Mineral phases in the Comet Halley dust particles

Details Mineral phases in the Comet Halley dust particles Mineral phases in the Comet Halley dust particles

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991geokh......789d&link_type=abstract

Geokhimiia (ISSN 0016-7525), June 1991, p. 789-795. In Russian.

Computer Science

Chemical Composition, Halley'S Comet, Interplanetary Dust, Mass Spectra, Mass Spectrometers, Minerals

Scientific paper

Results are presented of the analyses of mass spectra of 517 grains collected from the Comet Halley dust, which were performed by the dust-impact mass spectrometers Puma 1,2 on board Vega. The results indicate the presence of H, C, N, O, Na, Mg, Al, Si, S, Ca, Cr, and Fe, distributed among silicates; oxides and hydroxides; carbonates and bicarbonates; sulfates and sulfides; and nitrates, cyanides, and rhodanides. These mineral components form various mixtures with organic matter.

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