Kepler-62e

Kepler-62 e is an extra solar planet orbiting the star Kepler-62. It is on the inner edge of its host star's habitable zone, so is likely to be enshrouded in a cloudy viel, and have a dense atmosphere (like Venus, though less hot). To be terraformed some of the atmosphere would need to be removed. It may or may not have large amounts of water on its surface (could be an ocean planet if the latter is true). It has a radius of approximately 1.61 Earth's and recieves 1.2 times the amount of solar flux.