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Detailed Reference Information |
Stockman, S.A. and Frey, H. (1995). Noachian and Hesperian modification of the original chryse impact basin topography. Geophysical Research Letters 22: doi: 10.1029/95GL01111. issn: 0094-8276. |
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We propose a new center and ring assignment for the original Chryse impact basin based upon photogeologic mapping of Noachian outcrops and re-examinations of the published geology using orthographic projections. While others have centered the Chryse impact on the topographic low associated with Hesperian volcanic and fluvial deposits, we suggest that the center of the Noachian-age excavation cavity was located approximately 800 km to the north, and that the basin topography was modified significantly from the Noachian into the Hesperian. Evolution of the topographic low included structural modification by a later impact centered in Acidalia, restricted volcanic deposition and loading, localized subsidence, and restricted deposition from the circum-Chryse outflow channels. ¿ American Geophysical Union 1995 |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Impact phenomena (includes cratering), Planetology, Solid Surface Planets, Surface materials and properties, Tectonophysics, Planetary tectonics |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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