|
|
Space Astro
|
Info for exoplanet "Pyagyu"
| Scientific (actual) data |
|---|
| Planet | TOI-2260 b |
| Planet status | Confirmed |
| Planet mass | 0.011 |
| Radius | 0.1445 |
| Orbital period | 0.352473 |
| Semi major axis | 0.0097 |
| Discovered | 2022 |
| Updated | 2022-01-30 |
| Tzero tr | 2458930 |
| Impact parameter | 0.77 |
| Temperature (kelvin) | 2609 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass detection type | Theoretical |
| Radius detection type | Primary Transit |
| Star name | TOI-2260 |
| Right ascension | 247.67° |
| Declination | 49.05° |
| Mag v | 10.5 |
| Star distance | 101.3 |
| Star mass | 0.99 |
| Star radius | 0.94 |
| Star temperature | 5534 |
| Wikipedia article | TOI-2260 b |
Back
| |
| Fictional info (?) |
|---|
| Suggested name | Pyagyu |
| Planet type | Hot planet |
| Pyagyu has been known to astronomers since the medieval. The planet is named after the deity Pyagyu, the bringer of hate.
When viewed from Chisepi Kya, this proximity to TOI-2260 means the planet can only be seen near the western or eastern horizon during the early evening or early morning.
Pyagyu's surface appears very rippled and is similar in appearance to the Moon's, indicating that it has been geologically inactive for billions of years.
It may also have a rocky core of heavier elements, but like the other hot planets, Pyagyu lacks a well-defined solid surface. |
| Atmosphere | Carbonyl sulfide | 61% |
| Helium | 32% |
| Carbon dioxide | 6% |
| Methane | 0.35% |
| Ammonia | 0.11% |
| Nitrogen | 1.7E-5% |
| Atmospheric pressure | 70 bar |
 |
| No known satellites |
| Google search for Pyagyu |
|
Website by Joachim Michaelis
|
|
|
|