Trace element study of H chondrites: Evidence for meteoroid streams

Multivariate statistical analyses, both linear discriminant analysis and logistic regression, of the volatile trace elemental concentrations in H4-6 chondrites reveal compositionally distinguishable subpopulations. Observed difference in volatile trace element composition between Antarctic and non-A...

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Main Author: Wolf, Stephen Frederic
Other Authors: Lipschutz, Michael E.
Format: Text
Language:English
Published: Purdue University 1993
Subjects:
Online Access:https://docs.lib.purdue.edu/dissertations/AAI9334441
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spelling ftpurdueuniv:oai:docs.lib.purdue.edu:dissertations-31245 2023-07-02T03:29:53+02:00 Trace element study of H chondrites: Evidence for meteoroid streams Wolf, Stephen Frederic Lipschutz, Michael E. 1993-01-01T08:00:00Z https://docs.lib.purdue.edu/dissertations/AAI9334441 ENG eng Purdue University https://docs.lib.purdue.edu/dissertations/AAI9334441 Theses and Dissertations Available from ProQuest Analytical chemistry|Astronomy|Astrophysics|Statistics text 1993 ftpurdueuniv 2023-06-12T21:25:20Z Multivariate statistical analyses, both linear discriminant analysis and logistic regression, of the volatile trace elemental concentrations in H4-6 chondrites reveal compositionally distinguishable subpopulations. Observed difference in volatile trace element composition between Antarctic and non-Antarctic H4-6 chondrites (Lipschutz and Samuels, 1991) can be explained by a compositionaily distinct subpopulation found in Victoria Land, Antarctica. This population of H4-6 chondrites is compositionally distinct from non-Antarctic H4-6 chondrites and from Antarctic H4-6 chondrites from Queen Maud Land. Comparisons of Queen Maud Land H4-6 chondrites with non-Antarctic H4-6 chondrites do not give reason to believe that these two populations are distinguishable from each other on the basis of the ten volatile trace element concentrations measured. ANOVA indicates that these differences are not the result of trivial causes such as weathering and analytical bias. Thermoluminescence properties of these populations parallels the results of volatile trace element comparisons. Given the differences in terrestrial age between Victoria Land, Queen Maud Land, and modern H4-6 chondrite falls, these results are consistent with a variation in H4-6 chondrite flux on a 300 ky timescale. This conclusion requires the existence of co-orbital meteoroid streams. Statistical analyses of the volatile trace elemental concentrations in non-Antarctic modern falls of H4-6 chondrites also demonstrate that a group of 13 H4-6 chondrites, Cluster 1, selected exclusively for their distinct fall parameters (Dodd, 1992) is compositionally distinguishable from a control group of 45 non-Antarctic modern H4-6 chondrites on the basis of the ten volatile trace element concentrations measured. Model-independent randomization-simulations based on both linear discriminant analysis and logistic regression verify these results. While ANOVA identifies two possible causes for this difference, analytical bias and group classification, a test validation ... Text Antarc* Antarctic Antarctica Queen Maud Land Victoria Land Purdue University: e-Pubs Antarctic Queen Maud Land ENVELOPE(12.000,12.000,-72.500,-72.500) Victoria Land
institution Open Polar
collection Purdue University: e-Pubs
op_collection_id ftpurdueuniv
language English
topic Analytical chemistry|Astronomy|Astrophysics|Statistics
spellingShingle Analytical chemistry|Astronomy|Astrophysics|Statistics
Wolf, Stephen Frederic
Trace element study of H chondrites: Evidence for meteoroid streams
topic_facet Analytical chemistry|Astronomy|Astrophysics|Statistics
description Multivariate statistical analyses, both linear discriminant analysis and logistic regression, of the volatile trace elemental concentrations in H4-6 chondrites reveal compositionally distinguishable subpopulations. Observed difference in volatile trace element composition between Antarctic and non-Antarctic H4-6 chondrites (Lipschutz and Samuels, 1991) can be explained by a compositionaily distinct subpopulation found in Victoria Land, Antarctica. This population of H4-6 chondrites is compositionally distinct from non-Antarctic H4-6 chondrites and from Antarctic H4-6 chondrites from Queen Maud Land. Comparisons of Queen Maud Land H4-6 chondrites with non-Antarctic H4-6 chondrites do not give reason to believe that these two populations are distinguishable from each other on the basis of the ten volatile trace element concentrations measured. ANOVA indicates that these differences are not the result of trivial causes such as weathering and analytical bias. Thermoluminescence properties of these populations parallels the results of volatile trace element comparisons. Given the differences in terrestrial age between Victoria Land, Queen Maud Land, and modern H4-6 chondrite falls, these results are consistent with a variation in H4-6 chondrite flux on a 300 ky timescale. This conclusion requires the existence of co-orbital meteoroid streams. Statistical analyses of the volatile trace elemental concentrations in non-Antarctic modern falls of H4-6 chondrites also demonstrate that a group of 13 H4-6 chondrites, Cluster 1, selected exclusively for their distinct fall parameters (Dodd, 1992) is compositionally distinguishable from a control group of 45 non-Antarctic modern H4-6 chondrites on the basis of the ten volatile trace element concentrations measured. Model-independent randomization-simulations based on both linear discriminant analysis and logistic regression verify these results. While ANOVA identifies two possible causes for this difference, analytical bias and group classification, a test validation ...
author2 Lipschutz, Michael E.
format Text
author Wolf, Stephen Frederic
author_facet Wolf, Stephen Frederic
author_sort Wolf, Stephen Frederic
title Trace element study of H chondrites: Evidence for meteoroid streams
title_short Trace element study of H chondrites: Evidence for meteoroid streams
title_full Trace element study of H chondrites: Evidence for meteoroid streams
title_fullStr Trace element study of H chondrites: Evidence for meteoroid streams
title_full_unstemmed Trace element study of H chondrites: Evidence for meteoroid streams
title_sort trace element study of h chondrites: evidence for meteoroid streams
publisher Purdue University
publishDate 1993
url https://docs.lib.purdue.edu/dissertations/AAI9334441
long_lat ENVELOPE(12.000,12.000,-72.500,-72.500)
geographic Antarctic
Queen Maud Land
Victoria Land
geographic_facet Antarctic
Queen Maud Land
Victoria Land
genre Antarc*
Antarctic
Antarctica
Queen Maud Land
Victoria Land
genre_facet Antarc*
Antarctic
Antarctica
Queen Maud Land
Victoria Land
op_source Theses and Dissertations Available from ProQuest
op_relation https://docs.lib.purdue.edu/dissertations/AAI9334441
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