HR: 17:30h
AN: P42C-07    [PDF]
TI: Sensitive Amino Acid Composition and Chirality Analysis in the Martian Regolith with a Microfabricated in situ Analyzer
AU: * Skelley, A M
EM: alison@zinc.cchem.berkeley.edu
AF: Department of Chemistry, UC Berkeley, Berkeley, CA 94720 United States
AU: Grunthaner, F J
AF: Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 United States
AU: Bada, J L
AF: Scripps Institution of Oceanography, UC San Diego, La Jolla, CA 92093 United States
AU: Mathies, R A
EM: rich@zinc.cchem.berkeley.edu
AF: Department of Chemistry, UC Berkeley, Berkeley, CA 94720 United States
AB: Recent advances in microfabricated "lab-on-a-chip" technologies have dramatically enhanced the capabilities of chemical and biochemical analyzers. The portability and sensitivity of these devices makes them ideal instruments for in situ chemical analysis on other planets. We have focused our initial studies on amino acid analysis because amino acids are more chemically resistant to decomposition than other biomolecules, and because amino acid chirality is a well-defined biomarker [1]. Previously, we developed a prototype electrophoresis chip, detection system and analysis method where the amino acids were labeled with fluorescein using FITC and then electrophoretically analyzed using g-cyclodextrin as the chiral resolution agent [2]. Extracts of the Murchison meteorite were analyzed, and the D/L ratios determined by microchip CE closely matched those from HPLC and GCMS and exhibited greater precision. Our microchip analyzer has now been further improved by establishing the capability of performing amino acid composition and chirality analyses using fluorescamine rather than FITC [3]. Fluorescamine is advantageous because it reacts more rapidly than FITC, and because excess reagent is hydrolyzed to a non-fluorescent product. Furthermore, the use of fluorescamine facilitates interfacing with the Mars Organic Detector (MOD) [4]. Fluorescamine-amino acids are separated using similar conditions as the FITC-aa, resulting in similar separation times and identical elution orders. Fluorescamine-aa are chirally resolved in the presence of hydroxy-propyl-b-cyclodextrin, and typical limits of detection are $\sim$ 50 nM. This work establishes the feasibility of combining fluorescamine labeling of amino acids with microfabricated CE devices to develop low-volume, high-sensitivity apparatus for extraterrestrial exploration. The stage is now set for the development of the Mars Organic Analyzer (MOA), a portable analysis system for amino acid extraction and chiral analysis that will combine the capabilities of microchip CE with the previously developed extraction capabilities of MOD [4]. Amino acids are first extracted from soil by sublimation to a cold finger coated with fluorescamine for solid phase labeling. Sample transfer between MOD and the CE device is achieved through a capillary sipper driven by microfabricated valves and pumps [5]. The construction of a portable MOA instrument will facilitate in situ studies of amino acids in Mars analog sites such as the Atacama Desert in Chile. Preliminary chiral analyses of Atacama soil extracts on the microfabricated CE device have shown amino acid detection down to low ppb concentrations. Future field tests in the Atacama Desert will explore the feasibility of the portable CE device for performing in situ amino acid analysis. This work will provide the technology base for the development the Mars Organic Laboratory (MOL), a portable device that will analyze a broad suite of biomolecules, including nucleobases, sugars, and organic acids and bases [6]. [1]J.L. Bada, G.D. McDonald, Icarus 114 (1995) 139. [2]L.D. Hutt, D.P. Glavin, J.L. Bada, R.A. Mathies, Anal. Chem. 71 (1999) 4000. [3]A.M. Skelley, R.A. Mathies, J. Chromatogr. A (2003) in press. [4]G. Kminek, J.L. Bada, O. Botta, D.P. Glavin, F. Grunthaner, Planet. Space Sci. 48 (2000) 1087. [5]W.H. Grover, A.M. Skelley, C.N. Liu, E.T. Lagally, R.A. Mathies, Sens. Actuators B 89 (2003) 325. [6]A.M. Skelley, F.J. Grunthaner, J.F. Bada, R.A. Mathies, in SPIE: Proceedings of the In-Situ Instrument Technologies Meeting, Pasadena, CA, 2002.
DE: 6200 PLANETOLOGY: SOLAR SYSTEM OBJECTS (New field)
DE: 6215 Extraterrestrial materials
DE: 6225 Mars
DE: 6297 Instruments and techniques
SC: Planetary Sciences [P]
MN: 2003 Fall Meeting