Space weathering of silicates simulated by nanosecond pulse UV excimer laser

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2005.10.016 Byline: R. Brunetto (a)(b), F. Romano (a), A. Blanco (a), S. Fonti (a), M. Martino (a), V. Orofino (a), C. Verrienti (a) Keywords: Spectroscopy; Experimental techniques; Radiation chemistry; Meteorites; Asteroids Abstract: Laser irradiation experiments have been performed on powdered silicates (othopyroxene, clinopyroxene, and olivine) using a nanosecond pulse UV excimer laser (193 and 248 nm) to simulate the effects of space weathering induced on minor bodies of the Solar System by micrometeorite bombardment. We have used different fluences (from 0.05 to 2 J/cm.sup.2) to weather the samples, experimenting below and above the ablation threshold. All the irradiated materials have shown reddening and darkening of their UV-vis-NIR reflectance spectra. In addition we have found that: (1) below ablation threshold, weathering effects increase with increasing number of laser pulses, and with increasing fluence, confirming that a thermal process is active; (2) above ablation threshold, weathering is much stronger and efficient than in the previous case, and is independent on the number of pulses. We show that astrophysical time-scales, i.e. times necessary to obtain similar effects on planetary objects, are of about 10.sup.8 yr for both olivine and pyroxene in the case of ablation. The time grows up to 10.sup.10 yr in the case of thermal effects. We infer that micrometeorite bombardment can be rightly simulated by laser irradiation only considering congruent laser ablation. Author Affiliation: (a) Dipartimento di Fisica, Universita di Lecce, via Arnesano, I-73100 Lecce, Italy (b) INAF-Osservatorio Astrofisico di Catania, via S. Sofia 78, I-95123 Catania, Italy Article History: Received 17 June 2005; Revised 26 September 2005