Highly labile elements

Certain elements of high lability are very responsive to thermal processes, being either highly volatile during primary nebular condensation or highly mobile by postaccretionary metamorphic or shock heating. Data for highly labile elements indicate that different thermal processes were important in...

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Bibliographic Details
Main Authors: Lipschutz, Michael E., Woolum, Dorothy S.
Language:unknown
Published: 1988
Subjects:
91
Antarc*
Antarctica
Online Access:http://ntrs.nasa.gov/search.jsp?R=19890040126
id ftnasantrs:oai:casi.ntrs.nasa.gov:19890040126
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19890040126 2023-05-15T13:41:01+02:00 Highly labile elements Lipschutz, Michael E. Woolum, Dorothy S. Unclassified, Unlimited, Publicly available JAN 1, 1988 http://ntrs.nasa.gov/search.jsp?R=19890040126 unknown http://ntrs.nasa.gov/search.jsp?R=19890040126 Accession ID: 89A27497 Copyright Other Sources 91 1988 ftnasantrs 2012-02-15T17:59:53Z Certain elements of high lability are very responsive to thermal processes, being either highly volatile during primary nebular condensation or highly mobile by postaccretionary metamorphic or shock heating. Data for highly labile elements indicate that different thermal processes were important in the genesis of each of the chondritic groups and a discussion of each is given. Contents of highly labile elements in a given group of contemporary falls differ from those of the same group that fell in Antarctica more than 0.1 Myr ago. This difference is due either to a time-dependent change in meteorite sources or, less likely, orbital variation of the meteorite flux to Earth. Other/Unknown Material Antarc* Antarctica NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic 91
spellingShingle 91
Lipschutz, Michael E.
Woolum, Dorothy S.
Highly labile elements
topic_facet 91
description Certain elements of high lability are very responsive to thermal processes, being either highly volatile during primary nebular condensation or highly mobile by postaccretionary metamorphic or shock heating. Data for highly labile elements indicate that different thermal processes were important in the genesis of each of the chondritic groups and a discussion of each is given. Contents of highly labile elements in a given group of contemporary falls differ from those of the same group that fell in Antarctica more than 0.1 Myr ago. This difference is due either to a time-dependent change in meteorite sources or, less likely, orbital variation of the meteorite flux to Earth.
author Lipschutz, Michael E.
Woolum, Dorothy S.
author_facet Lipschutz, Michael E.
Woolum, Dorothy S.
author_sort Lipschutz, Michael E.
title Highly labile elements
title_short Highly labile elements
title_full Highly labile elements
title_fullStr Highly labile elements
title_full_unstemmed Highly labile elements
title_sort highly labile elements
publishDate 1988
url http://ntrs.nasa.gov/search.jsp?R=19890040126
op_coverage Unclassified, Unlimited, Publicly available
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Other Sources
op_relation http://ntrs.nasa.gov/search.jsp?R=19890040126
Accession ID: 89A27497
op_rights Copyright
_version_ 1766144493221838848

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