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Space Astro
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Info for exoplanet "Teja"
| Scientific (actual) data |
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| Planet | HD 34445 f |
| Planet status | Confirmed |
| Mass sini | 0.119 |
| Orbital period | 676.8 |
| Semi major axis | 1.543 |
| Orbit eccentricity | 0.031 |
| Discovered | 2017 |
| Updated | 2017-11-06 |
| Omega | 212 |
| K | 2.74 |
| Publication | Published in a refereed paper |
| Detection type | Radial Velocity |
| Mass detection type | Radial Velocity |
| Star name | HD 34445 |
| Right ascension | 79.42° |
| Declination | 7.35° |
| Mag v | 7.31 |
| Star distance | 46.5 |
| Star metallicity | 0.14 |
| Star mass | 1.07 |
| Star radius | 1.38 |
| Star sp type | G0V |
| Star age | 8.5 |
| Star temperature | 5836 |
| Wikipedia article | HD 34445 f |
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| Fictional info (?) |
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| Suggested name | Teja |
| Planet type | Cold planet |
| It is named after the deity Teja, the spirit of war.
An observer on Teja would therefore see only one sunset every four years.
The rotational period and seasonal cycles of Teja are likewise similar to those of Raxlas, as is the tilt that produces the seasons. Teja is the site of Celestium 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.
There are ongoing investigations assessing the present habitability potential of Teja, as well as the possibility of extant life.
In late February 2800, Teja was visited by the New Horizons probe, which used Teja's gravity to increase its speed and bend its trajectory en route to Raxlas. |
| Atmosphere | Helium | 37% |
| Sulfur dioxide | 29% |
| Formaldehyde | 23% |
| Ethane | 5.9% |
| Methane | 2.5% |
| Hydrogen peroxide | 1.1% |
| Xenon | 0.82% |
| Atmospheric pressure | 0.0016 bar |
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| No known satellites |
| Google search for Teja |
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Website by Joachim Michaelis
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