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Space Astro
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Info for exoplanet "Tayonedelia Des"
Scientific (actual) data |
Planet | HD 119445 b |
Planet status | Confirmed |
Mass sini | 37.6 |
Orbital period | 410.2 |
Semi major axis | 1.71 |
Orbit eccentricity | 0.082 |
Discovered | 2009 |
Updated | 2016-08-21 |
K | 413.5 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Radial Velocity |
Star name | HD 119445 |
Right ascension | 205.62° |
Declination | 41.67° |
Mag v | 6.304 |
Star metallicity | 0.04 |
Star mass | 3.9 |
Star radius | 20.5 |
Star sp type | G6 |
Star temperature | 5083 |
Wikipedia article | HD 119445 b |
Back
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Fictional info (?) |
Suggested name | Tayonedelia Des |
Planet type | Cold planet |
This planet is named after the deity Tayonedelia Des, the messenger of the sky.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to HD 119445, which reoccurs over the so-called synodic period approximately every 116 days.
It is radically different from Earth in other respects. Tayonedelia Des is by far the hottest planet in its solar system, with a mean surface temperature of 718°K (445°C).
Tayonedelia Des is the site of Olympus Mons, 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.
The two polar ice caps appear to be made largely of sand. In November 2500, NASA reported finding a large amount of underground ice in the Utopia Planitia region of Tayonedelia Des. |
Atmosphere | Sulfur dioxide | 94% |
Water vapor | 5.4% |
Hydrogen deuteride (HD) | 0.024% |
Atmospheric pressure | 1.4 bar |
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No known satellites |
Google search for Tayonedelia des |
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Website by Joachim Michaelis
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