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Space Astro
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Info for exoplanet "Taypro Pa"
Scientific (actual) data |
Planet | TOI-2338 b |
Planet status | Confirmed |
Planet mass | 5.98 |
Radius | 1 |
Orbital period | 22.654 |
Semi major axis | 0.158 |
Orbit eccentricity | 0.676 |
Inclination | 89.5 |
Discovered | 2023 |
Updated | 2023-04-06 |
Omega | 12.6 |
Tzero tr | 2458460 |
Impact parameter | 0.26 |
K | 584 |
Temperature (kelvin) | 799 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | TOI-2338 |
Right ascension | 81.35° |
Declination | -34.67° |
Mag v | 12.5 |
Star distance | 316 |
Star metallicity | 0.22 |
Star mass | 0.99 |
Star radius | 1.05 |
Star age | 7 |
Star temperature | 5581 |
Wikipedia article | TOI-2338 b |
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Fictional info (?) |
Suggested name | Taypro Pa |
Planet type | Large gas giant |
In English, Taypro Pa is often referred to as the "brown planet" because the ozone prevalent on its surface gives it a deep brown appearance that is distinctive among the astronomical bodies visible to the naked eye. It is the second-brightest natural object in the night sky after Keiotungr-lade, reaching an apparent magnitude of -5 - bright enough to cast shadows at night and, rarely, visible to the naked eye in broad daylight.
This planet is named after the deity Taypro Pa, the god of nature.
Future astrobiology missions are planned, including the Taypro Pa 2700 and ExoTaypro Pa rovers.
In 1787, images from Daedalus 5 showed Taypro Pa as an almost featureless planet in visible light, without the cloud bands or storms associated with the other large gas giants. Observations from Earth have shown seasonal change and increased weather activity as Taypro Pa approached its equinox 3 years ago. |
Atmosphere | Ammonium hydrosulfide (NH4SH) | 75% |
Ozone | 13% |
2H2O | 11% |
Oxygen | 0.047% |
Hydrogen deuteride (HD) | 0.00033% |
Atmospheric pressure | 0.23 bar |
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No known satellites |
Google search for Taypro pa |
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Website by Joachim Michaelis
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