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Space Astro
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Info for exoplanet "Yoinya Ryo"
Scientific (actual) data |
Planet | Kepler-296 d |
Planet status | Confirmed |
Radius | 0.186 |
Orbital period | 19.8503 |
Semi major axis | 0.118 |
Orbit eccentricity | 0.33 |
Discovered | 2014 |
Updated | 2021-02-05 |
Tconj | 2454970 |
Impact parameter | 0.26 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | Kepler-296 d, 2MASS J19060960+4926143 d, K01422.02, KIC 11497958 d, KOI-1422 d, KOI-1422.02, Kepler-296 A d, WISE J190609.59+492614.2 d |
Star name | Kepler-296 |
Right ascension | 286.54° |
Declination | 49.44° |
Mag j | 13.391 |
Mag h | 12.807 |
Mag k | 12.6 |
Star distance | 226 |
Star metallicity | -0.08 |
Star mass | 0.5 |
Star radius | 0.48 |
Star sp type | M2 V |
Star temperature | 3740 |
Star alternate names | Kepler-296, 2MASS J19060960+4926143, KIC 11497958, KOI-1422, Kepler-296 A, WISE J190609.59+492614.2 |
Wikipedia article | Kepler-296 d |
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Fictional info (?) |
Suggested name | Yoinya Ryo |
Planet type | Planet |
Orbiting within Nokya's orbit, Yoinya Ryo is an inferior planet and never appears to venture far from Kepler-296; its maximum angular distance from Kepler-296 (elongation) is 26 degrees.
The planet is named after the deity Yoinya Ryo, the god of the sky.
Yoinya Ryo is the site of Titanic Gravis, the biggest volcano and second-highest known mountain in its solar system, and of Valles Marineris, one of the largest canyons in its solar system. |
Atmosphere | 2H2O | 87% |
Nitric oxide | 13% |
Ammonia | 0.18% |
Atmospheric pressure | 0.4 bar |
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No known satellites |
Google search for Yoinya ryo |
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Website by Joachim Michaelis
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