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Space Astro
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Info for exoplanet "Osuf Ij"
| Scientific (actual) data |
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| Name | Kepler-1894 Ab |
| Planet status | Confirmed |
| Radius | 0.107 |
| Orbital period | 2.76266 |
| Semi major axis | 0.0385 |
| Orbit eccentricity | 0 |
| Inclination | 87.48 |
| Discovered | 2017 |
| Updated | 2024-06-27 |
| Tzero tr | 2454970 |
| Impact parameter | 0.46 |
| Temperature (kelvin) | 1231 |
| Publication | Announced on a website |
| Detection type | Primary Transit |
| Alternate names | KOI-3022 b, KOI-3022.01 |
| Star name | Kepler-1894 A |
| Right ascension | 295.59° |
| Declination | 49.67° |
| Mag v | 15.452 |
| Mag i | 15.167 |
| Mag j | 14.078 |
| Mag h | 13.761 |
| Mag k | 13.648 |
| Star distance | 935.191 |
| Star metallicity | 0 |
| Star mass | 0.96 |
| Star radius | 0.817 |
| Star sp type | G5V |
| Star age | 0.5 |
| Star temperature | 5467 |
| Star alternate names | KIC 11618601, KOI-3022 |
| Wikipedia article | Kepler-1894 Ab |
Back
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| Fictional info (?) |
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| Suggested name | Osuf Ij |
| Planet type | Hot planet |
| As seen relative to the fixed stars, it rotates on its axis exactly three times for every five revolutions it makes around Kepler-1894 A.
The nitric oxide has probably photodissociated, and the free argon has been swept into interplanetary space by the solar wind because of the lack of a carbon dioxide layer.
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 | Argon | 48% |
| Carbon monoxide | 44% |
| Nitric oxide | 7.4% |
| Carbon dioxide | 0.11% |
| Xenon | 0.0011% |
| Atmospheric pressure | 31 bar |
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| No known satellites |
| Google search for Osuf ij |
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Website by Joachim Michaelis
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