Direct dating of overprinting fluid systems in the Martabe epithermal gold deposit using highly retentive alunite

<p>The Martabe gold deposits in Sumatra formed in a shallow crustal epithermal environment associated with intermediate mafic intrusions adjacent to an active right-lateral wrench system. Gas/fluid temperatures reached 200–350 <span class="inline-formula"><sup>∘</sup&g...

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Bibliographic Details
Main Authors: J. Muston, M. Forster, D. Vasegh, C. Alderton, S. Crispin, G. Lister
Format: Article
Language:English
Published: Copernicus Publications 2023-04-01
Series:Geochronology
Online Access:https://gchron.copernicus.org/articles/5/153/2023/gchron-5-153-2023.pdf
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Summary:<p>The Martabe gold deposits in Sumatra formed in a shallow crustal epithermal environment associated with intermediate mafic intrusions adjacent to an active right-lateral wrench system. Gas/fluid temperatures reached 200–350 <span class="inline-formula"><sup>∘</sup></span>C. The structural geology suggests episodic switches in stress orientations during a Plio-Pleistocene seismotectonic evolution. Different mineralisation events may have been associated with oscillations in this earthquake cycle, so samples containing alunite were collected for <span class="inline-formula"><sup>40</sup></span>Ar <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="e653eaf840568ee76bb20ba3bf368ae0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-5-153-2023-ie00001.svg" width="8pt" height="14pt" src="gchron-5-153-2023-ie00001.png"/></svg:svg></span></span> <span class="inline-formula"><sup>39</sup></span>Ar geochronology to constrain the timing. <span class="inline-formula"><sup>39</sup></span>Ar diffusion experiments were performed to constrain variation in argon retentivity. The age spectra were produced by incremental step-heating with heating times chosen so similar percentages of <span class="inline-formula"><sup>39</sup></span>Ar gas release occurred during as many steps as possible. This ensured the detail necessary for analysis of the complex morphology of these spectra by applying the method of asymptotes and limits, which enabled recognition of different growth events of alunite in overprinting fluid systems. It was possible to provide estimates as to the frequency of individual events and their duration. The heating schedule also ensured that Arrhenius data populated the inverse temperature axis with sufficient detail to allow modelling. Activation energies were between 370–660 kJ mol<span class="inline-formula"><sup>−1</sup></span>. Application of Dodson's recursion determined closure temperatures that range from 400–560 <span class="inline-formula"><sup>∘</sup></span>C for a cooling rate of 100 <span class="inline-formula"><sup>∘</sup></span>C Ma<span class="inline-formula"><sup>−1</sup></span>. Such estimates are higher than any temperature to be expected in the natural system, giving confidence that the ages represent the timing of growth during periods of active fluid movement and alteration: a hypothesis confirmed by modelling age spectra using the MacArgon program. We conclude that gold in the Purnama pit resulted from overprinting fluid rock interactions during very short mineralisation episodes at <span class="inline-formula">∼2.25</span> and <span class="inline-formula">∼2.00</span> Ma.</p>
ISSN:2628-3697
2628-3719