Kepler-35
Autor(es): Karistus SolHorizon
Data de publicación:
Última actualización:
Kepler-35, aka KOI-2937, is a binary system composed of a G-type main sequence star and a K-type main sequence star located about 6254.19 lightyears from the solar system. Both stars are orbited by a low-density sub-Jupiter which completes a full revolution in a little over 1/3 of a year.
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