English

Space weathering simulations through controlled growth of iron nanoparticles on olivine

Earth and Planetary Astrophysics 2014-05-15 v2

Abstract

Airless planetary bodies are directly exposed to space weathering. The main spectral effects of space weathering are darkening, reduction in intensity of silicate mineral absorption bands, and an increase in the spectral slope towards longer wavelengths (reddening). Production of nanophase metallic iron (npFe0^{0}) during space weathering plays major role in these spectral changes. A laboratory procedure for the controlled production of npFe0^{0} in silicate mineral powders has been developed. The method is based on a two-step thermal treatment of low-iron olivine, first in ambient air and then in hydrogen atmosphere. Through this process, a series of olivine powder samples was prepared with varying amounts of npFe0^{0} in the 7-20 nm size range. A logarithmic trend is observed between amount of npFe0^{0} and darkening, reduction of 1 {\mu}m olivine absorption band, reddening, and 1 {\mu}m band width. Olivine with a population of physically larger npFe0^{0} particles follows spectral trends similar to other samples, except for the reddening trend. This is interpreted as the larger, ~40-50 nm sized, npFe0^{0} particles do not contribute to the spectral slope change as efficiently as the smaller npFe0^{0} fraction. A linear trend is observed between the amount of npFe0^{0} and 1 {\mu}m band center position, most likely caused by Fe2+^{2+} disassociation from olivine structure into npFe0^{0} particles.

Keywords

Cite

@article{arxiv.1404.2956,
  title  = {Space weathering simulations through controlled growth of iron nanoparticles on olivine},
  author = {T. Kohout and J. Čuda and J. Filip and D. Britt and T. Bradley and J. Tuček and R. Skála and G. Kletetschka and J. Kašlík and O. Malina and K. Šišková and R. Zbořil},
  journal= {arXiv preprint arXiv:1404.2956},
  year   = {2014}
}