Computer Science
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.315..733r&link_type=abstract
Nature (ISSN 0028-0836), vol. 315, June 27, 1985, p. 733-736.
Computer Science
33
Carbon, Cosmochemistry, Extraterrestrial Matter, Graphite, Meteoritic Composition, Cosmic Dust, Cosmology, Geochemistry, Low Temperature, Solar System, Temperature Effects, Samples, Extraterrestrial, Graphite, Carbon, Geochemistry, Solar System, Stratosphere, Phases, Thermal Effects, Cosmic Dust, Interplanetary Dust, Comparisons, Temperature, Electron Microscopy, Analysis, Data
Scientific paper
A description is presented for the most common carbon phase in carbon-rich chondritic porous (CP) aggregate collected from the stratosphere by NASA researchers as part of the Cosmic Dust Program. An extraterrestrial origin was confirmed for the samples by microscopic examinations. The sample grains contained 45 percent carbon-rich phases and 30 percent low-temperature phases. Studies of the d002 interlayer spacing of the carbon clumps indicated that graphitization occurred at metamorphic temperatures after solar nebular condensation, yet early in solar system formation. Graphitized terrestrial materials served as a useful reference against which the CP materials were compared.
MacKinnon Ian D. R.
Rietmeijer Frans J. M.
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