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Sun and Protosolar Nebula - Working Group Report
Authors:Kallenbach  R  Robert  F  Geiss  J  Herbst  E  Lammer  H  Marty  B  Millar  TJ  Ott  U  Pepin  RO
Institution:(1) International Space Science Institute, Hallerstrasse 6, CH-3012 Bern;(2) Lab. de Minéralogie, Muséum National d'Histoire Naturelle, 61, rue Buffon, F-75005, Paris;(3) The Ohio State Physics Dept. Smith Lab., College of Mathematical and Physical Sciences, 174 W. 18th Ave., Columbus, OH 43210, USA;(4) Space Research Institute, Austrian Academy of Sciences, A-8042 Graz, Austria;(5) Centre de Recherches Pétrographiques et Géochimiques, CNRS UPR, 9046, rue Notre-Dame des Pauvres, BP 20, F-54501 Vandoevre-les Nancy-Cedex;(6) Department of Physics, UMIST, P.O. Box 88, Manchester, M60 1QD, UK;(7) Max-Planck-Institut für Chemie, Postfach 3060, D-55020 Mainz, Germany;(8) School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota, 55455
Abstract:Volatile isotope abundances are tracers for the evolutionary processes of the solar system. At the same time they carry information on the galactic nucleosynthetic sources, from which solar matter originates. This working group report summarizes the present knowledge and addresses unresolved issues regarding fractionation of isotopes of volatile elements in the solar system. This revised version was published online in August 2006 with corrections to the Cover Date.
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