Odale-Articles-Mistastin
IMPACT CRATER EXPLORATIONS
by: Charles O'Dale
MISTASTIN IMPACT CRATER
*Maskelynite: A type of naturally occurring glass having the composition of plagioclase series feldspar, created by the vitrification of plagioclase by shock melting in meteorites and meteorite impacts. Image courtesy of NASA. |
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The Mistastin Impact Crater, a heavily eroded complex meteorite crater is technically a “central peak basin structure”. The structure’s rim includes a 26 km diameter ring of low hills that have an elevation of up to 670 m above sea level. These hills surround a depression, the centre of which is filled by the 16 km diameter Lake Mistastin. The lake surface is 338 m above sea level, and about 150 m lower than the mean regional elevation. It contains a horseshoe shaped island ~3 km in diameter, which rises ~130 m above lake level. The island consists largely of shocked basement lithologies and is the eroded remanent of a central uplift (Grieve 2006).
The crater was originally thought to be volcanic in origin. In 1968 it was confirmed as a meteorite impact site with the discovery of shock metamorphism features, specifically PDF in quartz, and poorly developed shatter cones (Taylor and Dence, 1969). |
Aerial Exploration
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The large depression made by the impact that created the Mistastin Meteorite Crater is illustrated in this image. When we cleared the western rim and entered the crater we were forced to fly below the crater rim level to stay out of the clouds.
The impact meteorite type may have been of iron composition (Wolfe et al., 1980). The target rock type is Precambrian, crystalline containing Proterozoic anorthosites, mangerite, granodiorite and quartz monzonite and exhibits a full range of shock features from brecciation to diaplectic glasses. If you ignored the lakes, the area almost looks like a moonscape. (Courtesy of NASA/LPI) Eastward moving glaciers have drastically reduced the surface expression of this structure, removing most of the impact melt sheet and breccias and exposing the crater floor. Glacial erosion has also imparted an eastward elongation to the crater that is particularly evident in the shape of the lake that occupies the central area of the structure. Isolated patches of fill and sub floor target rocks are preserved (Taylor and Dense, 1969). At the time of the impact 36 million years ago, the continents were approximately in their present positions and a moderate biological extinction had occurred which is associated with a microtektite and an iridium impregnated geological layer. The earliest apes made their appearance 10 million years later. |
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The image left was taken from about 1000’ over the western rim of the crater. On the margins of the lake are vestiges of the 80 m thick impact melt sheet that contain evidence of meteoritic features in quartz, feldspar and diaplectic glasses (maskelynite). The impact melt sheet is visible in this image as the plateau just to the left of center at the edge of the lake. In the far background the eastern rim is visible between the clouds.
The sheet of impact melt (image right - Courtesy of GISP)overlies a thin layer of breccia on the crater floor and has an exposed thickness of 80 m at its base. The melt is fine grained, glassy with numerous country rock inclusions. At higher levels it is medium grained with micro-porphyritic and poikilitic textures similar to many Apollo 16 melt rocks. Reaction, assimilation and local partial melting of the inclusions occur and the partial melts show varying degrees of mixing with the impact melt#. # The passage of the shock wave through the rock changes the structure of some of the enclosed minerals. IE: change is possible in the feldspar mineral plagioclase. The shock wave can break down the structure of the mineral, changing parts of it into a diapletic glass (glass formed at high-pressure in the solid-state) which is isotropic, or uniform in all directions. |
| We had to gain over 1000’ in altitude to safely clear the northern rim of the crater/basin. We continued our flying explorations further north. |
Side Note
| North of the Mistastin Impact Crater is some fascinating geology. In particular I wanted to share with you this image of the Fraser River Valley in Labrador, typical of the scenery we flew over in our exploration. This is one area of Canada I want to explore by foot!! |
References
Grieve, R.A.F., Impact Structures in Canada. Geological Association of Canada, 2006.
Taylor, E. C., Dence, M. R., A probable meteorite origin for Mistastin Lake, Labrador. Canadian Journal of Earth Sciences, v. 6, pp. 39-45. 1969.
Wolf, R., Woodrow, A.B. and Grieve,R.A.F., Meteoritic material at four Canadian impact craters. Geochimica et Cosmochimica Acta, v. 44, pp. 1015-1022. 1980.