Metal recycling tracked by mercury and helium isotopes in platinum-palladium nuggets from Corrego Bom Sucesso, Brazil

被引:5
作者
Cabral, Alexandre Raphael [1 ,2 ]
Deng, Changzhou [3 ]
Yin, Runsheng [3 ]
Yakubovich, Olga, V [4 ,5 ]
Stuart, Finlay M. [6 ]
Tupinamba, Miguel [7 ]
Lehmann, Bernd [8 ]
机构
[1] Univ Fed Minas Gerais UFMG, Ctr Pesquisa Prof Manoel Teixeira Costa, Inst Geociencias, BR-31270901 Belo Horizonte, MG, Brazil
[2] Ctr Desenvolvimento Tecnol Nucl CDTN, BR-31270901 Belo Horizonte, MG, Brazil
[3] Chinese Acad Sci, Inst Geochem, State Key Lab Ore Deposit Geochem, Guiyang 550081, Peoples R China
[4] St Petersburg State Univ, Inst Earth Sci, Unversitetskaya Emb 7-9, St Petersburg 199034, Russia
[5] Inst Precambrian Geol & Geochronol RAS, Makarova Emb 2, St Petersburg 199034, Russia
[6] Scottish Univ, Environm Res Ctr, Rankine Ave, E Kilbride G75 0QF, Lanark, Scotland
[7] Univ Estado Rio de Janeiro, Fac Geol, Tektos Geotecton Res Grp, BR-20550050 Rio De Janeiro, RJ, Brazil
[8] Tech Univ Clausthal, Mineral Resources, Adolph Roemer Str 2a, D-38678 Clausthal Zellerfeld, Germany
关键词
Platinum-palladium nuggets; Mercury isotopes; Helium isotopes; Corrego Bom Sucesso; Minas Gerais; Brazil; MINAS-GERAIS; HYDROTHERMAL FLUIDS; GOLD DEPOSITS; AR ISOTOPES; NOBLE-GASES; ORIGIN; HE; FRACTIONATION; MINERALS; MANTLE;
D O I
10.1016/j.chemgeo.2022.120752
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The enigmatic botryoidal nuggets of platinum (Pt) and palladium (Pd) from Corrego Born Sucesso in the southern Serra do Espinhaco, Minas Gerais, Brazil, are considered to have formed during supergene alteration of placer deposits. This requires hitherto unidentified precious-metal enrichment processes and is inconsistent with Pt-Os age of 180 Ma that entails formation at depth, as recently proposed. Here we report the first mercury (Hg) and helium (He) isotopic determinations of Pt-Pd nuggets. Mercury isotopic compositions have a mass-independent fractionation (MIF) signature with an odd-mass deficit (Delta Hg-199 = - 0.22 +/- 0.04; 1SD, n = 15), which requires aqueous photochemical reduction of Hg (II). Extremely low He-3/He-4 (<0.001 R-a) and extremely high concentrations of He (up to 1.9 x 10(17) at/g) are indicative of nugget formation from He-enriched fluids within the quartzite sequence of the Espinhaco basin, not from meteoric surface water. The data are consistent with a nugget-forming setting in the deep biosphere, as a result of groundwater interaction with Pt-Pd-Hg minerals in Pan-African-Brasiliano post-orogenic veins. We propose that the negative Hg-MIF signature was inherited from the vein minerals that originally acquired their Hg from Earth's surface during the intracratonic sedimentation of the Proterozoic Espinhaco basin.
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页数:8
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