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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 3.

TIR spectra of Trojans 624 Hektor, 911 Agamemnon, and 1172 Aneas (J. Emery et al. 2006), compared to the inverted reflectance and emissivity of Y-86720 and B-7904. Gaps in the meteorite spectra near 16 μm are a region of low signal-to-noise due to low beam splitter throughput.

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