Kepler-625 is a star with 1.04 times the mass of the Sun, and 0.96 times its radius. It is located 2481.09 light years away from the solar system and is estimated to be 1.51 billion years old, as compared to the Sun which is roughly 4.6 billion years old.
Kepler-625 is known to have 2 exoplanets in orbit around it.
Kepler-625 b was discovered by the Kepler observatory, in 2016-05, using the transit method. Its semi-major axis is 0.08 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of Kepler-625 b is 4.611 times the mass of Earth. The radius of Kepler-625 b is 1.990 that of Earth. With a mass below 5 Earth masses, a density of 3.22, and a semi-major axis of 0.0768 astronomical units, Kepler-625 b could, potentially, be an ocean world - a planet with no dry land.
Kepler-625 c was discovered by the Kepler observatory, in 2016-05, using the transit method. Its semi-major axis is 0.05 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of Kepler-625 c is 1.158 times the mass of Earth. The radius of Kepler-625 c is 1.050 that of Earth. At less than 1.5 Earth masses, Kepler-625 c is a regular terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.