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Space Astro
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Info for exoplanet "Iojul Tus"
Scientific (actual) data |
Planet | HD 113538 c |
Planet status | Confirmed |
Mass sini | 0.93 |
Orbital period | 1818 |
Semi major axis | 2.44 |
Orbit eccentricity | 0.2 |
Angular distance | 0.153797 |
Discovered | 2010 |
Updated | 2015-01-08 |
Omega | 280 |
Tperi | 2456740 |
K | 22.6 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Radial Velocity |
Star name | HD 113538 |
Right ascension | 196.24° |
Declination | -52.44° |
Mag v | 9.06 |
Star distance | 15.8 |
Star metallicity | -0.24 |
Star mass | 0.585 |
Star radius | 0.53 |
Star sp type | K9V |
Star age | 4.3 |
Star temperature | 4462 |
Wikipedia article | HD 113538 c |
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Fictional info (?) |
Suggested name | Iojul Tus |
Planet type | Cold planet |
Iojul Tus's atmosphere is similar to Nereke'kivitania's in its primary composition of carbonyl sulfide and xenon, but it contains more "ices" such as water, ammonia, and methane, along with traces of other hydrocarbons. This planet is named after the deity Iojul Tus, the goddess of hate.
Iojul Tus's surface appears very cratered and is similar in appearance to the Moon's, indicating that it has been geologically inactive for billions of years.
Iojul Tus is the site of Robusto Mountain, 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.
Because of its fast rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator).
Its north and south poles, therefore, lie where most other planets have their equators. |
Atmosphere | Carbonyl sulfide | 63% |
Xenon | 34% |
Sulfur dioxide | 2.7% |
Hydrogen | 1.9E-5% |
Carbon monoxide | 0% |
Atmospheric pressure | 60 bar |
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Moon | Dysno | Large irregular ice planetoid |
Hionn'theethe | Small round crater-filled planetoid |
Teproanan-cyl | Small irregular ice asteroid |
Google search for Iojul tus |
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Website by Joachim Michaelis
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