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Space Astro
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Info for exoplanet "Jugyuna Shu"
Scientific (actual) data |
Planet | Kepler-892 b |
Planet status | Confirmed |
Radius | 0.251 |
Orbital period | 13.7521 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454980 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J18523111+4353176 b, K01569.01, KIC 8009350 b, KOI-1569 b, KOI-1569.01 |
Star name | Kepler-892 |
Right ascension | 283.13° |
Declination | 43.89° |
Mag j | 13.968 |
Mag h | 13.378 |
Mag k | 13.335 |
Star distance | 640 |
Star metallicity | -0.04 |
Star mass | 0.75 |
Star radius | 0.72 |
Star age | 5.01 |
Star temperature | 4747 |
Star alternate names | 2MASS J18523111+4353176, KIC 8009350, KOI-1569 |
Wikipedia article | Kepler-892 b |
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Fictional info (?) |
Suggested name | Jugyuna Shu |
Planet type | Cold planet |
Orbiting within Rimi Repu's orbit, Jugyuna Shu is an inferior planet and never appears to venture far from Kepler-892; its maximum angular distance from Kepler-892 (elongation) is 36 degrees.
When viewed from Rimi Repu, Jugyuna Shu can reach an apparent magnitude of -3, bright enough for its reflected light to cast shadows, and making it on average the third-brightest object in the night sky. This cold planet is named after the deity Jugyuna Shu, the goddess of war.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Kepler-892, which reoccurs over the so-called synodic period approximately every 99 days.
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 | Neon | 73% |
Hydrogen chloride | 11% |
Hydrogen peroxide | 5.3% |
Ozone | 4.8% |
Methane | 3.1% |
Ammonia | 1.8% |
Krypton | 1.0E-6% |
Atmospheric pressure | 90 bar |
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No known satellites |
Google search for Jugyuna shu |
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Website by Joachim Michaelis
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