Geochemical and geological units of Mare Humorum - Definition using remote sensing and lunar sample informationMare Humorum has been found to contain at least nine distinct units. Mare basalt units typical of those at the Apollo 12 and 15 sites and central Mare Serenitatis exist also in Mare Humorum, but the early, high-titanium basalts typical of Mare Tranquillitatis and southeast Mare Serenitatis are absent. Basalts containing about 5% TiO2, not sampled at any Apollo site, also are found in Mare Humorum. Emplacement of extensive low-titanium basalts occurred in Mare Humorum in roughly the same period as emplacement of similar basalts at Apollo 12 and central Mare Serenitatis. These were followed by emplacement of the higher titanium basalts during a later period. These and other units are characterized and their extent mapped using a combination of remote sensing and Apollo sample studies. The results are interpreted in the context of the evolution of the Humorum region.
Document ID
19780062849
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Pieters, C. (Massachusetts Inst. of Tech. Cambridge, MA, United States)
Mccord, T. B. (MIT Cambridge, Mass., United States)
Head, J. W. (Brown University Providence, R.I., United States)
Adams, J. B. (MIT, Cambridge, Mass.; Washington, University Seattle, Wash., United States)
Zisk, S. (Haystack Observatory Westford, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46758
Funding Number(s)
CONTRACT_GRANT: NSG-7048 CONTRACT_GRANT: NASA ORDER S-217 CONTRACT_GRANT: NGR-40-002-116 CONTRACT_GRANT: NSG-7047