“…Io's visible reflectance spectra, notably an absorption edge near 0.4 µm, resemble those of elemental sulfur and certain sulfur compounds (Wamsteker et al 1974, Nash and Fanale 1977, Nelson and Hapke 1978, Fanale et al 1979, Smythe et al 1979, Veverka et al 1979, Pieri et al 1984, Sasson et al 1985, Nash 1987, Nash and Moses 1988. Consistent with the composition of Io's atmosphere, neutral cloud, and plasma torus, no conclusive evidence of silicates on Io has been obtained by reflectance spectroscopy, although Galileo SSI data indicate a 0.9-µm feature possibly due to Fe-Mg silicates (Geissler et al 1999).…”