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<article language="en">
	<journal>
		<journal_title>Stephan Mueller Special Publication Series</journal_title>
		<journal_url>www.stephan-mueller-spec-publ-ser.net</journal_url>
		<issn>1868-4556</issn>
		<eissn>1868-4564</eissn>
		<volume_number>4</volume_number>
		<volume_title>Geology, geophysics and tectonics of Northeastern Russia: a tribute to Leonid Parfenov</volume_title>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/smsps-4-289-2009</doi>
	<article_url>http://www.stephan-mueller-spec-publ-ser.net/4/289/2009/</article_url>
	<abstract_html>http://www.stephan-mueller-spec-publ-ser.net/4/289/2009/smsps-4-289-2009.html</abstract_html>
	<fulltext_pdf>http://www.stephan-mueller-spec-publ-ser.net/4/289/2009/smsps-4-289-2009.pdf</fulltext_pdf>
	<start_page>289</start_page>
	<end_page>311</end_page>
	<publication_date>2009-09-17</publication_date>
	<article_title content_type="html">Comparison of Cretaceous granitoids of the Chaun tectonic zone to those of the Taigonos Peninsula, NE Asia: rock chemistry, composition of rock forming minerals, and conditions of formation</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>P. L. Tikhomirov</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>M. V. Luchitskaya</name>
			<email>luchitskaya@ginras.ru</email>
		</author>
		<author numeration="3" affiliations="2">
			<name>I. R. Kravchenko-Berezhnoy</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Moscow State University, Moscow, Russia</affiliation>
		<affiliation numeration="2" content_type="html">Geological Institute, Russian Academy of Sciences, Moscow, Russia</affiliation>
	</affiliations>
	<abstract content_type="html">The Cretaceous granitoid complexes of the Eastern Taigonos and the Prybrezhny
Taigonos belts (southern part of the Taigonos Peninsula), Tanyurer pluton of
the Okhotsk-Chukotka volcanic belt, and the Peekiney, Moltykan, and Telekay
plutons of the Chaun tectonic zone are discussed in relation to their
structural position, petrography, rock and mineral chemistry and
physicochemical conditions of melt crystallization. These granitoid plutons
were generated through melting of a compositionally heterogeneous crustal
source, with direct contribution from mafic melts produced in the mantle
wedge above active or extinct Benioff zones. Variations of the trace-element
composition of granitoids are controlled to a greater extent by local
compositional peculiarities of the source regions than by the geodynamic
regime as such. The final crystallization of these plutons occurred at
comparatively shallow depths, between 1–2 and 6–7 km, in a temperature
interval of 700–770&amp;deg;C. The depth of emplacement of the bodies
decreases with increasing distance from the areas with oceanic and
transitional type crust, as does the degree of incompatible element
enrichment of the mantle and crustal sources of melts. Variations in fo&lt;sub&gt;2&lt;/sub&gt;
values at the late stages of crystallization of the plutons reach
3–4 orders of magnitude, exceeding the limits of the
quartz-fayalite-magnetite (QFM) and nickel-nickel oxide (NNO) buffer
equilibria, which likely results from local variations of the source
composition.</abstract>
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</article>

