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Space Astro
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Info for exoplanet "Gyoma-se"
Scientific (actual) data |
Planet | Kepler-1647 (AB) b |
Planet status | Confirmed |
Planet mass | 1.52 |
Radius | 1.06 |
Orbital period | 1107.59 |
Semi major axis | 2.7205 |
Orbit eccentricity | 0.0581 |
Inclination | 90.0972 |
Discovered | 2015 |
Updated | 2016-10-14 |
Omega | 155.046 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Radius detection type | Primary Transit |
Star name | Kepler-1647 (AB) |
Right ascension | 298.15° |
Declination | 40.66° |
Mag v | 13.78 |
Star mass | 2.1885 |
Star radius | 1.79 |
Star temperature | 6210 |
Wikipedia article | Kepler-1647 (AB) b |
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Fictional info (?) |
Suggested name | Gyoma-se |
Planet type | Cold gas giant |
Its orbital period around Kepler-1647 (AB) of 1100 earth days is the longest of all the planets in its solar system.
Gyoma-se and Byubo Ryoryo are cold gas giants rich in rock. It is named after the deity Gyoma-se, the creator of the sea.
Gyoma-se's axis has the smallest tilt of any of its solar system's planets.
Gyoma-se was one of the first planets to have its motions plotted across the sky - as early as the second millennium BC.
Liquid water cannot exist on the surface of Gyoma-se due to low atmospheric pressure, which is less than 6 percent of Earth's, except at the highest elevations for limited periods. In November 2800, NASA reported finding a large amount of underground ice in the Utopia Planitia region of Gyoma-se.
Surrounding Gyoma-se is a thin planetary ring system and a powerful magnetosphere.
Future targets for exploration in the Gyoma-se system include the probable ice-covered liquid ocean of its moon Shumi. |
Atmosphere | Sulfur dioxide | 85% |
2H2O | 14% |
Helium | 0.24% |
Ammonium hydrosulfide (NH4SH) | 0.16% |
Atmospheric pressure | 22 bar |
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Moon | Shumi | Small round rocky moon |
Chugyu Yoryu | Large almost round rocky moon |
Myuryo-mugagyo | Large slightly egg-shaped oceanic moon |
Google search for Gyoma-se |
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Website by Joachim Michaelis
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