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Space Astro
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Info for exoplanet "Gachu-puryu"
Scientific (actual) data |
Planet | LTT 9779 b |
Planet status | Confirmed |
Planet mass | 0.09225 |
Radius | 0.4211 |
Orbital period | 0.792064 |
Semi major axis | 0.01679 |
Orbit eccentricity | 0 |
Inclination | 76.39 |
Discovered | 2019 |
Updated | 2023-07-11 |
Tzero tr | 2459040 |
K | 19.65 |
Temperature (kelvin) | 2000 |
Publication | Submitted to a professional journal |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Alternate names | TOI-193 b |
Star name | LTT 9779 |
Right ascension | 358.67° |
Declination | -37.63° |
Mag v | 9.76 |
Star distance | 80.6 |
Star metallicity | 0.25 |
Star mass | 1 |
Star radius | 0.92 |
Star sp type | G8 |
Star temperature | 5445 |
Wikipedia article | LTT 9779 b |
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Fictional info (?) |
Suggested name | Gachu-puryu |
Planet type | Small hot gas planet |
The planet is named after the deity Gachu-puryu, the spirit of chaos.
An observer on Gachu-puryu would therefore see only one day every four years.
Optical ground-based telescopes are typically limited to resolving features about 285 kilometers across when Gachu-puryu is closest because of Earth's atmosphere.
Gachu-puryu has been explored on several occasions by robotic spacecraft, most notably during the early Pioneer and Frontier flyby missions and later by the Hotchins orbiter. The latest probe to visit the planet is Racer, which entered into orbit around Gachu-puryu after a lengthy ride. |
Atmosphere | 2H2O | 85% |
Ozone | 14% |
Ethane | 0.2% |
Carbonyl sulfide | 0.13% |
Atmospheric pressure | 2.7 bar |
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Moon | Ponyu'chu | Small round oceanic asteroid |
Shigu'behi Ooza | Small slightly egg-shaped gaseous asteroid |
Gisho-pyo | Small slightly egg-shaped gaseous asteroid |
Uikyagyo Kyuhe | Medium-sized slightly egg-shaped rocky moon |
Beyu | Large round rocky asteroid |
Ryapyu | Small irregular ice planetoid |
Nahebu | Large potato shaped gaseous asteroid |
Google search for Gachu-puryu |
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Website by Joachim Michaelis
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