Raman Detection Threshold Measurements for Acetic Acid in Martian Regolith Simulant JSC-1 in the Presence of Hydrated Metallic Sulfates
Keith Andrew, Kristopher A. Andrew, Melinda Thomas, Alicia, Pesterfield, Quentin Lineberry, Eric V. Steinfelds

TL;DR
This study measures the Raman detection thresholds of acetic acid in Martian regolith simulant with hydrated metallic sulfates, aiding future Mars biosignature detection efforts.
Contribution
It provides the first quantitative Raman detection thresholds for acetic acid in Martian-like conditions, informing future rover biosignature searches.
Findings
Raman peak at 1608 cm-1 identified for acetic acid detection.
Detection threshold ranges from 120 to 160 ppmv for Fe and Mg sulfates.
Raman spectroscopy can potentially detect biosignatures in Martian regolith.
Abstract
Several measurements, including the data from the laser spectrometer in the Sample Analysis at Mars instrument suite on the Curiosity Rover in Gale crater, have measured seasonal variations in atmospheric methane at the 0.7 ppbv (parts per billion volume) level. As a result, models have been proposed to understand the methane production including novel chemical, geological, meteorological, and biological mechanisms. Biological models often rely on methanogenic extremophile archaea which might be similar to some Earth based organisms which can be studied exhaustively in a laboratory setting. Such organisms might thrive in a subsurface ecosystem involving water and methane and as such could leave a unique biosignature in the Martian regolith that could be preserved over extended periods of time. The resulting mixture of carboxyl, acetyl and hydroxyl groups blended with the metallic…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Methane Hydrates and Related Phenomena
