This HiRISE image covers the southwest portion of the terraces and floor of Holden Crater situated in southwest Margaritifer Terra.

December 19, 2009

This HiRISE image covers the southwest portion of the terraces and floor of Holden Crater situated in southwest Margaritifer Terra.

Breccia is a rock typically consisting of rock fragments of various sizes and shapes that have been broken, tumbled and cemented together in sudden geologic event (e.g., a landslide, a flashflood or even an impact-cratering event). If it were not for the dark sandy dunes dispersed throughout, this image could easily fool an expert into thinking that this image is actually a photograph of a hand sample of an impact breccia.

The prefix "mega" implies that the breccia consists of clasts, or rock fragments, that are typically bigger than a large house or a building. The rectangular megaclast near the center of the image is a colossal 50 x 25 meters (approximately 150 X 75 feet). The crater likely experienced extensive modification by running water, which is supported by observations of drainage and deposition into the crater from a large channel (Uzboi Valles) breaching Holden's southwest rim.

While it is possible that the megabreccia formed from a catastrophic release of water into the crater, a more likely possibility is that it formed from the impact that created the approximately 150 kilometer-in-diameter Holden Crater. Popigai Crater, a terrestrial crater of half the size of Holden, possesses a similar occurrence of megabreccia with a comparable range in megaclast size to the Holden Crater example.

An impact-generated megabreccia deposit, as observed in terrestrial craters, typically lies beneath the crater floor, so the exhumation of the megabreccia may be the result of down-cutting and erosion of water that once flowed through Uzboi Valles.

Credits

NASA/JPL-Caltech/University of Arizona

ENLARGE

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