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Geology; August 2003; v. 31; no. 8; p. 669-672; DOI: 10.1130/G19552.1
© 2003 Geological Society of America
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Imaging the mountainless root of the 1.8 Ga Cheyenne belt suture and clues to its tectonic stability

Jason A. Crosswhite1 and Eugene D. Humphreys1

1 Department of Geological Sciences, 1272 University of Oregon, Eugene, Oregon 97403, USA

Receiver-function analysis across the Cheyenne belt, an Archean–Proterozoic suture, images a 100-km-wide zone of 50–60-km-thick crust. This thick crust is thought to be a remnant from the original 1.8 Ga suturing event. The thick and presumably buoyant crust is remarkable in that it is not associated with a large topographic or gravitational anomaly, suggesting isostatic balance and a high-density mass at depth to compensate the crustal root. These features could account for the lithosphere's long-term stability. The presence of eclogite below the crustal root is a likely source for the high-density mass, as it would not produce a seismically unusual Moho, yet it would provide the required excess mass.

Key Words: seismic discontinuities • seismic studies • suture zones • isostasy • Cheyenne belt




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