Fenrir
- For the Imperial Bloodline of the same name, see Line of Fenrir.
| ||
| Orbital characteristics | ||
| Mass (Kg) | 1.56E+23 | |
| Radius (Km) | 1,850 | |
| Solar Day (h) | 36.9 | |
| Orbital Period (days) | 2.14 | |
| Semi-Major Axis (Km) | 440,141(km) | |
| Periapsis (AU) | .003 | |
| Apoapsis (AU) | .003 | |
| Albedo | .01 | |
| Surface Temperature (K) | 151 | |
| Surface Gravity (m/s^2) | 3.05 | |
| Axial Tile (degrees) | 1.5 | |
| Inclination (degrees) | .2 | |
| Orbital Speed (Km/s) | 21.2 | |
| Satellites | None | |
Fenrir is the moon which most closely orbits the planet Chrysos.
North Polar Regions
The North Polar region of Fenrir is characterized by its cold and rugged terrain, dominated by thick ice caps and frozen methane lakes. This region experiences extremely low temperatures due to its tilt, resulting in a predominantly icy landscape. The surface is dotted with large, jagged ice formations and deep crevasses caused by the constant freezing and thawing cycles. Occasional geysers of water and methane erupt through the ice, driven by geothermal activity beneath the surface. The polar region is shrouded in darkness for most of its year, with brief periods of sunlight creating a stark contrast in the icy wilderness.
Equatorial Regions
The Equatorial region of Fenrir presents a more temperate climate compared to its poles, featuring a mixture of rocky and sandy terrains. This region receives the most sunlight, making it the warmest part of the moon. The landscape includes expansive plains of dark basalt rock, interspersed with areas of fine, golden dust. The equatorial zone experiences significant geological activity, including frequent volcanic eruptions that contribute to the formation of vast lava plains. The presence of various mineral deposits suggests that the equator may have once harbored liquid water. Dust storms occasionally sweep across the plains, reshaping the landscape and revealing new geological features.
Southern Polar Regions
The South Polar region of Fenrir, like the North Polar region, is dominated by ice and cold temperatures. The terrain is a mix of smooth ice fields and rugged, rocky outcrops, creating a visually striking contrast. The South Pole is home to several large subglacial lakes, kept liquid by geothermal heat from the moon's interior. These lakes are of particular interest to scientists studying the potential for microbial life. The dynamic interplay between ice and geothermal activity results in unique formations such as ice caves and meltwater channels.
