Kepler-725

作者：Galaxy-Leaper

發佈日期：

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.

請在此 翻譯 協助翻譯本頁。

在 Celestia 中開啟（建議） 或 下載

如何安裝附加元件？請在此 查閱 了解。