GSA Connects 2022 meeting in Denver, Colorado

Paper No. 223-12
Presentation Time: 11:00 AM

CAMBRIAN A-TYPE GRANITES IN PRYDZ BAY, EAST ANTARCTICA: SR-ND-HF-PB-O ISOTOPIC CONSTRAINTS ON MAGMA SOURCES AND THE ORIGIN OF HIGH CONCENTRATIONS OF HEAT-PRODUCING ELEMENTS


MAAS, Roland1, GREW, Edward2, CHRISTY, Andrew3, YATES, Martin2, CARSON, Christopher4, BODORKOS, Simon4 and BOGER, Steven1, (1)School of Geography, Earth and Atmospheric Sciences, University of Melbourne, Parkville, VIC 3010, Australia, (2)School of Earth and Climate Sciences, University of Maine, Orono, ME 04469, (3)Christy Mineralogical Consulting, PO Box 517, Hamilton, QLD 4007, Australia, (4)Geosciences Australia, PO Box 378, Canberra, ACT 2601, Australia

Cambrian (519-494 Ma) syn- to post-kinematic granites intrude polymetamorphic granulite-facies gneisses for 170 km along Prydz Bay. The granites range from fine-grained, foliated biotitic veins (<1 m) in the northeast to km-scale unfoliated biotite-hornblende plutons with K-feldspar phenocrysts in the southwest. Accessories include garnet and monazite in the NE; allanite, titanite, chevkinite-perrierite and fayalite in the SW; and fluorite in both. Whole-rock compositions have features reported in A-type granites, e.g., high Fe, Na+K, K/Na, F, HFSE (322-1625 ppm Zr), LREE (107-2101 ppm Ce) and Th (up to 878 ppm Th; Th/U = 28-142). The ratios La/LuN (85-976) and Sr/Y (up to 45) are higher toward the NE than in the SW (respectively 10 to 85; <10). High La/LuN ratios in the NE are associated with higher initial 87Sr/86Sr = 0.716-0.756 and lower εNd = −11.4 to −13.1), while the inverse applies in the SW, where 87Sr/86Sr = 0.7095-0.7300 and εNd = −7.7 to −11.0. Initial εHf (−6.8 to −13.8) correlates strongly with εNd. The Hf-Nd isotopic data plot slightly above the global crustal Hf-Nd array. Magma δ18O values, estimated from quartz δ18O, range narrowly (8.5 to 9.8‰) except for an intrusion with 87Sr/86Sr ≈ 0.752 and δ18O = 11-11.4‰. Initial Pb isotope compositions from leached feldspars are characterized by high 207Pb/204Pb (15.71-15.77) and low 206Pb/204Pb (17.7-18.16), a signature requiring Pb isotope evolution in an old, high-U/Pb reservoir (≥ 2 Ga), followed by a low-U/Pb (µ<<10) stage for several 100 Ma prior to granite formation. Lowering of U/Pb (avg. 3.6 ppm U) may be related to U removal from older crustal protoliths at ca. 1 Ga during the first of two granulite facies events in Prydz Bay gneisses; the second event at ca. 0.5 Ga had much less impact. By contrast, initial 208Pb/204Pb (ca. 38.6) points to magma sources in early Paleozoic continental crust with typical Th/Pb (ω≈40-50). Pb isotope signatures thus indicate magma sources in Proterozoic rocks with low U and near-average Th concentrations. The high Th concentrations (avg. 172 ppm), which dominate the high heat production of the Cambrian granites (Carson et al. 2014, J Geol Soc London 171, 9-12), thus appear to result from the magmatic processes generating the A-type granites rather than from Th-rich source rocks.