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KOI-433.02 m : ウィキペディア英語版 | KOI-433.02 m
KOI-433.02 m is a predicted exomoon around the candidate planet KOI-433.02. If the planet, observed by the Kepler telescope is confirmed, it is expected that, based on the general rule for planet-to-satellite(s) mass ratio of 10,000:1〔Bate et al 2003 (Monthly Notices of RSA, vol. 341, pp. 213-229)〕 one or more satellites could exist in orbit around it. If a single moon indeed existed, based on this predicted mass and the orbital properties of its parent planet and star, it could have an ESI rating of 0.93,〔http://phl.upr.edu/library/notes/latestlistofpotentialhabitableexoplanetsandexomoons (appears as simply 433.02 m)〕 meaning it would not only be the most Earth-like exomoon, but the most Earth-like planetary mass object overall, as the highest ESI rating for a planet is 0.88.〔http://phl.upr.edu/projects/habitable-exoplanets-catalog〕 However, it has not been observed, merely predicted.〔http://phl.upr.edu/library/notes/latestlistofpotentialhabitableexoplanetsandexomoons (appears as simply 433.02 m)〕 ==Comparison to Earth==
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