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Spectral Similarity in the Thermal Infrared between Sulfide-rich Carbonaceous Chondrite Meteorites, Jupiter Trojans, and Other D- and P-type Asteroids

  • Authors: Helena C. Bates, Ashley J. King, Kerri L. Donaldson Hanna, Audrey C. Martin, Joshua P. Emery, Neil E. Bowles, Sara S. Russell

Helena C. Bates et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

The reflectance spectra of Y-86720 (blue) and B-7904 (green), with the reflectance spectra of olivine/Fe-sulfide mixtures from R. Sultana et al. (2023). Gaps in the meteorite reflectance spectra near 16 μm are a region of low signal-to-noise due to low beam splitter throughput.

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