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Noble gases in the Murchison meteorite - Possible relics of s-process nucleosynthesisThe Murchison carbonaceous chondrite contains a new type of xenon component, enriched by up to 50 percent in five of the nine stable xenon isotopes, mass numbers 128 to 132. This component is released at 1200 to 1600 C from a severely etched mineral fraction. Krypton shows a similar but smaller enrichment in the isotopes 80 and 82. Neon and helium released in the same interval also are quite anomalous, being highly enriched in the isotopes 22 and 3. These patterns are strongly suggestive of three nuclear processes believed to take place in red giants: the s process (neutron capture on a slow time scale), helium burning, and hydrogen shell burning. If this interpretation is correct, then primitive meteorites contain yet another kind of alien, presolar material: dust grains ejected from red giants.
Document ID
19780057309
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Srinivasan, B.
(Chicago Univ. Chicago, IL, United States)
Anders, E.
(Chicago, University Chicago, Ill., United States)
Date Acquired
August 9, 2013
Publication Date
July 7, 1978
Publication Information
Publication: Science
Volume: 201
Subject Category
Lunar And Planetary Exploration
Accession Number
78A41218
Funding Number(s)
CONTRACT_GRANT: NGL-14-001-010
Distribution Limits
Public
Copyright
Other

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