Stability of reagents used for chiral amino acid analysis during spaceflight missions in high-radiation environments
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Updated: Feb 5, 2026

Enzymatic Cascade Reactions for the Synthesis of Chiral Amino Alcohols from L-lysine
Published on: February 16, 2018
Jessica S Creamer1, Maria F Mora1, Peter A Willis1
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
Abstract:
The search for biosignatures on spaceflight missions requires in situ instrumentation capable of highly selective and sensitive organic analyses. To this end, CE-LIF is a uniquely promising technique, capable of determining the type, abundance, and chirality of amino acids present in environmental samples at nanomolar concentrations. However, this type of assay requires several reagents that have not yet been used on spaceflight missions. A key concern, particularly for future missions to Europa, is the survivability of these critical components for CE separation and LIF detection under high levels of radiation. Here we present an investigation of the chemical stability of the reagents and associated fused silica capillary after a total ionizing dose of 300 krad, exceeding the predicted total ionizing dose for the potential Europa Lander Mission payload by two-fold. Neither the fused silica capillary nor the fluorescent dye (5-carboxyfluorescein succinimidyl ester) showed significant change in performance following irradiation. Following the irradiation of the pre-mixed background electrolyte, both migration time and resolution were affected. However, when the reagents (sodium tetraborate, sodium taurocholate, and γ-cyclodextrin) and the acetonitrile solution were irradiated separately and mixed afterwards, there was no change in the separation performance.
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