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Space Astro
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Info for exoplanet "Sosaosi Mona"
Scientific (actual) data |
Planet | Kepler-977 b |
Planet status | Confirmed |
Radius | 0.234 |
Orbital period | 26.8533 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454980 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19260389+4214535 b, K01847.01, KIC 6776401 b, KOI-1847 b, KOI-1847.01, WISE J192603.88+421453.2 b |
Star name | Kepler-977 |
Right ascension | 291.52° |
Declination | 42.25° |
Mag j | 13.434 |
Mag h | 13.018 |
Mag k | 12.92 |
Star distance | 664 |
Star metallicity | -0.01 |
Star mass | 0.87 |
Star radius | 0.83 |
Star age | 4.57 |
Star temperature | 5315 |
Star alternate names | 2MASS J19260389+4214535, KIC 6776401, KOI-1847, WISE J192603.88+421453.2 |
Wikipedia article | Kepler-977 b |
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Fictional info (?) |
Suggested name | Sosaosi Mona |
Planet type | Cold planet |
When viewed from Ditanrhea, Sosaosi Mona can reach an apparent magnitude of -3, bright enough for its reflected light to cast shadows, and making it on average the third-brightest object in the night sky. It is named after the deity Sosaosi Mona, the messenger of fear.
Sosaosi Mona is gravitationally locked with Kepler-977 in a 5:4 spin-orbit resonance, and rotates in a way that is unique in its solar system.
As the closest planet to Ditanrhea, Sosaosi Mona has been a prime target for early extra solar exploration.
Its apparent magnitude reaches -3, which is surpassed only by Ditanrhea, Larisma, and Kepler-977. Optical ground-based telescopes are typically limited to resolving features about 285 kilometers across when Sosaosi Mona is closest because of Earth's atmosphere.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
Atmosphere | Hydrogen chloride | 67% |
Oxygen | 16% |
Ammonia | 15% |
Xenon | 1.3% |
Helium | 0.0068% |
Ozone | 0% |
Atmospheric pressure | 0.7 bar |
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No known satellites |
Google search for Sosaosi mona |
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Website by Joachim Michaelis
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