Abstract

We performed in situ infrared spectroscopic measurements of OH bands in a forsterite single crystal between −194 and 200 °C. The crystal was synthesized at 2 GPa from a cooling experiment performed between 1,400 and 1,275 °C at a rate of 1 °C per hour under high silica-activity conditions. Twenty-four individual bands were identified at low temperature. Three different groups can be distinguished: (1) Most of the OH bands between 3,300 and 3,650 cm−1 display a small frequency lowering (<4 cm−1) and a moderate broadening (<10 cm−1) as temperature is increased from −194 to 200 °C. The behaviour of these bands is compatible with weakly H-bonded OH groups associated with hydrogen substitution into silicon tetrahedra; (2) In the same frequency range, two bands at 3,617 and 3,566 cm−1 display a significantly anharmonic behaviour with stronger frequency lowering (42 and 27 cm−1 respectively) and broadening (~30 cm−1) with increasing temperature. It is tentatively proposed that the defects responsible for these OH bands correspond to H atoms in interstitial position; (3) In the frequency region between 3,300 and 3,000 cm−1, three broad bands are identified at 3,151, 3,178 and 3,217 cm−1, at −194 °C. They exhibit significant frequency increase (~20 cm−1) and broadening (~70 cm−1) with increasing temperature, indicating moderate H bonding. These bands are compatible with (2H)Mg defects. A survey of published spectra of forsterite samples synthesized above 5 GPa shows that about 75 % of the incorporated hydrogen belongs to type (1) OH bands associated with Si substitution and 25 % to the broad band at 3,566 cm−1 (type (2); 3,550 cm−1 at room temperature). The contribution of OH bands of type (3), associated to (2H)Mg defects, is negligible. Therefore, solubility of hydrogen in forsterite (and natural olivine compositions) cannot be described by a single solubility law, but by the combination of at least two laws, with different activation volumes and water fugacity exponents.

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