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Space Astro
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Info for exoplanet "Amuvat"
| Scientific (actual) data |
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| Name | Kepler-1858 b |
| Planet status | Confirmed |
| Radius | 0.21599 |
| Orbital period | 88.0716 |
| Semi major axis | 0.3575 |
| Inclination | 89.79 |
| Discovered | 2017 |
| Updated | 2024-06-20 |
| Tzero tr | 2455050 |
| Impact parameter | 0.347 |
| Temp calculated | 325 |
| Publication | Announced on a website |
| Detection type | Primary Transit |
| Radius measurement type | Primary Transit |
| Alternate names | KOI-2553 b, KOI-2553.01 |
| Star name | Kepler-1858 |
| Ra | 292.31° |
| Dec | 46.63° |
| Mag v | 15.959 |
| Mag i | 15.338 |
| Mag j | 14.219 |
| Mag h | 13.742 |
| Mag k | 13.663 |
| Star distance | 833.055 |
| Star metallicity | 0.207 |
| Star mass | 0.84 |
| Star radius | 0.773 |
| Star sp type | K1V |
| Star age | 0.7 |
| Star temperature | 5058.9 |
| Star alternate names | KIC 9832208, KOI-2553 |
| Wikipedia article | Kepler-1858 b |
Back
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| Fictional info (?) |
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| Amuvat |
| Cold planet |
| It has the longest rotation period (445 days) of any planet in its solar system and rotates in the opposite direction to most other planets.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Kepler-1858, which reoccurs over the so-called synodic period approximately every 64 days.
As seen relative to the fixed stars, it rotates on its axis exactly three times for every five revolutions it makes around Kepler-1858. |
| Atmosphere | Xenon | 99% |
| 0.0016 bar |
| 0 × Earth |
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| Moon | Cequde-bedaro-r | Very small almost round ice moon |
| Fewil | Small irregular crater-filled moon |
| Faza Boce | Very small almost round rocky moon |
| Ehazes-omavode | Huge slightly egg-shaped rocky planetoid |
| Sivu Sidu'zubas | Very small slightly egg-shaped rocky planetoid |
| Elil-ozave | Medium-sized almost round oceanic comet |
| Unibal-er | Very small potato shaped gaseous asteroid |
| Google search for Amuvat |
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Website by Joachim Michaelis
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