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Space Astro
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Info for exoplanet "Ketsu Bobahe"
Scientific (actual) data |
Planet | AU Mic b |
Planet status | Confirmed |
Planet mass | 0.116 |
Radius | 0.4571 |
Orbital period | 8.46303 |
Semi major axis | 0.08305 |
Orbit eccentricity | 0.012 |
Inclination | 89.9904 |
Discovered | 2020 |
Updated | 2023-02-20 |
Omega | 356.2 |
Tzero tr | 2458330 |
Impact parameter | 0.0032 |
K | 11.2 |
Temperature (kelvin) | 569.5 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | AU Mic |
Right ascension | 311.29° |
Declination | -31.34° |
Mag v | 8.6 |
Star distance | 9.79 |
Star mass | 0.5 |
Star radius | 0.75 |
Star sp type | M1V |
Star age | 0.022 |
Star temperature | 3700 |
Wikipedia article | AU Mic b |
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Fictional info (?) |
Suggested name | Ketsu Bobahe |
Planet type | Terrestrial |
When viewed from Myopya, Ketsu Bobahe 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 Ketsu Bobahe, the bringer of fear.
An observer on Ketsu Bobahe would therefore see only one day every five years.
The nitric oxide has probably photodissociated, and the free carbon monoxide has been swept into interplanetary space by the solar wind because of the lack of a planetary magnetic field.
The rotational period and seasonal cycles of Ketsu Bobahe are likewise similar to those of Earth, as is the tilt that produces the seasons.
Liquid water cannot exist on the surface of Ketsu Bobahe due to low atmospheric pressure, which is less than 8 percent of Earth's, except at the highest elevations for short periods. |
Atmosphere | Carbon monoxide | 65% |
Formaldehyde | 31% |
Nitric oxide | 2.3% |
Carbon dioxide | 0.82% |
Krypton | 0.66% |
Neon | 0.059% |
Sulfur dioxide | 0.0043% |
Hydrogen peroxide | 0% |
Atmospheric pressure | 0.23 bar |
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No known satellites |
Google search for Ketsu bobahe |
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Website by Joachim Michaelis
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