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Laboratory duplication of comb layering in the Rhum pluton

Published online by Cambridge University Press:  05 July 2018

Colin H. Donaldson*
Affiliation:
Department of Geology, University of St. Andrews, Scotland Lunar Science Institute, 3303 NASA Road 1, Houston, Texas 77058, USA

Summary

The changes in olivine morphology and grain size upwards through comb-layered olivine eucrite and peridotite varieties of harrisite in the Rhum layered pluton are systematic, from abundant small granular crystals, to fewer and larger hopper crystals, to highly elongate branching crystals, which are preferentially elongate along the a axis and perpendicular to the plane of the layering. These changes have been reproduced in the laboratory by cooling water-bearing melts (P = 5 kb) of harrisite at 14 and 30 °/hr. These cooling rates represent maximum values for natural crystallization of comb-layered harrisite. Other experiments suggest that the oriented branching olivines in the rock crystallized at 30–50 °C supercooling. The results indicate that continuous, rather than abrupt, changes in the degree of supercooling and supersaturation of the magma can cause formation of comb layers. They also indicate that while field relations point to growth of most comb layers along a thermal gradient in the magma, this is not an essential condition for comb layer formation. Growth could be along a compositional gradient instead. During crystallization of a comb layer, both nucleation rate and the number of crystals suspended in magma close to the layer are essentially zero. Conditions initiating and terminating comb layer formation and the origin of the rapid vectorial crystallization are discussed. It is suggested that some comb layers could form without change in degree of supercooling, due to rapid removal of crystals suspended in the magma causing the enhanced growth rate and branching style of growth of the remaining crystals. Multiple origins of comb-layered rocks may therefore be possible.

Type
Research Article
Copyright
Copyright © The Mineralogical Society of Great Britain and Ireland 1977

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Footnotes

1

Present address: Department of Geology, University of Manchester, Manchester MI3 9PL, England.

References

Bryhni, (I.) and Dons, (J. A.), 1975. Lithos, 8, 113.CrossRefGoogle Scholar
Chalmers, (B.), 1963. Principles of Solidification (New York).Google Scholar
Donaldson, (C. H.), 1974. Geol. Soc. Am. Bull. 85, 1721.2.0.CO;2>CrossRefGoogle Scholar
Donaldson, (C. H.), 1975a. A Petrogenetic Study of Harrisite in the Isle of Rhum Pluton, Scotland. (Unpubl. Ph.D. thesis, Univ. St. Andrews).Google Scholar
Donaldson, (C. H.), 1975b. J. Geol. 83, 33.CrossRefGoogle Scholar
Donaldson, (C. H.), 1976. Contrib. Mineral. Petrol. 57, 187.CrossRefGoogle Scholar
Doremus, (R. M.), 1973. Glass Science (New York).Google Scholar
Drever, (H. I.) and Johnston, (R. J.), 1972. Meteoritics, 7, 327.CrossRefGoogle Scholar
Duba, (A.), 1972. J. Geophys. Res. 77, 2483.CrossRefGoogle Scholar
Eitel, (W.), 1965. Silicate Science vol. III. Dry Silicate Systems (Academic Press).Google Scholar
Harker, (A.), 1908. The Geology of the Small Isles of Inverness-shire. (Mem. Geol. Surv., Scotland.)Google Scholar
Hess, (H. H.), 1939. Trans. Am. Geophys. Union, 3, 430.CrossRefGoogle Scholar
Jackson, (E. D.), 1971. Fortschr. Mineral. 48, 128.Google Scholar
Kirkpatrick, (R. J.), 1975. Am. Mineral. 60, 798.Google Scholar
Knight, (C. A.), 1967. The Freezing of Supercooled Liquids (van Nostrand).Google Scholar
Lofgrcn, (G. E.) and Donaldson, (C. H.), 1975. Contrib. Mineral. Petrol. 49, 309.CrossRefGoogle Scholar
Moore, (J. G.) and Lockwood, (J. F.), 1973. Geol. Soc. Am. Bull. 84, 1.2.0.CO;2>CrossRefGoogle Scholar
Mutanen, (T.), 1974. Bull. Geol. Soc. Finland, 46, 53.CrossRefGoogle Scholar
Platten, (I. M.) and Watterson, (J. S.), 1969. Nature, 223, 286.CrossRefGoogle Scholar
Shaw, (H. R.), 1972. Am. J. Sci. 272, 870.CrossRefGoogle Scholar
Taubeneck, (W. H.) and Poldervaart, (A.), 1960. Geol. Soc. Am. Bull. 71, 1395.CrossRefGoogle Scholar
Van Diver, (B. B.) and Magetti, (M.), 1973. Geol. Soc. Am. Annual Meet. Abstr. 7, 846.Google Scholar
Wadsworth, (W. J.), 1961. Philos. Trans. R. Soc. B244, 21.Google Scholar
Wager, (L. R.), 1968. In Basalts (eds. Hess, H. H. and Poldervaart, A.) (Interscience, N.Y.)Google Scholar
Wager, (L. R.) and Brown, (G. M.), 1951. Geol. Mag. 88, 166.CrossRefGoogle Scholar
Wager, (L. R.) and Brown, (G. M.), 1968. Layered Igneous Rocks (Oliver and Boyd).Google Scholar
Wager, (L. R.) and Brown, (G. M.), and Wadsworth, (W. J.), 1960. J. Petrol. 1, 73.CrossRefGoogle Scholar
Walton, (D.) and Chalmers, (B.), 1959. Trans. Metall. Soc. AIME, 215, 447.Google Scholar