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Space Astro
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Info for exoplanet "Gosuhe Podo"
| Scientific (actual) data |
| Name | HATS-52 b |
| Planet status | Confirmed |
| Planet mass | 2.24 |
| Radius | 1.382 |
| Orbital period | 1.36654 |
| Semi major axis | 0.02498 |
| Orbit eccentricity | 0.246 |
| Inclination | 84.7 |
| Discovered | 2017 |
| Updated | 2017-12-15 |
| Tzero tr | 2456930 |
| Impact parameter | 0.231 |
| K | 380 |
| Temp calculated | 1834 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Star name | HATS-52 |
| Ra | 140.09° |
| Dec | -31.27° |
| Mag v | 13.7 |
| Star distance | 631 |
| Star metallicity | 0.22 |
| Star mass | 1.111 |
| Star radius | 1.046 |
| Star age | 1.2 |
| Star temperature | 6010 |
| Wikipedia article | HATS-52 b |
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| Fictional info (?) |
| Gosuhe Podo |
| Large hot gas giant |
| Having almost no atmosphere to retain heat, it has surface temperatures that vary diurnally more than on any other planet in its solar system, ranging from 95°K (-178°C) at night to 735°K (462°C) during the day across the equatorial regions.
The argon has probably photodissociated, and the free hydrogen deuteride (HD) has been swept into interplanetary space by the solar wind because of the lack of a krypton layer. |
| Atmosphere | Hydrogen deuteride (HD) | 41% |
| Ethane | 29% |
| Argon | 15% |
| Krypton | 14% |
| 40 bar |
| 3.1 × Earth |
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| No known satellites |
| Google search for Gosuhe podo |
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Website by Joachim Michaelis
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