Use of Major- and Minor-Element Mapping to Measure Chemical Variability in Diogenite Pyroxenes

Details Use of Major- and Minor-Element Mapping to Measure Chemical Variability in Diogenite Pyroxenes Use of Major- and Minor-Element Mapping to Measure Chemical Variability in Diogenite Pyroxenes

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28..441s&link_type=abstract

Meteoritics, vol. 28, no. 3, volume 28, page 441

Computer Science

Achondrites, Diogenites, Electron Microprobe, Elemental Mapping, Garland, Pyroxenes, Roda

Scientific paper

Diogenite orthopyroxene grains have been shown to exhibit chemical variability within individual meteorite samples, e.g., the population groups reported by Hewins [1]. Our previous work [2] has shown a great deal of inter- and intragrain variability in OPX. The Garland diogenite, for example, appears to have two distinct populations of OPX, based on Cr/Al ratios. However, within individual crystals, excursions of Cr/Al ratios are present that may span a wide range within each population group. We are presently conducting SIMS analysis of OPX in diogenites and, therefore, the chemical variability of analyzed pyroxenes must be completely determined in order to find that portion of the crystal that most accurately records the igneous, rather than the metamorphic history. Optical analysis alone is not sufficient to categorize the pyroxene crystals. For example, numerous grains in EET 83246 appear to be zoned, with changes in interference colors toward the rims. However, EDS mapping indicates that the rims are chemically similar to the cores; the interference colors are interpreted to be due to some sort of grain abrasion process that occurred during brecciation. Backscattered image mapping at low magnification can identify intergrain variations and gross intragrain chemical variations, but this must be followed up with more detailed elemental mapping. Our microprobe employs a Link (Oxford) eXL II analyzer with full-stage automation, so that we can combine EDS maps of major elements with WDS maps of minor elements (Al, Ti, Mn, Cr). Large area maps (>1 mm) are produced using stage rastering to avoid defocusing of the WDS spectrometers. In a final step, quantitative elemental maps of target grains are produced, whereby the characteristic X-ray intensity collected at each map pixel is background suppressed and fitted against a standard intensity to yield an apparent concentration. Appropriate standards, close to the composition of the mapped grain, are used such that the apparent concentration is close to the real (ZAF-corrected) concentration. A number of grains have been mapped in Roda, Garland, EET 83246 and LEW 88008. Except for Garland, OPX grains are relatively homogeneous. Some large Roda grains show very fine (100) augite lamellae along with small augite blebs and scattered spinel along relict grain boundaries. Orthopyroxenes in Garland exhibit rare zoning and thin augite lamellae. Both symmetrical and asymmetrical zoning are evident in elemental maps; an example of nearly symmetrical zoning is shown in the Fe and Mg quantitative maps in Fig. 1, which appears in the hard copy (note a companion abstract [3] that illustrates a microprobe traverse across this grain). In addition, some grains show evidence of partial relict rims, indicating that the grains are brecciated fragments of larger, zoned grains. These brecciated pieces may explain some, but not all, of the intragrain variability seen in Garland. Because Cr decreases toward the rim while Al remains relatively constant, those fragments from the grain core will have higher Cr/Al ratios than fragments from the rim. Acknowledgment: This research was supported by NASA Grant NAGW-3347 and the Institute of Meteoritics. References: [1] Hewins R. (1980) LPSC XI, 441-443. [2] Papike J. J. et al. (1993) LPSC XXIV, 1109-110. [3] Papike J. J. and Spilde M. N. (1993), this volume.

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