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Space Astro
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Info for exoplanet "Vosfar"
| Scientific (actual) data |
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| Planet | TOI-4184 b |
| Planet status | Confirmed |
| Planet mass | 6.6 |
| Radius | 0.2168 |
| Orbital period | 4.90198 |
| Semi major axis | 0.0336 |
| Inclination | 89.43 |
| Discovered | 2023 |
| Updated | 2023-06-28 |
| Tzero tr | 2459480 |
| Impact parameter | 0.306 |
| Temperature (kelvin) | 412 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass detection type | Theoretical |
| Radius detection type | Primary Transit |
| Star name | TOI-4184 |
| Right ascension | 43.83° |
| Declination | -79.41° |
| Mag v | 17.1 |
| Star distance | 69.2 |
| Star metallicity | -0.27 |
| Star mass | 0.24 |
| Star radius | 0.252 |
| Star sp type | M5.5 |
| Star age | 6.7 |
| Star temperature | 3225 |
| Wikipedia article | TOI-4184 b |
Back
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| Fictional info (?) |
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| Suggested name | Vosfar |
| Planet type | Large hot gas giant |
| It is a large hot gas giant planet with a mass one-thousandth that of TOI-4184, but two-and-a-half times that of all the other planets in its solar system combined. The interior of Vosfar is mainly composed of ices and rock. This large hot gas giant is named after the deity Vosfar, the god of the sky.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to TOI-4184, which reoccurs over the so-called synodic period approximately every 180 days.
Vosfar is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light.
Vosfar's thick atmosphere make observation of its surface challenging in infrared light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 36 years ago. |
| Atmosphere | Helium | 53% |
| Ammonia | 39% |
| Carbonyl sulfide | 7.6% |
| Hydrogen | 1.0E-6% |
| Atmospheric pressure | 80 bar |
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| No known satellites |
| Google search for Vosfar |
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Website by Joachim Michaelis
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