The History of Water in Martian Magmas From Thorium Maps.

ABSTRACT: Water inventories in Martian magmas are poorly constrained. Meteorite-based estimates range widely, from 10² to >10⁴ ppm H₂O, and are likely variably influenced by degassing. Orbital measurements of H primarily reflect water cycled and stored in the regolith. Like water, Th behaves incompatibly during mantle melting, but unlike water Th is not prone to degassing and is relatively immobile during aqueous alteration at low temperature. We employ Th as a proxy for original, mantle-derived H₂O in Martian magmas. We use regional maps of Th from Mars Odyssey to assess variations in magmatic water across major volcanic provinces and through time. We infer that Hesperian and Amazonian magmas had ∼100-3,000 ppm H₂O, in the lower range of previo

SUBMITTER: Black BA 

PROVIDER: S-EPMC9285613 | biostudies-literature | 2022 Jun

REPOSITORIES: biostudies-literature