DIAGENETIC ALTERATION AND CONCRETION FORMATION IN THE JURASSIC BRUSHY BASIN MEMBER OF THE MORRISON FORMATION, COLORADO PLATEAU, USA: AN ANALOG STUDY FOR THE YELLOWKNIFE BAY FORMATION AT GALE CRATER, MARS
Concretions are present in both the terrestrial and martian rocks and are important because they record fluid/rock (and biota, on Earth) interactions and can preserve organics and micro- and macro-fossils. Yellowknife Bay formation concretions exhibit uniform morphology and are enriched in Fe, Mg and Cl relative to the host rock. By comparison, Brushy Basin Member concretions exhibit much more diverse mineralogies, sizes, and morphologies within areas of tens of square centimeters despite similar lithology in both the terrestrial and martian rocks. The geochemistry of the Brushy Basin Member concretions is quite similar to the host rock with only slight enrichment of certain elements which implies limited transport of reactants. The diversity of concretion mineralogy and morphology with restricted reactant transport suggests the concretions form in diagenetic microenvironments and are likely influenced by biotic interaction. In contrast, uniform concretion morphology and mineralogy in the Yellowknife Bay formation indicate abiotic precipitation mechanisms. Although the Yellowknife Bay formation represents a potentially habitable paleoenvironment, the record of biotic interaction in diagenetic reactions and concretion formation is lacking.