HD 219134 g
HD 219134 g, also known as HR 8832 g, is an unconfirmed exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. It has a minimum mass of 11 Earth Masses, suggesting that it could be a high-mass ocean planet or a Neptune-like ice giant. Unlike HD 219134 b and HD 219134 c it was not observed by the Spitzer Space Telescope and thus its radius and density are unknown. It resides closer to the star than the inner edge of the system's (empirical) habitable zone, defined by the recent  Venus limit. If it has an Earth-like composition, it would have a radius 1.9 times that of Earth. However, since it is probably an ocean planet or Mini-Neptune, it is likely larger. Characteristics. Mass, Radius, and Temperature. HD 219134 g is a sub-Neptune-mass exoplanet with a minimum mass of 10.81 and an unknown radius, as it is not known to transit. However, due to the high metal content of the host star, the planet might not be an ice giant. For a rock-iron composition, HD 219134 g would be about 1.9 , which seems unlikely for  a planet of this mass. A more plausible rock-water composition would put the planet at about 2.4 . In the absence of an atmosphere, and assuming an albedo of 0.3, it has an equilibrium temperature of , but with an atmosphere it is likely to have a surface temperature much higher, that is if it has a rocky surface. So, it is rather unlikely to be habitable. Orbit. HD 219134 g takes about 94.2 days to orbits its star at a distance of 0.3753 AU. This is comparable to Mercury's orbit of 88 days at about 0.38 AU. However, due  to the lower luminosity of the host star, HD 219134 g is closer to Venus' situation. The eccentricity of the planet's orbit is believed to be close to zero, indicating a very circular orbit. Host Star. The planet HD 219134 g orbits the K3V orange dwarf HD 219134, also known as HR 8832. It is 79% the radius and 80% the mass of the Sun with 26% the luminosity. It has a temperature of 4699 K and is around 11 billion years old. For comparison, the Sun has a temperature of 5778 K and is 4.55 billion years old . The apparent magnitude of the star, or how bright it appears from Earth, is around 5. Therefore, it is just visible to the unaided eye to most observers.