2015
DOI: 10.1089/ast.2014.1220
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Selection of Portable Spectrometers for Planetary Exploration: A Comparison of 532 nm and 785 nm Raman Spectroscopy of Reduced Carbon in Archean Cherts

Abstract: Knowledge and understanding of the martian environment has advanced greatly over the past two decades, beginning with NASA's return to the surface of Mars with the Pathfinder mission and its rover Sojourner in 1997 and continuing today with data being returned by the Curiosity rover. Reduced carbon, however, is yet to be detected on the martian surface, despite its abundance in meteorites originating from the planet. If carbon is detected on Mars, it could be a remnant of extinct life, although an abiotic sour… Show more

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Cited by 21 publications
(16 citation statements)
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“…This OM is interpreted to reside in the nano-pores and void spaces of Py1 and Py2. The relative heights and shapes of disorder-induced 'D' (∼1315 Δcm -1 ) and or-der-induced 'G' (∼1600 Δcm -1 ) Raman bands of the OM are consistent with literature data of thermally mature Archean OM elsewhere in the Dresser Formation (Harris et al, 2015). This characteristic precludes an origin of OM in the stromatolites from post-metamorphic contamination.…”
Section: Organic Matter In Sulfidesupporting
confidence: 89%
“…This OM is interpreted to reside in the nano-pores and void spaces of Py1 and Py2. The relative heights and shapes of disorder-induced 'D' (∼1315 Δcm -1 ) and or-der-induced 'G' (∼1600 Δcm -1 ) Raman bands of the OM are consistent with literature data of thermally mature Archean OM elsewhere in the Dresser Formation (Harris et al, 2015). This characteristic precludes an origin of OM in the stromatolites from post-metamorphic contamination.…”
Section: Organic Matter In Sulfidesupporting
confidence: 89%
“…This band results from the movement of the oxygen atom in a Si-O-Si, a totally symmetric stretching mode. This band indicates the presence of crystalline silica (SiO 2 ) [13]. We observed similar bands at other spots of the Shivalinga.…”
Section: Resultssupporting
confidence: 80%
“…A similar argument was made for the width of the D1 peak (FWHM(D1)) as correlated to maturity [52] and showing a good correlation with burial temperature down to 150 °C. However, when a non-negligible fraction of H is within a non-aromatic structure in OM, this correlation no longer applies [6,37,61] or at least is not necessarily expected. Indeed, when D1/(G+D2) vs H:C is plotted for the PPRG sample set (Fig.…”
Section: Resultsmentioning
confidence: 99%