Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments

During their delivery to Earth, extraterrestrial dust particles (EDPs) are heated via aerodynamic braking in the upper atmosphere, liberating volatile and organic species. This study investigates the influence of atmospheric entry heating on this liberation process from Murchison (an EDP analogue),...

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Main Author: Wilson, Rebecca
Format: Thesis
Language:unknown
Published: 2010
Subjects:
Online Access:https://oro.open.ac.uk/62003/
https://oro.open.ac.uk/62003/1/13837661.pdf
https://doi.org/10.21954/ou.ro.0000f233
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spelling ftopenunivgb:oai:oro.open.ac.uk:62003 2023-06-11T04:05:38+02:00 Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments Wilson, Rebecca 2010 application/pdf https://oro.open.ac.uk/62003/ https://oro.open.ac.uk/62003/1/13837661.pdf https://doi.org/10.21954/ou.ro.0000f233 unknown https://oro.open.ac.uk/62003/1/13837661.pdf Wilson, Rebecca <http://oro.open.ac.uk/view/person/rcw93.html> (2010). Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments. PhD thesis The Open University. Thesis Public PeerReviewed 2010 ftopenunivgb https://doi.org/10.21954/ou.ro.0000f233 2023-05-28T06:00:11Z During their delivery to Earth, extraterrestrial dust particles (EDPs) are heated via aerodynamic braking in the upper atmosphere, liberating volatile and organic species. This study investigates the influence of atmospheric entry heating on this liberation process from Murchison (an EDP analogue), in order to assess the EDP contribution of biologically significant material to the early Earth. Experimental simulations used a filament pulse pyrolyser to flash heat Murchison, replicating early Earth EDP atmospheric entry conditions. These simulations determined that the dehydration of phyllosilicates, the decomposition of organic and carbonate materials released H 2 O, organic carbon and CO 2 , respectively. Further characterisation of the released organic species (using GCxGC-TOFMS) identified a range of aliphatic, aromatic, PAH, O-bearing, S-bearing and N-bearing species; including biomolecule precursors. Relative abundances of these organic species were dependant not only on simulation peak temperature and duration, but also on their reaction with other fragments, which may have led to their production as secondary products. In a complimentary study, comprehensive volatile organic analysis of Antarctic micrometeorites (AMMs) identified a range of aromatic, aliphatic, N-bearing, S-bearing, S-N-bearing and O-bearing species. Variations in the distribution of AMM aromatic species in comparison to the EDP analogue (as used in simulations) are consistent with i) the liberation of species during atmospheric entry heating ii) the alteration of organic material during Antarctic weathering processes and iii) a contribution from terrestrial sources. Alternatively, these deviations could reflect a different source (parent body) composition. This investigation demonstrates that the abundance and composition of volatile and organic species liberated and retained in EDPs during entry heating (and their subsequent atmospheric reactions), may have played a role in atmospheric and climate development. EDPs additionally served ... Thesis Antarc* Antarctic The Open University: Open Research Online (ORO) Antarctic Murchison ENVELOPE(144.250,144.250,-67.317,-67.317)
institution Open Polar
collection The Open University: Open Research Online (ORO)
op_collection_id ftopenunivgb
language unknown
description During their delivery to Earth, extraterrestrial dust particles (EDPs) are heated via aerodynamic braking in the upper atmosphere, liberating volatile and organic species. This study investigates the influence of atmospheric entry heating on this liberation process from Murchison (an EDP analogue), in order to assess the EDP contribution of biologically significant material to the early Earth. Experimental simulations used a filament pulse pyrolyser to flash heat Murchison, replicating early Earth EDP atmospheric entry conditions. These simulations determined that the dehydration of phyllosilicates, the decomposition of organic and carbonate materials released H 2 O, organic carbon and CO 2 , respectively. Further characterisation of the released organic species (using GCxGC-TOFMS) identified a range of aliphatic, aromatic, PAH, O-bearing, S-bearing and N-bearing species; including biomolecule precursors. Relative abundances of these organic species were dependant not only on simulation peak temperature and duration, but also on their reaction with other fragments, which may have led to their production as secondary products. In a complimentary study, comprehensive volatile organic analysis of Antarctic micrometeorites (AMMs) identified a range of aromatic, aliphatic, N-bearing, S-bearing, S-N-bearing and O-bearing species. Variations in the distribution of AMM aromatic species in comparison to the EDP analogue (as used in simulations) are consistent with i) the liberation of species during atmospheric entry heating ii) the alteration of organic material during Antarctic weathering processes and iii) a contribution from terrestrial sources. Alternatively, these deviations could reflect a different source (parent body) composition. This investigation demonstrates that the abundance and composition of volatile and organic species liberated and retained in EDPs during entry heating (and their subsequent atmospheric reactions), may have played a role in atmospheric and climate development. EDPs additionally served ...
format Thesis
author Wilson, Rebecca
spellingShingle Wilson, Rebecca
Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
author_facet Wilson, Rebecca
author_sort Wilson, Rebecca
title Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
title_short Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
title_full Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
title_fullStr Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
title_full_unstemmed Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments
title_sort organic material in micrometeorites: processes affecting its delivery to planetary environments
publishDate 2010
url https://oro.open.ac.uk/62003/
https://oro.open.ac.uk/62003/1/13837661.pdf
https://doi.org/10.21954/ou.ro.0000f233
long_lat ENVELOPE(144.250,144.250,-67.317,-67.317)
geographic Antarctic
Murchison
geographic_facet Antarctic
Murchison
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation https://oro.open.ac.uk/62003/1/13837661.pdf
Wilson, Rebecca <http://oro.open.ac.uk/view/person/rcw93.html> (2010). Organic Material in Micrometeorites: Processes Affecting Its Delivery to Planetary Environments. PhD thesis The Open University.
op_doi https://doi.org/10.21954/ou.ro.0000f233
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