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Using Fluid-Mobile Elements to Decipher an Aqueous History Preserved in the Sedimentary Rocks of Gale Crater, Mars

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Figure

Figure 1-1: Elemental trends in APXS data for Gusev Crater, Meridiani Planum, and Gale Crater
Figure 1-2: APXS results for Zn and Ni on Mars. The average soils (arrow), generally accepted to be representative of the composition of the average Mars crust [e.g., Yen et al., 2005; Taylor and McLennan, 2010], are enriched in both Ni and Zn relative to
Figure 1-4: APXS results compared to whole rock bulk elemental data for Martian meteorites and relatively unaltered volcanics from Maunakea, Hawai’i
Figure 1-5: Curiosity’s traverse in Gale Crater, Mars, over the first 1550 sols. Rover waypoints are indicated, APXS targets are denoted (red circles), and the approximate division between the Bradbury group to the north and the Mt
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Outline

APXS Deployment and Dataset Methods Maunakea Sedimentary Deposits Alteration Trends in the Mount Sharp Group Conclusion Conclusions and Future Work Chapter Summary and Key Points Overview of Gale Crater Geologic Setting Zn and Ge Occurrence and Distribution Diagenetic Mobilization and Fractionation

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