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Raman spectroscopy in astrobiology
Abstract
Raman spectroscopy is proposed as a valuable analytical technique for planetary exploration because it is sensitive to organic and inorganic compounds and able to unambiguously identify key spectral markers in a mixture of biological and geological components; furthermore, sample manipulation is not required and any size of sample can be studied without chemical or mechanical pretreatment. NASA and ESA are considering the adoption of miniaturised Raman spectrometers for inclusion in suites of analytical instrumentation to be placed on robotic landers on Mars in the near future to search for extinct or extant life signals. In this paper we review the advantages and limitations of Raman spectroscopy for the analysis of complex specimens with relevance to the detection of bio- and geomarkers in extremophilic organisms which are considered to be terrestrial analogues of possible extraterrestial life that could have developed on planetary surfaces.
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“Raman spectroscopy has proved to be very successful in detecting the complex biomolecules of microbial colonies in the most hostile environments on Earth, and has the advantage of no requirement for reagents or sample preparation, although Raman scattering is a photon-inefficient process (Ellery and Wynn-Williams, 2003; Jorge Villar and Edwards, 2006; Tarcea et al., 2008; Marshall et al., 2010).”
From The Astrobiology Primer v2.0 (2016) · cites this paper as Jorge Villar and Edwards, 2006
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Alteration Assemblages in Martian Meteorites: Implications for Near-Surface Processes
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Catling, D. C. (1999) · Journal of Geophysical Research: Planets · doi:10.1029/1998je001020 · Cited by 148
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Cited by
Sorted by citations
Domagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136
“A biosignature is defined as any characteristic element, molecule, substance, or feature that can be used as evidence of past or present life and is distinct from an abiogenic Mars Arctic and Antarctic sites, including permafrost and ice surfaces in the Canadian High Arctic, Siberia, Svalbard, Norway, and the Antarcti…”
Metadata
- Authors
- Jorge Villar, S. E., & Edwards, H. G. M.
- Affiliations
- University of Bradford (GB)
- Venue
- Analytical and Bioanalytical Chemistry
- Published
- 2005-09-03
- Volume
- 384
- Issue
- 1
- Pages
- 100-113
- ISSN
- 1618-2642 (ISSN-L)
- 1618-2650
- OpenAlex
- W2012986343
- Cited by
- 157
- References
- 2
- Citations by year
- 2026: 2 · 2025: 7 · 2024: 7 · 2023: 4 · 2022: 1 · 2021: 8 · 2020: 26 · 2019: 3 · 2018: 2 · 2017: 6 · 2016: 4 · 2015: 15 · 2014: 16 · 2013: 11 · 2012: 12
- Type
- book review
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Analytical and Bioanalytical Chemistry (publishedVersion)
- PubMed (publishedVersion)
- Funders
- Engineering and Physical Sciences Research Council (EP/D03194X/1)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Life Sciences › Biochemistry, Genetics and Molecular Biology › Biophysics › Spectroscopy Techniques in Biomedical and Chemical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Keywords
- Raman spectroscopy, astrobiology, planetary exploration, Mars, biosignatures, geochemical markers, extremophiles, organic compounds, inorganic compounds, extraterrestrial life detection
- MeSH terms
- Sensitivity and Specificity, Space Flight, Spectrum Analysis, Raman, Biomarkers, Mars, Exobiology
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