Kepler 232

Kepler-232 B is a Neptune-like Exoplanet that orbits a G-type star. Its mass is 9.69 Earths, it takes 4.4 days to complete one orbit of its star, and is 0.05

Kepler-232 c has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-232 c are still unknown, the object is highly unlikely to be a

Kepler-232 b is a Confirmed extrasolar planet exoplanet that orbits the star Kepler 232 in the constellation of Cygnus

Kepler-232 c Planet Status Confirmed. Discovered in 2014. Publication Status Announced on a website. Update 2021-02-05. Mass Masssini Semi-Major Axis

Kepler-232 b is a Neptune-like exoplanet that orbits a G-type star. Its mass is 9.69 Earths, it takes 4.4 days to complete one orbit of its star, and is 0.054 AU from its star. Its discovery was announced in 2014.

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Fictional info Suggested name Pobyupya Byu Planet type Warm planet It is named after the deity Pobyupya Byu, the god of the sky. When viewed from Gepia, this proximity to Kepler-232 means the planet can only be seen near the western or eastern horizon during the early evening or early morning.

This is the Kepler-232 . The star Kepler-232 islocated about 4575.8 light-years 1403.0 pc away from our Solar System. The star Kepler-232 has apparent magnitude of 14.2, with absolute magnitude of 3.4. Number of Extrasolar Planets 2 Name of the 1 Planet Kepler-232 b radius 0.275000 mass 0.023640 orbital distance 0.054000

The Orbital Period, or to say it another way, Kepler-232 c's year is 11.379349 days or 0.03 Earth Years. By the time, the Earth has completed a full year, the planet will have completed 32.08 orbits of its star . The Semi-Major Axis is the furthest point from its star in its orbit.

Quantised Inertia