Sephton, M. A. and Gilmour, I.
|DOI (Digital Object Identifier) Link:||http://dx.doi.org/10.1002/mas.1006|
|Google Scholar:||Look up in Google Scholar|
The carbonaceous chondrite meteorites contain evidence of the formation of the solar system, part of which is present within organic matter. In recent years, compound-specific isotope analysis (CSIA) has been useful in deciphering this complex record. The current published data set provides an insight into the source environments and reaction mechanisms that have contributed to the final state of the organic constituents in carbonaceous chondrites. This review summarises the CSIA data and related key interpretations.
|Item Type:||Journal Article|
|Keywords:||extraterrestrial; meteorites; carbonaceous chondrites; organic molecules; isotopes; compound-specific isotope analysis; gas chromatography-isotope ratio mass spectrometry|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 6044 not found.|
|Date Deposited:||29 Jun 2006|
|Last Modified:||14 Jan 2016 15:56|
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