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Space Astro
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Info for exoplanet "Saaedei'tha"
Scientific (actual) data |
Planet | HD 202772 A b |
Planet status | Confirmed |
Planet mass | 1.008 |
Radius | 1.562 |
Orbital period | 3.30896 |
Semi major axis | 0.0519 |
Orbit eccentricity | 0.047 |
Inclination | 84.2 |
Discovered | 2018 |
Updated | 2018-10-05 |
Omega | 88 |
Tconj | 2458330 |
Tzero tr | 2458330 |
Impact parameter | 0.416 |
K | 96.9 |
Temperature (kelvin) | 2132 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | HD 202772 A |
Right ascension | 319.7° |
Declination | -26.62° |
Mag v | 8.32 |
Star distance | 147.2 |
Star metallicity | 0.29 |
Star mass | 1.703 |
Star radius | 2.614 |
Star age | 1.8 |
Star temperature | 6230 |
Star alternate names | TIC 290131778 |
Wikipedia article | HD 202772 A b |
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Fictional info (?) |
Suggested name | Saaedei'tha |
Planet type | Hot gas giant |
It is the second-brightest natural object in the night sky after Cali, reaching an apparent magnitude of -5 - bright enough to cast shadows at night and, rarely, visible to the naked eye in broad daylight.
It is named after the deity Saaedei'tha, the creator 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 202772 A, which reoccurs over the so-called synodic period approximately every 191 days.
Saaedei'tha is the site of Titanic Gravis, the largest volcano and second-highest known mountain in its solar system, and of Valles Marineris, one of the largest canyons in its solar system. |
Atmosphere | Neon | 64% |
Nitric oxide | 16% |
Helium | 15% |
Ammonia | 5% |
Atmospheric pressure | 1.8 bar |
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No known satellites |
Google search for Saaedei'tha |
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Website by Joachim Michaelis
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