Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments

Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the M...

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Bibliographic Details
Published in:Planetary and space science 2016-02, Vol.121, p.53-59
Main Authors: Brolly, Connor, Parnell, John, Bowden, Stephen
Format: Article
Language:English
Subjects:
Carbon
ExoMars
Extraterrestrial environments
Mars (planet)
Mars missions
Mars surface
Organic carbon
Oxidation
Oxidised carbon
Raman spectroscopy
Sediments
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Summary:Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the Martian surface. If organic carbon (one of the building blocks of life) is present within the accessible Martian sediments, it is very likely that it will have experienced some oxidation. ESA׳s ExoMars mission set to fly in 2018, has on board a miniaturised Raman spectrometer. As Raman spectroscopy is sensitive to carbonaceous material and will be primarily used to characterise organics, it is essential that the effect oxidation has on the Raman carbon signal is assessed. Oxidised carbonaceous shales were analysed using Raman spectroscopy to assess this issue. Results show that haematite has a band which occurs in the same frequency as the carbon D band, which cannot be distinguished from each other. This can lead to a misidentification of the carbon D band and a misinterpretation of the carbon order. Consequently, caution must be taken when applying Raman spectroscopy for organic carbon analysis in oxidised terrestrial and extraterrestrial environments, including on Mars. •The haematite 2LO mode occurs in the same frequency as the carbon D band.•The haematite band overprints the carbon D band in all oxidised samples.•This leads to a misidentification of the Carbon D band in oxidised samples.•The carbon order can be misinterpreted as a result of this.•Caution must be taken when using Raman spectroscopy in oxidising environments.
ISSN:0032-0633
1873-5088
DOI:10.1016/j.pss.2015.12.008