Destinations

List of nearest terrestrial exoplanet candidates

From Wikipedia, the free encyclopedia

This list of nearest terrestrial exoplanets candidates contains possible terrestrial (“rocky”) exoplanets at a distance of up to 50 light-years from the Solar System, ordered by increasing distance.

They may be composed primarily of silicate rocks and/or metals. Within the Solar System, the terrestrial planets are the inner planets closest to the Sun.

There are no scientific consensus about terrestrial composition of the most of the planets in the list. Sources in the first column confirm the possibility of terrestrial composition.

Name Image (artist concept) Mass (M) Radius Density Surface Gravity Temperature Semi-major axis(AU) Eccentricity Earth SImilarity Index Planetary Habitability Index Main
source
Star Distance from theSun (ly)
Gliese 876 d[1]
Gl876 planet1 h.jpg
6,8 0,021 0,21 No. Surface temperature estimate: 157-377°C[2] [3] Gliese 876 15
Gliese 581 e
Planet Gliese 581 e.png
≥1,7 0,029 0 No. It is unlikely to possess an atmosphere due to its high temperature [4] Gliese 581 20
Gliese 581 c [5]
ESO - The Planetary System in Gliese 581 (by).jpg
≥5,6 0,072 0 Probably no. Likely to lie outside the habitable zone[6] [7] Gliese 581 20
Gliese 581 d [8]
Planet Gliese 581 d.png
≥5,6 0,218 0 Possibly. Lies within the habitable zone[9] [10] Gliese 581 20
61 Virginis b[11]
Artist concept 61vir b.png
≥5,1 0,050 0,12 No. Orbits too close to the star [12] 61 Virginis 28
HD 85512 b[13]
HD 85512 b (Artists's impression).jpg
≥3,6 0.26 0.11 Possibly. Considered to be the best candidate for habitability (as of August 25, 2011)[14] [15] HD 85512 36
55 Cancri e
Newneptune nasa big.jpg
8,6 0,016 0,17 No. Orbits too close to the star [16] 55 Cancri 40
HD 40307 b[17]
HD 40307 B.jpg
≥4,2 0,047 0 No. Orbits too close to the star [18] HD 40307 42
HD 40307 c[19]
HD 40307 C.jpg
≥6,8 0,081 0 No. Orbits too close to the star [20] HD 40307 42
HD 40307 d[21]
Planets of HD 40307.jpg
≥9,2 0,134 0 No. Orbits too close to the star [22] HD 40307 42

[edit]See also

List of potential habitable exoplanets

From Wikipedia, the free encyclopedia

Gliese 581 d is one of a few potential habitable exoplanets confirmed so far

This is a list of potential habitable exoplanets candidates ranked by similarity with Earth using the Earth Similarity Index(ESI). The index was made by the Planetary Habitability Laboratory at UPR-Arecibo.

Contents

[hide]

[edit]Methodology

[edit]Earth Similarity Index (ESI)

The ESI or the “easy scale,” measures how similar are planets to Earth in a scale from zero to one, with one being identical to Earth. ESI values between 0.8 and 1.0 correspond to Earth-like planets with a rocky composition that is able to hold a terrestrial atmosphere under temperate conditions. The ESI is a function of the planet’s radiusdensityescape velocity, and surface temperature.

[edit]Standard Primary Habitability (SPH)

The SPH measures the thermal-water climate suitability of a planet for land primary producers (vegetation) in a scale from zero to one, with one being more habitable. It is correlated with the global distribution of vegetation and net primary productivity. The SPH is a function of surface temperature and relative humidity. Only the thermal component of the SPH is used for exoplanets, assuming that water is present.

[edit]Habitable Zones Distance (HZD)

The HZD is a measure of how far a planet is from the center of its parent star habitable zone (HZ) in habitable zone units (HZU). Planets inside the HZ have HZD values between -1 to +1 HZU, with zero being the exact center of the HZ. The negative and positive values correspond to locations closer and farther to the star, respectively. The HZD is a function of the star’s luminosity and temperature, and the planet’s distance.

[edit]Planetary Class (pClass)

The pClass classifies planetary bodies with a combination of three thermal zones and seven mass categories. The thermal zones are hot, warm, and cold. They are related to the orbital position of the body with respect to the HZ, warm being the HZ. The mass divisions are asteroidan, mercurian, subterran, terran, superterran, neptunian, and jovian. The classification can be used for any solar and extrasolar planets including moons.

[edit]Habitable Class (hClass)

The hClass is a classification only for habitable worlds (Earth-size planets inside the HZ) in five thermal categories. The categories are hypopsychroplanets (Class hP, very cold planets), psychroplanets (Class P, cold planets), mesoplanets (Class M, medium temperature planets; not to be confused with Isaac Asimov‘s coinage mesoplanet), thermoplanets(Class T, hot planets), and hyperthermoplanets (Class hT, very hot planets). These names where inspired by the names used in microbiology to describe the growth temperatures of microbial life. Class M planets also have the thermal surface requirements to support complex life (0-50°C), a name familiar from science fiction. The other categories represent conditions only habitable by extremophilic life. The generic Class NH is used for non habitable planets.

[edit]List

For comparison purposes, four solar terrestrial planets are included in the list. The only three confirmed exoplanets in the data, HD 85512 bGliese 581 d and Kepler-22b, still rank very low as compared to the NASA Kepler candidates.

Rank Name ESI SPH HZD Combined pClass hClass Status
N/A Earth 1.00 0.72 -0.50 0.74 warm terran mesoplanet non-exoplanet
1 KOI 736.01 0.98 0.63 -0.59 0.67 warm terran mesoplanet Kepler candidate
2 KOI 899.03 0.94 0.99 -0.74 0.73 warm terran mesoplanet Kepler candidate
3 KOI 494.01 0.93 0.00 -0.33 0.53 warm terran psychroplanet Kepler candidate
4 KOI 314.02 0.92 0.34 -0.86 0.47 warm terran mesoplanet Kepler candidate
5 KOI 663.02 0.92 0.95 -0.78 0.7 warm subterran mesoplanet Kepler candidate
6 KOI 784.01 0.91 0.46 -0.81 0.52 warm terran mesoplanet Kepler candidate
7 KOI 610.01 0.90 0.05 -0.91 0.35 warm terran mesoplanet Kepler candidate
8 KOI 947.01 0.90 0.05 -0.36 0.53 warm terran psychroplanet Kepler candidate
9 KOI 812.02 0.88 0.18 -0.83 0.41 warm terran mesoplanet Kepler candidate
10 KOI 817.01 0.87 0.22 -0.82 0.42 warm superterran mesoplanet Kepler candidate
11 KOI 1422.02 0.86 0.00 -0.06 0.6 warm terran psychroplanet Kepler candidate
12 KOI 812.03 0.86 0.00 0.01 0.62 warm terran psychroplanet Kepler candidate
13 KOI 952.03 0.84 0.33 -0.79 0.46 warm terran mesoplanet Kepler candidate
14 KOI 1361.01 0.83 0.03 -0.27 0.53 warm superterran psychroplanet Kepler candidate
15 KOI 463.01 0.83 0.00 0.34 0.5 warm terran psychroplanet Kepler candidate
16 KOI 701.03 0.81 0.76 -0.65 0.64 warm superterran mesoplanet Kepler candidate
17 KOI 227.01 0.81 0.00 -0.93 0.29 warm terran thermoplanet Kepler candidate
18 KOI 255.01 0.80 0.91 -0.66 0.68 warm superterran mesoplanet Kepler candidate
19 KOI 854.01 0.79 0.00 0.54 0.42 warm terran hypopsychroplanet Kepler candidate
20 KOI 1026.01 0.79 0.00 0.80 0.33 warm terran hypopsychroplanet Kepler candidate
21 HD 85512 b 0.79 0.00 -0.95 0.28 warm superterran thermoplanet Confirmed
22 KOI 448.02 0.78 0.01 -0.18 0.54 warm superterran psychroplanet Kepler candidate
23 Kepler-22b 0.75 0.00 -0.59 0.39 warm superterran mesoplanet Confirmed
24 KOI 268.01 0.74 0.00 -0.94 0.27 warm superterran thermoplanet Kepler candidate
25 KOI 87.01 0.71 0.03 -0.79 0.32 warm superterran mesoplanet Kepler candidate
26 Gliese 581 d 0.70 0.00 0.79 0.3 warm superterran psychroplanet Confirmed
N/A Mars 0.66 0.00 0.33 0.44 warm subterran hypopsychroplanet non-exoplanet
N/A Mercury 0.60 0.00 -1.46 0.05 hot mercurian non-habitable non-exoplanet
N/A Venus 0.44 0.00 -0.93 0.17 warm terran non-habitable non-exoplanet