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List of potentially habitable exoplanets

Adapted from Wikipedia Β· Discoverer experience

A stunning image showing the formation of a new planet around a young star, captured by a powerful telescope.

This list shows planets outside our solar system that might be able to support life. These planets are called exoplanets. The information comes from the Habitable Worlds Catalog and data from the NASA Exoplanet Archive. The catalog is kept by the Planetary Habitability Laboratory at the University of Puerto Rico at Arecibo.

For a planet to possibly support life, it needs to be at a distance from its star where liquid water can exist on its surface. The planet also needs the right conditions, like having the right kind of air and protection from harmful energy from its star. These conditions include planetary habitability, geophysical and geodynamical aspects, atmospheric density, radiation levels, and the star's plasma environment. Scientists study these planets to learn more about where life might exist beyond Earth.

Main list

This is a list of special stars called exoplanets that might be able to support life. These stars are in the right place around their suns to have temperatures that allow for liquid water, and they are either smaller than 10 times the size of Earth or have a radius less than 2.5 times that of Earth. Even though they are on this list, it doesn’t mean they can definitely support life. Some of the bigger ones might not be rocky like Earth and could be more like mini-Neptunes. Earth is also listed here so we can compare, and Venus and Mars are included just for reference.

ObjectStarStar typeMass (MβŠ•)Radius (RβŠ•)Density (g/cm3)Flux (FβŠ•)Teq (K)Period (days)Distance (ly)Refs/notes
Earth
(reported for reference)
SunG2V1.001.005.5141.00255365.250Only planet confirmed to support life
Venus
(reported for reference)
SunG2V0.8150.9505.2431.911244.261224.700.0000042
Mars
(reported for reference)
SunG2V0.1070.5333.9340.431209.8686.980.0000058–0.000042
55 Cancri Bc55 Cancri BM4Vβ‰₯5.3β€”β€”0.320033.740.9
Gliese 12 bGliese 12M4V0.71 or 0.950.904+0.037
βˆ’0.034
5.3 or 7.11.6Β±0.231512.739.7Near inner edge of HZ, might resemble Venus
Gliese 163 cGliese 163M3Vβ‰₯6.80β€”β€”1.2527725.649
Gliese 180 dGliese 180M2Vβ‰₯7.56β€”β€”0.26β€”106.339
Gliese 251 cGliese 251M3Vβ‰₯3.84β€”β€”β€”β€”53.618.2
Gliese 357 dGliese 357M2Vβ‰₯6.10β€”β€”0.3820055.731
Gliese 433 dGliese 433M2Vβ‰₯5.22β€”β€”1.06β€”36.129.6
Gliese 514 bGliese 514M1Vβ‰₯5.20β€”β€”0.28+0.51
βˆ’0.166
202140.425Highly eccentric
Gliese 555 bGliese 555M4Vβ‰₯5.46β€”β€”0.521436.220.4
Gliese 625 bGliese 625M2Vβ‰₯2.82β€”β€”β€”14.62821.1Likely too hot
Gliese 667 CcGliese 667 CM1Vβ‰₯3.81~1.54β€”0.8827728.123.62
GJ 1002 bGJ 1002M5Vβ‰₯1.08~1.03β€”0.6723110.315.8
GJ 1002 cGJ 1002M5Vβ‰₯1.361.1β€”0.2618221.215.8
GJ 1061 cGJ 1061M5V1.81+0.13
βˆ’0.11
~1.18β€”1.452756.712
GJ 1061 dGJ 1061M5V1.67+0.17
βˆ’0.16
~1.16β€”0.6921813.012
GJ 3293 dGJ 3293M2Vβ‰₯7.60β€”β€”0.5922348.166
GJ 3998 dGJ 3998M1Vβ‰₯6.07β€”β€”β€”41.858
HD 20794 dHD 20794G8Vβ‰₯5.82β€”β€”β€”β€”647.619.7Highly eccentric orbit
HD 216520 cHD 216520K0Vβ‰₯9.44β€”β€”1.28β€”154.464
HIP 38594 bHIP 38594M0Vβ‰₯8.10β€”β€”1.34β€”60.758
K2-72eK2-72M2V~2.211.29β€”1.3026124.2217
K2-155dK2-155K?V4.271.64β€”β€”28940.6290
K2-288BbK2-288 BM3V4.271.91β€”0.4420731.4214
K2-332bK2-332M3.5Vβ€”2.20β€”1.17β€”17.7402
Kepler-22bKepler-22G5V~9.1 or ~352.38β€”1.10261289.9635
Kepler-62eKepler-62K2V4.5+14.2
βˆ’2.6
1.61β€”1.15264122.4981
Kepler-62fKepler-62K2V2.8Β±0.41.41β€”0.41204267.3981
Kepler-155cKepler-155M0Vβ€”2.24β€”1.05β€”52.7957
Kepler-174dKepler-174K3Vβ€”2.19β€”0.59206247.41,254
Kepler-186fKepler-186M1V1.44+2.33
βˆ’1.12
1.17β€”0.29188129.9579
Kepler-283cKepler-283K5Vβ€”1.82β€”0.8924892.71,526
Kepler-296eKepler-296K7V2.961.52β€”1.4127634.1737
Kepler-296fKepler-296K7Vβ€”1.80β€”0.4422563.3737
Kepler-440bKepler-440K6Vβ€”1.91β€”1.44273101.1981
Kepler-442bKepler-442K5V2.36+5.9
βˆ’1.3
1.35β€”0.70233112.31,193
Kepler-443bKepler-443K3Vβ€”2.35β€”0.89247177.72,615
Kepler-705bKepler-705M?Vβ€”2.11β€”0.7724356.1903
Kepler-725 cKepler-725G9V9.7β€”β€”β€”207.52,526
Kepler-1229bKepler-1229M?V2.5401.40β€”0.3221386.8865
Kepler-1410bKepler-1410K?Vβ€”1.78β€”1.0727460.91196
Kepler-1455bKepler-1455K?Vβ€”2.10β€”1.3049.31280
Kepler-1540bKepler-1540K?Vβ€”2.49β€”0.78250125.4799
Kepler-1544 bKepler-1544K2Vβ€”1.78β€”0.84248168.81092
Kepler-1606bKepler-1606G7Vβ€”2.07β€”1.64277196.42710
Kepler-1649cKepler-1649M5V1.201.06β€”0.7523719.5301
Kepler-1652bKepler-1652M?Vβ€”1.60β€”0.8424438.1822
Kepler-1653bKepler-1653K?Vβ€”2.17β€”1.04258140.32461
Kepler-1701bKepler-1701K?Vβ€”2.22β€”1.42275169.11904
LHS 1140 bLHS 1140M4V5.601.735.9Β±0.30.4322624.749Likely an ocean world with an atmosphere
LP 890-9 cLP 890-9M6Vβ€”1.37β€”0.912728.46105
Luyten bLuyten's StarM3Vβ‰₯2.89~1.35β€”1.0625818.6512.3
Proxima Centauri bProxima CentauriM5Vβ‰₯1.07:β€Š16β€Š1.17Β±0.23β€”0.7022811.1864.25Affected by stellar flare, possibly affected by high radiation flux
Ross 128 bRoss 128M4Vβ‰₯1.40~1.80β€”1.482809.8711.0
Ross 508 bRoss 508M4Vβ‰₯4.00β€”β€”1.32β€”10.837
Struve 2398 BcStruve 2398M4Vβ‰₯3.4β€”β€”37.911.5
Teegarden's Star bTeegarden's StarM7Vβ‰₯1.05~1.02β€”1.152644.9112.5
Teegarden's Star cTeegarden's StarM7Vβ‰₯1.11~1.04β€”0.3719911.412.5
L 98-59 fL 98-59M3Vβ‰₯2.97β€”β€”>128923.0734.6
TOI-700 dTOI-700M2V~1.721.14β€”0.8724637.4101
TOI-700 eTOI-700M2V0.820.95β€”1.2727327.8101
TOI-715 bTOI-715M4V3.021.55β€”0.6723419.29137
TOI-2094 AbTOI-2094M3V1.90β€”0.9818.8164
TOI-2257 bTOI-2257M3V5.712+4.288
βˆ’2.311
2.20β€”0.57+1.68
βˆ’0.31
256+61
βˆ’17
35.2188Highly eccentric
TOI-2285 bTOI-2285M4V4.11.75β€”β€”28427137Likely too hot
TOI-7166 bTOI-7166M4V2.01β€”1.0724912.9115
TRAPPIST-1eTRAPPIST-1M8V0.690.925.650.652306.141Confirmed to be rocky. Possibly has an atmosphere.
TRAPPIST-1fTRAPPIST-1M8V1.041.043.3 Β± 0.90.372009.241Confirmed to be rocky
TRAPPIST-1gTRAPPIST-1M8V1.321.134.1860.2518212.441Confirmed to be rocky
Wolf 1069 bWolf 1069M5Vβ‰₯1.26~1.08β€”0.6525015.631.2
Wolf 1061cWolf 1061M3Vβ‰₯3.41~1.60β€”1.3027117.913.8

Current candidates

This is a list of special faraway planets that might be able to support life. These planets are in the right place around their stars to possibly have liquid water, and they are smaller than Earth or not too much heavier. Earth is listed here for comparison, while Venus and Mars are included just for reference.

ObjectStarStar typeMass (MβŠ•)Radius (RβŠ•)Density (g/cm3)Flux (FβŠ•)Teq (K)Period (days)Distance (ly)Refs/notes
Earth
(reported for reference)
SunG2V1.001.005.5141.00255365.250Only planet confirmed to support life
Venus
(reported for reference)
SunG2V0.8150.9505.2431.911244.261224.700.0000042
Mars
(reported for reference)
SunG2V0.1070.5333.9340.431209.8686.980.0000058–0.000042
Gliese 180 cGliese 180M2Vβ‰₯6.40β€”β€”0.7823924.339
HD 40307 gHD 40307K2Vβ‰₯7.09β€”β€”0.67226197.842
HD 137010 bHD 137010K3V1.06β€”0.29355146
Kepler-452bKepler-452G2V~51.63β€”1.11261384.81799
KOI-4878.01KOI-4878F8V~1.9+1.1
βˆ’0.5
1.05β€”1.04+1.1
βˆ’0.34
257449.01,075
KOI-5715.01KOI-5715K3Vβ€”1.932601902,964
Lacaille 9352 dLacaille 9352M0Vβ‰₯8.3β€”β€”50.710.7
LTT 1445 AdLTT 1445AM2Vβ‰₯2.72β€”β€”β€”24.322.4
Tau Ceti fTau CetiG8Vβ‰₯3.93β€”β€”0.2719064211.9Has been only in HZ for less than 1 Gya
TOI-715.02TOI-715M4V1.066Β±0.0920.48+0.12
βˆ’0.17
25.6137
WD 1054–226 bWD 1054–226DAZ~1β€”β€”1.04118 The surface temperature might be high enough for habitability

Previous candidates

Some planets that were once thought to be good places for life have been studied more closely and found to not be as suitable.

For example, Gliese 581 d and g, Gliese 667 Ce and f, Gliese 682 b and c, Kapteyn b, Gliese 229 Ac, HD 85512 b, and Gliese 832 c were once thought to be in zones where life might exist, but later studies suggested they might not be.

Other planets like Gliese 180 b, Tau Ceti e, HD 85512 b, and Kepler-69c were also thought to be possibly habitable, but better models show they are outside the zones where life could thrive.

Kepler-438b was once considered potentially habitable but was later found to face strong flares that could remove its atmosphere, making it less likely to support life.

K2-3d and K2-18b were also thought to be good candidates for habitability, but recent studies show they are more like gaseous planets and not likely to support life.

Kepler-1638b was once thought to be a smaller planet that could support life, but newer measurements show it is more likely a large, icy planet with less chance for habitability.

KOI-1686.01 was once thought to be a habitable planet but was later found to be a false detection. Other planets like Kepler-577b and Kepler-1649b were also once considered habitable but are no longer thought to be so.

TRAPPIST-1 d was thought to be a place where life might exist, but recent data suggests it likely does not have an atmosphere like Earth's, making it less likely to support life.

Images

The Crab Nebula: A colorful view of a star's explosion remnant captured by the Hubble Space Telescope.
The Curiosity rover drilling into a rock on Mars, with the Yellowknife Bay area and Mount Sharp visible in the background.
A stunning view of Earth rising over the lunar horizon, captured by astronauts during the Apollo 8 mission.
A colorful collection of planets in our solar system, showing Mercury, Venus, Earth with its Moon, Mars, Jupiter, Saturn, Uranus, and Neptune, each captured by space probes.
An artist's rendering of HE 1523-0901, one of the oldest known stars in our galaxy, located about 7,500 light-years from Earth.

Related articles

This article is a child-friendly adaptation of the Wikipedia article on List of potentially habitable exoplanets, available under CC BY-SA 4.0.

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