|
|
Space Astro
|
Info for exoplanet "Hyuma"
Scientific (actual) data |
Name | TOI-2445 b |
Planet status | Confirmed |
Planet mass | 0.006 |
Radius | 0.12267 |
Orbital period | 0.371128 |
Semi major axis | 0.0064 |
Discovered | 2022 |
Updated | 2024-06-04 |
Tzero tr | 2459140 |
Impact parameter | 0.27 |
Temperature (kelvin) | 1060 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass measurement type | Theoretical |
Radius measurement type | Primary Transit |
Star name | TOI-2445 |
Right ascension | 43.32° |
Declination | 0.05° |
Mag v | 15.7 |
Star distance | 48.6 |
Star mass | 0.25 |
Star radius | 0.27 |
Star sp type | M |
Star temperature | 3330 |
Wikipedia article | TOI-2445 b |
Back
| |
Fictional info (?) |
Suggested name | Hyuma |
Planet type | Hot planet |
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to TOI-2445, which reoccurs over the so-called synodic period approximately every 191 days.
A prominent result is the "great orange spot", a giant storm that is known to have existed for centuries since it was first detected by scanner.
Wind speeds can reach 135 metres per second. |
Atmosphere | Carbonyl sulfide | 97% |
Ozone | 2.4% |
Carbon monoxide | 0.077% |
Ethane | 0.0079% |
Helium | 0.0012% |
Atmospheric pressure | 0.006 bar |
 |
No known satellites |
Google search for Hyuma |
|
Website by Joachim Michaelis
|
|
|
|