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Space Astro
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Info for exoplanet "Dusnis Dilmal"
| Scientific (actual) data |
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| Name | HAT-P-24 Ab |
| Planet status | Confirmed |
| Planet mass | 0.685 |
| Radius | 1.242 |
| Orbital period | 3.35524 |
| Semi major axis | 0.0465 |
| Orbit eccentricity | 0.067 |
| Inclination | 88.6 |
| Angular distance | 0.000152 |
| Discovered | 2010 |
| Updated | 2024-07-31 |
| Omega | 197 |
| Tzero tr | 2455220 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Alternate names | TOI-511.01 |
| Star name | HAT-P-24 A |
| Right ascension | 108.83° |
| Declination | 14.26° |
| Mag v | 11.76 |
| Mag j | 10.79 |
| Mag h | 10.59 |
| Mag k | 10.54 |
| Star distance | 405 |
| Star metallicity | -0.16 |
| Star mass | 1.191 |
| Star radius | 1.317 |
| Star sp type | F8IV-V |
| Star age | 2.8 |
| Star temperature | 6373 |
| Star alternate names | TOI-511 |
| Wikipedia article | HAT-P-24 Ab |
Back
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| Fictional info (?) |
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| Suggested name | Dusnis Dilmal |
| Planet type | Hot gas giant |
| It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 83°K (-190°C), and has a complex, layered cloud structure with sulfur dioxide thought to make up the lowest clouds, and krypton the uppermost layer of clouds.
As seen relative to the fixed stars, it rotates on its axis exactly five times for every four revolutions it makes around HAT-P-24 A. |
| Atmosphere | Krypton | 75% |
| Sulfur dioxide | 25% |
| Helium | 0.003% |
| Ammonia | 8.0E-5% |
| Atmospheric pressure | 9 bar |
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| No known satellites |
| Google search for Dusnis dilmal |
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Website by Joachim Michaelis
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