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Space Astro
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Info for exoplanet "Sekuru Gobyu"
| Scientific (actual) data |
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| Name | TOI-544 b |
| Planet status | Confirmed |
| Planet mass | 0.00909 |
| Radius | 0.1802 |
| Orbital period | 1.54835 |
| Semi major axis | 0.0225 |
| Orbit eccentricity | 0 |
| Discovered | 2022 |
| Updated | 2023-10-25 |
| Tperi | 2459200 |
| Tzero tr | 2459200 |
| Impact parameter | 0.66 |
| K | 2.17 |
| Temperature (kelvin) | 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 |
| Right ascension | 82.29° |
| Declination | -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 (?) |
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| Suggested name | Sekuru Gobyu |
| Planet type | 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% |
| Atmospheric pressure | 27 bar |
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| No known satellites |
| Google search for Sekuru gobyu |
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Website by Joachim Michaelis
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