Publication Date:
2019-07-17
Description:
We calculate that approximately 10% of martian atmospheric Kr-80 formed by neutron capture on Mars in approx. 0.5 Ga. The regolith contains even larger amounts of n-capture Kr-80 and Ar-36, which may provide clues to the evolution of the martian regolith and atmosphere. Additional information is contained in the original extended abstract.
Keywords:
Lunar and Planetary Science and Exploration
Type:
Lunar and Planetary Science XXXII; LPI-Contrib-1080
Format:
text
Permalink