Abstract
Silicate minerals are the commonest accessible materials on Earth. Thanks to the strong affinity of silicon for oxygen and the low density of the resulting oxides (3 g/cm3) compared with the average global density (5.5 g/cm3). Well over 90% of the crust is made up of silicates. Other elements are concentrated in the upper layers of the Earth when they form particularly stable simple oxides or complex oxides with Si02, and just eight elements together account for nearly 99% of the crustal mass. After oxygen and silicon itself come aluminum, iron, and four alkali or alkaline earth elements. Aluminosilicates are therefore the principal terrestrial minerals. Iron is believed from the evidence of meteoritic and stellar abundances, and the Earth’s density profile, to be the most abundant element in the whole Earth (35 wt. %), but it represents only 5% of the mass, and the less than 2% of the atoms in the crust. No other useful Mössbauer element is sufficiently plentiful for it to appear as a significant constituent of common natural minerals (e.g., Sn 2 ppm; Sb 0.2 ppm; Dy 3 ppm). The striking fact that 94% of the crust, by volume, is made of oxygen reflects the large ionic radius of O2−, 1.40 Å, and the elementary principle of crystal chemistry that the structures of oxides, silicates included, are basically closely packed arrays of oxygen anions with small metallic cations in the interstices. Figure 1 summarizes the composition of the crust by mass, number of atoms, and volume, thereby situating in a global context the subject matter of this chapter—silicate minerals containing iron along with varying amounts of other major elements.
Round and round the rugged rocks The ragged rascals ran.
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Coey, J.M.D. (1984). Mössbauer Spectroscopy of Silicate Minerals. In: Long, G.J. (eds) Mössbauer Spectroscopy Applied to Inorganic Chemistry. Modern Inorganic Chemistry, vol 1. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-0462-1_14
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