Spectral alteration of the Meteorite Epinal (H5) induced by heavy ion irradiation: a simulation of space weathering effects on near-Earth asteroids

By G. Strazzulla, E. Dotto, R. Binzel, R. Brunetto, M. Barucci, A. Blanco, V. Orofino. 2005

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/cf70ca5de4f00b24d1d37db6e193f4b26316309a

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Citations in the corpus

Irradiation of olivine by 4 keV He+: Simulation of space weathering by the solar wind (2009, background): “[39] Recent experiments in Catania [Brunetto and Strazzulla, 2005; Strazzulla et al., 2005; Brunetto et al., 2006b] have shown that higher-energy (60 – 400 keV) heavy ions can also cause significant alteration of spectral reflectance but at much lower ion fluences than used by Hapke [2001].”
Mercury’s Weather-Beaten Surface: Understanding Mercury in the Context of Lunar and Asteroidal Space Weathering Studies (2014, background): “…and Wehner 1964; Hapke 1965, 1966, 1968, 1973, 2001; KenKnight et al. 1967; Nash 1967; Hapke et al. 1970, 1975; Yin et al. 1972, 1975; Yin and Tsang 1976; Dukes et al. 1999; Davoisne et al. 2008; Brunetto and Strazzulla 2005; Strazzulla et al. 2005; Brunetto et al. 2006b; Loeffler et al. 2009).”
Space weathering and the interpretation of asteroid reflectance spectra (2010, unknown): “” Strazzulla et al. (2005) modeled the spectral effects of space weathering using a beam of 60 keV argon ions to simulate heavy”
Sources and physical processes responsible for OH/H2O in the lunar soil as revealed by the Moon Mineralogy Mapper (M3) (2011, background): “Heavier ions (especially He at ∼4% of solar wind particles) and other heavy species, with greater incident energies, also play a significant role in the sputtering process [Behrisch, 1983; Brunetto and Strazzulla., 2005; Strazzulla et al., 2005].”
Density of asteroids (2012, background): “…have allowed to understand the space weathering processes on the surfaces of olivines-and pyroxenes-rich S-complex asteroids (see, Chapman, 1996; Strazzulla et al., 2005; Vernazza et al., 2006, 2009a, among many others), including the related end-members A-and V-types (Brunetto et al., 2007;…”
Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification (2012, methodology): “These ion fluences are equivalent to exposure times of ∼ 0.1 × 106 to 1.3×106 years at about 1 AU from the Sun (calculated as in Strazzulla et al., 2005).”
Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, background): “…and diopside also confirm this very well-known effect of ion/laser irradiation on silicates and OCs [Yamada et al., 1999; Sasaki et al., 2001, 2002; Brunetto & Strazzulla, 2005; Marchi et al., 2005; Strazzulla et al., 2005; Brunetto et al., 2006; Loeffler et al., 2009; Fu et al., 2012] (see Append.”