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Materials and formation of the Imbrium basinA study of Imbrium basin deposits has been conducted, including geologic mapping, analysis of orbital geochemical data, earth-based near-IR spectroscopy, and analytical modeling. The morphologic facies of the deposits display an unusual bilateral symmetry with respect to the main rim of the basin, which is thought to be 1160 km in diameter and composed of Apennine-Carpathian-Alpes mountain ranges. The Imbrium ring structure consists of six concentric rings ranging from 550-3200 km in diameter. The evolution of the target for the Imbrium basin impact is discussed. It is suggested that the Imbrium impact, which occurred 3.85 Gyrs ago, formed a basin predominantly by a proportional-growth crater-forming mechanism.
Document ID
19890023491
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Spudis, Paul D.
(USGS, Branch of Astrogeology, Flagstaff AZ, United States)
Hawke, B. Ray
(Geological Survey Flagstaff, AZ, United States)
Lucey, Paul G.
(Hawaii, University Honolulu, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1988
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Country: United States
Start Date: March 16, 1987
End Date: March 20, 1987
Accession Number
89A10862
Distribution Limits
Public
Copyright
Other

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