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. Author manuscript; available in PMC: 2020 Oct 28.
Published in final edited form as: J Geophys Res Planets. 2020 Feb 21;125(3):e2019JE006011. doi: 10.1029/2019je006011

Figure 5.

Figure 5.

Laboratory spectra asymmetric Gaussian fitting results for RELAB and USGS spectra. These demonstrate the tendency of the centroid and asymmetry to decrease with increasing Fo#. This plot includes all 16 laboratory olivine spectra that have grain size <70 microns.