SOUTHERN AUSTRALIA AND SIBERIA: A COMPARISON OF TWO LITHOSPHERIC TRANSECTS
Oliver F. Gaul1, William L. Griffin1,2 and Suzanne Y. O'Reilly1
1 GEMOC, Macquarie, 2 CSIRO Exploration and Mining
Two lithospheric transects have been constructed, in southern
Australia and Siberia, using data from mantle xenocrysts brought
to the Earth's surface by kimberlitic and basaltic activity. The
southern Australian transect extends from the Eyre Peninsula of
central South Australia to Jugiong in southeastern New South Wales.
This transect encompasses both cratonic and fold belt environments
and crosses the Tasman Line, which separates Archean/Proterozoic
western Australia from the Phanerozoic accreted terrains of eastern
Australia. The Siberian transect also crosses a number of terrains
from the Archean Eastern Siberian craton in the south to Proterozoic
mobile belts in the north. These two transects provide an opportunity
to examine the changes in lithospheric structure and chemistry
from cratonic to off-craton environments. Comparison of the two
transects can be used to determine what patterns are common to
both cratons and what factors are independent of tectonic setting.
Samples studied consist of garnet and chromite heavy mineral concentrates
and were analysed by electron microprobe (major elements) and
proton microprobe or laser ablation ICPMS (minor and trace elements).
Temperature and pressure estimates have been made for each garnet
grain through the use of the single mineral Ni-thermometer and
Cr-barometer (Ryan and Griffin, 1996). These data have been used
to estimate model conductive paleogeotherms for each locality.
Results show a wide range of geotherms from 35 mWm-2 in the Archean
of Siberia, through 40-43 mWm-2 in Proterozoic regions of both
transects, to in excess of 50 mWm-2 in Phanerozoic eastern Australia.
Estimates of lithospheric thickness, based on trace element concentrations
in garnet, vary from 240 km in the core of the Siberian craton,
through 160-170 km in Proterozoic sections, to ~100 km in eastern
Australia.
Temperature and pressure estimates for garnet also allow the construction
of "chemical sections". These are plots of garnet chemistry
against depth which provide a useful tool for interpreting changes
in a number of variables with depth within the lithosphere.
Results from these chemical sections reveal some interesting patterns:
minor rock types are more commonly harzburgitic in Archean sections and wehrlitic in Phanerozoic areas
Cr2O3 content of garnet is lower in younger sections
a steady trend to higher Y/Ga and lower Zr/Y ratios in garnet exists between Archean and Phanerozoic lithosphere
the pattern of metasomatic activity appears to vary little between Archean and Phanerozoic times
TiO2 in garnet increases with depth in most sections regardless
of age
A method for estimating olivine Mg content from garnet chemistry
has been developed which involves the inversion of the O'Neill
and Wood (1979) garnet-olivine Fe-Mg exchange thermometer. The
Ni-temperature of a given garnet grain can be used, in conjunction
with the Mg, Fe and Ca content of the garnet, to solve for olivine
Mg and Fe content. The Mg content of olivine is an important indicator
of the degree to which lithospheric mantle has been depleted through
the extraction of basaltic melts. Also, because olivine is the
most common mineral in the lithospheric mantle, the Mg content
of olivine is one of the main factors in determining the density
of mantle rocks. Results of this procedure show an overall decrease
in olivine Mg content with depth in most sections. There is also
a trend to more Fe-rich compositions in younger areas. Values
in the shallow portions of sections range from Mg# >94 in Archean
areas to Mg# of 90-91 in Phanerozoic sections. This indicates
a lower degree of depletion in younger lithospheric sections and
could also account for a density increase of ~0.03 g/cc due to
olivine chemistry alone.
References
O'Neill, H. StC. and Wood, B. J. 1979. An experimental study of
Fe-Mg partitioning between garnet and olivine and its calibration
as a geothermometer. Contributions to Mineralogy and Petrology,
70, 59-70.
Ryan, C. G. & Griffin, W. L. 1996. Garnet geotherms: Pressure-temperature
data from Cr-pyrope garnet xenocrysts in volcanic rocks. Journal
of Geophysical Research, 101, 5611-5625.
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