By analyzing impact glass, the evolution of the impact melt at the Mistastin Lake impact structure was investigated. Impact glass clasts are present in a range of impactites, including polymict breccias and clast-rich impact melt rock, and from a variety of settings within the crater. From the glass clasts analyzed, three petrographic subtypes of impact glass were identified based on their clast content, prevalence of schlieren, color, texture, and habit. Several alteration phases were also observed replacing glass and infilling vesicles; however, textural observations and quantified compositional data allowed for the identification of pristine impact glass. Although the various types of glasses show significant overlap in their major oxide composition, several subtle variations in the major oxide chemistry of the glass were observed. To investigate this variation, a least-squares mixing model was implemented utilizing the composition of the glass and the known target rock chemistry to model the initial melt composition. Additionally, image analysis of the glass clasts was used to investigate whether the compositional variations correlated to textural difference in the lithologies. We propose that the textural and compositional dichotomy observed is a product of the evolution, assimilation, and emplacement of the glass. The dichotomy is reflective of the melt either being ballistically emplaced (group 2 glasses: occurring in melt-poor polymict breccias at lowermost stratigraphic position outside the transient crater) or the result of late-stage melt flows (group 1 glasses, occurring in melt-bearing polymict breccias and impact melt rocks at higher stratigraphic positions outside the transient crater).
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Smithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USASmithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USA
Corrigan, C. M.
Evans, T.
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Smithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USASmithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USA
Evans, T.
Andrews, B. J.
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Smithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USASmithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USA
Andrews, B. J.
Loring, S.
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Smithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USASmithsonian Inst, Natl Museum Amer Hist, 10th St & Constitut Ave NW, Washington, DC 20056 USA
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Univ Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Univ Western Ontario, Inst Earth & Space Explorat, London, ON N6A 5B7, CanadaUniv Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Tolometti, G. D.
Erickson, T. M.
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NASA Johnson Space Ctr, ARES Div, Jacobs JETS, Mailcode XI3, Houston, TX 77058 USAUniv Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Erickson, T. M.
Osinski, G. R.
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Univ Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Univ Western Ontario, Inst Earth & Space Explorat, London, ON N6A 5B7, CanadaUniv Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Osinski, G. R.
Cayron, C.
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Ecole Polytech Fed Lausanne EPFL, PX Grp Chair, Lab ThermoMech Met LMTM, Rue Maladiere 71b, Neuchatel CH-2000, SwitzerlandUniv Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Cayron, C.
Neish, C. D.
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Univ Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada
Univ Western Ontario, Inst Earth & Space Explorat, London, ON N6A 5B7, CanadaUniv Western Ontario, Dept Earth Sci, London, ON N6A 5B7, Canada