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Space Astro
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Info for exoplanet "Pinov-ah"
Scientific (actual) data |
Planet | HIP 36985 b |
Planet status | Confirmed |
Mass sini | 29 |
Orbital period | 8500 |
Semi major axis | 7 |
Orbit eccentricity | 0.55 |
Discovered | 2019 |
Updated | 2019-12-06 |
Omega | 50 |
K | 480 |
Publication | Published in a refereed paper |
Detection type | Radial Velocity |
Mass detection type | Spectrum |
Star name | HIP 36985 |
Right ascension | 114.03° |
Declination | -3.11° |
Mag v | 9.9 |
Star distance | 14.07 |
Star mass | 0.621 |
Star sp type | M1V |
Star age | 0.26 |
Wikipedia article | HIP 36985 b |
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Fictional info (?) |
Suggested name | Pinov-ah |
Planet type | Cold planet |
This planet is named after the deity Pinov-ah, the spirit of the underworld.
At this time it may appear as a bright star-like object, but is often far more difficult to observe than Gysapo.
Pinov-ah is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light.
As the closest planet to Gysapo, Pinov-ah has been a prime target for early interplanetary exploration.
The smooth Borealis basin in the northern hemisphere covers 30 percent of the planet and may be a giant impact feature.
Pinov-ah is primarily composed of hydrogen chloride with a significant part of its mass being water vapor, though water vapor comprises only about a small fraction of the number of molecules. |
Atmosphere | Hydrogen chloride | 93% |
Water vapor | 5.3% |
Carbon dioxide | 1.4% |
Atmospheric pressure | 40 bar |
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No known satellites |
Google search for Pinov-ah |
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Website by Joachim Michaelis
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