title: Next generation laser-based standoff spectroscopy techniques for Mars exploration.
abstract: In the recent Mars 2020 Rover Science Definition Team Report, the National Aeronautics and Space Administration (NASA) has sought the capability to detect and identify elements, minerals, and most importantly, biosignatures, at fine scales for the preparation of a retrievable cache of samples. The current Mars rover, the Mars Science Laboratory Curiosity, has a remote laser-induced breakdown spectroscopy (LIBS) instrument, a type of quantitative elemental analysis, called the Chemistry Camera (ChemCam) that has shown that laser-induced spectroscopy instruments are not only feasible for space exploration, but are reliable and complementary to traditional elemental analysis instruments such as the Alpha Particle X-Ray Spectrometer. The superb track record of ChemCam has paved the way for other laser-induced spectroscopy instruments, such as Raman and fluorescence spectroscopy. We have developed a prototype remote LIBS-Raman-fluorescence instrument, Q-switched laser-induced time-resolved spectroscopy (QuaLITy), which is approximately 70 000 times more efficient at recording signals than a commercially available LIBS instrument. The increase in detection limits and sensitivity is due to our development of a directly coupled system, the use of an intensified charge-coupled device image detector, and a pulsed laser that allows for time-resolved measurements. We compare the LIBS capabilities of our system with an Ocean Optics spectrometer instrument at 7 m and 5 m distance. An increase in signal-to-noise ratio of at least an order of magnitude allows for greater quantitative analysis of the elements in a LIBS spectrum with 200-300 μm spatial resolution at 7 m, a Raman instrument capable of 1 mm spatial resolution at 3 m, and bioorganic fluorescence detection at longer distances. Thus, the new QuaLITy instrument fulfills all of the NASA expectations for proposed instruments.
authors.affiliation: Hawai'i Institute for Geophysics and Planetology, University of Hawai'i, Mānoa, 1680 East West Road, Honolulu, Hawai'i 96822 USA.
authors.forename: Patrick J
authors.initials: PJ
authors.lastname: Gasda
authors.forename: Tayro E
authors.initials: TE
authors.lastname: Acosta-Maeda
authors.forename: Paul G
authors.initials: PG
authors.lastname: Lucey
authors.forename: Anupam K
authors.initials: AK
authors.lastname: Misra
authors.forename: Shiv K
authors.initials: SK
authors.lastname: Sharma
authors.forename: G Jeffrey
authors.initials: GJ
authors.lastname: Taylor