User:Kepler-1229b/sandbox/KOI-7923.01

KOI-7923.01
KOI-7923.01 is a potential extrasolar planet in the habitable zone of its host star (KIC 9084569) in the constellation Cygnus. It was discovered by the Kepler spacecraft in 2017.

KOI-7923.01, if it was confirmed to exist, would have an orbit of 395 days, a radius of 97% of the Earth's, and surface temperature roughly similar to Earth's polar regions.

In 2017, KOI-7923.01 was considered a potential habitable planet.