K2-332 b

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The planet is confirmed to exist and was discovered by the K2 "Second Light" mission in 2016. It was originally referred to by its EPIC designation. The average transit time is 2 hours and 2 minutes and the average depth is 0.6508%.[1][2][4][5] The object's star is within the 2MASS catalog.[5]

Characteristics

Mass, radius, and temperature

The planet has an estimated mass of 5.47 earths, and at a radius of more than twice that of the Earth, the density corresponds to that of a watery or gaseous Mini-Neptune rather than a rocky Super-Earth. It has an equilibrium temperature of 266 K (−7 °C; 19 °F), somewhat higher than Earth's.[3][5]

Orbit and host star

The planet orbits within the inner part of the habitable zone, about 1/3 of the way between the runaway G limit for Super-Earths and the absolute inner edge. Its orbital period is 17.7 days, but the planet has an unknown semi-major axis. Its star is a dim red dwarf with about 20% the mass and size of the sun. In its habitable-zone orbit, the planet receives 1.17 times the insolation Earth gets from the sun.[1][2][3][4][5]

Habitability

See also

References

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