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NASA NTRS · 20150011126

Using Dust from Asteroids as Regolith Microsamples

Cohen, Barbara·Chabot, Nancy·Klima, Rachel·Ernst, Carolyn·Rivkin, Andy·Postberg, Frank·Sternovsky, Zoltan
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Abstract

More robust links need to be forged between meteorites and their parent bodies to understand the composition, diversity and distribution of the asteroids. A major link can be sample analysis of the parent body material and comparison with meteorite data. Dust is present around all airless bodies, generated by micrometeorite impact into their airless surfaces, which in turn lofts regolith particles into a "cloud" around the body. The composition, flux, and size distribution of dust particles can provide insight into the geologic evolution of airless bodies. For example, the Cassini Cosmic Dust Analyzer detected salts and minerals emitted by plumes at Enceladus, evidence for a subsurface ocean with a silicate seafloor. Dust analysis instruments may enable future missions to obtain elemental, isotopic and mineralogical composition of regolith particles without returning the samples to terrestrial laboratories.

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Cohen, Barbara, Chabot, Nancy, Klima, Rachel, Ernst, Carolyn, Rivkin, Andy, Postberg, Frank, Sternovsky, Zoltan. 2015-03-16. Using Dust from Asteroids as Regolith Microsamples. https://ntrs.nasa.gov/citations/20150011126

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