Lithos, 23 (1989) 63-83 63
Elsevier Science Publishers B.V., Amsterdam -- Printed in The Netherlands
The Wuluma granite, Arunta Block, central Australia: An
example of in situ, near-isochemical granite formation in a
granulite-facies terrane
W.J. COLLINS ~, R.H. FLOOD 2, R.H. VERNON 2 and S.E. SHAW2
~ Department of Geology, The University of Newcastle, Newcastle, N.S. IV.. 2308 (Australia)
2School of Earth Sciences, Macquarie University, Sydney, N.S. 141.. 2109 (Australia)
LITHOS
Collins, W.J., Flood, R.H., Vernon, R.H. and Shaw, S.E., 1989. The Wuluma granite, Arunta Block, cen-
tral Australia: An example of in situ, near-isochemical granite formation in a granulite-facies terrane.
In: R. Gorbatschev (Editor), Proterozoic Geochemistry. Lithos, 23: 63-83.
The Wuluma granite is a small, elongate, relatively undeformed pluton in the Proterozoic Strangways
Metamorphic Complex, central Australia. The complex constitutes a supracrustal assemblage that under-
went granulite-facies metamorphism 1800 Ma ago. Metamorphism was associated with at least three phases
of folding that ultimately produced upright, regional, doubly plunging F3 folds and isobaric cooling en-
sued. Generation of the Wuluma granite occurred at ~ 1750 Ma, based on Rb-Sr isotopic data, during
syn-D3 regional retrogression and rehydration of the terrane.
Contacts between the granite and gneisses are invariably gradational. At the pluton margin, banded
gneisses grade along strike into granite containing abundant biotite schlieren that parallel regional struc-
tures. Granite and pegmatite dykes cut these rocks. Inwards from the contact, the granite is more homo-
geneous, containing diffuse parallel schlieren and small aligned rectangular feldspar crystals, indicating
flow of magma. Rafts of unmelted granofels form a ghost layering; they mimic macroscopic F3 folds and
show only minor retrogressive metamorphic effects. At the pluton core, the granite is homogeneous and
structurally isotropic, containing some subrounded granofelsic inclusions, very diffuse schlieren and dis-
aggregated pegrnatite dykes. Thus, it appears that an isoclinallyfolded, vertical body ofquartzofeldspathic
gneiss was melted "in situ" to form the pluton, which did not break away from the source. The body
resembles a tapered diapir and we term this type of pluton a regional migmatite terrane granite.
Geochemical data are consistent with the granite forming by anatexis of quartzofeldspathic migmatitic
gneisses with appropriate composition. The chemical similarity of both rock types implies derivation of
the granite by either partial melting and retention of residual material in the magma or more complete
melting, followed by solidification virtually in situ. The latter interpretation is preferred, although biotite
melanosome has been incorporated into the magmas. Migmatitic gneisses, with feldspar proportions cor-
responding to ternary minima compositions, are argued to have melted during influx of an externally
derived aqueous fluid associated with pegmatites. Field evidence shows that slightly different gneisses
melted to produce slightly different granite compositions, even on outcrop scale; the compositions of
migmatites and derivative granite both range from 67% to 77% SIO2. Therefore, crystal fractionation did
not produce the geochemical variation. Rather, in situ crystallization of the granite resulted in a compo-
sition near-isochemical to that of the precursors, but with a coarser, obviously granitic texture.
(Accepted February 10, 1989)
Introduction
Experimental studies have shown that granitic
magmas can be derived from a wide range of crustal
rock types (e.g., Tuttle and Bowen, 1958; Green,
1976; Clemens and Wall, 1981). Commonly the
process envisaged involves the granite magma being
formed by 20-30% partial melting; in these in-
stances the composition of the source rock is far re-
moved from the derived granitic melt and is diffi-
cult to infer, unless substantial assumptions are
made about the relationship between the granite
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