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Noachian and Hesperian modification of the original Chryse impact basin topographyWe prospose a new center and ring assignment for the original Chryse impact basin based upon photogeologic mapping of Noachian outcrops and re-examination 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 outlfow channels.
Document ID
19950056940
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Stockman, S. A.
(Science Systems and Applications, Lanham, MD United States)
Frey, H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
May 15, 1995
Publication Information
Publication: Geophysical Research Letters
Volume: 22
Issue: 10
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
95A88539
Funding Number(s)
PROJECT: RTOP 151-02-50
Distribution Limits
Public
Copyright
Other

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