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Space Astro
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Info for exoplanet "Zabumya"
Scientific (actual) data |
Planet | TOI-2364 b |
Planet status | Confirmed |
Planet mass | 0.225 |
Radius | 0.768 |
Orbital period | 4.01975 |
Semi major axis | 0.04871 |
Orbit eccentricity | 0 |
Inclination | 88.98 |
Discovered | 2022 |
Updated | 2022-10-31 |
Tzero tr | 2459060 |
Impact parameter | 0.21 |
K | 29.7 |
Temperature (kelvin) | 1091 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | TOI-2364 |
Right ascension | 89.13° |
Declination | -5.01° |
Star distance | 218.63 |
Star metallicity | 0.344 |
Star mass | 0.954 |
Star radius | 0.886 |
Star age | 3.5 |
Star temperature | 5306 |
Wikipedia article | TOI-2364 b |
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Fictional info (?) |
Suggested name | Zabumya |
Planet type | Hot gas giant |
Zabumya is similar in composition to Byaneko Bon, and both have different bulk chemical composition from that of the larger hot gas giants. The planet is named after the deity Zabumya, the messenger of the sky.
When viewed from Byaneko Bon, this proximity to TOI-2364 means the planet can only be seen near the western or eastern horizon during the early evening or early morning.
It is radically different from Byaneko Bon in other respects.
Zabumya is primarily composed of hydrogen chloride with a significant part of its mass being molecular hydrogen, though molecular hydrogen comprises only about a limited amount of the number of molecules.
In 1787, images from Daedalus 3 showed Zabumya as an almost featureless planet in visible light, without the cloud bands or storms associated with the other hot gas giants. |
Atmosphere | Hydrogen chloride | 85% |
Molecular hydrogen | 6.3% |
Sulfur dioxide | 6% |
Ammonium hydrosulfide (NH4SH) | 1.4% |
Neon | 0.28% |
Methane | 0.029% |
Atmospheric pressure | 1.5 bar |
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No known satellites |
Google search for Zabumya |
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Website by Joachim Michaelis
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