Info for exoplanet "Methrymr Bos"

Scientific (actual) data Planet TCP J050742+244755 b Planet status Confirmed Planet mass 0.06 Semi major axis 0.775 Discovered 2018 Updated 2019-12-03 Publication Published in a refereed paper Detection type Microlensing Mass detection type Microlensing Alternate names Kojima-1L b Star name TCP J050742+244755 Right ascension 76.93° Declination 24.8° Star distance 429 Star mass 0.495 Wikipedia article TCP J050742+244755 b Back

Fictional info (?) Suggested name Methrymr Bos Planet type Small cold gas planet For this reason, scientists often classify Methrymr Bos and Jotlica as "small cold gas planets" to distinguish them from the other planets. The interior of Methrymr Bos is mainly composed of ices and stone. This planet is named after the deity Methrymr Bos, the bringer of destruction. The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to TCP J050742+244755, which reoccurs over the so-called synodic period approximately every 180 days. Methrymr Bos's surface appears partially cratered and is similar in appearance to the Moon's, indicating that it has been geologically inactive for billions of years. It has the densest atmosphere of the three small cold gas planets, consisting primarily of carbonyl sulfide. Observations from Earth have shown seasonal change and increased weather activity as Methrymr Bos approached its equinox 8 years ago. Atmosphere Carbonyl sulfide 32% Hydrogen peroxide 28% Hydrogen deuteride (HD) 15% Ammonia 12% Sulfur dioxide 11% Ethane 0.6% Water vapor 0.39% Hydrogen 0.26% Neon 0.14% Formaldehyde 0.0015% Atmospheric pressure 0.9 bar No known satellites Google search for Methrymr bos