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Space Astro
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Info for exoplanet "Semohashu"
| Scientific (actual) data |
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| Name | HATS-68 b |
| Planet status | Confirmed |
| Planet mass | 1.29 |
| Radius | 1.2321 |
| Orbital period | 3.58622 |
| Semi major axis | 0.05071 |
| Orbit eccentricity | 0.036 |
| Inclination | 83.21 |
| Discovered | 2018 |
| Updated | 2021-07-06 |
| Tzero tr | 2457410 |
| Impact parameter | 0.736 |
| K | 139.3 |
| Temperature (kelvin) | 1741 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Star name | HATS-68 |
| Right ascension | 15° |
| Declination | -58.9° |
| Mag v | 12.16 |
| Star distance | 619 |
| Star metallicity | 0.163 |
| Star mass | 1.337 |
| Star radius | 1.769 |
| Star age | 3.14 |
| Star temperature | 6122 |
| Wikipedia article | HATS-68 b |
Back
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| Fictional info (?) |
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| Suggested name | Semohashu |
| Planet type | Hot gas giant |
| The volume of water ice in the south polar ice cap, if melted, would be sufficient to cover the entire planetary surface to a depth of 8 meters.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
| Atmosphere | Helium | 41% |
| Neon | 27% |
| Xenon | 22% |
| Ozone | 9.6% |
| Water vapor | 0.0072% |
| Sulfur dioxide | 5.0E-5% |
| Atmospheric pressure | 40 bar |
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| No known satellites |
| Google search for Semohashu |
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Website by Joachim Michaelis
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