Abstract

We present a novel, innovative approach to gas chromatography-mass spectrometry (GC-MS) based on micro-electro-mechanical systems (MEMS) columns that improve the current, state-of-the-art by dramatically reducing the size, mass, and power resources for deploying GC for future landed missions. The outlet of the MEMS GC column was coupled to a prototype of the MAss Spectrometer for Planetary EXploration (MASPEX) through a heated transfer line into the ion source. MEMS GC-MS experiments were performed to demonstrate linearity of response and establish limit of detection (LOD) to alkanes (organics), fatty acid methyl esters (FAMEs) and chemically derivatized amino acids (biological molecules). Linearity of response to each chemical family was demonstrated over two orders of magnitude dynamic range and limit of detection (LOD) values were single to tens (4–43) of picomoles per 1 μl injection volume. MEMS GC column analytical performance was also demonstrated for a “Mega Mix” of chemical analytes including organics and biological molecules. Chromatographic resolution exceeded 200, retention time reproducibility was << 1% RSD (majority ≤ 0.3%), and peak capacity values calculated to be 124 ± 2 over a 435 s retention time window. The 5.5 m MEMS column was also shown to be a suitable alternative to traditional commercial columns for use in comprehensive two-dimensional gas chromatography (GC × GC). Mass spectra collected from MASPEX showed close consistency with National Institute of Technology (NIST) reference mass spectra and were used for high confidence identification of all eluting analytes.

Highlights

  • The search for life, whether extinct or extant, is a high-priority goal for the National Aeronautics and Space Administration’s (NASA’s) Planetary Science Division (Green et al, 2021)

  • We present the sensitivity of the mechanical systems (MEMS) GC-MS setup as well as the reproducibility of the device to demonstrate the achievements of two of the three benchmarks for life detection

  • This experiment was performed to test the linear response in terms of sample analyte injected on-column mass and the peak area response from the total ion chromatogram constructed from the microchannel plate (MCP) detector

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Summary

Introduction

The search for life, whether extinct or extant, is a high-priority goal for the National Aeronautics and Space Administration’s (NASA’s) Planetary Science Division (Green et al, 2021). Multiple astrobiology-focused mission concepts are in development to evaluate prebiotic chemistry and habitability (e.g., concentration of CHNOPS elements), to detect biosignatures, and to detect life. Another important need is to distinguish between biotic and abiotic sources of complex organics. An Enceladus life detection mission in particular has strong scientific justification based on recent findings from the Cassini mission (Cable et al, 2021) These astrobiology-focused landed mission concepts are expected to identify individual organic molecules within potentially complex mixtures at low (1 nM) concentrations (Hand et al, 2017; MacKenzie et al, 2021a, 2021b)

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