Kepler-1520

Autor(es): LukeCEL Gurren Lagann

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Kepler-1520, also known as KOI-3794, is a K-type main sequence star about 2,017 light-years away in the constellation Cygnus. Its sole planet is one of a few known to have dust tails around it, which is caused by its surface evaporating from its very tight proximity to its host star

Kepler-1520 b

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