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A note against a small-body origin for shergottites, nakhlites, and chassignitesWith the possible exception of Brachina, shergottites, nakhlites, and chassignites all crystallized about 1.3 b.y. ago on the same planet, and they were probably ejected from it together about 180 m.y. ago. No breccias from the parent planet have yet been identified, thus a dominantly impact-processed surface or a small body internal melt scenario is virtually untenable. These meteorites must have formed in a magmatic complex, and on a planet from which it was difficult to remove material: as far as we know, it only happened once. Everything known about shergottites, nakhlites, and Chassigny is consistent with an igneous origin on Mars.
Document ID
19830034147
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Ryder, G.
(Northrop Services Lunar Curatorial Laboratory Houston, TX, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 15, 1982
End Date: March 19, 1982
Accession Number
83A15365
Funding Number(s)
CONTRACT_GRANT: NAS9-15425
Distribution Limits
Public
Copyright
Other

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