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


Citar

Texto integral

Acesso aberto Acesso aberto
Acesso é fechado Acesso está concedido
Acesso é fechado Somente assinantes

Resumo

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.

Sobre autores

V. Prokofiev

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

Autor responsável pela correspondência
Email: vpr2004@rambler.ru
Rússia, Moscow, 119017

K. Lobanov

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

Email: vpr2004@rambler.ru
Rússia, Moscow, 119017

A. Pek

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

Email: vpr2004@rambler.ru
Rússia, Moscow, 119017

M. Chicherov

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

Email: vpr2004@rambler.ru
Rússia, Moscow, 119017

A. Borovikov

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

Email: vpr2004@rambler.ru
Rússia, Novosibirsk, 630090

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML

Declaração de direitos autorais © Pleiades Publishing, Ltd., 2019