The dust grains from 9P/Tempel 1 before and after the encounter with Deep Impact

Science

Volumn 310, Issue 5746, 2005, Pages 278-280

  Harker, David E ^a   Woodward, Charles E ^b   Wooden, Diane H ^c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b University of Minnesota   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AMORPHOUS MATERIALS; ASTROPHYSICS; CRYSTALLINE MATERIALS; MAGNESIUM PRINTING PLATES; OLIVINE; PLANETS; SILICATES; SPECTRUM ANALYZERS;

DEEP IMPACT; GEMINI-N; SPECTRAL ENERGY DISTRIBUTION;

DUST;

CARBON; OLIVINE; PYROXENE; SILICATE; UNCLASSIFIED DRUG;

COMET;

ARTICLE; ASTRONOMY; COMET; COMET 9P/TEMPEL 1; DEEP IMPACT PROGRAM; DUST; ENERGY TRANSFER; MASS; MATHEMATICAL ANALYSIS; PARTICLE RADIATION; PRIORITY JOURNAL; SPACE FLIGHT; SPECTROSCOPY;

COSMIC DUST; METEOROIDS; ORGANIC CHEMICALS; SILICATES; SPECTROPHOTOMETRY, INFRARED;

EID: 26844485951     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1119143     Document Type: Article

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32. D.E.H. and C.E.W. acknowledge support from the NSF (AST03-07466). D.E.H. and D.H.W. acknowledge support from the NASA Planetary Astronomy Program (RTOP 344-32-21-04). We thank S. Fisher, C. Trujillo, and C. Trancho for their support Based on observations obtained at the Gemini Observatory (Gemini observing program GN-2005A-DD-9), which is operated by the Association of Universities for Research in Astronomy, Inc. under a cooperative agreement with the NSF on behalf of the Gemini partnership: the NSF (United States), the Particle Physics and Astronomy Research Council (UK), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil), and CONICET (Argentina).