Kepler-725

Autor(i): Galaxy-Leaper

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Kepler-725, also known as KOI-918, is a G-type main sequence star located 2,528.538 light-years away from Earth. As of August 2025, signals from two planets have been detected, one being a gas giant and the other a sub-Neptune or hydrogen ocean planet. Among them, Kepler-725 c was discovered using the Transit Timing Variation. Recent studies indicate that Kepler-725 c has a relatively high orbital inclination and eccentricity, which significantly reduces the planet's habitability.

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