Image Details
Caption: Figure 14.
Left: spectra of the LL-chondrite Chelyabinsk corresponding to five different grain sizes plus a slab from Bowen et al. (2023). All spectra are normalized to unity at 0.55 μm. Right: Band I and II depths as a function of grain size measured from the Chelyabinsk spectra. Uncertainties are smaller than the symbols.
© 2024. The Author(s). Published by the American Astronomical Society.