2004 Denver Annual Meeting (November 7–10, 2004)

Paper No. 2
Presentation Time: 1:45 PM

QUANTITATIVE 3D PETROGRAPHY USING X-RAY TOMOGRAPHY: APPLICATION TO BISHOP TUFF PUMICE CLASTS


GUALDA, Guilherme A.R., The Department of the Geophysical Sciences, The Univ of Chicago, 5734 S. Ellis Ave, Chicago, IL 60637 and RIVERS, Mark, Consortium for Advanced Radiation Sources, The Univ of Chicago, Building 434A, 9700 South Cass Ave, Argonne, IL 60439, ggualda@uchicago.edu

Textures are traditionally studied using the petrographic microscope, which limits observations to 2D sections of 3D objects. Given the difficulty in retrieving information on shapes, sizes and spatial distribution of objects in 3D from random sections, a method that can yield observations in 3D is highly desirable.

X-ray tomography yields a 3D map of the linear x-ray attenuation coefficient, which is a function of the atomic number and density of the material, and the x-ray energy used. Based on the compositional contrasts between different phases, various phases can be identified in a rock.

Pumice clasts, characterized by isolated crystals surrounded by a low-density matrix, are ideal for the application of this technique. We present our first results obtained using x-ray tomography for pumice clasts from the Bishop Tuff. Samples studied are from units F7, F8 and Ig2Ea and are representative of the variability in density and crystal contents observed in the early erupted Bishop.

Data were collected on the GeoSoilEnvironCARS beamline at the Advanced Photon Source, Argonne National Laboratory, using a 22 keV monochromatic x-ray beam. Image analysis was performed using the software Blob3D.

Intensity contrasts in the resulting images allow the separation of magnetite, sanidine, quartz (including minor plagioclase), glass and vesicles. Crystals smaller than 5 voxels in diameter cannot be quantified properly, mostly due to noise in the images. This constrains the spatial resolution of the resulting images; there is a trade-off between sample size and spatial resolution. We employed multiple runs with samples of varying sizes (5-10 mm) to obtain adequate resolution (voxel sizes, 7-17 μm).

We have previously studied quartz size distributions in Bishop pumice clasts using a crushing, sieving, and winnowing procedure. The agreement between our new and previous results is very good; in particular, we confirm the scarcity of quartz crystals smaller than 100 μm. We also obtained magnetite and sanidine size distributions, which are similar to those for quartz, emphasizing the significance of this depletion in small crystals.

We have just obtained our first vesicle size distributions. Integrated analysis of the crystal and vesicle size data will provide a critical test for our hypothesis of bubble rising in the Bishop magma.