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Space Astro
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Info for exoplanet "Teserus Is"
Scientific (actual) data |
Name | Kepler-53 c |
Planet status | Confirmed |
Planet mass | 0.11 |
Radius | 0.283 |
Orbital period | 38.5583 |
Discovered | 2012 |
Updated | 2023-01-13 |
Tconj | 2455000 |
Tzero tr | 2455000 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass measurement type | Spectrum |
Radius measurement type | Theoretical |
Alternate names | 2MASS J19215082+4033448 c, K00829.03, KIC 5358241 c, KOI-829 c, KOI-829.03, WISE J192150.81+403344.9 c |
Star name | Kepler-53 |
Right ascension | 290.46° |
Declination | 40.56° |
Mag v | 16 |
Mag j | 14.252 |
Mag h | 13.906 |
Star distance | 1420.1 |
Star mass | 0.98 |
Star radius | 0.89 |
Star temperature | 5858 |
Star alternate names | 2MASS J19215082+4033448, KIC 5358241, KOI-829, WISE J192150.81+403344.9 |
Wikipedia article | Kepler-53 c |
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Fictional info (?) |
Suggested name | Teserus Is |
Planet type | Small cold gas planet |
It is a small cold gas planet planet with a mass one-thousandth that of Kepler-53, but two-and-a-half times that of all the other planets in its solar system combined.
As seen from Kepler-53, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
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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 19 meters.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
Atmosphere | Carbonyl sulfide | 61% |
Hydrogen | 38% |
Atmospheric pressure | 0.7 bar |
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No known satellites |
Google search for Teserus is |
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Website by Joachim Michaelis
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