SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains

Comet dust is primitive and shows significant diversity. Our knowledge of the properties of primitive cometary particles has expanded significantly through microscale investigations of cosmic dust samples (anhydrous interplanetary dust particles (IDPs), chondritic porous (CP) IDPs and UltraCarbonace...

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Main Authors: D. H. Wooden, H. A. Ishii, M. E. Zolensky
Format: Text
Language:unknown
Published: The Royal Society 2017
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Online Access:https://dx.doi.org/10.6084/m9.figshare.4933271
https://rs.figshare.com/articles/journal_contribution/SUPPL_Chondrites_Chondrules_Complimentarity_and_The_Depletion_Pattern_from_Cometary_dust_the_diversity_of_primitive_refractory_grains/4933271
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spelling ftdatacite:10.6084/m9.figshare.4933271 2023-05-15T13:37:49+02:00 SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains D. H. Wooden H. A. Ishii M. E. Zolensky 2017 https://dx.doi.org/10.6084/m9.figshare.4933271 https://rs.figshare.com/articles/journal_contribution/SUPPL_Chondrites_Chondrules_Complimentarity_and_The_Depletion_Pattern_from_Cometary_dust_the_diversity_of_primitive_refractory_grains/4933271 unknown The Royal Society https://dx.doi.org/10.1098/rsta.2016.0260 Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 CC-BY Astrophysics Solar System, Solar Physics, Planets and Exoplanets Interstellar and Intergalactic Matter Text article-journal Journal contribution ScholarlyArticle 2017 ftdatacite https://doi.org/10.6084/m9.figshare.4933271 https://doi.org/10.1098/rsta.2016.0260 2021-11-05T12:55:41Z Comet dust is primitive and shows significant diversity. Our knowledge of the properties of primitive cometary particles has expanded significantly through microscale investigations of cosmic dust samples (anhydrous interplanetary dust particles (IDPs), chondritic porous (CP) IDPs and UltraCarbonaceous Antarctic micrometeorites, Stardust and Rosetta ), as well as through remote sensing ( Spitzer IR spectroscopy). Comet dust are aggregate particles of materials unequilibrated at submicrometre scales. We discuss the properties and processes experienced by primitive matter in comets. Primitive particles exhibit a diverse range of: structure and typology; distribution of constituents; concentration and form of carbonaceous and refractory organic matter; Mg- and Fe-contents of the silicate minerals; sulfides; existence/abundance of type II chondrule fragments; high-temperature calcium–aluminium inclusions and ameboid-olivine aggregates; and rarely occurring Mg-carbonates and magnetite, whose explanation requires aqueous alteration on parent bodies. The properties of refractory materials imply there were disc processes that resulted in different comets having particular selections of primitive materials. The diversity of primitive particles has implications for the diversity of materials in the protoplanetary disc present at the time and in the region where the comets formed. Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics
Solar System, Solar Physics, Planets and Exoplanets
Interstellar and Intergalactic Matter
spellingShingle Astrophysics
Solar System, Solar Physics, Planets and Exoplanets
Interstellar and Intergalactic Matter
D. H. Wooden
H. A. Ishii
M. E. Zolensky
SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
topic_facet Astrophysics
Solar System, Solar Physics, Planets and Exoplanets
Interstellar and Intergalactic Matter
description Comet dust is primitive and shows significant diversity. Our knowledge of the properties of primitive cometary particles has expanded significantly through microscale investigations of cosmic dust samples (anhydrous interplanetary dust particles (IDPs), chondritic porous (CP) IDPs and UltraCarbonaceous Antarctic micrometeorites, Stardust and Rosetta ), as well as through remote sensing ( Spitzer IR spectroscopy). Comet dust are aggregate particles of materials unequilibrated at submicrometre scales. We discuss the properties and processes experienced by primitive matter in comets. Primitive particles exhibit a diverse range of: structure and typology; distribution of constituents; concentration and form of carbonaceous and refractory organic matter; Mg- and Fe-contents of the silicate minerals; sulfides; existence/abundance of type II chondrule fragments; high-temperature calcium–aluminium inclusions and ameboid-olivine aggregates; and rarely occurring Mg-carbonates and magnetite, whose explanation requires aqueous alteration on parent bodies. The properties of refractory materials imply there were disc processes that resulted in different comets having particular selections of primitive materials. The diversity of primitive particles has implications for the diversity of materials in the protoplanetary disc present at the time and in the region where the comets formed.
format Text
author D. H. Wooden
H. A. Ishii
M. E. Zolensky
author_facet D. H. Wooden
H. A. Ishii
M. E. Zolensky
author_sort D. H. Wooden
title SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
title_short SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
title_full SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
title_fullStr SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
title_full_unstemmed SUPPL. Chondrites, Chondrules, Complimentarity and The Depletion Pattern from Cometary dust: the diversity of primitive refractory grains
title_sort suppl. chondrites, chondrules, complimentarity and the depletion pattern from cometary dust: the diversity of primitive refractory grains
publisher The Royal Society
publishDate 2017
url https://dx.doi.org/10.6084/m9.figshare.4933271
https://rs.figshare.com/articles/journal_contribution/SUPPL_Chondrites_Chondrules_Complimentarity_and_The_Depletion_Pattern_from_Cometary_dust_the_diversity_of_primitive_refractory_grains/4933271
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation https://dx.doi.org/10.1098/rsta.2016.0260
op_rights Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
cc-by-4.0
op_rightsnorm CC-BY
op_doi https://doi.org/10.6084/m9.figshare.4933271
https://doi.org/10.1098/rsta.2016.0260
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