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Origin of picritic green glass magmas by polybaric fractional fusionA preliminary presentation is given of a model which explains the picritic lunar mare green glass compositions as composites or magmas derived by polybaric fractional melting. The model accommodates changes in source composition and solidus temperature. As in the Klein and Langmuir model, the final compositions of the melts signify only average depths of melting. The onset of melting is deeper, final segregation is shallower.
Document ID
19920048256
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Longhi, John
(Lamont-Doherty Geological Observatory Palisades, NY, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1992
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Country: United States
Start Date: March 18, 1991
End Date: March 22, 1991
Sponsors: Lunar and Planetary Institute, NASA, American Association of Petroleum Geologists
Accession Number
92A30880
Funding Number(s)
CONTRACT_GRANT: NAG9-329
Distribution Limits
Public
Copyright
Other

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