T249 Rifting, Drifting, and Accretion of Microcontinental Terranes: A Recipe for Accretionary Orogens (Posters)
Tuesday, 29 October 2013
9:00 AM - 6:30 PM
Hall D
DOES THE MEGUMA TERRANE EXTEND INTO SOUTHERN BRITAIN?
Paper number: T249-1
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM
Authors
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R. NanceOhio University, Athens, OH
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James A. BraidSt. Francis Xavier University, Antigonish, NS
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Brendan MurphySt. Francis Xavier University, Antigonish, NS
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Nicolle DupuisSt. Francis Xavier University, Antigonish, NS
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Robin K. ShailSchool of Geography, Archaeology and Earth Resources, Penryn, N/A
Abstract
But while the unexposed basements of Avalonia and Meguma are thought to be isotopically similar, the Meguma sedimentary cover contains scarce Mesoproterozoic zircons. Hence, felsic magmas produced by crustal melting in the Meguma terrane (e.g. the ~370 Ma South Mountain Batholith) are isotopically more juvenile (εNd = -5 to -1, TDM = 1.3 Ga) than the rocks they intrude (εNd -12 to -7, TDM = 1.7 Ga) – a distinctive relationship also recognized for the Sierra Norte Batholith (~330 Ma; εNd = +1 to -3, TDM = 0.9–1.2 Ga) and its Late Devonian host rocks (εNd = –5 to –11) in southern Spain, where it has been used to suggest the possible presence of Meguma basement beneath the South Portuguese Zone. Available data for the Cornubian batholith of SW England (~270-290 Ma; εNd = -5 to -7, TDM = 1.3–1.8 Ga) and the Devonian metasediments it intrudes (εNd = –8 to –11) suggests this may also be true of that part of southern Britain (Rhenohercynian Zone) with which the South Portuguese Zone is traditionally correlated.