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Measuring the Effects of Regolith Porosity on Mid-IR Spectra of the Allende Meteorite

Mid-infrared (MIR; 5–35 μ m) spectroscopy of laboratory meteorites does not often match asteroid spectra, making it difficult to constrain the parent bodies of meteorites using the MIR. To potentially improve the number of meteorite–asteroid matches, we simulated the effects of regolith porosity on...

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Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Lonnie D. Dausend, Audrey C. Martin, Joshua P. Emery
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2025-01-01
Saila:The Planetary Science Journal
Gaiak:
Sarrera elektronikoa:https://doi.org/10.3847/PSJ/ada778
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