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Space Astro
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Info for exoplanet "Bekyufu Rya"
| Scientific (actual) data |
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| Name | SRGeJ0411 b |
| Planet status | Confirmed |
| Planet mass | 40 |
| Radius | 1.1 |
| Orbital period | 0.0270915 |
| Inclination | 83 |
| Discovered | 2024 |
| Updated | 2024-03-24 |
| Temp measured | 2200 |
| Publication | Published in a refereed paper |
| Detection type | Timing |
| Mass measurement type | Timing |
| Star name | SRGeJ0411 |
| Right ascension | 62.88° |
| Declination | 68.9° |
| Star distance | 324 |
| Star mass | 0.84 |
| Star radius | 0.01 |
| Star sp type | WD |
| Star temperature | 13790 |
| Wikipedia article | SRGeJ0411 b |
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| Fictional info (?) |
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| Suggested name | Bekyufu Rya |
| Planet type | Huge cold gas giant |
| It is a huge cold gas giant planet with a mass one-thousandth that of SRGeJ0411, but two-and-a-half times that of all the other planets in its solar system combined. The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to SRGeJ0411, which reoccurs over the so-called synodic period approximately every 139 days.
Its north and south poles, therefore, lie where most other planets have their equators. |
| Atmosphere | Ammonium hydrosulfide (NH4SH) | 99% |
| Atmospheric pressure | 2.3 bar |
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| No known satellites |
| Google search for Bekyufu rya |
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Website by Joachim Michaelis
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