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Space Astro
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Info for exoplanet "Ourosha'a"
Scientific (actual) data |
Planet | Kepler-1101 b |
Planet status | Confirmed |
Radius | 0.22 |
Orbital period | 81.3151 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2455010 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19381665+4540165 b, K02107.01, KIC 9225395 b, KOI-2107 b, KOI-2107.01, WISE J193816.64+454016.2 b |
Star name | Kepler-1101 |
Right ascension | 294.57° |
Declination | 45.67° |
Mag j | 13.793 |
Mag h | 13.422 |
Mag k | 13.314 |
Star distance | 897 |
Star metallicity | -0.04 |
Star mass | 0.94 |
Star radius | 0.91 |
Star age | 4.27 |
Star temperature | 5614 |
Star alternate names | 2MASS J19381665+4540165, KIC 9225395, KOI-2107, WISE J193816.64+454016.2 |
Wikipedia article | Kepler-1101 b |
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Fictional info (?) |
Suggested name | Ourosha'a |
Planet type | Cold planet |
Ourosha'a is the strangest and most crater filled planet in its solar system.
This cold planet is named after the deity Ourosha'a, the messenger of the sea.
The rotational period and seasonal cycles of Ourosha'a are likewise similar to those of Earth, as is the tilt that produces the seasons. Ourosha'a is the site of Celestium Gravis, the most active volcano and second-highest known mountain in its solar system, and of Valles Marineris, one of the largest canyons in its solar system.
Ourosha'a is primarily composed of ammonium hydrosulfide (NH4SH) with a significant part of its mass being hydrogen deuteride (HD), though hydrogen deuteride (HD) comprises only about a limited fraction of the number of molecules. Because of its fast rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). |
Atmosphere | Ammonium hydrosulfide (NH4SH) | 73% |
Hydrogen deuteride (HD) | 15% |
Argon | 9.6% |
Ozone | 2% |
Carbon monoxide | 0.21% |
Atmospheric pressure | 100 bar |
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No known satellites |
Google search for Ourosha'a |
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Website by Joachim Michaelis
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