Correlated microanalysis of cometary organic grains returned by Stardust |
| |
| Authors: | Bradley T De GREGORIO Rhonda M STROUD George D CODY Larry R NITTLER A L DAVID KILCOYNE Sue WIRICK |
| |
| Institution: | 1. Materials Science and Technology Division, Naval Research Laboratory, Washington, District of Columbia, USA;2. ESCG/NASA Johnson Space Center, Houston, Texas, USA;3. Geophysical Laboratory, Carnegie Institution of Washington, Washington, District of Columbia, USA;4. Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, District of Columbia, USA;5. Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California, USA;6. National Synchrotron Light Source, Brookhaven National Laboratory, Upton, New York, USA |
| |
| Abstract: | Abstract– Carbonaceous matter in Stardust samples returned from comet 81P/Wild 2 is observed to contain a wide variety of organic functional chemistry. However, some of this chemical variety may be due to contamination or alteration during particle capture in aerogel. We investigated six carbonaceous Stardust samples that had been previously analyzed and six new samples from Stardust Track 80 using correlated transmission electron microscopy (TEM), X‐ray absorption near‐edge structure spectroscopy (XANES), and secondary ion mass spectroscopy (SIMS). TEM revealed that samples from Track 35 containing abundant aliphatic XANES signatures were predominantly composed of cometary organic matter infilling densified silica aerogel. Aliphatic organic matter from Track 16 was also observed to be soluble in the epoxy embedding medium. The nitrogen‐rich samples in this study (from Track 22 and Track 80) both contained metal oxide nanoparticles, and are likely contaminants. Only two types of cometary organic matter appear to be relatively unaltered during particle capture. These are (1) polyaromatic carbonyl‐containing organic matter, similar to that observed in insoluble organic matter (IOM) from primitive meteorites, interplanetary dust particles (IDPs), and in other carbonaceous Stardust samples, and (2) highly aromatic refractory organic matter, which primarily constitutes nanoglobule‐like features. Anomalous isotopic compositions in some of these samples also confirm their cometary heritage. There also appears to be a significant labile aliphatic component of Wild 2 organic matter, but this material could not be clearly distinguished from carbonaceous contaminants known to be present in the Stardust aerogel collector. |
| |
| Keywords: | |
|
|
