Author name: Robert J. Bodnar

Fluids in Planetary Systems

At our first inaugural meeting last April, we sifted through several pages of potential topics. Some had been suggested by the councils of the par- ticipating societies; others had been gathered at meetings, while talking to colleagues. We strived to choose topics that would be of interest to a wide part of our membership – in each of these issues, mineralogists, geochemists, and petrologists should find at least one article of great interest to them – but also topics where exciting developments are underway. We also needed to find guest editors and authors willing to work under very tight deadlines. It you are interested in proposing a topic, you can download a propos- al form from our web site. We are already developing themes for 2006 and 2007. Here is what you can look forward to in 2005.

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Microscale Chemistry: Raman Analysis of Fluid and Melt Inclusions

Raman spectroscopy is a commonly applied nondestructive analytical technique for characterizing fluid and melt inclusions. The exceptional spatial resolution (~1 µm) and excellent spectral resolution (≤1 cm−1) permits the characterization of micrometer-scale phases and allows quantitative analyses based on Raman spectral features. Data provided by Raman analysis of fluid and melt inclusions has significantly advanced our understanding of complex geologic processes, including preeruptive volatile contents of magmas, the nature of fluids in the deep crust and upper mantle, the generation and evolution of methane-bearing fluids in unconventional hydrocarbon reservoirs. Anticipated future advances include the development of Raman mass spectroscopy and the use of Raman to monitor reaction progress in synthetic and natural fluid inclusion microreactors.

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