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Space Astro
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Info for exoplanet "Oriwi Tun"
Scientific (actual) data |
Planet | HD 33844 b |
Planet status | Confirmed |
Mass sini | 1.96 |
Orbital period | 551.4 |
Semi major axis | 1.6 |
Orbit eccentricity | 0.15 |
Discovered | 2013 |
Updated | 2015-12-24 |
Omega | 211 |
K | 33.5 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Radial Velocity |
Star name | HD 33844 |
Right ascension | 78.15° |
Declination | -14.95° |
Star distance | 100.9 |
Star mass | 1.75 |
Star sp type | K0 III |
Star age | 2.1 |
Star temperature | 4827 |
Wikipedia article | HD 33844 b |
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Fictional info (?) |
Suggested name | Oriwi Tun |
Planet type | Cold planet |
This cold planet is named after the deity Oriwi Tun, the bringer of destruction.
Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Oriwi Tun's distance from HD 33844 is only about two-thirds (or 106 pct) of its distance at aphelion.
Oriwi Tun is a cold planet and is sometimes called Emet Etex-ih's "sister planet" because of their similar size, mass, proximity to HD 33844, and bulk composition.
Its apparent magnitude reaches -3, which is surpassed only by Emet Etex-ih, Imare Medon, and HD 33844.
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). |
Atmosphere | Oxygen | 54% |
Formaldehyde | 41% |
Ozone | 3.4% |
Ammonia | 0.82% |
Ammonium hydrosulfide (NH4SH) | 0.18% |
Krypton | 0.039% |
Carbon dioxide | 1.8E-5% |
Atmospheric pressure | 7 bar |
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No known satellites |
Google search for Oriwi tun |
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Website by Joachim Michaelis
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