Marine Micropaleontology, 15 (1990) 365-378 365
Elsevier Science Publishers B.V., Amsterdam -- Printed in The Netherlands
Significance of Devonian-Carboniferous Radiolarians
from Accretionary Terranes of the New England Orogen,
Eastern Australia
JONATHAN AITCHISON
Department of Geology and Geophysics, University of New England, Armidale, NSW 2351 (Australia)
(Received August, 1~88; revised and accepted March, 1989)
Abstract
Aitchison, J.C., 1990. Significance of Devonian-Carboniferous radiolarians from accretionary terranes of the New
England orogen, eastern Australia. Mar. Micropaleontol., 15: 365-378.
Radiolarians provide age constraints for many previously undated terranes in the New England Orogen (NEO), a
tectonic collage developed along the eastern margin of Australia.
Djungati terrane, the age range of which was previously unknown, contains two distinctive siliceous sedimentary
lithofacies. The oldest is a thick sequence of red, ribbon-bedded cherts which probably accumulated in a deep ocean-
floor setting far from land. Middle Silurian through Late Devonian radiolarians have been recovered from these cherts.
Green tuffaceous cherts which contain a latest Devonian (Famennian) radiolarian fauna depositionaUy overlie the
lower red ribbon-bedded chert sequence. These cherts are intercalated with volcaniclastic sediments and the fauna
which they contain can be used to constrain the timing of accretion of older rocks into a subduction complex.
Anaiwan terrane, which was also previously undated, contains thin ribbon-bedded cherts which are depositionally
overlain by tuffaceous chert, siliceous siltstones and volcaniclastic sediments. Latest Devonian (?late Famennian)
and Early Carboniferous radiolarians have been recovered from these cherts and tuffaceous siltstones.
Radiolarians also occur in fine-grainedsiliceous sediments of the Yarrimie Formation, part of the Gamilaroi terrane.
These radiolarians are of Late Devonian (Frasnian) affinity and their presence indicates that blocks of limestone,
which contain Givetian conodonts and corals and were previously thought to indicate the age of the Yarrimie For-
mation, are allochthonous.
Introduction
The geology of eastern Australia is domi-
nated by a tectonic collage of terranes known
locally as the New England Orogen (NEO). The
detailed geology of the NEO is not well known
due to structural complexity and poor expo-
sure. Recent detailed work has shown the oro-
gen to be a complex collage ofterranes (Fig. 1 )
which were accreted to the eastern margin of
Australia at various times during the late Pa-
leozoic (Flood and Aitchison, 1988a, b). Early
plate tectonic models for this portion of eastern
Australia assumed a relatively simple active
plate margin during the Paleozoic (Leitch, 1974,
1975; Cawood, 1983; Harrington and Korsch,
1985; Murray et al., 1987). However, previous
models for the tectonic development of the NEO
are inconsistent with the available data (Flood,
1988) and the interrelationships of many of the
terranes present are unknown. Although some
terranes are moderately fossiliferous (e.g.,
Gamilaroi terrane), macrofossils are generally
scarce and previous tectonic models have been
based on assumed ages. Recent radiolarian
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