Kepler-175 is a Sun-like F-type star (about 0.97 solar masses, 6,064 K, 1.01 solar radii), 1,312 light-years from Earth. Kepler-175 b is a planet with 2.6 Earth radii, with an orbital period of 11.9 days, at 0.105 AU from its star, discovered in 2014 via transit. Kepler-175 c is a planet with 3.1 Earth radii, with an orbital period of 34.0 days, at 0.213 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.