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| Naji, M. |
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| Motta, Antonella |
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| Aletan, Dirar |
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| Mohamed, Tarek |
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| Ertürk, Emre |
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| Taccardi, Nicola |
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| Kononenko, Denys |
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| Petrov, R. H. | Madrid |
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| Alshaaer, Mazen | Brussels |
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| Bih, L. |
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| Casati, R. |
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| Muller, Hermance |
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| Kočí, Jan | Prague |
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| Šuljagić, Marija |
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| Kalteremidou, Kalliopi-Artemi | Brussels |
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| Azam, Siraj |
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| Ospanova, Alyiya |
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| Blanpain, Bart |
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| Ali, M. A. |
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| Popa, V. |
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| Rančić, M. |
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| Ollier, Nadège |
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| Azevedo, Nuno Monteiro |
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| Landes, Michael |
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| Rignanese, Gian-Marco |
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Stefani, Stefania
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (3/3 displayed)
- 2022Reflectance of silicate glasses in the mid-infrared region (MIR): Implications for planetary researchcitations
- 2017FT-IR and μ-IR analysis of Carbonaceous Chondrite meteorites characterization as possible analogue of next sample returned materials
- 2017Laboratory experiments on ammoniated clay minerals with relevance for asteroid (1) Ceres
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article
FT-IR and μ-IR analysis of Carbonaceous Chondrite meteorites characterization as possible analogue of next sample returned materials
Abstract
In this work, the Fourier Transform Infrared Spectroscopy (FT-IR) and Infrared μ-spectroscopy (μ-IR) techniques have been applied on four Carbonaceous Chondrites (CC) meteorites, as possible analogues of the Hayabusa2 and Osiris-REx space missions asteroid targets. The analysed CC meteorites belong to CV, CI and CM classes. Chondrules, CAIs, and mineral inclusions, have been identified and analysed in detail in the spectral region 8-14 μm (μ-IR analysis). CC packed powders have been analysed using a FT-IR spectrometer in the spectral range of 2-14 μm. The absorption bands, Christiansen and Reststrahlen features, of the main minerals have been identified. We plan to compare the FT-IR spectral results with C-type asteroids data collected by in-flight spectrometers (e.g. 1Ceres, 10Hygeia etc.)....