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Space Astro
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Info for exoplanet "Bapyonyo Bi"
Scientific (actual) data |
Planet | Kepler-218 c |
Planet status | Confirmed |
Radius | 0.28 |
Orbital period | 44.6996 |
Semi major axis | 0.248 |
Discovered | 2014 |
Updated | 2021-02-05 |
Tconj | 2455010 |
Impact parameter | 0.52 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19413907+4615592 c, K00711.01, KIC 9597345 c, KOI-711 c, KOI-711.01, WISE J194139.08+461559.6 c |
Star name | Kepler-218 |
Right ascension | 295.41° |
Declination | 46.27° |
Mag j | 12.732 |
Mag h | 12.386 |
Mag k | 12.311 |
Star distance | 669.02 |
Star metallicity | 0.194 |
Star radius | 1.06 |
Star temperature | 5502 |
Star alternate names | 2MASS J19413907+4615592, KIC 9597345, KOI-711, WISE J194139.08+461559.6 |
Wikipedia article | Kepler-218 c |
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Fictional info (?) |
Suggested name | Bapyonyo Bi |
Planet type | Cold planet |
The planet is named after the deity Bapyonyo Bi, the messenger of fear.
An observer on Bapyonyo Bi would therefore see only one winter every four years.
Bapyonyo Bi's axis has the smallest tilt of any of its solar system's planets.
Two spacecraft have visited Bapyonyo Bi: Wayfinder 8 flew by 23 years ago; and Messenger, launched 15 years ago, orbited Bapyonyo Bi over 55 times in four years before exhausting its reactor and crashing into the planet's surface 5 years later.
Bapyonyo Bi's dense clouds render observation of its surface difficult in ultraviolet light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 32 years ago. |
Atmosphere | Xenon | 65% |
Nitric oxide | 34% |
Nitrogen | 0.23% |
Ozone | 0.15% |
Hydrogen deuteride (HD) | 0.012% |
Oxygen | 0.0096% |
Atmospheric pressure | 0.002 bar |
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Moon | Nshoda Ikyu | Small almost round ice asteroid |
Jasegu Kyore Mo | Large almost round ice moon |
Homyakyu Rupase | Large potato shaped rocky moon |
Nunasa-yope | Huge almost round rocky moon |
Ipyomona-bya | Large almost round crater-filled moon |
Google search for Bapyonyo bi |
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Website by Joachim Michaelis
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