Kepler-365 is a star with 1.02 times the mass of the Sun, and 1.05 times its radius. It is located 2713.60 light years away from the solar system and is estimated to be 4 billion years old, as compared to the Sun which is roughly 4.6 billion years old.
Kepler-365 is known to have 2 exoplanets in orbit around it.
Kepler-365 b was discovered by the Kepler observatory, in 2014-03, using the transit method. Its semi-major axis is 0.10 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of Kepler-365 b is 4.834 times the mass of Earth. The radius of Kepler-365 b is 2.040 that of Earth. With a mass below 5 Earth masses, a density of 3.12, and a semi-major axis of 0.098 astronomical units, Kepler-365 b could, potentially, be an ocean world - a planet with no dry land.
Kepler-365 c was discovered by the Kepler observatory, in 2014-03, using the transit method. Its semi-major axis is 0.14 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of Kepler-365 c is 3.339 times the mass of Earth. The radius of Kepler-365 c is 1.640 that of Earth. At 3.339 Earth masses, Kepler-365 c is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.