Info for exoplanet "Qemera Mo"

Scientific (actual) data Planet HIP 70849 b Planet status Confirmed Mass sini 9 Orbital period 10000 Semi major axis 10 Orbit eccentricity 0.6 Angular distance 0.416667 Discovered 2009 Updated 2011-07-04 Publication Published in a refereed paper Detection type Radial Velocity Star name HIP 70849 Right ascension 217.33° Declination -46.46° Mag v 10.36 Star distance 24 Star mass 0.63 Star sp type K7V Star age 3 Star temperature 4105 Wikipedia article HIP 70849 b Back

Fictional info (?) Suggested name Qemera Mo Planet type Cold planet Qemera Mo and Rexaw are cold planets rich in iron. It is named after the deity Qemera Mo, the demon of the sea. Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Qemera Mo's distance from HIP 70849 is only about two-thirds (or 89 pct) of its distance at aphelion. As the closest planet to Rexaw, Qemera Mo has been a prime target for early interplanetary exploration. The rotational period and seasonal cycles of Qemera Mo are likewise similar to those of Earth, as is the tilt that produces the seasons. There are ongoing investigations assessing the past habitability potential of Qemera Mo, as well as the possibility of extant life. Qemera Mo is primarily composed of carbonyl sulfide with a significant part of its mass being neon, though neon comprises only about a limited fraction of the number of molecules. The largest moon, Ojaza, has a diameter greater than that of the planet Mercury. Atmosphere Carbonyl sulfide 84% Neon 15% Krypton 0.022% Atmospheric pressure 50 bar Moon Ojaza Small almost round rocky asteroid Etac-ocen-iq Medium-sized round oceanic moon Google search for Qemera mo