LITHOSPHERIC MANTLE TYPES IN EASTERN CHINA
W.L. Griffin, S.Y. O'Reilly, GEMOC Macquarie and X. Xu (Earth
Sciences, Univ. of Nanjing, Nanjing, China).
Mantle-derived xenoliths and garnet xenocrysts in volcanic rocks
have been used to investigate the composition and thermal state
of the subcontinental lithospheric mantle (SCLM) beneath different
tectonic domains in eastern China. Paleozoic kimberlites in Liaoning
and Shandong provinces, within the Sino-Korean craton, sample
typical Archean mantle: 180-220 km thick, low geotherm (35-40
mW/m2), and abundant clinopyroxene-free harzburgites. Both sections
are significantly more depleted on average than Kaapvaal SCLM.
The two areas differ markedly from one another in bulk compostion
and rock-type stratigraphy, suggesting that they represent separate
microcontinents, each with their own SCLM, that were accreted
into the Sino-Korean craton. Lamproites on the Proterozoic Yangtze
craton sample a distinctly different, typically Proterozoic lithosphere:
thinner (²150 km), hotter (45 mW/m2 geotherm), and dominated
by moderately depleted lherzolite, with essentially no cpx-free
harzburgite. The Proterozoic crust of the Cathaysia block has
been extensively intruded by the Mesozoic Yanshanian granitoids
(with Proterozoic Nd model ages), whose generation commonly is
regarded as a result of subduction processes. The known SCLM beneath
this province consists largely of fertile (²5% melt extraction)
lherzolites. This material is distinctly less depleted than either
Proterozoic SCLM, or peridotites generated in oceanic or convergent-margin
settings, and it is similar to fertile lithosphere found beneath
other young extensional areas, including the Red Sea (Zabargad
Is.). The present SCLM beneath Cathaysia may have been generated
by asthenospheric upwelling related to post-subduction extension.
This upwelling provided the heat source for generation of the
Yanshanian granitoids, and required displacement, or rifting and
dispersal, of any pre-existing Proterozoic lithosphere, and the
delamination of any "oceanic" or sub-arc SCLM developed
during the convergent phase. This model may also explain the rarity
of typical "oceanic" SCLM in xenolith suites from Phanerozoic
mobile belts in eastern Australia and central Asia.
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