Geochemistry: Supernova olivine from cometary dust

Science

Volumn 309, Issue 5735, 2005, Pages 737-741

  Messenger, Scott ^a   Keller, Lindsay P ^a   Lauretta, Dante S ^b  

^a NASA JOHNSON SPACE CENTER   (United States)

^b UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AGGREGATES; CONDENSATION; DUST; GRAIN SIZE AND SHAPE; MICROSTRUCTURE; PLANETARY SURFACE ANALYSIS; SILICATES;

EQUILIBRIUM CONDENSATION; INTERPLANETARY DUST PARTICLES; SUPERNOVA;

GEOCHEMISTRY;

NITROGEN; SILICATE; IRON DERIVATIVE; ISOTOPE; MAGNESIUM DERIVATIVE; OLIVINE; OXYGEN; SILICON;

COMET; DUST; GEOCHEMISTRY; OLIVINE;

ARTICLE; ASTRONOMY; CHEMICAL COMPOSITION; COOLING; CRYSTAL STRUCTURE; ORGANIC MATTER PRODUCTION; POLYMERIZATION; PRIORITY JOURNAL; THERMAL ANALYSIS; TRANSMISSION ELECTRON MICROSCOPY; CRYSTALLIZATION; TEMPERATURE;

COSMIC DUST; CRYSTALLIZATION; IRON COMPOUNDS; ISOTOPES; MAGNESIUM COMPOUNDS; METEOROIDS; NITROGEN; NITROGEN ISOTOPES; OXYGEN ISOTOPES; SILICATES; SILICON; TEMPERATURE;

EID: 23044472339     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1109602     Document Type: Article

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68. This is the inaugural paper from the newly established Robert M. Walker Laboratory for Space Science at Astromaterials Research and Exploration Science, NASA Johnson Space Center. This research was supported by NASA Cosmochemistry grants to S.M., L.P.K., and D.S.L. This work was enabled by the NanoSIMS ion microprobe designed by G. Slodzian. We thank A. Heger and S. Woosley for generously sharing unpublished supernova model data. The revision of this paper benefited from careful reviews by two anonymous reviewers.