Space weathering simulations through controlled growth of iron nanoparticles on olivine
arXiv:1404.2956 · doi:10.1016/j.icarus.2014.04.004
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 (npFe) during space weathering plays major role in these spectral changes. A laboratory procedure for the controlled production of npFe 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 npFe in the 7-20 nm size range. A logarithmic trend is observed between amount of npFe and darkening, reduction of 1 μm olivine absorption band, reddening, and 1 μm band width. Olivine with a population of physically larger npFe particles follows spectral trends similar to other samples, except for the reddening trend. This is interpreted as the larger, ~40-50 nm sized, npFe particles do not contribute to the spectral slope change as efficiently as the smaller npFe fraction. A linear trend is observed between the amount of npFe and 1 μm band center position, most likely caused by Fe disassociation from olivine structure into npFe particles.
References in corpus (1)
Cited by in corpus (5)
- Space weathering simulations through controlled growth of iron nanoparticles on olivine
- Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene
- Thermal Alteration and Differential Sublimation Can Create Phaethons "Rock Comet" Activity and Blue Color
- (433) Eros and (25143) Itokawa surface properties from reflectance spectra
- Spectroscopic Mapping of Callisto with HST/STIS and Implications for its Surface Composition