Mathematics – Logic
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p51g1201w&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #P51G-1201
Mathematics
Logic
[5494] Planetary Sciences: Solid Surface Planets / Instruments And Techniques, [6281] Planetary Sciences: Solar System Objects / Titan, [9805] General Or Miscellaneous / Instruments Useful In Three Or More Fields
Scientific paper
This contribution will describe the initial stages of a new ASTID-funded research program initiated in Fall 2009 aimed at lab-on-a-chip system development for astrobiological investigations on Titan. This technology development builds off related work at JPL and Berkeley [1-3] on the ultrasensitive compositional and chiral analysis of amino acids on Mars in order to search for signatures of past or present life. The Mars-focused instrument system utilizes a microcapillary electrophoresis (μCE) system integrated with on-chip perfluoropolyether (PFPE) membrane valves and pumps for automated liquid sample handling, on-chip derivitization of samples with fluorescent tags, dilution, and mixing with standards for data calibration. It utilizes a four-layer wafer stack design with CE channels patterned in glass, along with a PFPE membrane, a pneumatic manifold layer, and a fluidic bus layer. Three pneumatically driven on-chip diaphragm valves placed in series are used to peristaltically pump reagents, buffers, and samples to and from capillary electrophoresis electrode well positions. Electrophoretic separation occurs in the all-glass channels near the base of the structure. The Titan specific lab-on-a-chip system under development here focuses its attention on the unique organic chemistry of Titan. In order to chromatographically separate mixtures of neutral organics such as polycyclic aromatic hydrocarbons (PAHs), the Titan-specific microfluidic platform utilizes the related technique of microcapillary electrochromatography (μCEC). This technique differs from conventional μCE in that microchannels are filled with a porous stationary phase that presents surfaces upon which analyte species can adsorb/desorb. It is this additional surface interaction that enables separations of species critical to the understanding of the astrobiological potential of Titan that are not readily separated by the μCE technique. We have developed two different approaches for the integration of these stationary phases into microdevices, both by the packing of submicron-sized beads, and by the growth of porous polymer monoliths inside empty channels via a photoinitiated chemical polymerization process. References: 1. “Monolithic photolithographically patterned Fluorocur™ PFPE membrane valves and pumps for in situ planetary exploration”, P. A. Willis et al., Lab Chip 8, 1024 (2008). 2. “The Urey Instrument: An Advanced In Situ Organic and Oxidant Detector for Mars Exploration”, A. Aubrey et al., Astrobiology 8, 583 (2008). 3. “Development and evaluation of a microdevice for amino acid biomarker detection and analysis on Mars” A. M. Skelley et al., PNAS 102, 1041 (2005).
Fisher Andrew
Greer Frank
Grunthaner Frank
Harrison Janalee
Hodyss R. P.
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