noise: evidence for only two planets". Monthly Notices of the Royal Astronomical Society 437 (4): 3540–3549. doi:10.1093/mnras/stt2148. Bibcode: 2014MNRAS.437.3540F. 
  19. ↑ 19.0 19.1 Suárez Mascareño, A. et al. (November 2022). "Two temperate Earth-mass planets orbiting the nearby star GJ 1002". Astronomy & Astrophysics 670: A5. doi:10.1051/0004-6361/202244991. Bibcode: 2023A&A...670A...5S. 
  20. ↑ "Exoplanet-catalog" (in en). 23 December 2022. https://exoplanets.nasa.gov/exoplanet-catalog/8721/gj-1002-c/. 
  21. ↑ 21.0 21.1 Dreizler, S.; Jeffers, S. V.; Liebing, F.; Gorrini, P.; Haswell, C. A.; Gaidos, E.; Barnes, J. R.; Sordo, F. Del et al. (2025-04-15). "RedDots: Planetary masses in the GJ 1061 system from planet-planet interaction". Astronomy & Astrophysics 698: A114. doi:10.1051/0004-6361/202452490. Bibcode: 2025A&A...698A.114D. 
  22. ↑ "3 Earth-sized Planets Found Around One of Earth's Nearest Neighbors" (in en). https://www.discovermagazine.com/3-earth-sized-planets-found-around-one-of-earths-nearest-neighbors-40232. 
  23. ↑ "3 Earth-sized Planets Found Around One of Earth's Nearest Neighbors" (in en). https://www.discovermagazine.com/3-earth-sized-planets-found-around-one-of-earths-nearest-neighbors-40232. 
  24. ↑ Stefanov, A. K.; Mascareño, A. Suárez; Hernández, J. I. González; Nari, N.; Rebolo, R.; Affer, L.; Micela, G.; Ribas, I. et al. (2025-02-06). "HADES RV Programme with HARPS-N at TNG. XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system". Astronomy & Astrophysics 695: A62. doi:10.1051/0004-6361/202452630. ISSN 0004-6361. Bibcode: 2025A&A...695A..62S. 
  25. ↑ Template:Cite EPE
  26. ↑ Nari, N.; Dumusque, X. et al. (28 January 2025). "Revisiting the multi-planetary system of the nearby star HD 20794. Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf" (in en). Astronomy & Astrophysics 693: A297. doi:10.1051/0004-6361/202451769. ISSN 0004-6361. Bibcode: 2025A&A...693A.297N. 
  27. ↑ "Exoplanet-catalog". 18 July 2016. https://exoplanets.nasa.gov/exoplanet-catalog/3343/k2-72-e/. 
  28. ↑ "K2-288 B b - NASA Science". 22 April 2019. https://science.nasa.gov/exoplanet-catalog/k2-288-b-b/. 
  29. ↑ "Confirmed Planet Overview Page: Kepler-22 b". NASA Exoplanet Science Institute. http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-22 b&type=CONFIRMED_PLANET. 
  30. ↑ "Confirmed Planet Overview Page: Kepler-62e". NASA Exoplanet Science Institute. http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-62 e&type=CONFIRMED_PLANET. 
  31. ↑ "Confirmed Planet Overview Page: Kepler-62f". NASA Exoplanet Science Institute. http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-62 f&type=CONFIRMED_PLANET. 
  32. ↑ "Confirmed Planet Overview Page: Kepler-296e". NASA Exoplanet Science Institute. http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-296 e&type=CONFIRMED_PLANET. 
  33. ↑ 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. doi:10.1088/0004-637X/809/1/7. Bibcode: 2015ApJ...809....7B. 
  34. ↑ "Confirmed Planet Overview Page: Kepler-296 f". NASA Exoplanet Science Institute. http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-296 f&type=CONFIRMED_PLANET. 
  35. ↑ Template:Cite EPE
  36. ↑ "Exoplanet-catalog-Exoplanet exploration-Kepler-1606b". 10 May 2016. https://exoplanets.nasa.gov/exoplanet-catalog/2252/kepler-1606-b/. 
  37. ↑ "Earth-Size, Habitable Zone Planet Found Hidden in Early NASA Kepler Data". 15 April 2020. https://exoplanets.nasa.gov/news/1637/earth-size-habitable-zone-planet-found-hidden-in-early-nasa-kepler-data/. 
  38. ↑ "Exoplanet catalog-Exoplanet exploration-Kepler-1701b". 4 September 2020. https://exoplanets.nasa.gov/exoplanet-catalog/7742/kepler-1701-b/. 
  39. ↑ Cadieux, Charles; Doyon, René; MacDonald, Ryan J.; Turbet, Martin; Artigau, Étienne; Lim, Olivia; Radica, Michael; Fauchez, Thomas J. et al. (2024-06-21). "Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS". The Astrophysical Journal 970 (1): L2. doi:10.3847/2041-8213/ad5afa. Bibcode: 2024ApJ...970L...2C. 
  40. ↑ Delrez, L. et al. (September 2022). "Two temperate super-Earths transiting a nearby late-type M dwarf". Astronomy & Astrophysics 667: A59. doi:10.1051/0004-6361/202244041. Bibcode: 2022A&A...667A..59D. 
  41. ↑ Astudillo-Defru, Nicola; Forveille, Thierry; Bonfils, Xavier; Ségransan, Damien; Bouchy, François; Delfosse, Xavier et al. (2017). "The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293". Astronomy and Astrophysics 602: A88. doi:10.1051/0004-6361/201630153. Bibcode: 2017A&A...602A..88A. https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html. 
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  43. ↑ Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John et al. (2016). "A terrestrial planet candidate in a temperate orbit around Proxima Centauri". Nature 536 (7617): 437–440. doi:10.1038/nature19106. PMID 27558064. Bibcode: 2016Natur.536..437A. https://www.nature.com/articles/nature19106. 
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  49. ↑ "Comparison of the L 98-59 exoplanet system with the inner Solar System" (in en). https://www.eso.org/public/images/eso2112b/. 
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