NanoSIMS

Washington University 

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Two year retrospective

June 2004

In the last two years our work with the NanoSIMS has been very successful. The downtime due to hardware problems went down dramatically and with the help of our own development efforts, we are now able to use the instrument for a large variety of scientific studies. Several significant discoveries in the study of presolar grains and IDPs have been made with the NanoSIMS in the short time this instrument has been available. This has resulted in numerous publications from our group, including four that were published in the journal Science (DAULTON et al., 2002; FLOSS et al., 2004; MESSENGER et al., 2003a; NGUYEN and ZINNER, 2004a).

Interplanetary dust particles (IDPs) are primitive samples of extraterrestrial material with a fine-grained heterogeneous matrix. We have used the NanoSIMS for extensive studies of the C, N, O, Mg/Al, Si, and S isotopic compositions of these particles on a sub-micrometer scale (FLOSS and STADERMANN, 2003; 2004; FLOSS et al., 2004; MESSENGER and KELLER, 2002; MESSENGER et al., 2003a; 2003b; STADERMANN and BRADLEY, 2003). This work led to the discovery of presolar silicates (MESSENGER et al., 2003a) and the first observation of C isotopic anomalies in these particles (FLOSS et al., 2004). Most recent results include the discovery of presolar corundum in IDPs (in preparation) and of presolar phases in Antarctic micrometeorites (in preparation).

Combined mineralogical and isotopic studies of presolar grains on TEM grids were used for the determination of SiC polytype distributions (DAULTON et al., 2002; 2003) and for the detailed characterization of high-density (CROAT et al., 2004; STADERMANN et al., 2004a) and low-density (CROAT et al., 2003a; 2003b; STADERMANN et al., 2002; 2003; 2004b) presolar graphite spherules and their sub-components. The latter project included O and Ti isotopic measurements of 100 nm sized 'presolar grains within presolar grains'.

Other lines of investigation looked at the O isotopic compositions of presolar spinel grains (ZINNER et al., 2002a; 2003b; 2004), as well as the C, N, and Si isotopic compositions of small SiC and Si3N4 particles (ZINNER et al., 2002b; 2003a). We used the multi-collection and combined mode capabilities of the NanoSIMS for C, N, O, Mg/Al, Si, K, Ca, and Ti isotopic studies of individual presolar graphites (AMARI et al., 2002; 2003a; 2004) and for C, Si, and Ti isotopic measurements in presolar SiC grains of type X and Z (AMARI et al., 2003b).

High-resolution NanoSIMS O isotopic imaging of >70,000 densely packed oxide grains was used to identify several hundred presolar spinel and corundum grains (NGUYEN et al., 2003a; 2003b; 2003c). A similar imaging study of grain size separates from Acfer 094 led to the discovery of presolar silicate stardust in meteorites (NGUYEN and ZINNER, 2004a; 2004b).

Some development work using the St. Louis NanoSIMS has been done in collaboration with CAMECA to quantify the aging characteristics of the new miniaturized electron multipliers (SLODZIAN et al., 2003) and to evaluate the 'QSA' effect (SLODZIAN et al., 2004). NanoSIMS imaging was used for test measurements of elemental distributions in aerosol particles (EBERT et al., 2004).

References

  • Amari S., Nguyen A., Zinner E., and Lewis R. S. (2002)
    Multi-element isotopic analysis of presolar graphite fraction KFA1 from the Murchison meteorite.
    Meteorit. Planet. Sci. 37, A11.
  • Amari S., Stadermann F. J., Zinner E., and Lewis R. S. (2003a)
    Continued study of presolar graphite from Murchison separate KFA1.
    Lunar Planet. Sci. XXXIV, Abstract #1864.
  • Amari S., Zinner E., Gallino R., and Lewis C. S. (2003b)
    Silicon and titanium isotopic analysis of silicon carbide grains of type X and Z.
    Meteorit. Planet. Sci. 38, A66.
  • Amari S., Zinner E., and Lewis R. S. (2004)
    Comparison study of presolar graphite separates KE3 and KFA1 from the Murchison meteorite.
    Lunar Planet. Sci. XXXV, Abstract #2103.
  • Croat T. K., Bernatowicz T., Amari S., Messenger S., and Stadermann F. J. (2003a)
    Structural, chemical, and isotopic microanalytical investigations of graphite from supernovae.
    Geochim. Cosmochim. Acta 67, 4705-4725.
  • Croat T. K., Bernatowicz T., Stadermann F. J., Messenger S., and Amari S. (2003b)
    TEM study of internal crystals in supernova graphites.
    Lunar Planet. Sci. XXXIV, Abstract #1470.
  • Croat T. K., Stadermann F. J., Zinner E., and Bernatowicz T. J. (2004)
    Coordinated isotopic and TEM studies of presolar graphites from Murchison.
    Lunar Planet. Sci. XXXV, Abstract #1353.
  • Daulton T. L., Bernatowicz T. J., Lewis R. S., Messenger S., Stadermann F. J., and Amari S. (2002)
    Polytype distribution in circumstellar silicon carbide.
    Science 296, 1852-1855.
  • Daulton T. L., Bernatowicz T. J., Lewis R. S., Messenger S., Stadermann F. J., and Amari S. (2003)
    Polytype distribution of circumstellar silicon carbide: Microstructural characterization by transmission electron microscopy.
    Geochim. Cosmochim. Acta 67, 4743-4767.
  • Ebert M., Stadermann F. J., and Weinbruch S. (2004)
    Characterization of individual aerosol particles and sampling artefacts by NanoSIMS.
    European Aerosol Conference, submitted.
  • Floss C. and Stadermann F. J. (2003)
    Complementary carbon, nitrogen and oxygen isotopic imaging of interplanetary dust particles: Presolar grains and an indication of a carbon isotopic anomaly.
    Lunar Planet. Sci. XXXIV, Abstract #1238.
  • Floss C. and Stadermann F. J. (2004)
    Isotopically primitive interplanetary dust particles of cometary origin: Evidence from nitrogen isotopic compositions.
    Lunar Planet. Sci. XXXV, Abstract #1281.
  • Floss C., Stadermann F. J., Bradley J., Dai Z. R., Bajt S., and Graham G. (2004)
    Carbon and nitrogen isotopic anomalies in an anhydrous interplanetary dust particle.
    Science 303, 1355-1358.
  • Messenger S. and Keller L. P. (2002)
    Oxygen isotopic analyses of crystalline silicates and oxides in interplanetary dust.
    Meteorit. Planet. Sci. 37, A99.
  • Messenger S., Keller L. P., Stadermann F. J., Walker R. M., and Zinner E. (2003a)
    Samples of stars beyond the solar system: Silicate grains in interplanetary dust.
    Science 300, 105-108.
  • Messenger S., Keller L. P., and Walker R. M. (2003b)
    Continued studies of stardust in IDPs.
    Lunar Planet. Sci. XXXIV, Abstract #1630.
  • Nguyen A., Zinner E., and Lewis R. S. (2003a)
    Identification of presolar spinel grains from a Murray residue by multi-detection raster imaging.
    Lunar Planet. Sci. XXXIV, Abstract #1637.
  • Nguyen A., Zinner E., and Lewis R. S. (2003b)
    Identification of small presolar oxide grains by multi-detection isotopic raster imaging.
    Meteorit. Planet. Sci. 38, A71.
  • Nguyen A., Zinner E., and Lewis R. S. (2003c)
    Identification of small presolar spinel and corundum grains by isotopic raster imaging.
    Publ. Astron. Soc. Australia 20, 382-388.
  • Nguyen A. N. and Zinner E. (2004a)
    Discovery of ancient silicate stardust in a meteorite.
    Science 303, 1496-1499.
  • Nguyen A. N. and Zinner E. (2004b)
    Discovery of presolar silicate grains in the Acfer 094 carbonaceous chondrite.
    Lunar Planet. Sci. XXXV, Abstract #1675.
  • Slodzian G., Hillion F., Stadermann F. J., and Horreard F. (2003)
    Oxygen isotopic measurements on the CAMECA Nanosims 50.
    Applied Surface Sci. 203-204, 798-801.
  • Slodzian G., Hillion F., Stadermann F. J., and Zinner E. (2004)
    QSA influences on isotopic ratio measurements.
    Applied Surface Sci. 231-232, 874-877.
  • Stadermann F. J., Bernatowicz T., Croat T. K., Zinner E., Messenger S., and Amari S. (2002)
    NanoSIMS isotopic measurements of individual TiC crystals in a single presolar graphite grain.
    Meteorit. Planet. Sci. 37, A136.
  • Stadermann F. J., Bernatowicz T., Croat T. K., Zinner E., Messenger S., and Amari S. (2003)
    Titanium and oxygen isotopic compositions of sub-micrometer TiC crystals within presolar graphite.
    Lunar Planet. Sci. XXXIV, Abstract #1627.
  • Stadermann F. J. and Bradley J. P. (2003)
    The isotopic nature of GEMS in interplanetary dust particles.
    Meteorit. Planet. Sci. 38, A123.
  • Stadermann F. J., Croat T. K., and Bernatowicz T. (2004a)
    NanoSIMS determination of carbon and oxygen isotopic compositions of presolar graphites from the Murchison meteorite.
    Lunar Planet. Sci. XXXV, Abstract #1758.
  • Stadermann F. J., Croat T. K., Bernatowicz T. J., Amari S., Messenger S., Walker R. M., and Zinner E. (2004b)
    Supernova graphite in the NanoSIMS: carbon, oxygen and titanium isotopic compositions of a spherule and its TiC sub-components.
    Geochim. Cosmochim. Acta, in press.
  • Zinner E., Amari S., Guinness R., and Jennings C. (2003a)
    Si isotopic measurements of small SiC and Si3N4 grains from the Indarch (EH4) meteorite.
    Meteorit. Planet. Sci. 38, A60.
  • Zinner E., Amari S., Guinness R., Nguyen A., and Lewis R. S. (2002a)
    Abundances and oxygen isotopic compositions of presolar spinel grains.
    Meteorit. Planet. Sci. 37, A154.
  • Zinner E., Amari S., Guinness R., Nguyen A., Stadermann F., Walker R. M., and Lewis R. S. (2003b)
    Presolar spinel grains from the Murray and Murchison carbonaceous chondrites.
    Geochim. Cosmochim. Acta 67, 5083-5095.
  • Zinner E., Amari S., Guinness R., Nguyen A., and Stadermann F. J. (2002b)
    Isotopic compositions of small presolar dust grains.
    Geochim. Cosmochim. Acta 66, A882.
  • Zinner E., Nittler L. R., Hoppe P., Gallino R., and Lewis R. S. (2004)
    Oxygen and magnesium isotopic ratios of presolar spinel grains.
    Lunar Planet. Sci. XXXV, Abstract #1337.

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