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Almandine garnet phenocrysts in a ~1 Ga rhyolitic tuff from central India

Published online by Cambridge University Press:  13 June 2008

SARBANI PATRANABIS-DEB ,
JUERGEN SCHIEBER  and
ABHIJIT BASU
SARBANI PATRANABIS-DEB
Affiliation:
Indian Statistical Institute, Kolkata 700108, India
JUERGEN SCHIEBER
Affiliation:
Department of Geological Sciences, Indiana University, Bloomington, IN 47405, USA
ABHIJIT BASU*
Affiliation:
Department of Geological Sciences, Indiana University, Bloomington, IN 47405, USA
*
‡Author for correspondence: basu@indiana.edu
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Abstract

We report on the newly discovered almandine garnet phenocrysts in rhyolitic ignimbrites (Sukhda Tuff) in the Precambrian Churtela Shale Formation of the Chhattisgarh Supergroup in central India. SHRIMP ages of igneous zircon from the ignimbrites range from 990 Ma to 1020 Ma. These ignimbrites exhibit characteristic eutaxitic texture with compacted curvilinear glass shards with triple junctions. Quartz (commonly embayed; bluish cathodoluminescence) and albite (altered but retaining ghosts of twinning) are common phenocrysts; others are apatite, ilmenite, rutile, magnetite, zircon, monazite and garnet. There are no metamorphic or granitic xenoliths in the ignimbrites. Garnet grains occur as isolated broken isotropic crystals with sharp or corroded boundaries in a very fine-grained groundmass of volcanic ash that consists principally of albite, quartz, magnetite and glass. They do not have any systematically distributed inclusions. A few have penetratively intergrown phenocrysts of apatite, ilmenite, rutile and zircon, which we interpret as subophitic texture. Extensive SEM-BSE imaging of more than 100 grains and electron microprobe traverses across about 30 grains showed no zoning or systematic compositional variability. Common (metamorphic) garnets are usually zoned with respect to Fe–Mg–Mn and typically have mineral inclusions. We infer, therefore, that these observed garnets are not metamorphic xenocrysts. The average major oxide composition of analysed garnets from five different horizons within the Sukhda Tuff, spanning approximately 300 m of the stratigraphic section, have very small standard deviation for each element, which is suggestive of a single magmatic source. Phenocrysts of quartz, including those in contact with coexisting garnets, show blue scanning electron CL, indicating rapid cooling from high temperature; this suggests that adjacent coexisting garnets are not slowly cooled restites. We conclude, on the basis of texture, mineral chemistry and absence of any indicative xenoliths or xenocrysts, that these almandine garnets (Al78.7Py12.3Gr7.4Sp1.6) are phenocrysts within the Sukhda Tuff. Almandine of such composition is stable under high pressure. We infer that almandine crystallized at lower crustal depths in a magma that ascended very rapidly and may have erupted explosively.

Keywords

ignimbritephenocrystalmandinerhyolitic tuffProterozoicIndiagarnet
Type
Original Article
Information
Geological Magazine , Volume 146 , Issue 1 , January 2009 , pp. 133 - 143
Copyright
Copyright © Cambridge University Press 2008

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