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Space Astro
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Info for exoplanet "Kupyono-ku"
Scientific (actual) data |
Planet | Kepler-256 e |
Planet status | Confirmed |
Radius | 0.21 |
Orbital period | 10.6816 |
Semi major axis | 0.096 |
Discovered | 2014 |
Updated | 2021-02-05 |
Tconj | 2454960 |
Impact parameter | 0.04 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19301930+4605506 e, K00939.04, KIC 9466668 e, KOI-939 e, KOI-939.04, WISE J193019.31+460550.5 e |
Star name | Kepler-256 |
Right ascension | 292.58° |
Declination | 46.1° |
Mag j | 13.824 |
Mag h | 13.496 |
Mag k | 13.424 |
Star distance | 1057.36 |
Star metallicity | 0.061 |
Star mass | 1.02 |
Star radius | 1.3 |
Star temperature | 5551 |
Star alternate names | 2MASS J19301930+4605506, KIC 9466668, KOI-939, WISE J193019.31+460550.5 |
Wikipedia article | Kepler-256 e |
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Fictional info (?) |
Suggested name | Kupyono-ku |
Planet type | Warm planet |
Kupyono-ku has been known to astronomers since the beginning of the space age. For this reason, scientists often classify Kupyono-ku and Pigamamyu-no as "warm planets" to distinguish them from the other planets. The planet is named after the deity Kupyono-ku, the bringer of prosperity.
Having almost no atmosphere to retain heat, it has surface temperatures that vary diurnally more than on any other planet in its solar system, ranging from 90°K (-183°C) at night to 735°K (462°C) during the day across the equatorial regions.
Future astrobiology missions are planned, including the Kupyono-ku 1900 and ExoKupyono-ku rovers. The volume of water ice in the south polar ice cap, if melted, would be sufficient to cover the entire planetary surface to a depth of 15 meters.
Kupyono-ku can easily be seen from Pigamamyu-no with the naked eye, as can its grayish coloring. |
Atmosphere | Neon | 47% |
Hydrogen deuteride (HD) | 42% |
Ammonium hydrosulfide (NH4SH) | 9.1% |
Helium | 1.6% |
Krypton | 0.00045% |
Atmospheric pressure | 4 bar |
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No known satellites |
Google search for Kupyono-ku |
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Website by Joachim Michaelis
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