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Global Distribution and Spectral Properties of Low‐Reflectance Material on Mercury
Author(s) -
Klima Rachel L.,
Denevi Brett W.,
Ernst Carolyn M.,
Murchie Scott L.,
Peplowski Patrick N.
Publication year - 2018
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2018gl077544
Subject(s) - impact crater , mercury (programming language) , carbon fibers , geology , terrain , mineralogy , reflectivity , carbon sequestration , environmental science , earth science , astrobiology , carbon dioxide , materials science , chemistry , geography , optics , composite material , physics , cartography , organic chemistry , composite number , computer science , programming language
We examine the global distribution and spectral properties of low‐reflectance material (LRM) across Mercury to estimate the relative carbon abundance of prominent exposures and to test hypotheses for the origin of carbon in LRM. Our mapping demonstrates that LRM is consistently excavated from depth and that the spectral curvature attributed to carbon becomes more subdued as these surface deposits age. We find that the 600‐nm band depth in LRM deposits is related to carbon content and can be used to estimate carbon enrichment. LRM deposits excavated by basins and large craters may be enriched with as much as 4 wt% carbon over the local mean. Regional deposits, associated with the most heavily cratered terrains, are enriched by an average of ~2.5 wt% carbon. The association of LRM with excavation from depth shows that the carbon in LRM is native to the planet, rather than deposited over time by impacts.