HiPOD: Sunday, 13 September 2020
Frosted Ground in the Southern Hemisphere in Late Fall

Frosted Ground in the Southern Hemisphere
This image was acquired within two weeks of the winter solstice, when the subsolar latitude is at its northernmost position.

At this location and time, the Sun barely peeks over the horizon in the mid-afternoon when MRO passes overhead, and carbon dioxide frost is building up on most of the surface.

In enhanced color, the frost appears blue. Slopes that face north receive more heat from the sun and appear reddish, indicating less frost is present. There may also be a small amount of water frost on the surface.

Mars is very different from Earth in that its main atmospheric component can condense onto the surface. The nitrogen that dominates Earth’s atmosphere never condenses onto the surface, although nitrogen in the atmospheres of frigid Triton and Pluto does form surface frost and ice.

ID: ESP_026388_1280
date: 13 March 2012
altitude: 252 km

https://uahirise.org/hipod/ESP_026388_1280
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

Black & white is less than 5 km across; enhanced color is less than 1 km. For full observation details, visit the ID link.