Geochemical investigations of microgranitoid enclaves in the S-type Cowra Granodiorite, Lachlan Fold Belt, SE Australia

Citation
Te. Waight et al., Geochemical investigations of microgranitoid enclaves in the S-type Cowra Granodiorite, Lachlan Fold Belt, SE Australia, LITHOS, 56(2-3), 2001, pp. 165-186
Citations number
98
Categorie Soggetti
Earth Sciences
Journal title
LITHOS
ISSN journal
00244937 → ACNP
Volume
56
Issue
2-3
Year of publication
2001
Pages
165 - 186
Database
ISI
SICI code
0024-4937(200103)56:2-3<165:GIOMEI>2.0.ZU;2-L
Abstract
The Cowra Granodiorite is a relatively mafic, enclave-rich, S-type pluton i n the Lachlan Fold Belt, which has been cited as a type example of a restit ic origin for all varieties of enclaves in Lachlan Fold Belt S-type granite s. Microgranitoid enclaves from the pluton are subordinate to metasedimenta ry Varieties and can be subdivided into two groups according to their mafic mineral assemblage: pyroxene microtonalites and biotite microgranites. No geochemical or isotopic distinction can be made between the two varieties. Petrographic evidence (acicular apatites, xenocrysts from the host granite) suggests an origin as mingled, mon mafic, magmas, which have been variably contaminated by the more felsic host magma. This is supported by the fact that the microgranitoid enclaves have isotopic compositions (Sr-87/Sr-86((i )) = 0.7095 to 0.7144, epsilon (Nd(i)) = - 9.2 to - 6.9) that are generally more primitive than, or similar to, those of the host granite (Sr-87/Sr-86 ((i)) = 0.7142, epsilon (ND(i)) = -8.8). The spread in isotopic composition s, like their trace element compositions, is considered to be the consequen ce of variable degrees of diffusive exchange between the felsic and more ma fic magmas during slow cooling. Several studied metasedimentary enclaves ar e not in isotopic equilibrium with their host granite and therefore cannot represent pristine samples of the hulk source region of the granite. Instea d, they represent portions of a lithologically and compositionally diverse source terrane or accidental xenoliths entrapped during emplacement. (C) 20 01 Elsevier Science B.V. All rights reserved.