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Space Astro
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Info for exoplanet "Ryuru"
Scientific (actual) data |
Planet | Kepler-924 b |
Planet status | Confirmed |
Radius | 0.274 |
Orbital period | 61.037 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2455010 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19224044+4023517 b, K01669.01, KIC 5183357 b, KOI-1669 b, KOI-1669.01, WISE J192240.44+402351.8 b |
Star name | Kepler-924 |
Right ascension | 290.67° |
Declination | 40.4° |
Mag j | 13.114 |
Mag h | 12.83 |
Mag k | 12.745 |
Star distance | 995 |
Star metallicity | 0.01 |
Star mass | 1.14 |
Star radius | 1.23 |
Star age | 3.09 |
Star temperature | 6167 |
Star alternate names | 2MASS J19224044+4023517, KIC 5183357, KOI-1669, WISE J192240.44+402351.8 |
Wikipedia article | Kepler-924 b |
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Fictional info (?) |
Suggested name | Ryuru |
Planet type | Cold planet |
This cold planet is named after the deity Ryuru, the bringer of prosperity.
As seen relative to the fixed stars, it rotates on its axis exactly five times for every four revolutions it makes around Kepler-924. An observer on Ryuru would therefore see only one summer every four years.
Ryuru's dense atmosphere make observation of its surface challenging in ultraviolet light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 24 years ago.
Surrounding Ryuru is a irregular planetary ring system and a powerful magnetosphere.
Wind speeds can reach 104 metres per second.
Planet is often inhabitated by unpredictable but interesting herbivores known to survive by devouring anything they find at night. Most Igeyu are not related to Hyabyu Jupyu but have 3 tentacles and vary in size from 70 to 90 cm. They can survive temperatures from -10 to 10°C and to some degree prolonged periods without food. |
Estimated population | 60000000 |
Atmosphere | Methane | 59% |
Water | 40% |
Oxygen | 0.11% |
Carbon dioxide | 0.096% |
Atmospheric pressure | 0.6 bar |
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No known satellites |
Google search for Ryuru |
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Website by Joachim Michaelis
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