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Space Astro
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Info for exoplanet "Wengj-wo"
Scientific (actual) data |
Planet | Kepler-1519 b |
Planet status | Confirmed |
Radius | 0.63 |
Orbital period | 240.799 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2455170 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19464029+4927426 b, K03762.01, KIC 11518142 b, KOI-3762 b, KOI-3762.01, WISE J194640.29+492742.6 b |
Star name | Kepler-1519 |
Right ascension | 296.67° |
Declination | 49.46° |
Mag j | 13.642 |
Mag h | 13.257 |
Mag k | 13.189 |
Star distance | 858 |
Star metallicity | -0.07 |
Star mass | 0.94 |
Star radius | 0.91 |
Star age | 3.98 |
Star temperature | 5644 |
Star alternate names | 2MASS J19464029+4927426, KIC 11518142, KOI-3762, WISE J194640.29+492742.6 |
Wikipedia article | Kepler-1519 b |
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Fictional info (?) |
Suggested name | Wengj-wo |
Planet type | Cold planet |
The interior of Wengj-wo is mainly composed of ices and rock. This planet is named after the deity Wengj-wo, the god of dreams.
At this time it may appear as a bright star-like object, but is often far more difficult to observe than Atyung.
Wengj-wo is the site of Ars Ridge, the tallest volcano and second-highest known mountain in its solar system, and of Valles Marineris, one of the largest canyons in its solar system.
In November 3300, NASA reported finding a large amount of underground ice in the Utopia Planitia region of Wengj-wo.
Wengj-wo can easily be seen from Atyung with the naked eye, as can its grayish coloring.
Because of its rapid rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). |
Atmosphere | Hydrogen chloride | 54% |
Molecular hydrogen | 44% |
Formaldehyde | 0.59% |
Ammonium hydrosulfide (NH4SH) | 0.00013% |
Atmospheric pressure | 21 bar |
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No known satellites |
Google search for Wengj-wo |
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Website by Joachim Michaelis
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