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Cambridge University Press, Apr 29, 2010 - Science
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How did the Solar System's chemical composition evolve? This textbook provides the answers in the first interdisciplinary introduction to cosmochemistry. It makes this exciting and evolving field accessible to undergraduate and graduate students from a range of backgrounds, including geology, chemistry, astronomy and physics. The authors - two established leaders who have pioneered developments in the field - provide a complete background to cosmochemical processes and discoveries, enabling students outside geochemistry to understand and explore the Solar System's composition. Topics covered include: - synthesis of nuclides in stars - partitioning of elements between solids, liquids and gas in the solar nebula - overviews of the chemistry of extraterrestrial materials - isotopic tools used to investigate processes such as planet accretion and element fractionation - chronology of the early Solar System - geochemical exploration of planets Boxes provide basic definitions and mini-courses in mineralogy, organic chemistry, and other essential background information for students. Review questions and additional reading for each chapter encourage students to explore cosmochemistry further.

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the building blocks of matter
Origin of the elements
elements and isotopes
a record of stellar nucleosynthesis and processes
a record of nebular and planetary processes
Chondrite classification
Cosmochemical and geochemical fractionations
Radioisotopes as chronometers
organic matter
Chemistry of anhydrous planetesimals
Chemistry of comets and other icebearing planetesimals
Chemistry of comets
Moon and Mars
Cosmochemical models for the formation of the solar system
Some analytical techniques commonly used

Chronology of the solar system from radioactive isotopes

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About the author (2010)

Harry (Hap) McSween is Chancellor's Professor at the University of Tennessee. He has conducted research on cosmochemistry for more than three decades and was one of the original proponents of the hypothesis that some meteorites are from Mars. He has been a co-investigator for four NASA spacecraft missions and serves on numerous advisory committees for NASA and the US National Research Council. Dr McSween has written or edited four books on meteorites and planetary science, and co-authored a textbook in geochemistry. He is a former President and Fellow of the Meteoritical Society, a Fellow of the American Academy of Arts and Sciences, recipient of the Leonard Medal, and has an asteroid named for him.

Gary Huss is a Research Professor and Director of the W. M. Keck Cosmochemistry Laboratory at the Hawaii Institute for Geophysics and Planetology, University of Hawaii at Manoa. In more than three decades of research on cosmochemistry, he was among the first to study presolar grains, the raw materials for the Solar System. He presently studies the chronology of the early Solar System. He comes from a family of meteorite scientists: his grandfather, H. H. Nininger, has been called the father of modern meteoritics, and his father, Glenn Huss, and grandfather were responsible for recovering over 500 meteorites previously unknown to science. Dr Huss is a former President and Fellow of the Meteoritical Society and also has an asteroid named for him.

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