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Space Astro
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Info for exoplanet "Pyanc Yao"
Scientific (actual) data |
Planet | Kepler-1696 b |
Planet status | Confirmed |
Radius | 0.251 |
Orbital period | 65.9409 |
Semi major axis | 0.3245 |
Inclination | 89.95 |
Discovered | 2020 |
Updated | 2021-02-05 |
Tzero tr | 2455060 |
Impact parameter | 0.0108 |
Temperature (kelvin) | 454 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19421825+4201241 b, K03361.01, KIC 6619815 b, KOI-3361 b, KOI-3361.01 |
Star name | Kepler-1696 |
Right ascension | 295.58° |
Declination | 42.02° |
Mag i | 15.284 |
Mag j | 14.245 |
Mag h | 13.913 |
Mag k | 13.969 |
Star distance | 1571.34 |
Star metallicity | -0.04 |
Star mass | 1.047 |
Star radius | 1.27 |
Star temperature | 5379 |
Star alternate names | 6619815, 2MASS J19421825+4201241, KIC 6619815, KOI-3361 |
Wikipedia article | Kepler-1696 b |
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Fictional info (?) |
Suggested name | Pyanc Yao |
Planet type | Cold planet |
The planet is named after the deity Pyanc Yao, the messenger of chaos.
At this time it may appear as a bright star-like object, but is often far more difficult to observe than Kyuzher Zhyi.
Pyanc Yao's thick clouds render observation of its surface challenging in infrared light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 52 years ago. Plans have been proposed for rovers or more complex missions, but they are hindered by Pyanc Yao's strong magnetosphere.
A prominent result is the "great white spot", a giant storm that is known to have existed for centuries since it was first detected by scanner. |
Atmosphere | Carbonyl sulfide | 81% |
Nitrogen | 18% |
Hydrogen chloride | 0.83% |
Helium | 0.00016% |
Krypton | 7.3E-5% |
Atmospheric pressure | 2.4 bar |
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No known satellites |
Google search for Pyanc yao |
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Website by Joachim Michaelis
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