Ming Zhang1, S.Y. O'Reilly1 and J. Stephenson2
1. GEMOC, Macquarie
2. Dept of Earth Sciences, James Cook University
INTRODUCTION
Basaltic magmas in continental settings are commonly formed by decompression
partial melting of an upwelling mantle plume or asthenosphere rising to
the base of the subcontinental lithospheric mantle (SCLM). The magmas may
contain components contributed by partial melting of small degrees of some
enriched SCLM and primary magmas can also be modified on their way to the
surface by interaction with the lithospheric wall rocks. Therefore, primitive
continental basalts erupted through different crustal domains (or at different
times) can record geochemical signatures of mantle reservoirs (mantle plume,
asthenospheric mantle, and SCLM) and can trace the secular evolution of
the SCLM which, in general, ties in closely with the evolutionary history
of the crustal domains mapped at the surface.
Late Cenozoic basalts in North Queensland (8.0-0.01 Ma) constrain the
nature and evolutionary history of their mantle sources. The widespread
basaltic volcanism in North Queensland (NQld) covers an area of ca 23,000
km2 with a total volume of more than 650 km3 (Stephenson, 1989).
Six of the NQld lava-field basaltic provinces (Atherton, McBride, Chudleigh
and Nulla at Townsville?Cairns area and McLean and Piebald near Cooktown)
were chosen for this study. The McBride and Chudleigh basalts erupted
largely through the Mesoproterozoic Georgetown Inlier. The McLean, Piebald,
Atherton and Nulla Provinces are located in various blocks of the Phanerozoic
Tasman foldbelts. The term "Atherton-Nulla Provinces" refers to the
Atherton, McBride, Chudleigh and Nulla Provinces, and the term "Cooktown
Provinces" refers to the McLean and Piebald Provinces.
In this study, we use detailed geochemical data, including Sr-Nd-Pb
isotopic ratios, of these basalts to constrain their petrogenesis and the
nature of their mantle reservoirs and to provide new information on the
Phanerozoic tectonic evolution of the Tasman foldbelt in eastern Australia.
The new data, combined with previously published data for Cenozoic basalts
from eastern Australia (eg McDonough et al., 1985; Ewart et al., 1988;
O'Reilly and Zhang, 1995; Zhang et al., 1999), allow general isotopic characterisation
of mantle sources for the widespread intraplate basalts in eastern Australia
during Cenozoic times. These data also document the locus of both
Pacific-MORB and Indian-MORB mantle reservoirs beneath eastern Australia
for two time slices (at ca. 35 Ma and present day) and thus provide additional
constraints on the movement of the two global-scale mantle reservoirs with
time and its relationship with regional plate-tectonic geodynamics.
PETROLOGY AND ELEMENTAL GEOCHEMISTRY
The NQld basaltic rocks are dominantly (>90%) undersaturated alkaline
basalts, with less than 10% olivine tholeiites. The alkaline basalts range
from strongly undersaturated nephelinite (found only in the Cooktown provinces),
nepheline hawaiite and basanite to moderately undersaturated alkali olivine
basalt and hawaiites. More than 75% of the samples contain mantle
xenoliths, reflecting their primitive nature.
SiO2 contents for the NQld basalts range from 40.3 to 51.7 wt%, with
nephelinites ?42 wt% and ol-tholeiites >50 wt%. MgO contents range
from 12.8 to 4.3 wt% with Mg/(Mg+Fe2+) of 0.70-0.49 (mostly > 0.61).
The basalts from the Atherton-Nulla Provinces differ significantly from
the Cooktown nephelinites in their high Al2O3 and low TiO2 (1.5-2.4 wt%
vs >2.5 wt%) and CaO/Al2O3 (<0.7 vs 0.7-1.2).
Most incompatible trace elements do not correlate with Mg/(Mg+Fe2+)
for the NQld basalts. All the NQld basalts are LREE-enriched with
chondrite-normalised La/Yb of 6-41. The Cooktown nephelinites have much
higher contents (up to a factor of 3) of strongly incompatible elements
such as Cs, Th, U, Nb, and light rare earth elements (LREE) and marginally
higher Sr, Ba, Zr, and Hf contents than the Atherton-Nulla basalts.
The Pb contents of about 80% of the analysed samples fall in a narrow range
of 1.4-2.6 ppm. Some Cooktown nephelinites have Ce/Pb ratios much
higher (up to 57) than the range for oceanic basalts (25±5).
The normalised incompatible element patterns of the Cooktown nephelinites
are characterised by strong enrichment in Nb, Ta, Th, U and LREE and depletion
in K and Rb. In contrast, the Atherton-Nulla basanites generally
show a gradual increase in strongly incompatible element abundances from
Rb to Nb or Ta and a general decrease from Nb (or Ta) to Yb. Enrichments
in K relative to Nb and in Sr relative to Nd are common.
Sr-Nd-Pb ISOTOPIC SYSTEMATICS
87Sr/86Sr ratios for the NQld basalts range from 0.70340 to 0.70472
and 143Nd/144Nd ratios range from 0.51302 to 0.51279 (_Nd_=+7.5 ? +3.0).
Although the ranges of Sr and Nd isotopic ratios for the NQld basalts overlap
those for the New South Wales (NSW) basalts, the NQld basalts clearly differ
from the latter in their high 87Sr/86Sr at a given _Nd, thus forming a
distinct high 87Sr/86Sr trend. The most depleted NQld samples are
similar to the most enriched Indian MORB, whereas the most depleted NSW
samples plot close to the enriched end of the Pacific MORB field.
Pb isotopic ratios range in 206Pb/204Pb from 17.86 to 18.62, in 207Pb/204Pb
from 15.51 to 15.62, and in 208Pb/204Pb from 37.74 to 38.55 for the NQld
basalts, ubiquitously displaying a Dupal Pb isotopic signature with _8/4Pb
= +32 ? +63 and _7/4Pb = +3.3 ? +10.9 (Fig. 1; Hart, 1984). On the
other hand, the NSW basalts are high in 206Pb/204Pb (18.70-19.14) and many
of them have negative _7/4Pb and _8/4Pb values, similar to the Pacific
MORB compositions (Zhang et al., 1999). In contrast to the nearly vertical
trends shown by the NSW basalts on the 206Pb/204Pb vs 87Sr/86Sr and _Nd
diagrams, the NQld basalts show a positive correlation between 206Pb/204Pb
and 87Sr/86Sr (Fig. 2) and a negative correlation between 206Pb/204Pb and
_Nd.
DISCUSSION
Mantle Sources of the North Queensland basalts
The simplest explanation for the coherent Sr, Nd and Pb isotope variations
in the NQld basalts (Figs 1 and 2) involves a mixing of two mantle source
components. The depleted one has low 87Sr/86Sr and 206Pb/204Pb, and
high 143Nd/144Nd, similar to the enriched Indian MORB. The depleted
isotopic signature most likely simply reflects an Indian-MORB asthenospheric
mantle source that has been widely recognised from many young basalts from
the Western Pacific arcs and back-arc basins (eg Hergt and Hawkesworth,
1994).
The complementary enriched mantle source points to a component with
high 87Sr/86Sr, moderately low 143Nd/144Nd and high 206Pb/204Pb, characteristic
of an enriched (EM2) mantle component. Many of the Atherton-Nulla
basalts have Sr-Nd-Pb isotopic ratios similar to the Tonga-Kermadec Arc
basalts (eg Ewart et al., 1994 and refs therein). In addition, they
have generally high Rb/Sr, K/Nb, K/U, Sr/La and Zr/Nb ratios. The
high 87Sr/86Sr trend of the NQld basalts is consistent with derivation
from a lithospheric mantle wedge modified by subduction-related processes.
We propose that the EM2 mantle source recognised in the Atherton-Nulla
basalts may have been derived from an SCLM modified by percolation of subduction-related
metasomatic fluids during the late Paleozoic when this part of the Tasman
foldbelt (Hodgkinson and Broken River Provinces) was built up by orogenic
magmatism and crustal accretion. This is consistent with Ewart et
al.'s (1988) suggestion that subduction-modified SCLM has played a significant
role in the generation of some eastern Australian basalts.
The Sr-Nd isotopic ratios of spinel peridotite xenoliths from the Atherton-Nulla
provinces form an even higher 87Sr/86Sr trend, above the trend defined
by the host basalts. Although we do not think these xenoliths represent
the direct mantle source for the basalts (which should be located in the
garnet peridotite stability field), these data are compatible with the
presence of a subduction-modified SCLM in North Queensland. Seven
spinel lherzolite xenoliths from Atherton produce a Sm-Nd "isochron" age
of 264 Ma (R=0.9754) with _Nd(t) = +8. This "age" may be relevant
to the timing of metasomatism of a moderately refractory upper mantle wedge
associated with or shortly after the regional Permo-Carboniferous post-orogenic
magmatism.
However, the NQld basalts show a general negative correlation between
206Pb/204Pb and 238U/204Pb (µ). Basalts from Cooktown and McBride
provinces also display a negative correlation between__Nd and Sm/Nd.
The decoupling between the isotopic systems and relevant parent/daughter
elements requires recent metasomatism to produce high U/Pb and LREE/HREE
in the isotopically depleted mantle source or melts generated therefrom
(such as the Cooktown nephelinites). The age of this event should
be younger than 40 m.y. as constrained by the high µ values (up to
170) of the low-206Pb/204Pb nephelinites. The diagnostic incompatible
element signatures of the Cooktown nephelinites include: (1) fractionated
incompatible element patterns with strong depletion of Rb, and K and strong
enrichment of Th, U, Nb and Ta and (2) high U/Pb, Th/Pb, Ce/Pb and La/Yb
accompanied by low K/Nb, K/U, K/Ba, Rb/Sr and Zr/Nb. These trace
element signatures are similar to those of the plume-derived HIMU-type
OIBs though their Pb isotope ratios bear little resemblance to one another.
A model to explain the incompatible element signatures (O'Reilly &
Zhang, 1995) invokes interaction between ascending asthenosphere-derived
melts and amphibole- and apatite-bearing mantle wall-rock in the upper
part of SCLM. Apatite not only has low Rb/Sr and Sr/La and high U/Pb,
Th/Pb and Ce/Pb, but also dominates the budget for U, Th, LREE, and Sr
in mantle xenoliths. Nb contents are low in mantle apatite, but high
in mantle amphibole. Thus, addition of a small proportion of mantle
apatite and amphibole would produce the observed incompatible element signatures
in the Cooktown nephelinites. Tectonically, metasomatism which produced
apatite and amphibole in the upper mantle wall-rocks may be connected with
low-degree partial melting from the east-migrating Indian Ocean asthenosphere
which has a long residence beneath eastern Gondwana (Zhang et al., 1999).
Alternatively, this event can be linked to the early Tertiary SSW-directed
subduction of the Phoenix-Pacific Plate north of Papua New Guinea (Johnson
et al., 1978). The presence of a high-velocity zone beneath the NQld
at depths of 300-600 km (van der Hilst et al., 1997) may be explained as
the manifestation of the down-going plate. In either case, this amphibole-
and apatite-type metasomatism is likely to be a precursor of the Cooktown
magmatism.
Isotopic Characterisation of Mantle Sources for Eastern Australian Basalts
The present database for the Sr-Nd-Pb isotopes of the Australian basalts
allow us to make a generalised characterisation of the radiogenic isotopic
signatures of mantle sources in eastern Australia. Sun et al .'s
(1989) four-component dynamic model to explain the isotopic and incompatible
element systematics of the Australian central-volcano and lava-field basalts
provides baseline information. A first-order approximation to explain
the new data comprises several two-component mixing relationships, each
reflecting dynamic interactions between two mantle components that contribute
to magma generation (Figs 1 and 2). The two source components for
the late Cenozoic NQld basalts (< 6 Ma) are an Indian-MORB asthenosphere
and an EM2-type SCLM. On the other hand, the NSW lava-field basalts
(55-14 Ma) can be accounted for by mixing between a Pacific-MORB asthenosphere
and an SCLM component that is isotopically similar to the inferred SCLM
component in NQld.
Alkaline basalts from the Victorian Newer Basalts Province have both
incompatible element patterns and Sr-Nd-Pb isotopic compositions similar
to the primitive central-volcano basalts. Therefore the Australian mantle
plume presently beneath the Bass Strait may have contributed to these basalts.
The early Tertiary Tasmanian alkaline basalts reflect mixing between an
Pacific-MORB source and a HIMU component connected to a HIMU plume presently
located near the Balleny Islands, Antarctica (Lanyon et al., 1993).
In addition, the NSW leucitites and the Dubbo basanites may have tapped
an EM1-type mantle source, likely residing in the SCLM beneath the western
part of the Lachlan Foldbelt with possible Precambrian basement.
Pacific- and Indian-MORB Mantle in Eastern Australia
Sr-Nd-Pb isotopic data demonstrate the presence of an Indian-MORB source
component for the Cooktown Provinces and a more diluted Indian-MORB source
component for the Atherton-Nulla Provinces in North Queensland during the
last 8 Ma. In southeastern Australia, Pacific-MORB isotope signatures
characterise some of the early (55-14 Ma) lava-field basalts. This discovery
further constrains the secular distribution of major asthenospheric mantle
reservoirs represented by the Pacific and Indian MORB sources during and
following the breakup of eastern Gondwana. These data, together with
plate reconstruction positioning, track the locus of the boundary of the
two reservoirs beneath the Australian continent (Fig. 3; Zhang et al.,
1999) and fill the gap between previous boundary locations of the Indian-MORB
and Pacific-MORB mantle sources in the region constrained from back-arc
basin basalts in the southwestern Pacific Ocean (eg Hergt and Hawkesworth,
1994).and ocean floor basalts in the Southern Ocean (eg Pyle et al., 1995).
We conclude that the Indian MORB source is a long-term asthenospheric reservoir
beneath most of eastern Gondwana continent and that the westward migration
of the Pacific MORB source may have been associated with the opening of
the Tasman Sea (at ca. 85-60 Ma) along a broad front southeast of the Australian
continent.
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Fig. 1 206Pb/204Pb vs 208Pb/204Pb diagram for lava-field basalts
from eastern Australia. NHRL, the Northern Hemisphere Reference Line from
Hart (1984).
Fig. 2 206Pb/204Pb vs 87Sr/86Sr diagram for lava-field basalts from eastern Australia.
Fig. 3 Distribution of Australian basalts with Pacific MORB and
Indian MORB geochemical signatures at two time slices, 35 Ma (fainter broad
lines) and 5 Ma (heavy lines) on palinspastic reconstructions. Faint and
heavy dashed lines represent inferred boundary between Indian MORB and
Pacific MORB-type basalts at 35 Ma and 0 Ma, respectively.