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Estimation of the depth of origin of basic magmas: A modified thermodynamic approach and a comparison with experimental melting studies
Authors:Donald J DePaolo
Institution:(1) Department of Earth and Space Sciences, University of California, 90024 Los Angeles, California, USA
Abstract:Thermodynamic calculations, modified after Nicholls et al. (1971), which relate the activity of silica in a lava to the temperature and pressure conditions at which the lava could be in equilibrium with a mantle mineral assemblage, have been extended to H2O-bearing magmas by using published experimental data to derive the dependence of 
$$a_{{\text{SiO}}_{\text{2}} }$$
on the weight fraction of H2O dissolved in a magma. A petrogenetic grid has been calculated which gives the P-T conditions under which a magma with a given 
$$a_{{\text{SiO}}_{\text{2}} }$$
at its liquidus at 1 atm could equilibrate with a mantle mineral assemblage containing olivine (ol) and orthopyroxene (opx) for different amounts of H2O in the magma at its source. This grid is in good agreement with the results of experimental studies as summarized by Green (1971) and Brey and Green (1975). The results show that the pressure at which a given magma composition can equilibrate with ol + opx increases for increasing amounts of H2O dissolved in the magma at depth.In addition, experimental data have been used to calculate the effect of olivine crystallization and removal on the 
$$a_{{\text{SiO}}_{\text{2}} }$$
in the residual liquid to assess the effect of low-pressure differentiation on 
$$a_{{\text{SiO}}_{\text{2}} }$$
. The results show that if 20 % olivine is added to a basalt magma, its calculated pressure of equilibration with ol+opx increases by sim4–5 kbar for a given temperature. The calculated effects of olivine removal and H2O addition on 
$$a_{{\text{SiO}}_{\text{2}} }$$
are reasonably consistent with the silicate mixing model of Burnham (1975).Thermodynamic calculations of this type may be useful for assessing the internal consistency of certain experimental data, and in extrapolating the results to other magma compositions. The application of these calculations to determining the possible depth of origin of natural lavas appears to be limited primarily by the difficulty in determining 
$$_{{\text{SiO}}_{\text{2}} }$$
in a lava at its liquidus temperature.
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