Abundance of presolar grains in comet Wild 2 and implications for transport and mixing in the solar nebula.

Stadermann F. J. and Floss C. (2008)
Lunar & Planet. Sci. 39, Abstract #1889.


ABSTRACT

In early 2006 NASA's Stardust mission successfully returned samples from comet Wild 2 for laboratory analysis. Among the surprise discoveries during the preliminary examination (PE) of the cometary matter was the observation that these samples are not just mixtures of ice and interstellar grains as previously speculated, but contain significant fractions of high-temperature minerals from the inner solar system. Only a single presolar grain with extremely anomalous O isotopic composition was found during the PE, indicating a relatively low presolar grain abundance. We have continued our search for presolar material in samples from Wild 2 by performing isotope imaging searches in C, N, O, and S at high spatial resolution and located two more presolar grains in the cometary material. With this additional data we can determine the presolar grain abundance in the Wild 2 samples with better statistical significance, compare the abundance to those in other types of solar system materials, and draw conclusions about basic solar nebula properties.


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