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Space Astro
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Info for exoplanet "Eisyaog En"
Scientific (actual) data |
Planet | WASP-158 b |
Planet status | Confirmed |
Planet mass | 2.79 |
Radius | 1.07 |
Semi major axis | 0.0517 |
Orbit eccentricity | 0 |
Inclination | 87.7 |
Discovered | 2018 |
Updated | 2018-05-15 |
Tzero tr | 2457620 |
Impact parameter | 0.32 |
K | 295 |
Temperature (kelvin) | 1590 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Star name | WASP-158 |
Right ascension | 4.15° |
Declination | -10.98° |
Mag v | 12.1 |
Star metallicity | 0.24 |
Star mass | 1.38 |
Star radius | 1.39 |
Star sp type | F6V |
Star age | 1.7 |
Star temperature | 6350 |
Wikipedia article | WASP-158 b |
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Fictional info (?) |
Suggested name | Eisyaog En |
Planet type | Large hot gas giant |
Eisyaog En 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. Eisyaog En is orbiting WASP-158 every @ORBITALPERIOD Earth days.
It is named after the deity Eisyaog En, the messenger of good fortune.
As seen relative to the fixed stars, it rotates on its axis exactly five times for every five revolutions it makes around WASP-158.
Eisyaog En was one of the first planets to have its motions plotted across the sky - as early as the second millennium BC.
Eisyaog En is the site of Celestium Gravis, the largest volcano and second-highest known mountain in its solar system, and of Valles Marineris, one of the largest canyons in its solar system.
A prominent result is the "great blue spot", a giant storm that is known to have existed for centuries since it was first detected by scanner. |
Atmosphere | Helium | 45% |
Hydrogen | 20% |
Neon | 20% |
Argon | 11% |
Carbon monoxide | 4.3% |
Ammonia | 0.032% |
Sulfur dioxide | 0.002% |
Atmospheric pressure | 100 bar |
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Moon | Yojeiq | Huge round ice moon |
Google search for Eisyaog en |
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Website by Joachim Michaelis
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