Popigai ZH-Glasses: Origin by Initial H2O Irregularities, Unstable Shock Flow and Quenching

Details Popigai ZH-Glasses: Origin by Initial H2O Irregularities, Unstable Shock Flow and Quenching Popigai ZH-Glasses: Origin by Initial H2O Irregularities, Unstable Shock Flow and Quenching

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1026v&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1026

Astronomy and Astrophysics

Astronomy

Scientific paper

Interesting fine-banded impact glasses known in some astroblemes and
among some tektite strewn fields are highly-mobile products of initial
shock melting and mixing, bearing the traces of unstable microflow
preserved by quenching.

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