Kepler-695 is an orange K-type dwarf (about 0.84 solar masses, 5,181 K, 0.80 solar radii), 843 light-years from Earth. Kepler-695 b is a planet with 9.2 Earth radii, with an orbital period of 3.0 days, discovered in 2016 via transit. The planet was found when it crossed the face of its star, producing periodic dips in brightness that reveal its size and orbital period to space-based photometry. The planet's large radius (9.2 Earth radii) indicates a bloated atmosphere heated by intense stellar radiation. At roughly 843 light-years, Kepler-695 lies far beyond the nearest stars yet remains reachable to large survey telescopes.