Compositional variation in late-stage differentiates in mare lavas, as indicated by silicate melt inclusionsQuestions regarding an interpretation of data from silicate melt inclusions are considered, taking into account the fragmental nature of the record, the possible effects of cooling rate on late-stage melt composition, and the crystallization of the trapped melt. New data related to 484 new analyses are provided in a separate table. Textural and mineralogical features and bulk chemical composition for an overall characterization of late-stage differentiates are discussed. A description is presented of a grouping and recognition of rock types on the basis of late-stage inclusion analyses. Attention is given to the bimodality of potassium values and the delineation of differentiation trends. It is found that many of the problems in interpretation and much of the scatter found in the composition of silicate melt inclusions in lunar samples can be attributed to the incomplete nature of the record and to crystallization after trapping.
Document ID
19780057751
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Roedder, E. (U.S. Geological Survey Reston, Va., United States)
Weiblen, P. W. (Minnesota, University Minneapolis, Minn., 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
78A41660
Funding Number(s)
CONTRACT_GRANT: NASA ORDER T-1170-A CONTRACT_GRANT: NSG-9050