K2-32

Author(en): Pan-STARRS

Veröffentlichungsdatum:

K2-32 is a binary star system of a K-type main-sequence star and a red dwarf star about 516.58 light-years away in the constellation Ophiuchus. The larger star (component A) has four confirmed planets (three neptunians and one terran) all found within 0.17 AU from their host, which is comparable to the solar distance of Mercury at perihelion

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