Kepler-1442

Autor(es): Pan-STARRS

Fecha de lanzamiento:

Kepler-1442, also known as KOI-3220, is an F-type main sequence star about 2,020 light-years away in the constellation Cygnus. A single neptunian planet is orbiting at a distance of 0.37 AU from its parent star, where in 2020 was speculated to harbor a superterran-mass satellite, but since deemed unlikely to exist according to follow-up studies

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