Light noble gas data in Guli massif carbonatites reveal the subcontinental lithospheric mantle as primary fluid source


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For better understanding of the fluid phase sources of carbonatites of Guli alkaline-ultrabasic intrusion (Maymecha-Kotuy complex) we have studied isotope composition of He and Ne in the carbonatites of different formation stages. The data definitely point to the subcontinental lithospheric mantle (SCLM) as a primary source of fluid phase of Guli carbonatites. The absence of plume signature in such a plume-like object (from petrological point of view) could be explained in terms that Guli carbonatites have been formed at the waning stage of plume magmatic activity with an essential input of SCLM components.

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A. Buikin

Vernadsky Institute of Geochemistry and Analytical Chemistry

编辑信件的主要联系方式.
Email: bouikine@mail.ru
俄罗斯联邦, Moscow, 119991

L. Kogarko

Vernadsky Institute of Geochemistry and Analytical Chemistry

Email: bouikine@mail.ru
俄罗斯联邦, Moscow, 119991

J. Hopp

Institut für Geowissenschaften der Universität Heidelberg

Email: bouikine@mail.ru
德国, Im Neuenheimer Feld 234-236, Heidelberg, D_69120

M. Trieloff

Institut für Geowissenschaften der Universität Heidelberg; Klaus-Tschira-Labor für Kosmochemie, Universität Heidelberg

Email: bouikine@mail.ru
德国, Im Neuenheimer Feld 234-236, Heidelberg, D_69120; Im Neuenheimer Feld 234-236, Heidelberg, 69120

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