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  • 1
    Publication Date: 2019-06-28
    Description: During the past decade interplanetary dust particles (IDPS) have been collected in the earth's stratosphere. Isotopic studies of these particles have demonstrated that many of them are greatly enriched in deuterium and at least some of them carry this enrichment in smaller subcomponents. Deuterium enrichments of a similar magnitude are seen in simple molecules in interstellar clouds. Deuterium enrichment in IDPs can be taken as evidence for the presence of interstellar material. It is not clear at this time whether the carriers of the isotopic anomalies represent true, unaltered interstellar dust grains, or whether they represent an altered component with a molecular 'memory' of original interstellar grains. The spectra of different components in the collected dust provide suggestive matches to similar components evident in the astronomical spectra of dust in comets, dense molecular clouds, and emission nebulae. The known extraterrestrial nature of the particles, the possible presence of interstellar material in them, and their spectral similarity to many astronomical objects all argue that the collected IDPs provide useful analogs for the modelling of interstellar dust.
    Keywords: Astrophysics
    Type: NASA-TM-112437 , NAS 1.15:112437 , Interstellar Dust; 403-413
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  • 2
    Publication Date: 2019-07-13
    Description: The purpose of the 1984-1985 ANSMET (Antarctic Search for Meteorites) expedition was to recover meteorites from the Main, Near Western, Middle Western, and Far Western icefields in the Allan Hills area and to carry out a reconnaissance of other nearby blue icefields. A brief summary of the locations and maps visited are provided.
    Keywords: Astrophysics
    Type: NASA/TM-1986-112433 , NAS 1.15:112433 , Smithsonian Contributions to the Earth Sciences; 30; 5-9
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  • 3
    Publication Date: 2019-08-15
    Description: We have seen that studies of nearby star-forming regions are beginning to reveal the first signs of protoplanetary disks. Studies of interstellar and interplanetary grains are starting to provide clues about the processing and incorporation of matter into the Solar System. Studies of meteorites have yielded isotopic anomalies which indicate that some of the grains and inclusions in these bodies are very primitive. Although we have not yet detected a true interstellar grain, some of these materials have not been extensively modified since their removal from the ISM. We are indeed close to seeing our interstellar heritage. The overlap between astronomical and Solar System studies is in its infancy. What future experiments, observations, and missions can be performed in the near future that will greatly enhance our understanding of star formation and the formation of the Solar System?
    Keywords: Astrophysics
    Type: NASA-TM-112436 , NAS 1.15:112436 , Galactic and Extragalactic Star Formation; 232; 311-327|Jun 24, 1987; Whistler; Canada
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