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HD 219134 h, also known as HR 8832 h, is an exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. It has a minimum mass of 108 Earth masses, which indicates that the planet is likely a gas giant. Unlike HD 219134 b and c it is not observed to transit and thus its radius and density are unknown.
HD 219134 (also known as Gliese 892 or HR 8832) is a main-sequence star in the constellation of Cassiopeia. It is smaller and less luminous than the Sun, with a spectral class of K3V, which makes it an orange-hued star. HD 219134 is relatively close to our system, with an estimated distance of 21.34 light years.
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HD 219134 c, also known as HR 8832 c, is a hot, dense, rocky exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia.Originally thought to be a little less than three times the mass of Earth, it is now known to be over 4.2 times the mass and 45% larger in radius, suggesting a rocky composition with a higher quantity of iron than Earth.
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HD 219134 b (or HR 8832 b) is one of at least five exoplanets orbiting HD 219134, a main-sequence star in the constellation of Cassiopeia. [ 3 ] [ 1 ] [ 4 ] [ 5 ] HD 219134 b has a size of about 1.5 R 🜨 , [ 2 ] and a density of 6.4 g/cm 3 and orbits at 21.25 light-years away. [ 3 ]