Kinetics of Gas–Solid Reactions in the Solar System and Beyond

Abstract

Research Article| November 01, 2018 Kinetics of Gas–Solid Reactions in the Solar System and Beyond Hiroko Nagahara Hiroko Nagahara Earth-Life Science Institute, Tokyo Institute of Technology, 2-12-1-IE−19 Ookayama, Meguro, 152−8550 Tokyo, Japan Search for other works by this author on: GSW Google Scholar Author and Article Information Hiroko Nagahara Earth-Life Science Institute, Tokyo Institute of Technology, 2-12-1-IE−19 Ookayama, Meguro, 152−8550 Tokyo, Japan Publisher: Mineralogical Society of America First Online: 09 Nov 2018 Copyright © 2018 by the Mineralogical Society of AmericaMineralogical Society of America Reviews in Mineralogy and Geochemistry (2018) 84 (1): 461–497. https://doi.org/10.2138/rmg.2018.84.12 Article history First Online: 09 Nov 2018 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Hiroko Nagahara; Kinetics of Gas–Solid Reactions in the Solar System and Beyond. Reviews in Mineralogy and Geochemistry 2018;; 84 (1): 461–497. doi: https://doi.org/10.2138/rmg.2018.84.12 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyReviews in Mineralogy and Geochemistry Search Advanced Search Evaporation and condensation of crystalline or amorphous materials at high temperature are the fundamental processes at low pressure in circumstellar environments such as protoplanetary disks and outflows around evolved stars and supernovae, where liquid is basically unstable. Condensation or evaporation of various dust species in a multi-elemental system causes elemental and/or isotopic fractionation, which are commonly found in astronomical observations or in presolar grains included in chondrites derived from late stage stars. Evaporation and condensation in the high temperature region of a protoplanetary disk may be related to chemical diversity of planets and planetesimals including asteroids. Evaporation and condensation are... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.