Images

read the article 'COBALT/Langley'
03.17.2017 COBALT/Langley
read the article 'COBALT/JPL team'
03.17.2017 COBALT/JPL team
read the article 'Mono Lake'
01.26.2017 Mono Lake
This image shows atomic hydrogen scattering sunlight in the upper atmosphere of Mars, as seen by the Imaging Ultraviolet Spectrograph on NASA's Mars Atmosphere and Volatile Evolution mission.
10.19.2016

MAVEN's Ultraviolet Views of Hydrogen's Escape from Mars

This image shows atomic hydrogen scattering sunlight in the upper atmosphere of Mars, as seen by the Imaging Ultraviolet Spectrograph on NASA's Mars Atmosphere and Volatile Evolution mission. About 400,000 observations, taken over the course of four days shortly after the spacecraft entered orbit around Mars, were used to create the image. Hydrogen is produced by the breakdown of water, which was once abundant on Mars' surface. Because hydrogen has low atomic mass and is weakly bound by gravity, it extends far from the planet (the darkened circle) and can readily escape.

Image Credit: NASA/University of Colorado

All Images




Search Icon