|
|
Space Astro
|
Info for exoplanet "Misha-pyobi"
Scientific (actual) data |
Planet | HAT-P-62 b |
Planet status | Confirmed |
Planet mass | 0.761 |
Radius | 1.073 |
Orbital period | 2.64532 |
Semi major axis | 0.03772 |
Orbit eccentricity | 0.1 |
Inclination | 87.93 |
Discovered | 2020 |
Updated | 2020-07-15 |
Tzero tr | 2457120 |
Impact parameter | 0.25 |
K | 110 |
Temperature (kelvin) | 1512 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | HAT-P-62 |
Right ascension | 74.5° |
Declination | 48.3° |
Star distance | 353.1 |
Star metallicity | 0.414 |
Star mass | 1.023 |
Star radius | 1.17 |
Star age | 8.1 |
Star temperature | 5629 |
Wikipedia article | HAT-P-62 b |
Back
| |
Fictional info (?) |
Suggested name | Misha-pyobi |
Planet type | Hot gas giant |
Misha-pyobi is similar in composition to Pasa, and both have different bulk chemical composition from that of the larger hot gas giants. This planet is named after the deity Misha-pyobi, the creator of war.
An observer on Misha-pyobi would therefore see only one sunrise every three years.
Misha-pyobi is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light.
The volume of water detected has been estimated to be equivalent to the volume of water in Earth's oceans.
Misha-pyobi is primarily composed of krypton with a significant part of its mass being hydrogen, though hydrogen comprises only about a tiny amount of the number of molecules. |
Atmosphere | Krypton | 64% |
Hydrogen | 35% |
2H2O | 0.38% |
Xenon | 0.0009% |
Atmospheric pressure | 1.1 bar |
|
No known satellites |
Google search for Misha-pyobi |
|
Website by Joachim Michaelis
|
|
|
|