Author(s): Gurren Lagann
Kepler-64, also known as KOI-6464 and PH1, is a quadruple star system consisting of an F-type main sequence star, a Sun-like star and two red dwarf stars about 7,163 light-years away in the constellation Cygnus. A gas giant planet about 2/3 the size of Saturn orbits two stars (components Aa and Ab) in the system. It is the first exoplanet discovered by the Planet Hunters project in 2012, and is the first known transiting exoplanet in a quadruple star system
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