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Serenitatis multi-ringed basin - Regional geology and basin ring interpretationNew topographic data allow a reassessment of the ring structure and distribution of facies of the Serenitatis basin (SB) and correlation with the younger and essentially same-size Orientale basin. Three major rings of the main (southern) SB are mapped: the Linne ring, outlined by mare ridges, average diameter 420 km; the Haemus ring, outlined by basin-facing scarps and massifs with crenulated borders, 610 km; and the Vitruvius ring, outlined by basin-facing linear scarps and massifs, 880 km. The second ring is interpreted as the rim of the transient cavity, while Serenitatis ejecta should be present in significant amounts at the junction of the Serenitatis and Imbrium third rings. The new reconstruction indicates that portions of the SB are better preserved than previously thought, consistent with recent stratigraphic and sample studies that suggest an age (as young as 3.87 plus or minus 0.04 b.y.) for SB which is older than, but close to, the time of formation of the Imbrium basin.
Document ID
19800035564
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Head, J. W., III
(Brown University Providence, R.I., United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1979
Publication Information
Publication: Moon and the Planets vol. 21
Subject Category
Lunar And Planetary Exploration
Accession Number
80A19734
Funding Number(s)
CONTRACT_GRANT: NGR-40-002-116
Distribution Limits
Public
Copyright
Other

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