Irradiation induced mineral changes of NWA10580 meteorite by infrared analysis

Gyollai, Ildikó and Biri, Sándor and Juhász, Zoltán and Király, Csilla and Pályi, Bernadett and Rácz, Richárd Péter and Rezes, Dánel and Sulik, Béla and Szabó, Máté and Szalai, Zoltán and Szávai, Péter and Szklenár, Tamás and Kereszturi, Ákos (2024) Irradiation induced mineral changes of NWA10580 meteorite by infrared analysis. Astronomy and Astrophysics, 683 (A162). pp. 1-12. (In Press)

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Abstract

Context. Identifying minerals on asteroid surfaces is difficult as space weathering modifies the minerals’ infrared spectra. This should be better understood for proper interpretation. Aims. We simulated the space weathering effects on a meteorite and recorded the alterations of the crystalline structure, such as the change in peak positions and full width at half maximum values. Methods. We used proton irradiation to simulate the effects of solar wind on a sample of NWA 10580 CO3 chondrite meteorites. After irradiation in three gradually increased steps with 1 keV ion energy, we used infrared microscopic reflectance and diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS) to identify and understand the consequences of irradiation. Results. We find negative peak shifts after the first and second irradiations at pyroxene and feldspar minerals, similarly to the literature, and this shift was attributed to Mg loss. However, after the third irradiation a positive change in values in wavenumber emerged for silicates, which could come from the distortion of SiO4 tetrahedra, resembling shock deformation. The full width at half maximum values of major bands show a positive (increasing) trend after irradiations in the case of feldspars, using IR reflection measurements. Comparing DRIFTS and reflection infrared data, the peak positions of major mineral bands were at similar wavenumbers, but differences can be observed in minor bands. Conclusions. We measured the spectral changes of meteorite minerals after high doses of proton irradiation for several minerals. We show the first of these measurements for feldspars; previous works only presented pyroxene, olivine, and phyllosilicates.

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