Astronomy:Kepler-155c

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Kepler 155c is an exoplanet in orbit around a K-type star 957 light-years away.[1]

Properties

Mass and radius

Kepler 155c is a Neptune-like planet with a mass of 5.65 Earth masses and a radius of 0.2 Jupiters (2.24 Earths.)[1] It has a density about half that of the Earth and a gravity of 1.126 Earth gravities.

Orbit

Kepler 155c orbits its star every 52.7 days at 0.242 AU. It has a low eccentricity.[1]

Star

Kepler 155 is a K-type main sequence star 957 light-years from Earth.[1] It is host to at least two planets, Kepler 155b and 155c.[2] The star has a temperature of 4508 K, a mass of 0.677 solar masses, and a radius 62% that of the Sun. Kepler 155's metallicity is similar to that of the Sun, at -0.04.[3]

Habitability

Kepler 155c is in the inner habitable zone of its star.[4] It is likely tidally locked due to its close stellar orbit and low eccentricity,[1] but since it is larger than Earth, if it is a water world, rather than an ice giant like NASA Exoplanet Exploration suggests, it could have an atmosphere that circulates air around the planet, making the planet habitable over a wide range of its regions.

Discovery

Kepler 155c was discovered in 2014 by the Kepler space telescope. Kepler used the transit method to find Kepler 155c.[2]

References