Share Email Print

Proceedings Paper

Trace isotopic analysis of micron-sized grains: Mo and Zr analysis of stardust (SiC and graphite grains)
Author(s): Michael J. Pellin; Guenther K. Nicolussi
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

Secondary Neutral Mass Spectrometry using resonant laser ionization can provide for both high useful yields and high discrimination while maintaining high lateral and depth resolutions. An example of the power of the method is measurement of the isotropic composition of Mo and Zr in 1-5 micrometers presolar SiC and graphite grains isolated form the Murchison CM2 meteorite for the first time. These grains have survived the formation of the Solar System, and isotopic analysis reveals a record of the stellar nucleosynthetic processes known as s-, p-, and r-process. Successful isotopic analysis of these elements requires both high selectivity and high efficiency. Resonant ionization spectroscopy is particularly useful and flexible in this application. While the sensitivity of this technique has often been reported in the past, we focus here on the very low noise properties of the technique. We further demonstrate the efficacy of noise removal by two complimentary methods. First we use the resonant nature of the signal to subtract background signal. Second we demonstrate that by choosing the appropriate resonance scheme background can often be dramatically reduced.

Paper Details

Date Published: 15 May 1998
PDF: 10 pages
Proc. SPIE 3270, Methods for Ultrasensitive Detection, (15 May 1998); doi: 10.1117/12.308373
Show Author Affiliations
Michael J. Pellin, Argonne National Lab. (United States)
Guenther K. Nicolussi, Argonne National Lab. and Univ. of Chicago (United States)

Published in SPIE Proceedings Vol. 3270:
Methods for Ultrasensitive Detection
Bryan L. Fearey, Editor(s)

© SPIE. Terms of Use
Back to Top