GSECARS Synchrotron Facility for Planetary Science Research

Overview
GSECARS receives funding from NASA’s Research Facilities for Planetary Science program (https://science.nasa.gov/researchers/planetary-science-enabling-facilities) to support planetary science research conducted by NASA-funded investigators using some of our beamlines. This support is focused primarily on experiments using the 13-ID-E X-ray microprobe and the 13-BM-D the full-field computed microtomography (CMT) instrument, which are the GSECARS instruments most heavily used by researchers in this field.
NASA-funded researchers receive assistance in experiment design and sample preparation to ensure that prepared samples are optimized for synchrotron analysis, particularly to take full advantage of the new beamline capabilities provided by the Advanced Photon Source upgrade (APS-U). This funding also supports data collection, data interpretation, and publication preparation using these beamlines.
Access is through the APS General User Program involving peer-review of beam time proposals. Support for focused ion beam section preparation at the University of New Mexico is also offered to planetary science researchers that require it through this program.
Main Techniques
X-ray Fluorescence (µXRF) mapping: Compositional analysis and mapping for elements with ~ 1 µm focused spot size and X-ray emission energies between ~ 2-28 keV. Multiple elements can be analyzed simultaneously. Minimum detection limits are sample dependent, but parts-per-million level detection is typical, and ppb level detection is possible for some samples.
X-ray Absorption Fine Structure (µXAFS): Microfocused XAFS to determine the speciation (local chemistry, quantitative determination of the local geometric structure around the absorbing atom) of elements. Both µ-XANES and µ-EXAFS are possible, depending on concentration, as is oxidation state mapping. For extraterrestrial materials, XAFS can be used for defining valence states of multivalent elements in minerals and glasses that can then be used as oxybarometry proxies in cosmochemical studies. Multivalent elements of particular importance to earth and planetary science studies include S, Ti, V, Mn, Cr, Eu, and Fe.
X-ray Diffraction (µXRD): Microdiffraction analysis for mineral identification with spatial resolutions of ~ 1 µm. Area detector readout at frame rates < 20 msec per frame possible using Eiger 1M area detector allowing for diffraction mapping and tomography, etc.
Fluorescence and Diffraction Computed Microtomography (fCMT and dCMT): Both element specific XRF and XRD tomography with micrometer spatial resolution are available. Tomographic slices of XRF and XRD intensity through the object are then reconstructed following the same methods utilized for absorption tomography.
Full-field X-ray Computed Microtomography (CMT): Absorption tomography using the 13-BM-D bending magnet source for non-destructive 3D characterization of internal microstructures of larger samples. Used to visualize primary mineral phases and their textures, chemical zoning within crystallites, orientation relations, as well as secondary reaction products. The full-field absorption CMT apparatus consists of a single crystal scintillator (which converts X-rays to visible light), a microscope objective (that magnifies the scintillator image), and a 1920×1200 pixel fast CMOS camera. Operational modes include monochromatic beam mode for element-specific applications, pink beam mode which provides more than 1,000 times higher intensity than the monochromatic mode, and white beam mode which provides the highest flux and the highest energy X-ray spectrum, at the expense of vertical beam size.
FIB Sectioning Capability: This project includes funding to support preparation of focused ion beam sections for use at 13-ID-E using the University of New Mexico ion beam facilities. These resources are available on an as-needed basis to users of the GSECARS facilities that require this specialized sample preparation procedure.
Science Highlights
Analysis of Extraterrestrial Samples Using Focused-beam X-ray Fluorescence and Diffraction Microtomography
This study describes developments at our 13-ID-E microprobe beamline for simultaneous synchrotron-based XRF and XRD microtomographic analysis of unsectioned extraterrestrial samples. These methods provide new opportunities for spatially resolved characterization of...
Mapping the redox state of the young Solar System using ytterbium valence state
On Earth, most rare earth elements (REE) usually occur as 3+ cations. The primary exceptions being the elements europium and cerium, which can also be found as 2+ and 4+ cations respectively. In the case of ytterbium (Yb), only 3+ states have been reported so far....
Sulfur in apatite from the Nakhla meteorite record a late-stage oxidation event
Maryjo Brounce, Jeremy W. Boyce, Francis M. McCubbin,
Sulfur in apatite from the Nakhla meteorite record a late-stage oxidation event,
Earth and Planetary Science Letters,
Volume 595, 2022, 117784,, ISSN 0012-821X.
Contacts
Tony Lanzirotti
PSEF PI and Primary Contact
University of Chicago
lanzirotti@uchicago.edu
Steve Sutton
PSEF Co-I
University of Chicago
sutton@cars.uchicago.edu
Adrian Brearley
PSEF Co-I
University of New Mexico
brearley@unm.edu
Important Links
Recent Publications from NASA-funded researchers
Hammouda, T., Frossard, P., Boyet, M., Bouvier, A., Newville, M., & Lanzirotti, A. (2024). Mapping the redox state of the young Solar System using ytterbium valence state. Geochimica et Cosmochimica Acta, 372, 124-133. https://doi.org/10.1016/j.gca.2024.03.018
Antonio Lanzirotti, Stephen R. Sutton, Matthew Newville, Adrian Brearley, Oliver Tschauner, “Focused-beam X-ray fluorescence and diffraction microtomographies for mineralogical and chemical characterization of unsectioned extraterrestrial samples,” Meteorit. Planet Sci. 59 (2), 395-418 (2024). https://doi.org/10.1111/maps.14130
Black, B. A., & Brounce, M. (2023). Linking impact melt redox with crustal weathering regime. Geology, 51(10), 978-982. https://doi.org/10.1130/G51405.1
Proteek Chowdhury, Maryjo Brounce, Jeremy W. Boyce, Francis M. McCubbin, “The Oxidation State of Sulfur in Apatite of Martian Meteorite-Shergotty,” J. Geophys. Res. – Planet 128 (6), e2022JE007634 (2023). https://doi.org/10.1029/2022JE007634
M.Darby Dyar, Molly McCanta, Antonio Lanzirotti, Cody J. Steven, Cai Ytsma, “Calibration for iron redox state and oxygen fugacity in silicate glasses from x-ray absorption spectroscopy,” Chem. Geol. 635, 121605 (2023). https://doi.org/10.1016/j.chemgeo.2023.121605
Guy N. Evans, Laurence A. Coogan, Betül Kaçar, William E. Seyfried, “Molybdenum in basalt-hosted seafloor hydrothermal systems: Experimental, theoretical, and field sampling approaches,” Geochim. Cosmochim. Acta 353, 28-44 (2023). https://doi.org/10.1016/j.gca.2023.05.018
Anthony Feldman, “Climatic Influences on Incipient Alteration in Mars-Relevant Ultramafic Soils,” Ph.D., University of Nevada, Las Vegas, 2023.
Cody J. Steven, M.Darby Dyar, Molly McCanta, Matthew Newville, Antonio Lanzirotti, “Wave vector and field vector orientation dependence of Fe K pre-edge X-ray absorption features in clinopyroxenes,” Am. Mineral. 108 (9), 1754-1763 (2023). https://doi.org/10.2138/am-2022-8547
Nicholas D. Tailby, Dustin Trail, Bruce Watson, Antonio Lanzirotti, Matthew Newville, Yanling Wang, “Eu speciation in apatite at 1 bar: An experimental study of valence-state partitioning by XANES, lattice strain, and Eu/Eu* in basaltic systems,” Am. Mineral. 108 (5), 789-813 (2023). https://doi.org/10.2138/am-2022-8388
Maryjo Brounce, Jeremy W. Boyce, Francis M. McCubbin, “Sulfur in apatite from the Nakhla meteorite record a late-stage oxidation event,” Earth Planet. Sci. Lett. 595, 117784 (2022). https://doi.org/10.1016/j.epsl.2022.117784
Jon M. Friedrich, Matthiew M. Chen, Stephanie A. Giordano, Olivia K. Matalka, Juliette W. Strasser, Kirstin A. Tamucci, Mark L. Rivers, Denton S. Ebel, “Size-frequency distributions and physical properties of chondrules from x-ray computed microtomography and digital data extraction,” Microsc. Res. Techniq. 85 (5), 1814-1824 (2022). https://doi.org/10.1002/jemt.24043