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Organic chemistry and mineral interactions in the solar system

Abstract

dc:description.abstract

The objective of this project was to develop methods to detect meteoritic organic compounds in situ, and to detelmine whether any associations exist between specific classes of compound and co-located minerals, thus indicating a possible common origin. Carbonaceous chondrites, (which comprise a small proportion of meteorites), contain a few per cent of organic material, heterogeneously distributed within their structure, the major part being macromolecular ("insoluble organic material", lOM). Model compounds were covalently bonded to "molecular tags", atoms or groups not normally present in meteorites, enabling easier detection against background signals when using analytical methods suitable for use in situ, such as Raman spectroscopy or SEM. Also, extra functionality was introduced to model compounds by ozone treatment, allowing a greater density of tags to be attached. Following development work with terrestrial models, meteorite samples were exposed to ozone, but oxalic acid was formed instead of the expected oxygenated IOM derivative. To determine if this result was due to an effect of the minerals present, whole rock samples and demineralised IOM were analysed, both before and after exposure to ozone. Isolated IOM behaved differently from that still in situ. Fresh samples ofIOM were isolated (using two literature methods), and their reactions and properties compared. The evidence obtained indicated that the structure of IOM had been modified on isolation, and that the modifications caused by the two methods were different. This shows that any data generated from isolated IOM does not necessarily directly relate to organic material still present within a meteorite. Using the data obtained in this study, and that previously reported, two-component models for the structure of lOM, and scenarios for its formation, were discussed.

Degree

thesis:*
Name dc:type.qualificationname
phd
Level dc:type.qualificationlevel
doctoral
Grantor dc:publisher.institution
The Open University
Year dc:date.issued
2013

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Goodyear, Michael David

Rights

Language dc:language
en

Chain of custody

source
Harvested from
The Open University
Base URL
oro.open.ac.uk/cgi/oai2
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
related terms
citation

Goodyear, Michael David. Organic chemistry and mineral interactions in the solar system. doctoral thesis, The Open University, 2013.