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Space Astro
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Info for exoplanet "Topihyu"
| Scientific (actual) data |
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| Name | WASP-178 b |
| Planet status | Confirmed |
| Planet mass | 1.41 |
| Radius | 1.94 |
| Orbital period | 3.34483 |
| Semi major axis | 0.0558 |
| Orbit eccentricity | 0 |
| Inclination | 85.7 |
| Discovered | 2019 |
| Updated | 2022-04-06 |
| Tzero tr | 2457480 |
| Lambda angle | 91.3 |
| Impact parameter | 0.628 |
| K | 123 |
| Temperature (kelvin) | 2402 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Alternate names | KELT-26 b |
| Molecules | SiO |
| Star name | WASP-178 |
| Right ascension | 227.27° |
| Declination | -42.71° |
| Mag v | 9.95 |
| Mag j | 9.8 |
| Star distance | 417 |
| Star metallicity | -0.06 |
| Star mass | 1.93 |
| Star radius | 1.801 |
| Star sp type | A1IV-V |
| Star age | 0.43 |
| Star temperature | 8640 |
| Star alternate names | KELT-26, HD 134004 |
| Wikipedia article | WASP-178 b |
Back
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| Fictional info (?) |
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| Suggested name | Topihyu |
| Planet type | Hot gas giant |
| The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. A prominent result is the "great yellow spot", a giant storm that is known to have existed for centuries since it was first seen by telescope. |
| Atmosphere | SiO | 99% |
| Atmospheric pressure | 17 bar |
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| No known satellites |
| Google search for Topihyu |
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Website by Joachim Michaelis
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