Isotopic systematics of He, Ar, S, Cu, Ni, Re, Os, Pb, U, Sm, Nd, Rb, Sr, Lu, and Hf in the rocks and ores of the Norilsk deposits


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

This paper reports the first results of a study of 11 isotope systems (3He/4He, 40Ar/36Ar, 34S/32S, 65Cu/63Cu, 62Ni/60Ni, 87Sr/86Sr, 143Nd/144Nd, 206–208Pb/204Pb, Hf–Nd, U–Pb, and Re–Os) in the rocks and ores of the Cu–Ni–PGE deposits of the Norilsk ore district. Almost all the results were obtained at the Center of Isotopic Research of the Karpinskii All-Russia Research Institute of Geology. The use of a number of independent genetic isotopic signatures and comprehensive isotopic knowledge provided a methodic basis for the interpretation of approximately 5000 isotopic analyses of various elements. The presence of materials from two sources, crust and mantle, was detected in the composition of the rocks and ores. The contribution of the crustal source is especially significant in the paleofluids (gas–liquid microinclusions) of the ore-forming medium. Crustal solutions were probably a transport medium during ore formation. Air argon is dominant in the ores, which indicates a connection between the paleofluids and the atmosphere. This suggests intense groundwater circulation during the crystallization of ore minerals. The age of the rocks and ores of the Norilsk deposits was determined. The stage of orebody formation is restricted to a narrow age interval of 250 ± 10 Ma. An isotopic criterion was proposed for the ore-bearing potential of mafic intrusions in the Norilsk–Taimyr region. It includes several interrelated isotopic ratios of various elements: He, Ar, S, and others.

About the authors

E. M. Prasolov

Karpinskii All-Russia Research Institute of Geology; Institute of Earth Sciences

Author for correspondence.
Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106; St. Petersburg

S. A. Sergeev

Karpinskii All-Russia Research Institute of Geology; Institute of Earth Sciences

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106; St. Petersburg

B. V. Belyatsky

Karpinskii All-Russia Research Institute of Geology

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106

E. S. Bogomolov

Karpinskii All-Russia Research Institute of Geology

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106

K. A. Gruzdov

Karpinskii All-Russia Research Institute of Geology

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106

I. N. Kapitonov

Karpinskii All-Russia Research Institute of Geology; Institute of Earth Sciences

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106; St. Petersburg

R. Sh. Krymsky

Karpinskii All-Russia Research Institute of Geology

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106

V. O. Khalenev

Karpinskii All-Russia Research Institute of Geology

Email: Edward_Prasolov@vsegei.ru
Russian Federation, St. Petersburg, 199106

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2018 Pleiades Publishing, Ltd.