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Sulfides and hollows formed on Mercury’s surface by reactions with reducing S-rich gases
Quantitative analyses of the experimental phases were performed with a JEOL JXA 8530F electron microprobe operated at 15 keV accelerating voltage and 15 nA beam current. The samples were analyzed with
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MER1 Pancam Science Raw Data Bundle
This bundle contains raw data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 1 (Opportunity). These data were produced by the science team.
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Smrekar_etal_2022_Supplementary_Tables1_2_3
See Smrekar et al., 2022 for additional explanation. Table 1: Derived parameters for coronae in Smrekar et al., (2022) and O’Rourke and Smrekar 32. Te (elastic thickness), Source (method in this study
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“Salt Tectonics” on Titan: radial labyrinths as topographic expressions of solid-state flow
Surface observations of Saturn’s moon Titan revealed features characterized as dissected, elevated plateaus with high valley density known as labyrinth terrains. Of this terrain class, a subtype refer
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ROSETTA-ORBITER 67P OSINAC 4 ESC2-MTP015 RDR-REFLECT V1.0
This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in reflectance units (normalized and thus without unit),...
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