The Permian Cornubian granite batholith, SW England; Part 1: Field, structural, and petrological constraints
Author:
Searle Michael P.123ORCID, Shail Robin K.1, Pownall Jonathan M.34, Jurkowski Christopher3, Watts Anthony B.3, Robb Laurence J.3
Affiliation:
1. 1Camborne School of Mines, Department of Earth and Environmental Science, University of Exeter (Penryn campus), Penryn, Cornwall TR10 9FE, UK 2. 2Oxford University Museum of Natural History, Parks Road, Oxford OX1 3PW, UK 3. 3Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, UK 4. 4Department of Geosciences and Geography, University of Helsinki, Gustaf Hällströmin katu, 00014 Helsinki, Finland
Abstract
Abstract
The Permian Cornubian granite batholith (295–275 Ma) in SW England includes seven major plutons and numerous smaller stocks extending for ~250 km from the Isles of Scilly in the WSW to Dartmoor in the ENE. The granites are peraluminous and classified as crustal melt S-type, predominantly two-mica granites, and biotite or tourmaline monzo- and syenogranites, with subordinate minor topaz granite and lithium mica granite. The granites and their host rocks are pervasively mineralized with tin (cassiterite), tungsten (wolframite, ferberite), copper (chalcopyrite, chalcocite, bornite), arsenic (arsenopyrite), and zinc (sphalerite) mineralized lodes. Quartz-muscovite selvedges (greisen-bordered) also contain enrichment of lithophile elements such as boron (tourmaline), fluorine (fluorite), and lithium (lithium-micas such as lepidolite and zinnwaldite). They are derived from both muscovite and biotite dehydration melting of pelitic-psammitic rocks and intruded from a common source along the length of the batholith. Pressure estimates from andalusite and cordierite-bearing hornfels in the contact metamorphic aureole (150 ± 100 MPa) show that the granites intruded to 3 km depth. Cupolas around the Land's End and Tregonning granites show aplite-pegmatite dikes and tourmaline + quartz + muscovite veins (greisen) that are frequently mineralized. Synchronous intrusions of lamprophyre dikes suggest an additional heat source for crustal melting may have been from underplating of alkaline magmas. The lack of significant erosion means that the source region is not exposed. In an accompanying paper (Part 2; Watts et al., 2024), gravity modeling reveals possible solutions for the shape and depth of the granite and the structure of the lower crust. We present a new model for the Land's End, Tregonning, and Carnmenellis granites showing a mid-crustal source composed of amphibolite facies migmatites bounded by prominent seismic reflectors, with upward expanding dikes feeding inter-connected granite laccoliths that show inflated cupolas with shallow contact metamorphism. The Cornubian granites intruded >90 m.y. after obduction of the Lizard ophiolite complex, and after Upper Devonian–Carboniferous Variscan compressional, and later extensional, deformation of the surrounding Devonian country rocks. Comparisons are made between the Cornubian batholith and the Patagonian batholith in Chile, the Himalayan leucogranites, and the Baltoro granite batholith along the Karakoram range in northern Pakistan.
Publisher
Geological Society of America
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