Geochemistry and Petrogenesis of Basaltic Rocks from North
Queensland: Has Subduction-Modified Mantle Played a Role?
Ming Zhang1, Jon Stephenson2, Suzanne Y O'Reilly1, Marc Norman1, Malcolm T McCulloch3
1, GEMOC, Macquarie University, Sydney, NSW 2109, Australia;
2, Dept of Earth Sciences, James Cook University, Townsville,
Qld 4811, Australia; 3, Research School of Earth Sciences, Australian
National University, Canberra, ACT 0200, Australia
INTRODUCTION
Cenozoic basaltic volcanism is widespread in North Queensland
(NQld) as a part of the eastern Australian volcanic zone. Basaltic
rocks from 7 volcanic provinces, including Atherton, McBride,
Chudleigh, Nulla and Mingela at Townsville-Cairns area and McLean
and Piebald near Cooktown, were chosen for this study. The basalts
are located cross the major tectonic boundaries between the Mesoproterozoic
Georgetown Inlier and the Phanerozoic Hodgkinson and Thomson fold
belts. The McBride Province is located mostly inside the Georgetown
Inlier, whereas the Mingela, Atherton, and Cooktown Provinces
are in the Phanerozoic fold belts. The Chudleigh and Nulla volcanoes
straddle the tectonic boundary. Most of the basalts occurring
as volcanic cones and long lava flows were erupted during a period
of 8.0-0.01 Ma, with an exception of the early Tertiary (44-31
Ma) plugs and dykes at Mingela (Stephenson, 1989). All these
basaltic provinces are recognised as lava field provinces.
Their age distribution does not show any relationship with the
northward motion of the Indo-Australian plate over a mantle plume
that resulted in the central volcano volcanism in eastern
Australia during at least the last 35 Ma. In the following text,
the term "Cairns" is used for Atherton, McBride, Chudleigh
and Nulla Provinces, and "Cooktown" for McLean and Piebald.
PETROLOGY AND GEOCHEMISTRY
Sixty-one basalt samples from North Queensland were analysed for
major (by XRF) and 40 trace elements (by XRF and ICPMS); up to
41 of them were also analysed for Sr-Nd-Pb isotopes (Pb isotope
data not available for Chudleigh and Mingela Provinces). Based
on a CIPW-norm classification (O'Reilly & Zhang, 1995), 57
samples are alkaline basalts, ranging from nephelinite (5%) and
basanite (16%) to alkali olivine basalt (5%) and hawaiite (67%),
and the rest are olivine tholeiite (7%). Mg numbers (Mg#=Mg/Mg+Fe2+)
range 0.70-0.49, with an average of 0.64 (MgO=12.8-4.3 wt%), and
average Ni content is 185 ppm (±60 ppm). The majority of
these basaltic rocks (including some hawaiites) contain abundant
mantle xenoliths and high-pressure megacrysts, indicating their
primitive or near-primitive nature.
Major and trace elements: In general, basalts from
Cairns area and Mingela are higher in SiO2, Al2O3, but lower in
TiO2, Sc, Y, Nb and La at a given Mg# than the lava field basalts
from New South Wales (NSW) and the Victorian Newer Basalts in
eastern Australia (Table 1). They also have CaO/Al2O3 (0.56±0.08)
lower than the NSW basaltic rocks (0.69±0.12), but similar
to the Newer Basalts (0.57±0.11). In contrast, the Cooktown
basalts are similar to many strongly alkaline basalts in NSW in
their SiO2, Al2O3 and TiO2 contents, but have higher CaO/Al2O3
(0.82±0.20) than the later. Y abundances of the Cooktown
samples are within the lower range for the NSW and Victorian basalts,
but marginally higher than the other NQld basalts, whereas Nb,
Th and LREE abundances are among the highest of all the basaltic
rocks discussed here. No well-defined correlations between Mg#
and minor and most incompatible trace elements are present for
the NQld basalts.
Incompatible element patterns: The primitive NQld
basalts exhibit three different types of incompatible element
patterns (Fig. 1). The majority of basalts from Cairns area are
moderately silica-undersaturated (eg alkali olivine basalts and
hawaiites). They display identical incompatible element patterns
with slight to moderate enrichments in K, Sr and P over Nb, Ta,
La, Zr and Hf, reflecting a lesser degree of enrichments in both
HFSE and LREE. On the other hand, strongly alkaline basalts (eg
lc-normative nephelinites), the predominant rock type in
Cooktown area and the subordinate in Cairns, show fractionated
incompatible element patterns similar to many NSW nephelinites,
basanites, and ne-hawaiites (eg Barrington, Kandos, and some from
Southern Highlands, Monaro and Dubbo; O'Reilly & Zhang, 1995),
with strong enrichments in Nb, Ta and LREE and relative depletions
to variable degree in Rb, K, Zr, Hf, and Ti. One moderately evolved
hawaiite and one ol-tholeiite from Cooktown are similar to the
majority of the Cairns basalts. The relative K-depletion in the
Cooktown basalts becomes more significant (ie decreasing K/Nb)
with increasing SiO2-undersaturation. The incompatible element
patterns of the early Tertiary Mingela basalts are similar to
the typical OIB, the Newer Basalts, and some NSW lava field basalts
(eg Blue Mts, Oberon, Grabben Gullen, and some Dubbo tholeiites).
They exhibit a peak at Nb and Ta and a gradual decrease in mantle-normalised
abundances from K to Yb, except for the presence of a slight Sr-enrichment,
which is almost ubiquitous in the NQld basalts. The differences
in the incompatible element patterns reflect the variations in
some incompatible element ratios (eg K/Nb=340±80 for Cairns
vs 180±80 for NSW; Table 1) and can be further illustrated
using element-ratio plots such as Rb/Sr vs K/Nb (Fig. 2) and Sr/La
vs K/Nb. For example, three distinct areas can be recognised
on the Figure 2. The Cooktown strongly alkaline rocks fall in
the area for the Barrington, Kandos and Dubbo alkaline basalts,
forming a trend pointing to the region defined by amphibole- and
apatite-bearing spinel peridotite xenoliths hosted by the Victorian
Newer Basalts. The Mingela samples plot close to the Newer Basalts,
Dubbo tholeiites and average OIB composition. The Cairns basalts
mostly plot outside the region for the other Australian basalts
and extend toward the N-MORB and the Kermadec-Tonga island arc
basalts (Ewart & Hawkesworth, 1987) due to their high K/Nb
and low Rb/Sr ratios.
Sample No. | |||||||||
SiO2 | 44.8 | ||||||||
Al2O3 | 4.45 | ||||||||
TiO2 | 0.21 | 2.9 | 1.3 | ||||||
Sc | 17.1 | ||||||||
Y | 4.55 | 29 | 28 | ||||||
Nb | 0.713 | 48.0 | 2.3 | ||||||
La | 0.687 | 37.0 | 2.50 | ||||||
K/Nb | 350 | 250 | 258 | ||||||
Zr/Nb | 15 | 5.8 | 32 | ||||||
Sr/La | 31 | 18 | 36 | ||||||
(La/Yb)n§ | 1.39 | 12.3 | 0.59 |
$, chondrite-normalised ratios; ¶, basaltic rocks from Kermadec-Tonga
arc (Ewart & Hawkesworth, 1987); *, estimated compositions
of primitive mantle, ave. OIB, and ave. normal MORB (Sun &
McDonough, 1989)
Figure 1 Incompatible element patterns for representative basaltic
rocks in North Queensland. Atherton and Chudleigh from Cairns
area and McLean from Cooktown area
Sr-Nd-Pb isotopic systematics: The NQld basaltic rocks have 87Sr/86Sr of 0.7034-0.7048 and 143Nd/144Nd of 0.51302-0.51279 (eNd=+7.5-+3.0) The Sr and Nd isotopic ratios correlate with neither their parent/daughter element ratios nor any fractionation or crustal contamination indicators such as Mg# and SiO2. Although the Sr and Nd isotopic ratios of the Cairns and Cooktown basalts are within the ranges of the NSW lava field basalts and the Victorian Newer Basalts, they differ in their high 87Sr/86Sr at a given 143Nd/144Nd, thus forming a high 87Sr/86Sr trend above the NSW and Victorian trend (Fig. 3). Coincident with this trend, spinel peridotite xenoliths found from the Cairns area are characterised by even higher 87Sr/86Sr at a given 143Nd/144Nd than their hosts (O'Reilly & Zhang, 1995). The most depleted NQld basalts are similar to relatively enriched Indian MORB, whereas the most enriched trend towards the EM2 component. In contrast to the high 87Sr/86Sr trend of the younger NQld basalts, the early Tertiary Mingela basalts plot with in the compositional range for the NSW and Victorian basalts.
Pb isotopic ratios of the NQld samples range in 206Pb/204Pb of
17.90-18.66, in 207Pb/204Pb of 15.56-15.63, and in 208Pb/204Pb
of 37.72-39.24, displaying Dupal signatures with D7/4Pb = +3.3-+12.5
and D8/4Pb = +32-+106. They differ from the NSW lava field basalts
in their generally low but variable 206Pb/204Pb and high D7/4Pb
(18.60-19.14 and -4.4-+6.7, respectively, for NSW basalts). Therefore,
on a 207Pb/204Pb vs 208Pb/204Pb plot (Fig. 4), the NQld basalts
form a subparallel trend below the NSW basalts, indicating the
presence of a source component with relatively low Th/U. The
Dupal-type Pb isotopic signature and the correlations between
87Sr/86Sr and 206Pb/204Pb and between 143Nd/144Nd and 206Pb/204Pb
also require contributions from mantle reservoirs of both an Indian-MORB
type and an EM2 type.
Figure 2 Rb/Sr vs K/Nb for the lava field basalts in eastern
Australia. amp- & ap-peridotites, amphibole- and apatite-bearing
spinel peridotite xenoliths in the Victorian Newer Basalts (O'Reilly
& griffin, 1988); Newer Basalts, after McDonough et al. (1985);
Kermadec basalts, after Ewart & Hawkesworth (1987)
Figure 3 87Sr/86Sr vs 143Nd/144Nd for the lava field basalts
in eastern Australia. Pacific and Indian MORB after Mahoney et
al. (1995).
CHARACTERISTICS OF THE MANTLE SOURCES
Three distinct mantle sources can be inferred from the Sr-Nd-Pb
isotope data. One is represented by the early Tertiary Mingela
basalts. It has both isotope and element signatures likely derived
from an OIB-type sublithospheric mantle source, possibly resulting
from interaction of an enriched deep mantle with the overlying
depleted asthenosphere of the Pacific-MORB type. A similar source
has been considered as one of the dominant mantle reservoirs for
some basalts in NSW and Victoria (O'Reilly & Zhang, 1995).
Figure 4 207Pb/204Pb vs 208Pb/204Pb for the lava field basalts
in eastern Australia.
The isotopic trends for the other NQld basalts can be simply interpreted
as mixing of two source components. One is likely to be an asthenospheric
Indian-MORB source that has been widely recognised in the late-Tertiary
to Present basalts from island arc and backarc basin settings
in the SW Pacific (eg the Kermadec-Tonga arc and the Lau basin,
Hawkins, 1995). This Indian-MORB-type asthenosphere is considered
to have at least partially replaced the previous Pacific-MORB-type
asthenosphere beneath the SW Pacific margins. The other is a
component with EM2 geochemical signatures, likely hosted in the
subcontinental lithospheric mantle (SCLM). However, this SCLM
component must be heterogeneous and is likely to have multiple
origins if the differences in element abundances and ratios between
the Cairns and Cooktown basalts are taken into account. The Cairns
basalts are characterised by relatively high K/Nb, Sr/La, Sr/Nd,
but low La/Yb. This, in connection with their relatively high
SiO2, Al2O3, but low TiO2, Y, HFSE and LREE abundances, indicates
that the SCLM beneath the Cairns area may have been heterogeneously
modified by subduction-related processes, probably during the
Paleozoic - early Mesozoic times when the Tasman Fold Belts were
formed by westward subduction of the proto-Pacific plate beneath
the eastern margin of the Australian continent. Isotopic signatures
of mantle xenoliths in the same region support this conclusion.
On the other hand, the incompatible element patterns of the Cooktown
alkaline basalts may require contributions from a metasomatised
SCLM source containing amphibole (± apatite), similar to
that for the Barrington nephelinites (O'Reilly and Zhang, 1995).
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