Oxidation state of Paleozoic subcontinental lithospheric mantle below the Pali Aike volcanic field in southernmost Patagonia
Oxidation state of Paleozoic subcontinental lithospheric mantle below the Pali Aike volcanic field in southernmost Patagonia
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巴塔哥尼亚最南端巴利艾克火山田下方古生代次大陆岩石圈地幔氧化态
DOI:
10.1016/j.lithos.2008.02.009
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发表时间:
2008-09
期刊:
影响因子:
3.5
通讯作者:
Stern, Charles R.
中科院分区:
文献类型:
--
作者:
Wang, Jian;Hattori, Keiko H.;Li, Jianping;Stern, Charles R.
Mantle xenoliths in the Quaternary Pali Aike alkaline basalts of southernmost Patagonia include lherzolites and harzburgites with and without garnet. The values of fO2for all xenoliths range from 0.33 logarithmic unit below the fayalite–magnetite–quartz buffer (FMQ−0.33) to FMQ+0.75, which overlap those for abyssal peridotites. The fO2data, together with the bulk rock and mineral compositions, suggest that the subcontinental lithospheric mantle (SCLM) below Pali Aike formed through the accretion of oceanic lithosphere. The oceanic accretion likely occurred in mid to late Paleozoic time when the southern Patagonian terrane formed along the southwest margin of Gondwana. Relict spinel inclusions in garnet suggest that garnet-facies peridotites formed from spinel-facies peridotites most likely in response to pressure increase during the accretion. Comparable fO2for garnet- and spinel-facies peridotites suggests that this spinel-garnet transformation was not accompanied by changes in fO2. Metasomatism by asthenosphere-derived melt through a slab window resulted in the formation of Ti-bearing minerals, and lowering of Mg and enrichment of Ti in bulk rocks and minerals. The replacement of olivine by orthopyroxene formed orthopyroxenites in extreme cases. No significant change in fO2is associated with this metasomatism since similar oxidation state is observed between un-metasomatized (FMQ−0.23 to +0.48) and metasomatized (FMQ−0.33 to +0.75) samples. This is explained by the fO2of the asthenospheric melt (~FMQ−0.50) similar to the SCLM prior to the metasomatism.
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影响因子:
3.1
作者:
M. McCanta;M. Dyar;M. Rutherford;J. Delaney
通讯作者:
M. McCanta;M. Dyar;M. Rutherford;J. Delaney
影响因子:
3.1
作者:
J. Selverstone;C. Stern
通讯作者:
J. Selverstone;C. Stern
影响因子:
3.9
作者:
Y. Niu
通讯作者:
Y. Niu
DOI:
10.1144/gsl.sp.2005.246.01.12
发表时间:
2005
期刊:
Geological Society, London, Special Publications
影响因子:
--
作者:
A. Rapalini
通讯作者:
A. Rapalini
影响因子:
1.8
作者:
W. Gosen
通讯作者:
W. Gosen