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Space Astro
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Info for exoplanet "Feqeneh Ekaj"
| Scientific (actual) data |
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| Name | TOI-912 b |
| Planet status | Confirmed |
| Planet mass | 0.016 |
| Radius | 0.1722 |
| Orbital period | 4.67807 |
| Semi major axis | 0.041 |
| Orbit eccentricity | 0.58 |
| Inclination | 88.7 |
| Discovered | 2025 |
| Updated | 2025-09-19 |
| Omega | -169 |
| Tzero tr | 2458630 |
| Impact parameter | 0.34 |
| K | 4.29 |
| Temperature (kelvin) | 551 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Star name | TOI-912 |
| Right ascension | 229.33° |
| Declination | -80.47° |
| Mag v | 12.67 |
| Mag j | 9.09 |
| Mag h | 8.47 |
| Mag k | 8.2 |
| Star distance | 26.089 |
| Star metallicity | -0.19 |
| Star mass | 0.418 |
| Star radius | 0.419 |
| Star sp type | M3V |
| Star age | 0.8 |
| Star temperature | 3572 |
| Star alternate names | L 20-1, TIC 406941612, 2MASS J15172165-8028225 |
| Wikipedia article | TOI-912 b |
Back
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| Fictional info (?) |
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| Feqeneh Ekaj |
| Hot planet |
| As seen from TOI-912, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
| Atmosphere | Carbon dioxide | 52% |
| Sulfur dioxide | 48% |
| Ammonia | 0.11% |
| 0.0021 bar |
| 1.4 × Earth |
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| No known satellites |
| Google search for Feqeneh ekaj |
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Website by Joachim Michaelis
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