Ore-Forming Fluids of the Gold-Bearing Interval of the Kola Superdeep Borehole


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This paper reports on the physical–chemical parameters and vertical distribution of different types of fluid inclusions in quartz from the Au-bearing interval of the Kola Superdeep Borehole. We assume that gold ore mineralization was formed when a deep flux of CO2 interacted with brines at depths of 10 205–9269 m due to tectonic factors. In this paper, we discussed the role of these processes in the formation of the orogenic gold deposits including the gold mineralization of the Southern Pechenga structural zone.

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V. Prokofiev

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences

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Email: vpr2004@rambler.ru
俄罗斯联邦, Moscow, 119017

K. Lobanov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences

Email: vpr2004@rambler.ru
俄罗斯联邦, Moscow, 119017

A. Pek

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences

Email: vpr2004@rambler.ru
俄罗斯联邦, Moscow, 119017

M. Chicherov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences

Email: vpr2004@rambler.ru
俄罗斯联邦, Moscow, 119017

A. Borovikov

Sobolev Institute of Geology and Mineralogy, Siberian Branch, Russian Academy of Sciences

Email: vpr2004@rambler.ru
俄罗斯联邦, Novosibirsk, 630090

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