This thesis will examine the possibility of using information available from present day measured martian, terrestrial, meteoritic and solar noble gas abundances to help constrain models of planetary evolution. It is divided into four main sections. The first introductory section reviews the role of noble gases in the investigation of planetary sses and histories. It also summarises "a best current" solar system evolution and planetary accretion model.
| Identifer | oai:union.ndltd.org:bl.uk/oai:ethos.bl.uk:493950 |
| Date | January 2008 |
| Creators | Edwards, Stephen |
| Publisher | University of Manchester |
| Source Sets | Ethos UK |
| Detected Language | English |
| Type | Electronic Thesis or Dissertation |
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