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Nd and Sr isotopic systematics of central Australian granulites: chronology of crustal development and constraints on the evolution of lower continental crust

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TLDR
In this paper, the authors reported the results of an isotopic analysis of granulite terrains in the Proterozoic Arunta Block of Central Australia, showing that the terrain cooled slowly, did not experience significant uplift until ∼ 1,000 Ma and remained at temperatures above 320°C until the late Palaeozoic.
Abstract
Nd and Sr isotopic data are reported for a granulite terrain in the Proterozoic Arunta Block of Central Australia. Sm-Nd data from a wide range of rock types define a crust formation age of 2,070±125 Ma and provide further evidence for voluminous crustal growth in the Proterozoic. An ɛ Nd value of +1.5±0.8 indicates a depleted mantle source for this crustal segment and there is no evidence for a large component of significantly older sialic crust. Field relationships, geochemistry and Rb-Sr data for mafic and felsic granulites indicate that intracrustal differentiation and polyphase deformation were followed by granulite facies metamorphism (Rb depletion) at ∼1,800 Ma. Rb-Sr data for strongly retrogressed granulites define an age of ∼1,700 Ma which is interpreted as the time of retrograde biotite growth. Partial melting at the presently exposed crustal level and anatexis at deeper crustal levels were broadly coeval with the retrograde metamorphism. Sm-Nd and Rb-Sr isotopic systematics of minerals indicate that the terrain cooled slowly, did not experience significant uplift until ∼1,000 Ma and remained at temperatures above 320° C until the late Palaeozoic. The mineral data are consistent with geological relationships and petrological evidence for a prolonged period of isobaric cooling followed by uplift late in the metamorphic evolution of the terrain. The granulite protoliths appear to have formed in a rift which closed within ∼280 Ma of initial separation. Deformation and granulite facies metamorphism at ∼1,800 Ma are interpreted to be a consequence of collision between the continental blocks which defined the rift. Regional retrogression and granitoid magmatism at ∼1,700 Ma are attributed to underthrusting of the granulites by lower grade rocks in the final stages of collision. Subsequent events in the cooling and uplift history appear to have been controlled by the presence of long-lived major faults in the crust and a prolonged history of episodic compression in the continental lithosphere. The results of this study suggest that granulite terrains, in general, cannot be equated with lower continental crust but instead represent assemblages of (mainly) supracrustal rocks which in some instances have been involved in major collision events.

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Citations
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An extended episode of early Mesoproterozoic metamorphic fluid flow in the Reynolds Range, central Australia*

TL;DR: The products of metamorphic fluid flow are preserved in zones within the marbles and metamorphosed semipelites of the Upper Calcsilicate Unit in the granulite portion of the Late Palaeoproterozoic Reynolds Range Group, northern Arunta Block, central Australia.
Journal ArticleDOI

Crustal growth in West Africa at 2.1 Ga

TL;DR: The most precise zircon U-Pb and Sm-Nd data for the more widespread Birimian terranes (sensu stricto), from this study and from the literature, cluster between 2.12 and 2.07 Ga.
Journal ArticleDOI

Tectonic evolution of Proterozoic Australia

John S. Myers, +2 more
- 01 Dec 1996 - 
TL;DR: This article proposed an alternative hypothesis in which numerous fragments of continental crust were assembled by plate tectonic processes, and the assembly was completed between 1300 and 1100 Ma when the crustal fragments were combined as an early component of the Rodinian supercontinent.

The Mean Age of Mantle and Crustal Reservoirs for the Planet Mars

S. B. Jacobsen, +1 more
TL;DR: Based on all available isotopic and trace element data for SNCs, the authors obtained a mean age of formation of the crust on Mars of 34 +/- 6 Ga, which is the same as the age of the Earth's crust.
Journal ArticleDOI

The persistent myth of crustal growth

TL;DR: From the extraterrestrial telescopic, space probe, meteorite and returned sample studies of planetary evolution, and terrestrial evidence for early differentiation of core and fluid spheres and continental crust, the authors feel the conclusion is inescapable that large terrestrial planets of our solar system underwent essentially immediate differentiation into relatively constant volume core, depleted mantle, enriched crust and fluid reservoirs.
References
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Journal ArticleDOI

Closure temperature in cooling geochronological and petrological systems

TL;DR: In this paper, a good approximation is obtained by relating τ to the slope of the cooling curve at the closure temperature of a geochronological system, which is defined as its temperature at the time corresponding to its apparent age.
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Sm-Nd isotopic evolution of chondrites

TL;DR: In this paper, it was shown that none of the analyzed meteorite samples deviated more than 0.5 e-units from a 4.6-AE reference isochron and defined an initial 4.5-AE value for CHUR using the Juvinas data of Lugmair.
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Neodymium isotopes in the Colorado Front Range and crust–mantle evolution in the Proterozoic

TL;DR: In this article, an empirical model is constructed that may provide accurate crust-formation ages f or rocks of all ages, based on the isotopic data of major rock types of the basement underlying the Rocky Mountains in Colorado.
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Nd isotopic variations and petrogenetic models

TL;DR: In this article, the authors analyzed the geochemical properties of a chondritic reservoir with high Fe, high Fe basalt, Ti basalt and alkali basalts and compared the results with the present value of the source regions of the earth.
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Precise determination of SmNd ratios, Sm and Nd isotopic abundances in standard solutions☆

TL;DR: In this article, the methods used for precise calibrations of Sm/Nd ratios and the average isotopic abundances obtained for normal Sm and Nd are given, and a mixed Sm-Nd normal solution with a precisely known Sm/nd ratio close to the nominal average chondritic value is described and the calibration discussed.
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