Impact craters are ubiquitous features on solid bodies in the solar system, but on Earth they’re rather annoyingly quickly eroded. The impact crater at Sudbury, Ontario is 1.85 Byr old with an initial diameter of between 150 and 260 kilometers. Sudbury remains an oblong scar on the Canadian shield, but little remains (or has been discovered/identified) of the ejecta. A recent paper by Cannon, et al. (2010) identified several localities of ejecta deposition in Michigan.
I had the opportunity in the Spring and Fall of 2011 to participate in a field trip to the Marquette area of Michigan, where there was supposed to be 40m of impact breccia in what the authors designate the McClure locality.
Estimates of crater ejecta distribution rely on a limited dataset of “small” nuclear explosions, a couple well-preserved terrestrial craters (Ries, Barringer Meteorite, Lonar, etc), and observations of lunar craters. Ejecta thickness is seen to decay following a power law where thickness t = 0.14 * (R^0.74) * [(r/R)^-3], where R = distance from crater center to site, and r = primary or transient crater radius. Using appropriate values here (R = 500km; r = 100km) gives a calculated ejecta thickness of ~30m at the Marquette area, a surprisingly spot on result.
But don’t get too bogged down by wishes and estimates and dry writing. The Sudbury impact didn’t deposit 40 meters of ejecta at this sole locality. Everywhere, in all directions at over 500 kilometers away would have been inundated with enough material to bury a ten story building!
Our first trip out in Spring 2011 had temporary success. We searched the area for a good hour or so, and our colleagues from Northwestern University eventually drove a bit further down the road and found a small outcrop. Hooray! Unfortunately, it was in an open pit of someone’s ongoing basement construction. Despite some fast talking by professors, the group was swiftly kicked out. A bit disheartened and rather hungry, we gave up for the trip and decided to look at a map before heading out on our next trip. At GSA we talked to THE ejecta guy, the one who found the outcrop and has published several papers on samples collected therefrom. Turns out we turned left where we should have gone right…
In October we returned and had almost immediate success!
This was the first convincing piece of ejecta I found, and afterward I was too excited hunting around to take more photos. We returned the next day and found a nice – but highly weathered – continuous cropping out of ~4 meters of ejecta (still no photos), but we couldn’t find the upper or lower contacts or clear-cut glassy lapilli (supposedly concentrated near the lower contact). Close to the crater, high volumes of ejected material essentially buries the surrounding terrain. Distal (far away) ejecta has less volume but higher energy, and so it interacts with the surface more during deposition and incorporates more local terrain. I believe starting at ~2.5 crater radii from the impact, local material starts to make up the majority of the “impact” layer. Although the exact transition distance is fuzzy, at ~5 crater radii at Marquette we would certainly expect extensive incorporation of locally derived material. The impact layer at the McClure locality is supposed to lie directly over a banded iron formation, though there’s also a chert layer down there. I almost forgot to sample the site and had to grab a quick couple of samples on the way out:
To access to the locality we sampled, turn right off of County Road 510 and park on the side of the road leading to the old bridge (no longer in service). The field photo was taken in the woods to the east of the road, where there are several large boulders and some really nice, smaller outcrops. The main outcrop (and where my sample was taken) is located near the arrow in the map below. I am not sure if the land is privately owned, so be courteous if you visit. In looking closer at the Cannon paper, it appears we weren’t at the exact McClure area, which they place at 46°33′N, 87°33′W (GMap link). Maybe we’ll try to check that out next fall. This was our sampled area:
W. F. Cannon, K. J. Schulz, J. Wright Horton Jr., and D. A. Kring (2010) The Sudbury impact layer in the Paleoproterozoic iron ranges of northern Michigan, USA. GSA Bulletin, v. 122, pp. 50-75; doi:10.1130/B26517.1
F. Hörz, R. Ostertag, and D. A. Rainey (1983) Bunte breccia of the Ries: Continuous deposits of large impact craters. Reviews of Geophysics and Space Physics, v. 21, pp. 1667-1725.
T. R. McGetchin, M. Settle, and J. W. Head (1973) Radial thickness variation in impact crater ejecta: Implications for lunar basin deposits. Earth and Planetary Science Letters, v. 20, pp. 226-236.