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Space Astro
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Info for exoplanet "Nebya'kuya"
Scientific (actual) data |
Planet | HD 133131 A b |
Planet status | Confirmed |
Mass sini | 1.43 |
Orbital period | 649 |
Semi major axis | 1.44 |
Orbit eccentricity | 0.32 |
Discovered | 2016 |
Updated | 2016-08-24 |
K | 36.68 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Star name | HD 133131 A |
Right ascension | 225.9° |
Declination | -27.84° |
Mag v | 8.4 |
Star distance | 47 |
Star metallicity | -0.306 |
Star mass | 0.95 |
Star sp type | G2V |
Star age | 9.7 |
Star temperature | 5799 |
Wikipedia article | HD 133131 A b |
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Fictional info (?) |
Suggested name | Nebya'kuya |
Planet type | Cold planet |
Nebya'kuya's atmosphere is similar to Ripyo's in its primary composition of xenon and hydrogen, but it contains more "ices" such as water, ammonia, and methane, along with traces of other hydrocarbons. It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 80°K (-193°C), and has a complex, layered cloud structure with hydrogen thought to make up the lowest clouds, and xenon the uppermost layer of clouds. This cold planet is named after the deity Nebya'kuya, the messenger of dreams.
The volume of water ice in the south polar ice cap, if melted, would be sufficient to cover the entire planetary surface to a depth of 16 meters.
In late February 2300, Nebya'kuya was visited by the New Horizons probe, which used Nebya'kuya's gravity to increase its speed and bend its trajectory en route to Ripyo. |
Atmosphere | Xenon | 99% |
Hydrogen | 0.36% |
Carbon dioxide | 0.07% |
Ammonium hydrosulfide (NH4SH) | 0.00073% |
Atmospheric pressure | 0.001 bar |
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Moon | Chumyu | Small slightly egg-shaped gaseous moon |
Sanezaso Sope | Small potato shaped rocky moon |
Gebipo Hyusa Jo | Medium-sized potato shaped gaseous asteroid |
Kizara-ruge | Medium-sized irregular rocky comet |
Zeryu Chacha-gyo | Large irregular rocky asteroid |
Nshuda | Large round oceanic comet |
Google search for Nebya'kuya |
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Website by Joachim Michaelis
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