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Space Astro
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Info for exoplanet "Uqedo-ci"
Scientific (actual) data |
Planet | HD 3167 d |
Planet status | Confirmed |
Mass sini | 0.0217 |
Orbital period | 8.492 |
Semi major axis | 0.07757 |
Orbit eccentricity | 0.36 |
Discovered | 2017 |
Updated | 2017-06-28 |
Omega | 176 |
Tconj | 2457810 |
K | 2.39 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Radial Velocity |
Star name | HD 3167 |
Right ascension | 8.74° |
Declination | 4.38° |
Mag v | 8.94 |
Mag j | 7.548 |
Mag h | 7.203 |
Star distance | 47.36 |
Star metallicity | -0.02 |
Star mass | 0.94 |
Star radius | 0.87 |
Star sp type | K0 V |
Star age | 5 |
Star temperature | 5528 |
Star alternate names | EPIC 220383386, HIP 2736, 2MASS J00345752+0422531, BD+03 68, K2-96, SAO 109291, TYC 0013-00894-1, WISE J003457.60+042251.4 |
Wikipedia article | HD 3167 d |
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Fictional info (?) |
Suggested name | Uqedo-ci |
Planet type | Warm planet |
It is the second-brightest natural object in the night sky after Dotynul-osu, reaching an apparent magnitude of -5 - bright enough to cast shadows at night and, rarely, visible to the naked eye in broad daylight.
The planet is named after the deity Uqedo-ci, the creator of hate.
As seen from HD 3167, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
Uqedo-ci's axis has the smallest tilt of any of its solar system's planets.
As the closest planet to Dotynul-osu, Uqedo-ci has been a prime target for early extra solar exploration.
The Uqedo-ci system has a unique configuration among those of the planets because its axis of rotation is tilted sideways, nearly into the plane of its solar orbit. Observations from Earth have shown seasonal change and increased weather activity as Uqedo-ci approached its equinox 4 years ago. |
Atmosphere | Helium | 52% |
2H2O | 48% |
Atmospheric pressure | 60 bar |
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No known satellites |
Google search for Uqedo-ci |
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Website by Joachim Michaelis
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