Kepler-1234

Author(s): SolHorizon

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Kepler-1234, also known as KOI-2424 and KIC 12453581, is a single K-type main-sequence star about 3,068.55 light-years away in the constellation Cygnus . A sub-Neptune-sized planet was discovered via the transit method in 2016, with an orbital period of 11.94 days . The planet Kepler-1234 b has a radius of approximately 2.81 times that of Earth, but its mass has not been determined .

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