Stable isotopes (O, C) and fluid inclusion study of quartz-carbonate veins from the antimony line, Murchison Greenstone Belt
Clicks: 1
ID: 305812
2014
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
0.0
/100
1 views
0 readers
AI Quality Assessment
Not analyzed
Readership in this journal
Ranked #7,674 of 8,486 articles by views in american journal of science
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 8,486 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
In the homogeneously deformed Murchison Greenstone Belt region, fluids circulations were focused along a localized deformation brittle-ductile zone, and the so-called Antimony Line. In order to trace the origin of the fluid, its composition, the temperature of the precipitation along the Antimony Line, we investigate the stable isotope (oxygen and carbon) and fluid inclusion compositions of the quartz-carbonate veins, as well as chemical analyses of the carbonates and ^40^Ar-^39^Ar dating on the fuchsite associated with the veins. Three types of fluid inclusions are recognized for the H~2~O-CO~2~-dominated (plus minor CH~4~-N~2~) fluid(s). Microthermometric measurements together with the paragenesis of the veins and host rocks indicate that the pressure-temperature of the precipitation is 350 to 450 °C, 200 to 300 MPa, which is an unusually high temperature for an antimony deposit. The carbonates are Fe-Mg-rich and are characterized by flat MREE and HREE patterns, with slight depletions in LREE. The oxygen isotope compositions of the quartz are rather homogeneous at the scale of the Antimony Line (δ^18^O~quartz~ = 10.9-14.3‰). In detail, subtle differences in the δ^18^O values for the quartz and carbonate exist depending on the sampling sites. These differences are likely due to minor temperature and/or host rock geochemistry variations along the Antimony Line. Data point to a metamorphic origin for the fluids responsible for the mineralization, which likely escaped from the nearby greenstone lithologies. Finally, we present an overview of the Murchison Greenstone Belt geological evolution by integrating the antimony metallogeny of the Antimony Line, which can be compared to that of an orogenic gold deposit.
| Reference Key |
openalex_W2331941650
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | Justine Jaguin, Philippe Boulvais, Marie‐Christine Boiron, Marc Poujol, Denis Gapais, Gilles Ruffet, Nicolas Briant |
| Journal | american journal of science |
| Year | 2014 |
| DOI |
10.2475/07.2014.03
|
| URL | |
| Keywords | Keywords not found |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.