Kepler-384 is a Sun-like G-type star (about 0.88 solar masses, 5,577 K, 0.88 solar radii), 896 light-years from Earth. Kepler-384 b is a planet with 1.1 Earth radii, with an orbital period of 22.6 days, at 0.148 AU from its star, discovered in 2014 via transit. Kepler-384 c is a planet with 1.1 Earth radii, with an orbital period of 45.3 days, at 0.236 AU from its star, discovered in 2014 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.