|
|
Space Astro
|
Info for exoplanet "Tebenutu"
| Scientific (actual) data |
|---|
| Name | TOI-4666 b |
| Planet status | Confirmed |
| Planet mass | 0.7 |
| Radius | 1.11 |
| Orbital period | 2.90892 |
| Semi major axis | 0.0333 |
| Orbit eccentricity | 0 |
| Inclination | 89.7 |
| Discovered | 2025 |
| Updated | 2025-10-14 |
| Tzero tr | 2459170 |
| Impact parameter | 0.07 |
| K | 142 |
| Temperature (kelvin) | 713 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Star name | TOI-4666 |
| Right ascension | 56.29° |
| Declination | -39.06° |
| Mag v | 15.3 |
| Star distance | 154.75 |
| Star metallicity | 0.79 |
| Star mass | 0.576 |
| Star radius | 0.585 |
| Star sp type | M2V |
| Star age | 3 |
| Star temperature | 3793 |
| Wikipedia article | TOI-4666 b |
Back
| |
| Fictional info (?) |
|---|
| Suggested name | Tebenutu |
| Planet type | Hot gas giant |
| As seen relative to the fixed stars, it rotates on its axis exactly two times for every four revolutions it makes around TOI-4666.
It has the densest atmosphere of all the hot gas giants, consisting mostly of hydrogen peroxide.
The smooth Borealis basin in the northern hemisphere covers 16 percent of the planet and may be a giant impact feature.
Its north and south poles, therefore, lie where most other planets have their equators. |
| Atmosphere | Hydrogen peroxide | 60% |
| Methane | 33% |
| Oxygen | 5.8% |
| Carbonyl sulfide | 0.0029% |
| Atmospheric pressure | 0.0014 bar |
 |
| No known satellites |
| Google search for Tebenutu |
|
Website by Joachim Michaelis
|
|
|
|