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Measurement of gas-phase species during Langmuir evaporation of forsterite

Nichols, R. H., Jr. and Grimley, R. T. and Wasserburg, G. J. (1998) Measurement of gas-phase species during Langmuir evaporation of forsterite. Meteoritics and Planetary Science, 33 (S4). A115-A116. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20140716-144324335

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Abstract

Forsterite, the most abundant mineral in meteorites, forms at high temperatures often associated with nebular processes. It evaporates congruently, and its equilibrium evaporation is rather well understood [e.g.]. For these reasons, in part, many recent studies have focused on the more difficult kinetics of the free (Langmuir or nonequilibrium) evaporation of this mineral.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.1998.tb01327.x/abstractPublisherArticle
http://dx.doi.org/10.1111/j.1945-5100.1998.tb01327.xDOIArticle
ORCID:
AuthorORCID
Wasserburg, G. J.0000-0002-7957-8029
Additional Information:© 1998 The Meteoritical Society. Article first published online: 4 Feb 2010. Supported by NASA grant NAGW3337 (GJW). Div. Cont. 8519 (999).
Funders:
Funding AgencyGrant Number
NASANAGW3337
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences8519
Lunatic Asylum Lab999
Issue or Number:S4
Record Number:CaltechAUTHORS:20140716-144324335
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140716-144324335
Official Citation:(1998), Abstracts. Meteoritics & Planetary Science, 33: A7–A172. doi: 10.1111/j.1945-5100.1998.tb01327.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:47273
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:16 Jul 2014 23:32
Last Modified:09 Mar 2020 13:19

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