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Space Astro
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Info for exoplanet "Bobawa"
| Scientific (actual) data |
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| Name | Kepler-1801 b |
| Planet status | Confirmed |
| Radius | 0.241701 |
| Orbital period | 10.4409 |
| Semi major axis | 0.0915 |
| Orbit eccentricity | 0 |
| Inclination | 84.89 |
| Discovered | 2017 |
| Updated | 2024-06-12 |
| Tzero tr | 2454970 |
| Impact parameter | 0.914 |
| Temperature (kelvin) | 829 |
| Publication | Announced on a website |
| Detection type | Primary Transit |
| Radius measurement type | Primary Transit |
| Alternate names | KOI-2172 b, KOI-2172.01 |
| Star name | Kepler-1801 |
| Right ascension | 295.16° |
| Declination | 39.2° |
| Mag v | 15.28 |
| Mag i | 14.856 |
| Mag j | 13.828 |
| Mag h | 13.481 |
| Mag k | 13.405 |
| Star distance | 839.332 |
| Star metallicity | -0.06 |
| Star mass | 0.95 |
| Star radius | 0.866 |
| Star sp type | G5V |
| Star age | 8.1 |
| Star temperature | 5455 |
| Star alternate names | 4173026 |
| Wikipedia article | Kepler-1801 b |
Back
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| Fictional info (?) |
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| Suggested name | Bobawa |
| Planet type | Warm planet |
| 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-1801, which reoccurs over the so-called synodic period approximately every 203 days.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
| Atmosphere | Ozone | 56% |
| 2H2O | 27% |
| Carbon dioxide | 9.8% |
| Hydrogen | 4.8% |
| Nitric oxide | 1.3% |
| Krypton | 0.26% |
| Water vapor | 0.25% |
| Molecular hydrogen | 0.003% |
| Neon | 0.00036% |
| Atmospheric pressure | 0.001 bar |
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| No known satellites |
| Google search for Bobawa |
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Website by Joachim Michaelis
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