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Space Astro
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Info for exoplanet "Riro"
| Scientific (actual) data |
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| Planet | TOI-5205 b |
| Planet status | Confirmed |
| Planet mass | 1.08 |
| Radius | 1.035 |
| Orbital period | 1.63076 |
| Semi major axis | 0.0199 |
| Orbit eccentricity | 0.02 |
| Inclination | 88.21 |
| Discovered | 2022 |
| Updated | 2022-09-23 |
| Omega | 318 |
| Tzero tr | 2459440 |
| K | 346 |
| Temperature (kelvin) | 737 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass detection type | Radial Velocity |
| Radius detection type | Primary Transit |
| Star name | TOI-5205 |
| Right ascension | 313.77° |
| Declination | 24.36° |
| Mag v | 15 |
| Star distance | 86.865 |
| Star metallicity | 0 |
| Star mass | 0.392 |
| Star radius | 0.394 |
| Star sp type | M4.0 |
| Star temperature | 3439 |
| Wikipedia article | TOI-5205 b |
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| Fictional info (?) |
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| Suggested name | Riro |
| Planet type | Hot gas giant |
| For this reason, scientists often classify Riro and Maze as "hot gas giants" to distinguish them from the other planets. The planet is named after the deity Riro, the god of war.
Riro's axis has the smallest tilt of any of its solar system's planets.
The 2H2O has probably photodissociated, and the free krypton has been swept into interplanetary space by the solar wind because of the lack of a planetary magnetic field.
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 | Krypton | 54% |
| Neon | 34% |
| 2H2O | 12% |
| Ozone | 0.05% |
| Water vapor | 3.0E-6% |
| Atmospheric pressure | 0.18 bar |
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| No known satellites |
| Google search for Riro |
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Website by Joachim Michaelis
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