Kepler-182 is a star in the constellation of Cygnus. The star is notable for having two planets in the circumstellar habitable zone.
With a mass the same as the Sun's and an age of five billion years, Kepler-182 has exhausted its core hydrogen and expanded away from the main sequence. It is now a subgiant contracting towards the red giant branch. It has a radius of and an effective temperature of , giving a bolometric luminosity of .
Two exoplanets orbit it. The first, Kepler-182b, has a radius of and orbits the parent star every 9.8 days. The second, Kepler-182c, has a radius of and orbits the parent star every 20.7 days.
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