Sources
of Cenozoic intra-plate magmatism in Central Asia:
implication from geochemistry and Sr-Nd-Pb isotope
data
V.M.Savatenkov*, E.A.Kudryashova**, A.M.Kozlovsky**,
V.V.Yarmolyuk**
* Institute of Precambrian Geology and Geochronology
RAS, St.-Petersburg; ** Institute of the Geology of Ore Deposits, Petrography,
Mineralogy, and Geochemistry RAS, Moscow, Russia.
During Later Cenozoic within Central Asia the series of independently
evolving volcanic areas (so-called Central Asian Volcanic Province (CAVP)) has
formed [1]. They are Udokan (UVA), Vitim (VVA), Southern
Baycalian (SBVA) and Khangai
(KVA) volcanic areas. They are situated far from lithospheric
plate margins and are characterized by predominance of sub-alkaline and
alkaline basalts. So, they relate to intra-plate processes. Geophysical studies
of CAVP [2] revealed presence of large-scale ledge of an asthenospheric
mantle (or hot field of mantle) with roof elevated on 100 km to surface.
Moreover, directly beneath some volcanic areas the local elevation attending
the 50 km to surface was discovered. These elevations were interpreted as
mantle diapires produced by thermal field of the
mantle. Because the feeding area was common the structurally separated volcanic
areas were developed simultaneously [1]. This fact also indicates the relation
of CAVP with mantle plumes. Volcanic areas are characterized by the duration of
development exceeding a few 10 Ma, as well as by relations to grabens systems, the stable character of magmatism, the regular migration corresponding to lithosphere
displacements over hot spot, and by the link to dome-like elevation at modern
relief.
The geochemical characteristics of the basalts from the different areas
of CAVP demonstrate no significant differences. The basalts show smooth
normalized REE spectrum with relative LREE enrichment. The trace element
enrichment implies that the basalts of CAVP correspond to OIB. However, CAPV
basalts show enrichment in Ba and K and depletion in
U, Th, Zr, Hf and heavy REE compared with OIB. Because geochemical
characteristics of basalts from different CAVP area are similar the source of
investigated basalts is common and melting environment is similar.
In spite of these similarities, some differences between the basalts
from different areas as well as basalts from single volcanic area occur. For
example, the basalts from SBVA and KVA contain lower MgO
compared with the basalts from UVA and VVA; that mean higher fractionating
degree. In addition, within KVA the basalts vary from high-Mg to low-Mg types. These
variations of chemical composition occur from centre to edge of KVA and they apparently
indicate different levels of magma generation. These levels appear to link with
mantle dome structure.
ÁIn εNd versus εSr space, the basalts from
CAVP form superposition confined by
two trends from PREMA-like mantle (FOZO [3]), one of which extend to EMI source
and other extend to EMII source. In according to the εNd
versus εSr
diagram, the basalts from SBVA and KVA derived from the source contained
mixture of EMI and EMII components. The basalts from VVA form trend from FOZO
to EMII [4]. End-member of the basalts from UVA accords with a weak depleted
mantle isotope signatures.
In 206Pb/204Pb versus 207Pb/204Pb
space, basalts from KVA and UVA also form some trend from FOZO. First group of
the samples forms array shifted to the field of
ancient (Archean) recycled material. The latter was
primarily enriched in U and then partly loosed it during Proterozoic
period. Other group of the samples forms trend toward the field of low-U/Pb ancient recycled material. This conclusion is in
agreement with low Th and U concentrations in the studied
basalts. End-member component of the basalts from UVA is a weak depleted
mantle. This suggests shorter history of enriched source evolution compared
with source of the basalts from KVA.
Thus geochemical and isotopic data demonstrate that source of the
studied basalts appear to be involved material of recycled lithosphere. The basalts
from KVA and SBVA generally exhibit low εNd value (up to -12), reflecting
recycled lithosphere was ancient. In addition, their Pb
isotope signature results from the long-term evolution of enriched source. In
contrast, isotope data on the basalts from UVA and VVA indicate the
shorter history of enriched source evolution. Sr-Nd-Pb
isotope differences between end-member sources of the basalts from southern
(KVA, SBVA) and northern (UVA, VVA) reflect sublithospheric
mantle heterogeneity. So, sublithospheric mantle apparently
contain buried lithosphere
fragments of different age. Based on SrãNdãPb isotopic results, we
suggest that common component for all of the studied basalts was
asthenospheric mantle with εSr
~ -15, εNd ~ +5, 206Pb/204Pb
~ 18.5, at least in Central Asia.
This work is supported by the Russian Academy
Foundation (grants 07-05-00876, 05-05-64000, 07-05-90100).
References:
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