Sub-surface alteration and related change in reflectance spectra of space-weathered materials

0561082 - GLÚ 2023 RIV FR eng J - Journal Article
Chrbolková, Kateřina - Halodová, P. - Kohout, Tomáš - Ďurech, J. - Mizohata, K. - Malý, P. - Dědič, V. - Penttilä, A. - Trojánek, F. - Jarugula, R.
Sub-surface alteration and related change in reflectance spectra of space-weathered materials.
Astronomy & Astrophysics. Roč. 665, September 2022 (2022), č. článku A14. ISSN 0004-6361. E-ISSN 1432-0746
Institutional support: RVO:67985831
Keywords : methods: laboratory: solid state * methods: data analysis * techniques: spectroscopic * planets and satellites: surfaces * solar wind * meteorites, meteors, meteoroids
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 6.5, year: 2022
Method of publishing: Open access
https://www.aanda.org/articles/aa/full_html/2022/09/aa43282-22/aa43282-22.html

Context. Airless planetary bodies are studied mainly by remote sensing methods. Reflectance spectroscopy is often used to derive their compositions. One of the main complications for the interpretation of reflectance spectra is surface alteration by space weathering caused by irradiation by solar wind and micrometeoroid particles.
Aims. We aim to evaluate the damage to the samples from H⁺ and laser irradiation and relate it to the observed alteration in the spectra.
Methods. We used olivine (OL) and pyroxene (OPX) pellets irradiated by 5 keV H⁺ ions and individual femtosecond laser pulses and measured their visible (VIS) and near-infrared (NIR) spectra. We observed the pellets with scanning and transmission electron microscopy. We studied structural, mineralogical, and chemical modifications in the samples. Finally, we connected the material observations to changes in the reflectance spectra.
Results. In both minerals, H+ irradiation induces partially amorphous sub-surface layers containing small vesicles. In OL pellets, these vesicles are more tightly packed than in OPX ones. Any related spectral change is mainly in the VIS spectral slope. Changes due to laser irradiation are mostly dependent on the material’s melting temperature. Of all the samples, only the laser-irradiated OL contains nanophase Fe particles, which induce detectable spectral slope change throughout the measured spectral range. Our results suggest that spectral changes at VIS-NIR wavelengths are mainly dependent on the thickness of (partially) amorphous sub-surface layers. Furthermore, amorphisation smooths micro-roughness, increasing the contribution of volume scattering and absorption over surface scattering.
Conclusions. Soon after exposure to the space environment, the appearance of partially amorphous sub-surface layers results in rapid changes in the VIS spectral slope. In later stages (onset of micrometeoroid bombardment), we expect an emergence of nanoparticles to also mildly affect the NIR spectral slope. An increase in the dimensions of amorphous layers and vesicles in the more space-weathered material will only cause band-depth variation and darkening.
Permanent Link: https://hdl.handle.net/11104/0334585