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. 2020 Sep 23;125(9):e2019JE006294. doi: 10.1029/2019JE006294

Figure 5.

Figure 5

(left) Context Mastcam and associated RMI images for ChemCam observations showing typical bedrock targets along Curiosity's traverse through Mt. Sharp. (right) ChemCam passive spectra and Mastcam spectra associated with DRTed targets demonstrating the spectral variability of the Murray formation. Both Stranraer and Oban were located on VRR and represent end‐members in the area; Stranraer had some of the deepest ferric absorptions along the traverse while Oban was a member of the “gray” class of rocks that contains coarse grained gray hematite. Observation IDs are Oban—Mastcam: Sol 1,905, product identifiers 0099940(08–21), RMI: CRO_566517863PRC_F0671358CCAM01904L1, CRO_566518772PRC_F0671358CCAM01904L1; Stranraer—Mastcam: Sol 2,007, product identifiers 01056000(1–7), RMI: CRO_575483031PRC_F0690408CCAM01005L1, CRO_575483650PRC_F0690408CCAM01005L1; Mason point—Mastcam: Sol 1,696, product identifiers 0088450(01–14), RMI: CRO_547960268PRC_F0630346CCAM01695L1, CRO_547961029PRC_ F0630346CCAM01695l; Precipice—Mastcam: Sol 1,532, product identifiers 00780900(1–7), RMI: CRO_533402746PRC_F0592830CCAM01531L1, CRO_533404002PRC_ F0592830CCAM01531.