Role of spectral resolution for infrared asteroid compositional analysis using meteorite spectra

In this work the potential mineral identification of meteorites is analysed for the mid-infrared range, to evaluate observational possibilities for future missions targeting small body surfaces. Three carbonaceous and three ordinary chondrite meteorites are examined by a diffuse reflection (DRIFT) i...

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Veröffentlicht in:arXiv.org 2020-05
Hauptverfasser: Skulteti, A, Kereszturi, A, Kereszty, Zs, Pal, B, Szabo, M, Cipriani, F
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description In this work the potential mineral identification of meteorites is analysed for the mid-infrared range, to evaluate observational possibilities for future missions targeting small body surfaces. Three carbonaceous and three ordinary chondrite meteorites are examined by a diffuse reflection (DRIFT) instrument, and the presence of principal minerals is confirmed by a powder diffraction method as well. The possibilities and constraints of mineral identifications in the mid-infrared are simulated by artificially degrading the spectral resolution. Our research shows that for the definite identification of principal mineral bands, a spectral resolution \(\leq 10\)~cm\(^{-1}\) (\(\leq 0.15 \mu\)m) is needed. At 20-100~cm\(^{-1}\) (0.3 - 1.5~\(\mu\)m) resolution the identification of these minerals is uncertain, and with a resolution \(>100\)~cm\(^{-1}\), it is almost impossible.
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subjects Asteroid missions
Fourier transforms
Infrared analysis
Meteorites
Meteors & meteorites
Minerals
Physics - Earth and Planetary Astrophysics
Physics - Instrumentation and Methods for Astrophysics
Spectra
Spectral resolution
title Role of spectral resolution for infrared asteroid compositional analysis using meteorite spectra
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