Kepler-1649 is a type-M red dwarf star estimated to be roughly ¼ the radius of the Sun with only two confirmed planets in its orbit, the other being
Kepler-1649c. Kepler-1649c is similar to
Earth from our own solar system in two ways: both
Kepler-1649c and Earth have orbits roughly twice the radius of the previous known planets (Kepler-1649b and Venus respectively), and they are of similar size.
Orbit Kepler-1649b takes only 8.6 Earth days to orbit
Kepler-1649. == References ==