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An experimental investigation of olivine morphology
Authors:Colin H Donaldson
Institution:(1) Department of Geology, University of St. Andrews, Scotland;(2) Lunar Science Institute, 3303 NASA Road 1, 77058 Houston, Texas, USA;(3) Present address: Department of Geology, University of Manchester, M13 9 PL Manchester, England
Abstract:Olivine crystals can adopt ten types of shape. Experimental crystallization of eight rock melts shows that there is a systematic change from polyhedral or granular olivines rarr hopper olivines rarr branching olivines rarr randomly oriented chain olivines rarr parallel-growth chain olivines rarr chain+lattice olivines rarr plate or feather olivines, with increase in cooling rate and with increase in degree of supercooling. This sequence involves changes from complete to progressively less complete crystals and from equant habit to elongate bladed habit (c>aGtb) to tabular habit (asimec Gt b). The sequence is not affected by the phase relations of the melt. The larger the olivine content of a melt the slower the cooling rate at which a particular olivine shape grows, whereas the lower the melt viscosity, the greater the cooling rate. Irrespective of the melt composition, comparable crystal shapes grow at the same degrees of supercooling. By comparison of the shapes of olivine crystals in experiments with those in rocks of similar composition, it is possible to deduce the cooling rate through the olivine crystallization interval and the approximate degree of supercooling at which the olivine crystals nucleated and grew in the rocks. The various shapes of skeletal olivines in many picrites, olivine-rich basalts and the Archaean ldquospinifexrdquo rocks are not due to rapid cooling, but to rapid olivine growth caused by the high normative olivine content of the magma.
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