Astron. Astrophys. 364, 282-292 (2000)

Steps toward interstellar silicate mineralogy

V. Thermal evolution of amorphous magnesium silicates and silica

D. Fabian, C. Jäger, Th. Henning, J. Dorschner and H. Mutschke

University of Jena, Astrophysical Institute and University Observatory (AIU), Schillergässchen 3, 07745 Jena, Germany

Received 17 December 1999 / Accepted 26 April 2000

Abstract

The thermally induced amorphous-to-crystalline transition has been studied for bulk sheets and micrometre-sized particles of magnesium silicate glass (), nanometre-sized amorphous magnesium silicate ( and smokes) and amorphous silica particles (). Silicate glass was produced by the shock-quenching of melts. Samples of nanometre-sized smoke particles have been obtained by the laser ablation technique.

Both the and the smokes have been found to consist of two particle species; particles of smaller size ranging in diametre from 10 nm to about 100 nm and bigger size ranging from a few 100 nm to almost 3 micrometres in diametre. Nanometre-sized particles have been shown to be depleted in magnesium whereas the micrometre-sized particles were found to be enriched in Mg. Generally, the particles are composed of nonstoichiometric magnesium silicates with compositions varying even inside of the particles. Frequently, the particles contained internal voids that are assumed to have been formed by thermal shrinkage or outgassing of the particles' interior during cooling.

Annealing at 1000 K transformed the magnesium silicate smokes into crystalline forsterite (c-), tridymite (a crystalline modification of SiO₂) and amorphous silica (a-SiO₂) according to the initial Mg/Si-ratio of the smoke. Crystallization took place within a few hours for the smoke and within one day for the smoke.

The glass evolved more slowly because crystallization started at the sample surface. It has been annealed at temperatures ranging from 1000 to 1165 K. In contrast to the smoke samples, glass crystallized as orthoenstatite (). Only after 50 hours of annealing at 1000 K, weak indications of forsterite and tridymite formation have been found in the X-ray diffraction spectra.

At a temperature of 1000 K, amorphous silica nanoparticles showed distinctly lower rates of thermal evolution compared with the magnesium silicates. At 1220 K, the timescale of crystallization of a- into cristobalite and tridymite amounts to 4.5 h.

From the experiments, crystallization parameters have been obtained: activation energy and velocity of crystal growth.

The spectra shown in this study will be made publically available in the electronic database (http://www.astro.uni-jena.de ).

Key words: stars: circumstellar matter stars: formation stars: AGB and post-AGB solar system: formation methods: laboratory

Send offprint requests to: D. Fabian (fabian@astro.uni-jena.de)

SIMBAD Objects

Contents

• 1. Introduction
• 2. Observational evidence for crystalline silicates in space
  • 2.1. Meteorites
  • 2.2. IDPs and cometary grains
  • 2.3. Circumstellar environment around young stars
  • 2.4. AGB and Post-AGB stars
• 3. Basic parameters of crystallization
• 4. Experimental
  • 4.1. Preparation and sample characterization
    • 4.1.1. Magnesium silicate glass ()
    • 4.1.2. Nanometre-sized particles ( and smoke)
  • 4.2. Annealing experiments
    • 4.2.1. Bulk and micrometre-sized glass
    • 4.2.2. Annealing of smoke
    • 4.2.3. Annealing of smoke
    • 4.2.4. Summary of and smoke evolution
    • 4.2.5. Annealing of amorphous silica nanoparticles
• 5. Discussion
• 6. Conclusions
• 7. Outlook
• Acknowledgements
• References

© European Southern Observatory (ESO) 2000

Online publication: December 15, 2000
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