Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering

Sho Sasaki (), Keiko Nakamura, Yoshimi Hamabe, Erika Kurahashi and Takahiro Hiroi
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Sho Sasaki: The University of Tokyo
Keiko Nakamura: Kobe University
Yoshimi Hamabe: The University of Tokyo
Erika Kurahashi: The University of Tokyo
Takahiro Hiroi: Brown University

Nature, 2001, vol. 410, issue 6828, 555-557

Abstract: Abstract ‘Space weathering’ is the term applied to the darkening and reddening of planetary surface materials with time, along with the changes to the depths of absorption bands in their optical spectra. It has been invoked to explain the mismatched spectra of lunar rocks and regolith, and between those of asteroids and meteorites1,2,3,4,5,6. The formation of nanophase iron particles on regolith grains as a result of micrometeorite impacts or irradiation by the solar wind has been proposed as the main cause of the change in the optical properties7,8. But laboratory simulations9,10,11,12,13,14 have not revealed the presence of these particles, although nano-second-pulse laser irradiation did reproduce the optical changes12. Here we report observations by transmission electron microscopy of olivine samples subjected to pulse laser irradiation. We find within the amorphous vapour-deposited rims of olivine grains nanophase iron particles similar to those observed in the rims of space-weathered lunar regolith grains15,16. Reduction by hydrogen atoms implanted by the solar wind is therefore not necessary to form the particles. Moreover, the results support the idea that ordinary chondrites came from S-type asteroids5, and thereby provides some constraints on the surface exposure ages of those asteroids.

Date: 2001
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DOI: 10.1038/35069013

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