Non-destructive X-ray Spectroscopy Methods for use in Study of Iron Age-Persian Period Arrowheads's

ORAL

Abstract

Non-destructive x-ray spectroscopy methods are commonly used to determine the composition and structure of unidentified samples.~ A novel application of these methods is to use a high energy ($>$80 keV) synchrotron source in the study of archeological artifacts thereby probing the bulk material instead of just the surface. Using x-ray fluorescence and diffraction, the raw materials and methods used in manufacturing arrowheads from several Iron Age-Persian Period Middle Eastern archaeological sites were investigated.~ The fluorescence spectrum provides information about the relative composition of the bulk while the 2D diffraction pattern can yield details about the composition of the majority bronze phase as well as highlight differences in thermo-mechanical techniques.~ The results obtained from analysis of the fluorescence spectra indicate that that the arrowheads are bronze, composed primarily of a leaded copper -- tin alloy.~ Additionally, after comparing the diffraction patterns to known standards, the percent weight of tin in the bronze alloys of select artifacts was determined. The addition of lead to copper-tin alloys, which would reduce the cost of the composite metal and improve the fluidity of the melt, may be more commonplace than previously thought.~ Data from both fluorescence and diffraction spectra will be presented.

–

Authors

  • Mitchell Miller

    Illinois Institute of Technology

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO

  • John Gaddy

    University of Southern California, University of Chicago, University of Toronto, Argonne National Laboratory, Illinois Institute of Technology, University of Northern Iowa, Universite Aix-Marseille 1, Universite Montpellier 2, University of Missouri, University of Missouri, Department of Physics and Astronomy and the Missouri Research Reactor, University of Missouri, Department of Physics and Astronomy, University of Missouri, the Missouri Research Reactor, Columbia Univ, Univ of Northern Iowa, University of Charleston, NASA Goddard Space Flight Center, Iowa State University, University of Colorado, NOAO, University of Toledo, University of Massachusetts, Smith College, Observatory of Bordeaux, Spitzer Science Center, University of Chile, SAO