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Space Astro
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Info for exoplanet "Dano Ryu"
Scientific (actual) data |
Planet | HD 212301 A b |
Planet status | Confirmed |
Mass sini | 0.4 |
Radius | 1.07 |
Orbital period | 2.24571 |
Semi major axis | 0.036 |
Orbit eccentricity | 0.0147 |
Angular distance | 0.000683 |
Discovered | 2005 |
Updated | 2019-12-13 |
Omega | 172.8 |
Tperi | 2453390 |
Tzero vr | 53549.2 |
K | 59.5 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Radius detection type | Theoretical |
Alternate names | HD 212301 b |
Star name | HD 212301 A |
Right ascension | 336.88° |
Declination | -77.72° |
Mag v | 7.77 |
Star distance | 52.7 |
Star metallicity | 0.18 |
Star mass | 1.05 |
Star sp type | F8 V |
Star age | 5.9 |
Star temperature | 5998 |
Star alternate names | HD 212301 |
Wikipedia article | HD 212301 A b |
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Fictional info (?) |
Suggested name | Dano Ryu |
Planet type | Hot planet |
Its orbital period around HD 212301 A of 2.2 earth days is the longest of all the planets in its solar system. Dano Ryu is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the valleys, deserts, and polar ice caps of Earth. Dano Ryu is orbiting HD 212301 A every 2.2 Earth days.
It is named after the deity Dano Ryu, the spirit of destruction.
Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Dano Ryu's distance from HD 212301 A is only about two-thirds (or 59 pct) of its distance at aphelion.
Dano Ryu was one of the first planets to have its motions plotted across the sky - as early as the second millennium BC. |
Atmosphere | Ammonium hydrosulfide (NH4SH) | 65% |
Ethane | 34% |
Water vapor | 0.00014% |
Atmospheric pressure | 40 bar |
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No known satellites |
Google search for Dano ryu |
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Website by Joachim Michaelis
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