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Space Astro
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Info for exoplanet "Totheus-medita"
Scientific (actual) data |
Name | Kepler-124 Ab |
Planet status | Confirmed |
Radius | 0.0946 |
Orbital period | 3.41046 |
Semi major axis | 0.0395 |
Orbit eccentricity | 0 |
Inclination | 70.06 |
Discovered | 2014 |
Updated | 2025-09-05 |
Tconj | 2454960 |
Impact parameter | 0.971 |
Temperature (kelvin) | 892 |
Publication | Announced on a website |
Detection type | Primary Transit |
Radius measurement type | Primary Transit |
Alternate names | 2MASS J19070067+4903536 b, K00241.03, KIC 11288051 b, KOI-241 b, KOI-241.03, WISE J190700.66+490353.5 b |
Star name | Kepler-124 A |
Right ascension | 286.75° |
Declination | 49.06° |
Mag j | 12.78 |
Mag h | 12.314 |
Mag k | 12.233 |
Star distance | 420.046 |
Star metallicity | -0.46 |
Star mass | 0.88 |
Star radius | 0.722 |
Star sp type | G9/K0V |
Star age | 1.82 |
Star temperature | 5188 |
Star alternate names | 2MASS J19070067+4903536, KIC 11288051, KOI-241, WISE J190700.66+490353.5 |
Wikipedia article | Kepler-124 Ab |
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Fictional info (?) |
Suggested name | Totheus-medita |
Planet type | Hot planet |
As seen from Kepler-124 A, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
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 9 meters.
Because of its fast rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). |
Atmosphere | Ethane | 83% |
Ammonium hydrosulfide (NH4SH) | 16% |
Carbonyl sulfide | 0.047% |
Atmospheric pressure | 40 bar |
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No known satellites |
Google search for Totheus-medita |
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Website by Joachim Michaelis
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