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Space Astro
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Info for exoplanet "Aesida"
| Scientific (actual) data |
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| Planet | Kepler-1336 b |
| Planet status | Confirmed |
| Radius | 0.177 |
| Orbital period | 23.1987 |
| Discovered | 2016 |
| Updated | 2021-02-05 |
| Tconj | 2454980 |
| Publication | Announced on a website |
| Detection type | Primary Transit |
| Alternate names | 2MASS J19450665+4653594 b, K02748.01, KIC 9962455 b, KOI-2748 b, KOI-2748.01, WISE J194506.64+465359.3 b |
| Star name | Kepler-1336 |
| Right ascension | 296.28° |
| Declination | 46.9° |
| Mag j | 12.819 |
| Mag h | 12.423 |
| Mag k | 12.366 |
| Star distance | 822 |
| Star metallicity | 0.05 |
| Star mass | 0.94 |
| Star radius | 1.3 |
| Star age | 12.3 |
| Star temperature | 5512 |
| Star alternate names | 2MASS J19450665+4653594, KIC 9962455, KOI-2748, WISE J194506.64+465359.3 |
| Wikipedia article | Kepler-1336 b |
Back
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| Fictional info (?) |
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| Suggested name | Aesida |
| Planet type | Cold planet |
| Aesida is the oldest planet known belonging to Kepler-1336 and one of the largest in its solar system. It is a cold planet planet with a mass one-thousandth that of Kepler-1336, but two-and-a-half times that of all the other planets in its solar system combined. Aesida's atmosphere is similar to Pekoer Rinyla's in its primary composition of 2H2O and hydrogen deuteride (HD), but it contains more "ices" such as water, ammonia, and methane, along with traces of other hydrocarbons. It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 65°K (-208°C), and has a complex, layered cloud structure with hydrogen deuteride (HD) thought to make up the lowest clouds, and 2H2O the uppermost layer of clouds. This cold planet is named after the deity Aesida, the god of dreams.
Aesida's surface appears slightly bruised and is similar in appearance to the Moon's, indicating that it has been geologically inactive for billions of years.
Liquid water cannot exist on the surface of Aesida due to low atmospheric pressure, which is less than 6 percent of Earth's, except at the lowest elevations for limited periods.
Aesida is primarily composed of 2H2O with a significant part of its mass being hydrogen deuteride (HD), though hydrogen deuteride (HD) comprises only about a tiny amount of the number of molecules.
In 3476, images from Frontier 7 showed Aesida as an almost featureless planet in visible light, without the cloud bands or storms associated with the other cold planets. |
| Atmosphere | 2H2O | 25% |
| Hydrogen deuteride (HD) | 22% |
| Ammonia | 21% |
| Nitric oxide | 12% |
| Argon | 8.6% |
| Hydrogen | 8.5% |
| Sulfur dioxide | 0.65% |
| Ammonium hydrosulfide (NH4SH) | 0.2% |
| Nitrogen | 0% |
| Atmospheric pressure | 0.0011 bar |
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| No known satellites |
| Google search for Aesida |
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Website by Joachim Michaelis
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