Image Details
Caption: Figure 7.
Molar content of fayalite (Fa) vs. ferrosilite (Fs) for NEOs with an ordinary chondrite-like composition whose spectra do not show the 2 μm band. Measured values for H- (green), L- (orange), and LL- (blue) ordinary chondrites from Nakamura et al. (2011) are also included. The error bars correspond to the uncertainties derived by Sanchez et al. (2020), 2.0 mol% for Fa and 1.4 mol% for Fs. Figure adapted from Nakamura et al. (2011).
© 2024. The Author(s). Published by the American Astronomical Society.