Mars: Its atmosphere and surface

Abstract

Spectral experiments on Mars Orbiter show that solar energy is absorbed by the planet and its atmosphere and eventually re-emitted in the infrared as thermal emission. The majority of the radiances at the north polar Mars area follows very closely the radiance from a black body of about 145 degrees kelvin, which indicates a frozen CO2 surface; the south polar region radiance indicates a temperature inversion in the atmosphere, and the emission of atmospheric dust as well as emissions from frozen CO2.