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Space Astro
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Info for exoplanet "Mipbian"
Scientific (actual) data |
Planet | 51 Peg b |
Planet status | Confirmed |
Planet mass | 0.47 |
Mass sini | 0.46 |
Radius | 1.9 |
Orbital period | 4.2308 |
Semi major axis | 0.052 |
Orbit eccentricity | 0.0069 |
Inclination | 80 |
Angular distance | 0.003537 |
Discovered | 1995 |
Updated | 2017-01-26 |
Omega | 54.1 |
Tperi | 2450400 |
Tzero vr | 2497 |
K | 55.65 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Radial Velocity |
Radius detection type | Theoretical |
Molecules | CO, H2O |
Star name | 51 Peg |
Right ascension | 344.36° |
Declination | 20.77° |
Mag v | 5.49 |
Star distance | 14.7 |
Star metallicity | 0.2 |
Star mass | 1.11 |
Star radius | 1.266 |
Star sp type | G2 IV |
Star age | 4 |
Star temperature | 5793 |
Wikipedia article | 51 Peg b |
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Fictional info (?) |
Suggested name | Mipbian |
Planet type | Hot gas giant |
It is the second-brightest natural object in the night sky after Fercli Culo, reaching an apparent magnitude of -5 - bright enough to cast shadows at night and, sometimes, visible to the naked eye in broad daylight.
It is named after the deity Mipbian, the spirit of love and beauty.
Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Mipbian's distance from 51 Peg is only about two-thirds (or 116 pct) of its distance at aphelion.
As the closest planet to Fercli Culo, Mipbian has been a prime target for early extra solar exploration.
Wind speeds can reach 99 metres per second. |
Atmosphere | H2O | 91% |
CO, | 8.9% |
Atmospheric pressure | 4 bar |
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No known satellites |
Google search for Mipbian |
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Website by Joachim Michaelis
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