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Space Astro
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Info for exoplanet "Epukes"
Scientific (actual) data |
Planet | Kepler-386 b |
Planet status | Confirmed |
Radius | 0.124 |
Orbital period | 12.3104 |
Semi major axis | 0.096 |
Discovered | 2014 |
Updated | 2021-02-05 |
Tconj | 2454970 |
Impact parameter | 0.8 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19192612+4841378 b, K02442.02, KIC 11080405 b, KOI-2442 b, KOI-2442.02, WISE J191926.15+484137.8 b |
Star name | Kepler-386 |
Right ascension | 289.86° |
Declination | 48.69° |
Mag j | 14.183 |
Mag h | 13.754 |
Mag k | 13.605 |
Star distance | 904.74 |
Star metallicity | -0.225 |
Star mass | 0.74 |
Star radius | 0.77 |
Star temperature | 5178 |
Star alternate names | 2MASS J19192612+4841378, KIC 11080405, KOI-2442, WISE J191926.15+484137.8 |
Wikipedia article | Kepler-386 b |
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Fictional info (?) |
Suggested name | Epukes |
Planet type | Warm planet |
Epukes and Utir are warm planets rich in rock. For this reason, scientists often classify Epukes and Utir as "warm planets" to distinguish them from the other planets. This warm planet is named after the deity Epukes, the bringer of nature.
Epukes is gravitationally locked with Kepler-386 in a 4:3 spin-orbit resonance, and rotates in a way that is unique in its solar system.
Epukes can easily be seen from Utir with the naked eye, as can its greenish coloring. Optical ground-based telescopes are typically limited to resolving features about 210 kilometers across when Epukes is closest because of Utir's atmosphere. |
Atmosphere | Hydrogen peroxide | 64% |
Ethane | 35% |
2H2O | 0.28% |
Hydrogen deuteride (HD) | 0.14% |
Water vapor | 0.091% |
Ozone | 0.078% |
Hydrogen | 0.025% |
Atmospheric pressure | 50 bar |
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Moon | Obene Pegyba | Large slightly egg-shaped rocky asteroid |
Ewezeto | Very small slightly egg-shaped gaseous asteroid |
Azus Eteh'omir | Huge irregular crater-filled asteroid |
Lulupop-i | Very small potato shaped gaseous comet |
Google search for Epukes |
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Website by Joachim Michaelis
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