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. Author manuscript; available in PMC: 2020 Aug 14.
Published in final edited form as: J Geophys Res Planets. 2017 Nov 21;122(12):2469–2488. doi: 10.1002/2017JE005331

Figure 6.

Figure 6.

VNIR reflectance spectra of smectites A – D and their oxidative products, collected in dry anaerobic conditions, except for the peroxide-treated samples which were measured in laboratory air. Gray dotted lines at ~0.55 μm and 0.87 μm highlight the spectral features of Fe3+ in hematite in peroxide-treated smectites.