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dc.contributor.authorSearle, MP
dc.contributor.authorShail, RK
dc.contributor.authorPownall, JM
dc.contributor.authorJurkowski, C
dc.contributor.authorWatts, AB
dc.contributor.authorRobb, LJ
dc.date.accessioned2024-04-09T10:57:04Z
dc.date.issued2024-04-04
dc.date.updated2024-04-08T22:44:20Z
dc.description.abstractThe 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.en_GB
dc.identifier.citationPublished online 4 April 2024en_GB
dc.identifier.doihttps://doi.org/10.1130/b37457.1
dc.identifier.urihttp://hdl.handle.net/10871/135710
dc.identifierORCID: 0000-0001-7200-5124 (Shail, Robin K)
dc.language.isoenen_GB
dc.publisherGeological Society of Americaen_GB
dc.rights© 2024 Geological Society of America. This version is made available under the CC-BY 4.0 license: https://creativecommons.org/licenses/by/4.0/  en_GB
dc.titleThe Permian Cornubian granite batholith, SW England; Part 1: Field, structural, and petrological constraintsen_GB
dc.typeArticleen_GB
dc.date.available2024-04-09T10:57:04Z
dc.identifier.issn0016-7606
dc.descriptionThis is the author accepted manuscript. The final version is available from the Geological Society of America via the DOI in this recorden_GB
dc.identifier.eissn1943-2674
dc.identifier.journalGSA Bulletinen_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2024-02-26
rioxxterms.versionAMen_GB
rioxxterms.licenseref.startdate2024-04-04
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2024-04-09T10:52:02Z
refterms.versionFCDAM
refterms.dateFOA2024-04-09T10:57:11Z
refterms.panelCen_GB
refterms.dateFirstOnline2024-04-04


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© 2024 Geological Society of America. This version is made available under the CC-BY 4.0 license: https://creativecommons.org/licenses/by/4.0/  
Except where otherwise noted, this item's licence is described as © 2024 Geological Society of America. This version is made available under the CC-BY 4.0 license: https://creativecommons.org/licenses/by/4.0/