Source of fluids forming distal Zn-Pb-Ag skarns: Evidence from laser ablation–inductively coupled plasma–mass spectrometry analysis of fluid inclusions from El Mochito, Honduras
- Iain M. Samson1,
- Anthony E. Williams-Jones2,
- Katherine M. Ault3,
- Joel E. Gagnon1 and
- Brian J. Fryer1
- 11Department of Earth and Environmental Sciences, University of Windsor, Windsor, Ontario N9B 3P4, Canada
- 22Department of Earth and Planetary Sciences, McGill University, Montreal, Quebec H3A 2A7, Canada
- 33Aurum Exploration Services, Kells, County Meath, Republic of Ireland
Abstract
The compositions of fluid inclusions trapped in garnet, pyroxene, and sphalerite, measured with laser ablation–inductively coupled plasma–mass spectrometry, from the distal, dominantly limestone-hosted, El Mochito Zn-Pb-Ag skarn, Honduras, are very similar to those of proximal magmatic fluids in granitoid-related mineral deposits. However, the El Mochito mineralizing fluids are chemically distinct from basinal brines, demonstrating that in distal skarns, magmatic fluids dominate, and that most element concentrations and ratios are unaffected by water-rock interaction. High fluid temperatures (~325–425 °C) throughout the paragenesis are also consistent with this hypothesis. A variety of elements and element ratios (e.g., Rb, Mn, K/Na, Mn/Na, Rb/Na, Zn/Na) clearly discriminates between magmatic fluids and basinal brines. Elevated Ca most likely resulted from carbonate dissolution along the flow path. Zinc and Pb contents indicate that the ore metals were precipitated in the deposit in proportions that approached their ratios in the fluid.
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- Received 29 May 2008.
- Revision received 15 August 2008.
- Accepted 19 August 2008.
- © 2008 Geological Society of America












