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Space Astro
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Info for exoplanet "Sekuru Gobyu"
| Scientific (actual) data |
| Name | TOI-544 b |
| Planet status | Confirmed |
| Planet mass | 0.00909 |
| Radius | 0.1802 |
| Orbital period | 1.54835 |
| Semi major axis | 0.0225 |
| Discovered | 2022 |
| Updated | 2023-10-25 |
| Tperi | 2459200 |
| Tzero tr | 2459200 |
| Impact parameter | 0.66 |
| K | 2.17 |
| Temp calculated | 999 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Alternate names | HD 290498 b |
| Star name | TOI-544 |
| Ra | 82.29° |
| Dec | -0.34° |
| Mag v | 11 |
| Star distance | 41.1 |
| Star mass | 0.85 |
| Star radius | 0.66 |
| Star temperature | 4369 |
| Star alternate names | HD 290498 |
| Wikipedia article | TOI-544 b |
Back
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| Fictional info (?) |
| Sekuru Gobyu |
| Hot planet |
| As seen from TOI-544, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
The hydrogen peroxide has probably photodissociated, and the free argon has been swept into interplanetary space by the solar wind because of the lack of a carbon monoxide layer. |
| Atmosphere | Argon | 60% |
| Ammonium hydrosulfide (NH4SH) | 24% |
| Hydrogen peroxide | 15% |
| Carbon monoxide | 0.42% |
| Hydrogen | 0.00031% |
| Nitric oxide | 3.3E-5% |
| 27 bar |
| 0.7 × Earth |
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| No known satellites |
| Google search for Sekuru gobyu |
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Website by Joachim Michaelis
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