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Kepler-445c
Kepler-445c is an exoplanet orbiting the Red dwarf star Kepler-445 every 5 days in the inner edge of the circumstellar habitable zone.〔http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-445+c&type=CONFIRMED_PLANET〕 PHL has currently not assessed the planet for Habitability.〔http://phl.upr.edu/projects/habitable-exoplanets-catalog〕 ==Physical Features==
With a radius of 2.5R⊕ it is likely a Water world or even a Mini-Neptune if gaseous. Due to its high radius it would have to have a mass of 15.9M⊕ According to the (PHL exoplanet density calculator ) to have a density similar of that of the Earth.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Kepler-445c」の詳細全文を読む
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