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Cosmic-ray exposure history at Taurus-LittrowRecent surface history at Taurus-Littrow is dominated by emplacement of the Central Cluster and Bright Mantle morphological units, both believed to have resulted from arrival of ejecta from a large primary crater, probably Tycho. This paper reports new noble gas data for eight Apollo 17 rocks. Kr-81 - Kr cosmic ray exposure ages for these rocks affirm the observation of a pronounced grouping of ages, reinforcing the photogeologic evidence for the site-wide nature of the Central Cluster event. The consequences of post-cratering shielding changes are considered and it is concluded that the differences can reasonably be attributed to these changes, particularly because of the greater likelihood of rollover and impact fragmentation of the relatively smaller rocks from which most age data have been obtained. These considerations also lead to a more refined age estimate of 109 plus or minus 4 m.y. for Central Cluster, the Bright Mantle, and Tycho.
Document ID
19780057817
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Drozd, R. J.
(Washington Univ. Saint Louis, MO, United States)
Hohenberg, C. M.
(Washington Univ. Saint Louis, MO, United States)
Morgan, C. J.
(Washington Univ. Saint Louis, MO, United States)
Podosek, F. A.
(Washington Univ. Saint Louis, MO, United States)
Wroge, M. L.
(Washington University St. Louis, Mo., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 14, 1977
End Date: March 18, 1977
Accession Number
78A41726
Funding Number(s)
CONTRACT_GRANT: NSG-07016
CONTRACT_GRANT: NGL-26-008-065
Distribution Limits
Public
Copyright
Other

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