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Space Astro
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Info for exoplanet "Evitu Ho"
Scientific (actual) data |
Planet | Kepler-430 b |
Planet status | Confirmed |
Radius | 0.29 |
Orbital period | 35.968 |
Semi major axis | 0.2244 |
Discovered | 2015 |
Updated | 2016-05-06 |
Temperature (kelvin) | 667 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Radius detection type | Primary Transit |
Alternate names | KOI-2365 b, 2MASS J19311407+4934460 b, K02365.01, KIC 11560897 b, KOI-2365.01, WISE J193114.06+493446.0 b |
Star name | Kepler-430 |
Right ascension | 292.81° |
Declination | 49.58° |
Mag j | 12.743 |
Mag h | 12.486 |
Star distance | 942.26 |
Star metallicity | 0.2 |
Star mass | 1.17 |
Star radius | 1.49 |
Star temperature | 5884 |
Star alternate names | KOI-2365, 2MASS J19311407+4934460, KIC 11560897, WISE J193114.06+493446.0 |
Wikipedia article | Kepler-430 b |
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Fictional info (?) |
Suggested name | Evitu Ho |
Planet type | Cold planet |
Evitu Ho and Eravi are cold planets rich in gas. It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 83°K (-190°C), and has a complex, layered cloud structure with methane thought to make up the lowest clouds, and hydrogen peroxide the uppermost layer of clouds. It is named after the deity Evitu Ho, the spirit of the underworld.
Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Evitu Ho's distance from Kepler-430 is only about two-thirds (or 33 pct) of its distance at aphelion.
Evitu Ho was one of the first planets to have its motions plotted across the sky - as early as the second millennium BC. |
Atmosphere | Hydrogen peroxide | 64% |
Methane | 30% |
Nitrogen | 3.7% |
Carbonyl sulfide | 1.3% |
Formaldehyde | 0.35% |
Oxygen | 0.0024% |
Nitric oxide | 6.2E-5% |
Carbon dioxide | 6.2E-5% |
Atmospheric pressure | 0.7 bar |
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No known satellites |
Google search for Evitu ho |
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Website by Joachim Michaelis
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