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Citations that are already defined on the page should be defined here so when we merge this list in we will not have to fix citations

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Info from http://phl.upr.edu/projects/habitable-exoplanets-catalog please cite where the data come from!

List of Exoplanets in the conservative habitable zone

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This is a list of the exoplanets that are more likely to have a rocky composition and maintain surface liquid water (i.e. 0.5 < Planet Radius ≤ 1.5 Earth radii or 0.1 < Planet Minimum Mass ≤ 5 Earth masses, and the planet is orbiting within the conservative habitable zone).

Object Star Star type Planet type Mass(M⊕) Radius(R⊕) Flux(F⊕) Teq(K) Period(Days) Distance(Ly) ESI Ref
Earth Sun G2V warm terran 1.00 1.00 1.00 255 365.25 - 1.00
Gliese 667 Cc Gliese 667 C M1.5V warm terran ≥3.8 1.1 - 1.5 - 2.0 0.88 247 28.143 ± 0.029 23.62 0.84 [1] [2]
Kepler-442b Kepler-442 K warm terran 8.2 - 2.3 - 1.0 1.34 0.70 233 112.3053 1291.6 0.84 [2]
Gliese 667 Cf Gliese 667 C M1.5V warm terran ≥ 2.7 1.0 - 1.4 - 1.8 0.56 221 39 23.62 0.77 [2]
Wolf 1061c Wolf 1061 M3V warm terran ≥ 4.3 1.1 - 1.6 - 2.0 0.60 223 17.9 13.8 0.76 [2]
Kapteyn b Kapteyn sdM1 warm terran ≥ 4.8 1.2 - 1.6 - 2.1 0.43 205 48.616 12.8 0.67 [2]
Kepler-62f Kepler-62 K2V warm terran 10.2 - 2.8 - 1.2 1.41 0.39 201 267.291 ~1200 0.67 [2]
Kepler-186f Kepler-186f M1V warm terran 4.7 - 1.5 - 0.6 1.17 0.29 188 129.9459 ~1200 0.61 [2]
Gliese 667 Ce Gliese 667 C M1.5V warm terran ≥ 2.7 1.0 - 1.4 - 1.8 0.30 189 62.2 23.62 0.60 [2]

List of Exoplanets in the optimistic habitable zone

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This is a list of the exoplanets that are less likely to have a rocky composition or maintain surface liquid water (i.e. 1.5 < Planet Radius ≤ 2.5 Earth radii or 5 < Planet Minimum Mass ≤ 10 Earth masses, or the planet is orbiting within the optimistic habitable zone).

Object Star Star type Planet type Mass(M⊕) Radius(R⊕) Flux(F⊕) Teq(K) Period(Days) Distance(Ly) ESI Ref
Kepler-438b Kepler-438 M warm terran 4.0 - 1.3 - 0.6 1.1 1.38 276 35.2 473 0.88 [2]
Kepler-296e Kepler-296 M warm terran 12.5 - 3.3 - 1.4 1.5 1.22 267 34.1 737 0.85 [2]
Kepler-62e Kepler-62 K warm Superterran 18.7 - 4.5 - 1.9 1.6 1.10 261 122.4 1200 0.83 [2]
Kepler-452b Kepler-452 G warm Superterran 19.8 - 4.7 - 1.9 1.6 1.11 261 384.8 1402 0.83 [2]
Gliese 832 c Gliese 832 M warm Superterran ≥ 5.4 1.2 - 1.7 - 2.2 1.00 253 35.7 16 0.81 [2]
K2-3d K2-3 M warm terran 11.1 1.5 1.46 280 44.6 137 0.80 [2]
Kepler-283c Kepler-283 K warm Superterran 35.3 - 7.0 - 2.8 1.8 0.90 248 92.7 1741 0.79 [2]
Tau Ceti e Tau Ceti G warm terran ≥ 4.3 1.1 - 1.6 - 2.0 1.51 282 168.1 12 0.78 [2]
Gliese 180 c Gliese 180 M Warm Superterran ≥ 6.4 1.3 - 1.8 - 2.3 0.79 239 24.3 38 0.77 [2]
Kepler-440b Kepler-440 K Warm Superterran 41.2 - 7.7 - 3.1 1.9 1.43 273 101.1 851 0.75 [2]
Gliese 180b Gliese 180 M Warm Superterran ≥ 8.3 1.3 - 1.9 - 2.4 1.23 268 17.4 38 0.75 [2]
HD 40307 g HD 40307 K Warm Superterran ≥ 7.1 1.3 - 1.8 - 2.3 0.68 227 197.8 42 0.74 [2]
Gliese 163 c Gliese 163 M Warm Superterran ≥ 7.3 1.3 - 1.8 - 2.3 0.66 230 25.6 49 0.73 [2]
K2-18 b K2-18 M Warm Superterran ? - 16.5 - 6.0 2.2 0.94 251 32.9 111 0.73 [2]
Kepler-61 b Kepler-61 K Warm Superterran ? - 13.8 - 5.2 2.2 1.27 267 59.9 1063 0.73 [2]
Kepler-443 b Kepler-443 K Warm Superterran ? - 19.5 - 7.0 2.3 0.89 247 177.7 2540 0.71 [2]
Kepler-22 b Kepler-22 G Warm Superterran ? - 20.4 - 7.2 2.4 1.11 261 289.9 619 0.71 [2]
Gliese 422 b Gliese 422 M Warm Superterran ≥ 9.9 1.4 - 2.0 - 2.6 0.68 231 26.2 41 0.71 [2]
K2-9 b K2-9 M Warm Superterran ? - 16.8 - 6.1 2.2 1.38 276 18.4 359 0.71 [2]
Gliese 3293 c Gliese 3293 M Warm Superterran ≥ 8.6 1.4 - 1.9 - 2.5 0.60 223 48.1 59 0.70 [2]
Kepler-298 d Kepler-298 K Warm Superterran ? - 26.8 - 9.1 2.5 1.29 271 77.5 1545 0.68 [2]
Kepler-174 d Kepler-174 K Warm Superterran ? - 14.8 - 5.5 2.2 0.43 206 247.4 1174 0.61 [2]
Kepler-296 f Kepler-296 M Warm Superterran 28.7 - 6.1 - 2.5 1.8 0.34 194 63.3 737 0.60 [2]
Gliese 682 c Kepler-296 M Warm Superterran ≥ 8.7 1.4 - 1.9 - 2.5 0.37 198 57.3 17 0.59 [2]
KOI-4427 b KOI-4427 M Warm Superterran 38.5 - 7.4 - 3.0 1.8 0.24 179 147.7 782 0.52 [2]

References

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  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. arXiv:1307.6984. Bibcode:2014MNRAS.437.3540F. doi:10.1093/mnras/stt2148.{{cite journal}}: CS1 maint: multiple names: authors list (link) CS1 maint: unflagged free DOI (link)
  2. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag PHL's Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo
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