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Space Astro
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Info for exoplanet "Aemir Ro"
Scientific (actual) data |
Planet | HD 8574 b |
Planet status | Confirmed |
Mass sini | 2.11 |
Orbital period | 227.55 |
Semi major axis | 0.77 |
Orbit eccentricity | 0.288 |
Angular distance | 0.017421 |
Discovered | 2003 |
Updated | 2009-10-07 |
Omega | 3.6 |
Tperi | 2451470 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Star name | HD 8574 |
Right ascension | 21.3° |
Declination | 28.57° |
Mag v | 7.12 |
Star distance | 44.2 |
Star metallicity | 0.05 |
Star mass | 1.17 |
Star radius | 1.37 |
Star sp type | F8 |
Star age | 7.13 |
Star temperature | 6080 |
Wikipedia article | HD 8574 b |
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Fictional info (?) |
Suggested name | Aemir Ro |
Planet type | Cold planet |
When viewed from Julthi Peauto, Aemir Ro can reach an apparent magnitude of -3, bright enough for its reflected light to cast shadows, and making it on average the third-brightest object in the night sky. For this reason, scientists often classify Aemir Ro and Julthi Peauto as "cold planets" to distinguish them from the other planets. The planet is named after the deity Aemir Ro, the bringer of war.
Liquid water cannot exist on the surface of Aemir Ro due to low atmospheric pressure, which is less than 3 percent of Julthi Peauto's, except at the lowest elevations for limited periods.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
Atmosphere | Xenon | 37% |
Ammonia | 25% |
Methane | 24% |
Molecular hydrogen | 5.9% |
Ammonium hydrosulfide (NH4SH) | 4.5% |
Formaldehyde | 2.9% |
Oxygen | 0.0034% |
Carbonyl sulfide | 0.0019% |
Carbon monoxide | 0.00059% |
Atmospheric pressure | 0.031 bar |
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No known satellites |
Google search for Aemir ro |
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Website by Joachim Michaelis
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