Chondritic micrometeorites from the Transantarctic Mountains

On the basis of morphological and petrographic characteristics, eight “giant” unmelted micrometeorites in the 300–1100 μm size range were selected from the Transantarctic Mountain micrometeorite collection, Victoria Land, Antarctica. Mineralogical and geochemical data obtained by means of scanning e...

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Published in:Meteoritics & Planetary Science
Main Authors: van Ginneken, Matthias, Folco, Luigi, Cordier, Carole, Rochette, Pierre
Format: Article in Journal/Newspaper
Language:unknown
Published: Wiley 2012
Subjects:
Online Access:https://kar.kent.ac.uk/88125/
https://doi.org/10.1111/j.1945-5100.2011.01322.x
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spelling ftkentuniv:oai:kar.kent.ac.uk:88125 2023-05-15T13:38:02+02:00 Chondritic micrometeorites from the Transantarctic Mountains van Ginneken, Matthias Folco, Luigi Cordier, Carole Rochette, Pierre 2012-01-27 https://kar.kent.ac.uk/88125/ https://doi.org/10.1111/j.1945-5100.2011.01322.x unknown Wiley van Ginneken, Matthias, Folco, Luigi, Cordier, Carole, Rochette, Pierre (2012) Chondritic micrometeorites from the Transantarctic Mountains. Meteoritics & Planetary Science, 47 (2). pp. 228-247. ISSN 1086-9379. E-ISSN 1945-5100. (doi:10.1111/j.1945-5100.2011.01322.x <https://doi.org/10.1111/j.1945-5100.2011.01322.x>) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:88125 </88125>) QB651 Planets Minor QE515 Geochemistry Article PeerReviewed 2012 ftkentuniv https://doi.org/10.1111/j.1945-5100.2011.01322.x 2023-03-12T19:19:15Z On the basis of morphological and petrographic characteristics, eight “giant” unmelted micrometeorites in the 300–1100 μm size range were selected from the Transantarctic Mountain micrometeorite collection, Victoria Land, Antarctica. Mineralogical and geochemical data obtained by means of scanning electron microscopy, electron probe microanalyses, and synchrotron X‐ray diffraction allow their classification as chondritic micrometeorites. The large size of the micrometeorites increases considerably the amount of mineralogical and geochemical information compared to micrometeorites in smaller size fractions, therefore allowing a better definition of their parent material. A large variety of material is observed: five micrometeorites are related to unequilibrated and equilibrated ordinary chondrite, one to CV chondrite, one to CM chondrite, and one to CI chondrite parent materials. Besides reporting the first occurrence of a CV‐like micrometeorite, our study shows that the abundance of chondritic material supports observations from recent studies on cosmic spherules that a large part of the micrometeorite flux in this size range is of asteroidal origin. Article in Journal/Newspaper Antarc* Antarctica Victoria Land University of Kent: KAR - Kent Academic Repository Transantarctic Mountains Victoria Land Meteoritics & Planetary Science 47 2 228 247
institution Open Polar
collection University of Kent: KAR - Kent Academic Repository
op_collection_id ftkentuniv
language unknown
topic QB651 Planets
Minor
QE515 Geochemistry
spellingShingle QB651 Planets
Minor
QE515 Geochemistry
van Ginneken, Matthias
Folco, Luigi
Cordier, Carole
Rochette, Pierre
Chondritic micrometeorites from the Transantarctic Mountains
topic_facet QB651 Planets
Minor
QE515 Geochemistry
description On the basis of morphological and petrographic characteristics, eight “giant” unmelted micrometeorites in the 300–1100 μm size range were selected from the Transantarctic Mountain micrometeorite collection, Victoria Land, Antarctica. Mineralogical and geochemical data obtained by means of scanning electron microscopy, electron probe microanalyses, and synchrotron X‐ray diffraction allow their classification as chondritic micrometeorites. The large size of the micrometeorites increases considerably the amount of mineralogical and geochemical information compared to micrometeorites in smaller size fractions, therefore allowing a better definition of their parent material. A large variety of material is observed: five micrometeorites are related to unequilibrated and equilibrated ordinary chondrite, one to CV chondrite, one to CM chondrite, and one to CI chondrite parent materials. Besides reporting the first occurrence of a CV‐like micrometeorite, our study shows that the abundance of chondritic material supports observations from recent studies on cosmic spherules that a large part of the micrometeorite flux in this size range is of asteroidal origin.
format Article in Journal/Newspaper
author van Ginneken, Matthias
Folco, Luigi
Cordier, Carole
Rochette, Pierre
author_facet van Ginneken, Matthias
Folco, Luigi
Cordier, Carole
Rochette, Pierre
author_sort van Ginneken, Matthias
title Chondritic micrometeorites from the Transantarctic Mountains
title_short Chondritic micrometeorites from the Transantarctic Mountains
title_full Chondritic micrometeorites from the Transantarctic Mountains
title_fullStr Chondritic micrometeorites from the Transantarctic Mountains
title_full_unstemmed Chondritic micrometeorites from the Transantarctic Mountains
title_sort chondritic micrometeorites from the transantarctic mountains
publisher Wiley
publishDate 2012
url https://kar.kent.ac.uk/88125/
https://doi.org/10.1111/j.1945-5100.2011.01322.x
geographic Transantarctic Mountains
Victoria Land
geographic_facet Transantarctic Mountains
Victoria Land
genre Antarc*
Antarctica
Victoria Land
genre_facet Antarc*
Antarctica
Victoria Land
op_relation van Ginneken, Matthias, Folco, Luigi, Cordier, Carole, Rochette, Pierre (2012) Chondritic micrometeorites from the Transantarctic Mountains. Meteoritics & Planetary Science, 47 (2). pp. 228-247. ISSN 1086-9379. E-ISSN 1945-5100. (doi:10.1111/j.1945-5100.2011.01322.x <https://doi.org/10.1111/j.1945-5100.2011.01322.x>) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:88125 </88125>)
op_doi https://doi.org/10.1111/j.1945-5100.2011.01322.x
container_title Meteoritics & Planetary Science
container_volume 47
container_issue 2
container_start_page 228
op_container_end_page 247
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