Published online by Cambridge University Press: 01 May 2009
When such minerals as mica, pyroxene, nepheline, fluorite, and hematite are mentioned to us, we can hardly avoid associating their genesis with very high temperatures, and if amphibole be added we are equally bound to imagine also the existence of high pressure. So deeply rooted is this, I might almost say, superstition that few petrographers, when they find such minerals lining the fissures or cavities in rocks, fail to immediately conclude that great heat, and sometimes pressure, is indicated by such an occurrence. No doubt that in the vast majority of cases they would be right, yet I hope to show in these notes that such minerals have occasionally been produced under little or no pressure at a temperature so low as to be insufficient to carbonize or even discolour the organic matter of bone, that is at a temperature considerably below that of an ordinary baking oven.
page 309 note 1 Brit. Assoc. Rep. 1881, pp. 130–135; quoted by Prestwich, “Controverted Questions of Geology,” pp. 240–241.Google Scholar
page 310 note 1 See H. J. Johnston-Lavis: British Association Reports for 1888 –89–90–92, and Notes on Pipernoid Structure of Igneous Rocks, “Natural Science,” vol. iii, No. 19, September, 1893, pp. 218–221.Google Scholar
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