Mid-infrared spectral evolution of amorphous magnesium and iron silicate smokes due to vacuum annealing at T greater than or equal to 1000 K

Details Mid-infrared spectral evolution of amorphous magnesium and iron silicate smokes due to vacuum annealing at T greater than or equal to 1000 K Mid-infrared spectral evolution of amorphous magnesium and iron silicate smokes due to vacuum annealing at T greater than or equal to 1000 K

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..497h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 497.

Computer Science

Infrared Spectra, Amorphous Materials, Magnesium, Silicates, Iron Compounds, Annealing, Vacuum, Smoke

Scientific paper

A natural explanation is presented for the similarity in spectra of amorphous silicate dust from a variety of comets and stars; this is the rapid evolution of initially amorphous silicates to the 'stall' spectrum, followed by the persistence of this signature over a long timescale in a cooling environment. It is predicted that most circumstellar and interstellar silicates are only half-way to the stall spectrum.

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