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Highly siderophile and strongly chalcophile elements in high-temperature geochemistry and cosmochemistry / editors, Jason Harvey, University of Leeds, UK, James M.D. Day, Scripps Institution of Oceanography, USA.

Contributor(s): Material type: TextTextSeries: Reviews in mineralogy and geochemistry ; Volume 81.Publisher: Chantilly, Virginia : Mineralogical Society of America, 2016Copyright date: ©2016Description: 1 online resource (798 pages) : illustrations, graphs, tablesContent type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9781501502095 (e-book)
Subject(s): Genre/Form: Additional physical formats: Print version:: Highly siderophile and strongly chalcophile elements in high-temperature geochemistry and cosmochemistry.DDC classification:
  • 549.112 23
LOC classification:
  • QE515 .H544 2016
Online resources:
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Enhanced descriptions from Syndetics:

Highly Siderophile and Strongly Chalcophile Elements in High Temperature Geochemistry and Cosmochemistry, Volume 81

This RiMG (Reviews in Mineralogy & Geochemistry) volume investigates the application of highly siderophile (HSE) and strongly chalcophile elements. This volume has its origin in a short course sponsored by the Mineralogical Society of America and the Geochemical Society held in San Diego, California on the 11thand 12th December 2015, ahead of the American Geophysical Union's Fall Meeting, which featured a session with the same title.

Topics in this volume include:

analytical methods and data quality experimental constraints applied to understanding HSE partitioning nucleosynthetic variations of siderophile and chalcophile elements HSE in the Earth, Moon, Mars and asteroidal bodies HSE and chalcophile elements in both cratonic and non-cratonic mantle, encompassing both sub-continental and sub-oceanic lithosphere the importance of the HSE for studying volcanic and magmatic processes, and an appraisal of the importance of magmatic HSE ore formation in Earth's crust.

Highly siderophile and strongly chalcophile elements comprise Re, Os, Ir, Ru, Pt, Rh, Pd, Au, Te, Se and S and are defined by their strong partitioning into the metallic phase, but will also strongly partition into sulfide phases, in the absence of metal. The chemical properties of the HSE mean that they are excellent tracers of key processes in high temperature geochemistry and cosmochemistry, having applications in virtually all areas of earth science. A key aspect of the HSE is that three long-lived, geologically useful decay systems exist with the HSE as parent (107Pd-107Ag), or parent-daughter isotopes (187Re-187Os and190Pt-186Os).

The material in this book is accessible for graduate students, researchers, and professionals with interests in the geochemistry and cosmochemistry of these elements, geochronology, magmatic ore bodies and the petrogenesis of platinum-group minerals.

Includes bibliographical references at the end of each chapters.

Description based on print version record.

Electronic reproduction. Ann Arbor, MI : ProQuest, 2016. Available via World Wide Web. Access may be limited to ProQuest affiliated libraries.

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