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Remote Sensing of Craters

How has remote sensing played a role in the search for or verification of a supposed impact crater? In two ways: 1) recognition of morphological features that are compatible with an impact origin (but this does not rule out certain volcanic craters) and 2) detection of shock-induced changes that may be sensed as spectral changes. The strategy is one of simply using remote sensing to single out landform anomalies consistent with an impact origin and then seeking confirmation by on-site inspection and examination of rocks for shock metamorphic effects (their absence leads to ambiguities, making volcanic craters an alternative). At least four new impact structures have been discovered through remote sensing.

A feel for what to look for, and the variations in morphologic expression owing to differences in erosional state, at a crater site can be gained by switching again to the Geological Survey of Canada's Web Page on Impact Cratering (http://gdcinfo.agg.emr.ca/crater/world_craters.html). Go to the list of individual craters and check these especially interesting sites: North America: Brent/Clearwater East and West/ Deep Bay/ New Quebec; South America: Araguainha; Africa: Aorounga/ Bosumtwi/Rotor Kamm/Vredefort; Europe: Ries; Asia: Bigach/Popigai; Australia: Henbury/Wolfe Creek.

With this practice behind you, we challenge you to find the crater in this Landsat scene:

If you succeed in the hunt, you will have pinpointed the 6 km (4 mile) wide Goat Paddock crater in Western Australia (click here for a closeup view [Goat Paddock2]). Interior Australia is the home of perhaps the most dramatic exposure of the central peak of a complex crater anywhere in the world, seen below in this aerial oblique view of a ringed mountain at the Gosses Bluff Crater.

The 6 km (4 mile)-wide ring consists of layers of resistant sandstone tilted at steep angles as the strata were driven upwards on end during the rebound of the crater floor into the peak. They have since been breached so that the lower interior now exposes softer rocks being eroded away. In the Large Format Camera photo below, taken from the Shuttle, this central peak stands out in sharp contrast to the folded rocks of the McDonnel Range to its north.

The outer sections of the crater have been nearly obliterated through erosion but are faintly expressed as a dark band in the photo; field studies show the approximate diameter of the full crater to be 22 km (14 miles).

Water often fills complex craters sufficiently intact to retain a central depression. A Seasat radar image of the Elgygytgyn Crater in Siberia (diameter = 18 km [12 miles]) is a good example; the aerial oblique view offers a different perspective.



A different kind is Manicouagan, a 100 km (60+ mile) structure in southern Quebec of Canada which has a great central peak area of igneous and metamorphic rocks, among which are feldpar-rich rocks in which much of the feldspar has transformed by shock into glass, known as maskelynite. Like Manson, there is a depression or moat between peak and (now eroded) rim that formed annular valleys which filled with water when a hydroelectric power dam blocked the draining rivers.

Because of this outline, astronauts journeying back from the Moon could see this crater from well out in space.

A SIR-B radar image of southern Ontario highlights two juxtaposed but unrelated craters, that are very different in age, in size, and in structural state.

The partially circular lake-filled structure on the right (east) is the 8 km (5 mile) wide Wanapitei crater estimated to have been formed 34 m.y. ago. The far larger Sudbury structure is evidenced by a pronounced elliptical pattern, more strongly expressed by the low hills to the north. This huge impact crater (some argue it was at least 245 km [150 miles] across when it was circular) was created about 1800 million years ago. It was subsequently deformed by the strong northwestward thrusting of the Grenville Province terrane against the Superior Province (containing Sudbury) more than 900 million years later. After Sudbury was initially excavated, magmas from deep in the crust invaded the breccia filling to emplace against its walls (some investigators think that the resulting norite rocks are actually melted target rocks). This igneous rock is host to vast deposits of nickel and copper, making this impact structure a multi-billion dollar source of ore minerals.

Radar can sharpen the appearance of an impact structure, as demonstrated with this aerial radar image of the Haughton crater (24 km; 15miles wide) in Canada. Although about 23 million years old, much of the crater's morphology has survived erosion.


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Code 935, Goddard Space Flight Center, NASA
Written by: Nicholas M. Short, Sr. email: nmshort@epix.net
and
Jon Robinson email: Jon.W.Robinson.1@gsfc.nasa.gov
Webmaster: Bill Dickinson Jr. email: rstwebmaster@gsti.com
Web Production: Christiane Robinson, Terri Ho and Nannette Fekete
Updated: 1999.03.15.