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Space Astro
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Info for exoplanet "Harlene Dys"
Scientific (actual) data |
Planet | L 98-59 d |
Planet status | Confirmed |
Planet mass | 0.0061 |
Radius | 0.1357 |
Orbital period | 7.45072 |
Semi major axis | 0.0486 |
Orbit eccentricity | 0.074 |
Inclination | 88.449 |
Discovered | 2018 |
Updated | 2021-08-06 |
Omega | 180 |
Tzero tr | 2451360 |
Impact parameter | 0.922 |
K | 1.5 |
Temperature (kelvin) | 416 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Alternate names | TOI-175 d |
Star name | L 98-59 |
Right ascension | 122.53° |
Declination | -68.31° |
Mag v | 11.7 |
Star distance | 10.623 |
Star metallicity | -0.5 |
Star mass | 0.32 |
Star radius | 0.291 |
Star temperature | 3500 |
Star alternate names | TOI-175 |
Wikipedia article | L 98-59 d |
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Fictional info (?) |
Suggested name | Harlene Dys |
Planet type | Warm planet |
The planet is named after the deity Harlene Dys, the messenger of the sky.
Liquid water cannot exist on the surface of Harlene Dys due to low atmospheric pressure, which is less than 7 percent of Jarnno's, except at the lowest elevations for short periods.
Planet is mostly occupied by friendly but poisonous bacteria that feed by killing the Pina plant. The Vigahali Ste are related to Cuditagaret, have wings and vary in length from 50 to 130 meters. Vigahali Ste are known to thrive at temperatures from -80 to -30°C and to some degree severe infection. |
Estimated population | 12000000 |
Atmosphere | Water | 70% |
Methane | 29% |
Carbon dioxide | 0.32% |
Oxygen | 0.027% |
Atmospheric pressure | 0.12 bar |
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No known satellites |
Google search for Harlene dys |
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Website by Joachim Michaelis
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