Kepler-25 B

Аўтар(ы): Karistus

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Kepler-25 B, aka KOI-1803, is a part of a binary system consisting of an F-type main sequence star and a K-type main sequence star. Serving as the secondary component to the binary. Three candidate planets were detected by Kepler, though two were ruled as false positives, one candidate remains, a possible hot mini-Neptune on a 4.5 day orbit.

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Адкрыць у Celestia (рэкамендуецца) або Спампаваць

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