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Space Astro
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Info for exoplanet "Misepiauto Ron"
Scientific (actual) data |
Planet | Kepler-935 b |
Planet status | Confirmed |
Radius | 0.12 |
Orbital period | 4.88084 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454970 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19400520+4637091 b, K01716.01, KIC 9838949 b, KOI-1716 b, KOI-1716.01, WISE J194005.20+463709.1 b |
Star name | Kepler-935 |
Right ascension | 295.02° |
Declination | 46.62° |
Mag j | 13.292 |
Mag h | 12.774 |
Mag k | 12.62 |
Star distance | 482 |
Star metallicity | -0.01 |
Star mass | 0.78 |
Star radius | 0.73 |
Star age | 3.8 |
Star temperature | 4830 |
Star alternate names | 2MASS J19400520+4637091, KIC 9838949, KOI-1716, WISE J194005.20+463709.1 |
Wikipedia article | Kepler-935 b |
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Fictional info (?) |
Suggested name | Misepiauto Ron |
Planet type | Cold planet |
It is named after the deity Misepiauto Ron, the goddess of destruction.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Kepler-935, which reoccurs over the so-called synodic period approximately every 174 days.
Misepiauto Ron's axis has the smallest tilt of any of its solar system's planets.
The Misepiauto Ron system has a unique configuration among those of the planets because its axis of rotation is tilted sideways, nearly into the plane of its solar orbit. In 1887, images from Frontier 8 showed Misepiauto Ron as an almost featureless planet in visible light, without the cloud bands or storms associated with the other cold planets. |
Atmosphere | Ammonium hydrosulfide (NH4SH) | 74% |
Molecular hydrogen | 26% |
Carbonyl sulfide | 0.029% |
Atmospheric pressure | 70 bar |
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No known satellites |
Google search for Misepiauto ron |
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Website by Joachim Michaelis
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