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It has been suggested that the recently discovered exoplanet GJ581d might be able to support liquid water due to its relatively low mass and orbital distance. However, GJ581d receives 35% less stellar energy than Mars and is probably locked in tidal resonance, with extremely low insolation at the poles and possibly a permanent night side. Under such conditions, it is unknown whether any habitable climate on the planet would be able to withstand global glaciation and / or atmospheric collapse.
Here we present three-dimensional climate simulations that demonstrate GJ581d will have a stable atmosphere and surface liquid water for a wide range of plausible cases, making it the first confirmed super-Earth (exoplanet of 2-10 Earth masses) in the habitable zone.
We find that atmospheres with over 10 bar CO2 and varying amounts of background gas (e.g., N2) yield global mean temperatures above 0 degrees Celsius for both land and ocean-covered surfaces. Based on the emitted IR radiation calculated by the model, we propose observational tests that will allow these cases to be distinguished from other possible scenarios in the future.
Two extrasolar planets, Gliese 667 Cb (GJ 667 Cb) and Gliese 667 Cc (GJ 667 Cc), have been found orbiting Gliese 667 C. Gliese Cc have masse of at least 3.9 times the mass of Earth (and are thus classified as super-Earth). It orbits the star every four weeks at a distance of 0.1235 AU.
Planet Cc was first mentioned in a pre-print made public on 21 November 2011. It was described as one of the best candidates yet found to harbor liquid water, and thus, potentially, support life on its surface. A detailed orbital analysis and refined orbital parameters for Gliese 667 Cc were presented.
Preliminary radial-velocity measurements indicate the presence of the super-Earth planet candidate Gliese 667 Cc, orbiting in an "extended habitable zone" where large quantities of CO2 and other greenhouse gases may make life possible (a planet similar to Gliese 581 d). The researchers noted that the radial-velocity signals from the system indicate the presence of other companions beyond the habitable zone, but that such planets would have unstable and eccentric orbits if they existed at all.
Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light-years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super-Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT-7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low density.
Gliese 1214 b is also significant because its parent star is relatively near the Sun and because it transits (crosses in front of) that parent star, which allows the planet's atmosphere to be studied using spectroscopic technologies.
HD 85512 b is an extrasolar planet orbiting Gliese 370 (a K-type or "orange dwarf") star approximately 36 light-years distance from Earth in the constellation of Vela (the Sail).
Due to its mass of at least 3.6 times the mass of Earth, HD 85512 b is classified as a super-Earth and is one of the smallest exoplanets discovered to be on the edge of the habitable zone. HD 85512 b, along with Gliese 581 d is considered to be one of the best candidates for habitability as of August 30, 2011
For the temperature to be below 270 K (-3.15° C), for a circular orbit, the planetary albedo should be 0.48 ± 0.05 and for an eccentricity of 0.11, the planetary albedo should be 0.52. If the planet has 50% cloud cover, water may exist in liquid form on the planet provided its atmosphere is similar to our own, thus making the planet habitable. Also, if the albedo of the planet is increased due to cloud cover, water could be present in its liquid form on the planet, which would mean that the planet is on the edge of habitability.
Based on the bolometric luminosity of its parent star, the planet would get 1.86 times as much sunlight as Earth, slightly less than Venus at 1.92, suggesting that it may have suffered a runaway greenhouse effect.
Using the measured stellar luminosity of Gliese 370 of 0.126 times that of our Sun, it is possible to calculate HD 85512 b's effective temperature a.k.a. black body temperature, which probably differs from its surface temperature. The effective temperature for HD 85512 b, assuming an aforementioned albedo, would be 24.138 °C (75 °F).
Kepler-22b is an extrasolar planet orbiting G-type star Kepler-22. It is located 600 light years away from Earth in the constellation of Cygnus. It was discovered by NASA's Kepler Space Telescope and is the first known transiting planet to orbit within the habitable zone of a Sun-like star.
It is thought that the object has a mass similar to that of Neptune (~35 Earth masses). Another possibility is that Kepler-22b is an "ocean-like" world. It might also be comparable to the water-rich planet GJ 1214 b although Kepler-22b, unlike GJ 1214b, is in the habitable zone.