Carbon stable isotope analyses of individual deep-sea spherules

Details Carbon stable isotope analyses of individual deep-sea spherules Carbon stable isotope analyses of individual deep-sea spherules

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988metic..23..339w&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 23, Dec. 1988, p. 339-347. Research supported by SERC.

Computer Science

3

Carbon Isotopes, Meteoritic Composition, Ocean Bottom, Radioactive Age Determination, Spherules, Abundance, Chondrites, High Temperature Environments, Potassium Isotopes, Strontium Isotopes

Scientific paper

Melted and unmelted samples of type S and type I deep-sea spherules are analyzed to determine their carbon isotopic composition. It is shown that there are four different sorts of carbonaceous materials in the spherules. All of the samples contain two forms of low temperature combustible carbon distinguished by isotopic composition in both type S and type I spherules. A high temperature carbon with a very minor C-13 enrichment is found in unmelted type S spherules. Also, all melted samples contain small amounts of high temperature carbon with an isotopic composition suggestive of handling blank.

Affiliated with

Also associated with

No associations

Rating

Carbon stable isotope analyses of individual deep-sea spherules does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Carbon stable isotope analyses of individual deep-sea spherules, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Carbon stable isotope analyses of individual deep-sea spherules will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1758903