Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...425..274h&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 425, no. 1, p. 274-285
Astronomy and Astrophysics
Astronomy
178
Comets, Infrared Astronomy, Interplanetary Dust, Interstellar Extinction, Late Stars, Silicates, Spectrum Analysis, Chondrites, Emission Spectra, Infrared Spectroscopy, Kuiper Airborne Observatory, Olivine, Stellar Models, Comets, Composition, Spectroscopy, Spectra, Astronomy, Composition, Silicate, Grains, Comparison, Idps, Interplanetary Dust, Particles, Emissions, Model, Laboratory Studies, Pyroxene, Olivine, Mineralogy, Crystalline, Mixing, Dust, Catalog, Data, Size, Shape, Wavelength, Infrared, Analysi
Scientific paper
We have analyzed the existing spectra of seven comets which show an emission feature at 7.8-13 micrometers. Most have been converted to a common calibration, taking into account the SiO feature in late-type standard stars. The spectra are compared with spectra of the Trapezium, interplanetary dust particles (IDPs), laboratory mineral samples, and small particle emission models. The emission spectra show a variety of shapes; there is no unique 'cometary silicate'. A peak at 11.20-11.25 micrometers, indicative of small crystalline olivine particles, is seen in only three comets of this sample, P/Halley, Bradfield 1987 XXIX, and Levy 1990 XX. The widths of the emission features range from 2.6 to 4.1 micrometers (FWHM). To explain the differing widths and the broad 9.8 micrometers maximum, glassy silicate particles, including both pyroxene and olivine compositions, are the most plausible candidates. Calculations of emission models confirm that small grains of glassy silicate well mixed with carbonaceous material are plausible cometary constituents. No single class of chondritic aggregate IDPs exhibits spectra closely matching the comet spectra. A mixture of IDP spectra, particularly the glass-rich aggregates, approximately matches the spectra of comets P/Halley, Levy, and Bradfield 1987 XXIX. Yet, if comets are simply a mix of IDP types, it is puzzling that the classes of IDPs are so distinct. None of the comet spectra match the spectrum of the Trapezium. Thus, the mineralogy of the cometary silicates is not the same as that of the interstellar medium. The presence of a component of crystalline silicates in comets may be evidence of mixing between high- and low-temperature regions in the solar nebula.
Hanner Martha S.
Lynch David K.
Russell Ray W.
No associations
LandOfFree
The 8-13 micron spectra of comets and the composition of silicate grains does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The 8-13 micron spectra of comets and the composition of silicate grains, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 8-13 micron spectra of comets and the composition of silicate grains will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1255917