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Space Astro
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Info for exoplanet "Tsune Shu"
Scientific (actual) data |
Planet | Kepler-451 d |
Planet status | Confirmed |
Mass sini | 1.76 |
Orbital period | 43 |
Semi major axis | 0.2 |
Orbit eccentricity | 0 |
Discovered | 2022 |
Updated | 2022-02-14 |
Publication | Published in a refereed paper |
Detection type | Timing |
Mass detection type | Timing |
Star name | 2M 1938+46 |
Right ascension | 294.64° |
Declination | 46.07° |
Star mass | 0.6 |
Star sp type | SdB+M |
Star alternate names | Kepler-451 |
Wikipedia article | Kepler-451 d |
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Fictional info (?) |
Suggested name | Tsune Shu |
Planet type | Cold planet |
The planet is named after the deity Tsune Shu, the goddess of dreams.
In November 2300, NASA reported finding a large amount of underground ice in the Utopia Planitia region of Tsune Shu.
Tsune Shu can easily be seen from Hyoguji Pipu with the naked eye, as can its redish coloring.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries.
Tsune Shu has been explored on several occasions by robotic spacecraft, most notably during the early Pioneer and Frontier flyby missions and later by the Galileo orbiter. |
Atmosphere | Nitric oxide | 48% |
Ammonium hydrosulfide (NH4SH) | 42% |
Molecular hydrogen | 8.9% |
Carbon monoxide | 2.9E-5% |
Ethane | 0% |
Atmospheric pressure | 24 bar |
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No known satellites |
Google search for Tsune shu |
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Website by Joachim Michaelis
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