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Crystallisation of amorphous Mg-Fe silicates produced from microwave-dried sol-gels

Published online by Cambridge University Press:  12 October 2020

Stephen P. Thompson
Affiliation:
Diamond Light Source, Harwell Science & Innovation campus, Didcot, Oxforshire OX11 0DE, UK email: stephen.thompson@diamond.ac.uk
Anna Herlihy
Affiliation:
Diamond Light Source, Harwell Science & Innovation campus, Didcot, Oxforshire OX11 0DE, UK email: stephen.thompson@diamond.ac.uk
Claire A. Murray
Affiliation:
Diamond Light Source, Harwell Science & Innovation campus, Didcot, Oxforshire OX11 0DE, UK email: stephen.thompson@diamond.ac.uk
Annabelle R. Baker
Affiliation:
Diamond Light Source, Harwell Science & Innovation campus, Didcot, Oxforshire OX11 0DE, UK email: stephen.thompson@diamond.ac.uk
Sarah J. Day
Affiliation:
Diamond Light Source, Harwell Science & Innovation campus, Didcot, Oxforshire OX11 0DE, UK email: stephen.thompson@diamond.ac.uk
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Abstract

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Amorphous Mg-Fe silicates are produced from microwave-dried sol-gels and their thermal crystallisation is studied via in situ synchrotron X-ray powder diffraction. Mg-pyroxene crystallised to forsterite, enstatite and cristobalite. The inclusion of 10% Fe formed only forsterite at much higher temperature, while pure Mg-olivine crystallised at a lower temperature than Mg-pyroxene. Cristobalite is observed as a high-temperature crystallite in the pure-Mg compositions. Crystallisation activation energies are derived and discussed in relation to protoplanetary disks.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

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Thompson, S. P., Herlihy, A., Murray, C. A. M., Baker, A. R., Day, S. J., Smith, A. J., & Snow, T. 2019, A&A, 624, A136Google Scholar