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Noachian and Hesperian modification of the original Chryse impact basin topographyWe propose a new center (35.5 W, 32.5 N) and ring assignment for the original Chryse impact basin based on photogeologic mapping and re-examination of the published geology. Noachian features in the Chryse Planitia area are the best indicators of the original ancient multiringed impact structure. While other workers have centered the Chryse impact on the topographic low associated with Hesperian volcanic and fluvial deposits, we suggest that the center of the original Noachian-age excavation cavity was located 800 km farther NE, and the basin topography was significantly modified over time.
Document ID
19940030956
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stockman, Stephanie
(Science Systems and Applications, Inc. Lanham, MD., United States)
Frey, Herbert
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Lunar and Planetary Inst., The Twenty-Fifth Lunar and Planetary Science Conference. Part 3: P-Z
Subject Category
Lunar And Planetary Exploration
Accession Number
94N35462
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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