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Kepler-69 System

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Exoplanetary Scratchpad

[SysBP Img]

Kepler-69, also known as 2MASS J19330262+4452080 and KOI-172, is a sun-like star a little dimmer and about a billion years older. The inner planet b is a hot super-Earth. Initially, planet c was thought to be the most Earth-like planet detected, and heralded as the first Super-Earth found in the habitable zone by Kepler around a sunlike star (candidacy announced with a batch of 461 candidates found in 2013). It is now thought to be more likely interior to the habitable zone, a "Super Venus", is 70% larger than Earth, and has a Venus-like period of 242 days.

Kepler-69 System Web PagesEdit

Kepler-69 System In the NewsEdit

Most Earth-Like Planet Detected (Jan 2013)Edit

Planets Confirmed (Apr 2013)Edit

See also Kepler-62 System

Planet c More like a Super-Venus(2013)Edit

See AlsoEdit

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