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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 2.

Figure 2.

Backscatter Mössbauer spectra for smectites A, B, C, and D and their oxidation products, offset for clarity. Each spectrum was normalized to a maximum peak intensity of 0.3. Mössbauer spectra of unaltered samples were acquired after some oxidation during storage (cf., Chemtob et al., 2015).