Kepler-1682 is a Sun-like G-type star (about 0.99 solar masses, 5,619 K, 0.84 solar radii), 1,160 light-years from Earth. Kepler-1682 b is a planet with 2.9 Earth radii, with an orbital period of 14.8 days, discovered in 2020 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. At roughly 1,160 light-years, Kepler-1682 lies far beyond the nearest stars yet remains reachable to large survey telescopes.