PRECIPITATION OF MN-BEARING NODULES IN SHALLOW SOFT SEDIMENTS IN GALE CRATER, MARS
Regionally in the Groken area, the grain size is progressing from mudstone to sandstone, suggesting a transition from low-energy lacustrine deposits to a higher-energy lake margin environment. There is evidence for shallow water wave ripples in nearby stratigraphy. Nodules at Groken occupy thin horizons ~1.4 mm thick. Results from the ChemCam instrument from 85 nodules show that 71% of nodules contained both Mn and P, showing a strong relationship between Mn, P, and nodule morphology. Results from the Sample Analysis at Mars (SAM) instrument at the nearby Mary Anning 3 target point to the local presence of S-bearing organic molecules and high molecular weight (HMW) molecules. Results from the CheMin instrument suggest that the high Mn and P materials are currently amorphous.
Manganese-rich nodular features are common in terrestrial lacustrine environments. Diagenetic ferromanganese concretions that are sub-mm to a few mm in diameter can form within a distinct sediment layer at or below the sediment surface in fine-grained sediments containing organic carbon. In this scenario, Mn-oxides are first deposited in sediments where oxygen is absent below the top layer. The oxides then dissolve by reduction with organic carbon to form Mn2+, which diffuses upward to the oxidizing interface and re-precipitates as Mn-oxides along a thin horizon. Due to the slightly lower redox potential of Fe2+, Fe-oxides and peak concentrations of dissolved Fe2+ are found just below the Mn-oxides. Amorphous Mn and Fe oxides have been shown to sorb P if it is available in solution. A similar diagenetic pathway may be applicable to the mm-scale Mn nodules that outcrop on the sediment surface at Groken.