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Space Astro
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Info for exoplanet "Taydime Sto"
| Scientific (actual) data |
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| Name | Kepler-1472 b |
| Planet status | Confirmed |
| Radius | 0.17 |
| Orbital period | 38.1313 |
| Discovered | 2016 |
| Updated | 2021-02-05 |
| Tconj | 2454990 |
| Publication | Announced on a website |
| Detection type | Primary Transit |
| Alternate names | 2MASS J19392463+4903268 b, K03345.01, KIC 11303322 b, KOI-3345 b, KOI-3345.01, WISE J193924.64+490326.8 b |
| Star name | Kepler-1472 |
| Right ascension | 294.85° |
| Declination | 49.06° |
| Mag j | 13.579 |
| Mag h | 13.308 |
| Mag k | 13.255 |
| Star distance | 1269 |
| Star metallicity | 0.03 |
| Star mass | 1.16 |
| Star radius | 1.25 |
| Star age | 3.09 |
| Star temperature | 6159 |
| Star alternate names | 2MASS J19392463+4903268, KIC 11303322, KOI-3345, WISE J193924.64+490326.8 |
| Wikipedia article | Kepler-1472 b |
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| Fictional info (?) |
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| Suggested name | Taydime Sto |
| Planet type | Cold planet |
| It has the longest rotation period (445 days) of any planet in its solar system and rotates in the opposite direction to most other planets.
It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 50°K (-223°C), and has a complex, layered cloud structure with molecular hydrogen thought to make up the lowest clouds, and carbonyl sulfide the uppermost layer of clouds. The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Kepler-1472, which reoccurs over the so-called synodic period approximately every 99 days. |
| Atmosphere | Carbonyl sulfide | 77% |
| Molecular hydrogen | 19% |
| Helium | 2.7% |
| Hydrogen chloride | 0.29% |
| Atmospheric pressure | 60 bar |
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| No known satellites |
| Google search for Taydime sto |
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Website by Joachim Michaelis
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