Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula

Details Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..227c&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 227.

Computer Science

1

Chondrites, Magnetite, Oxygen 17, Solar Corona, Asteroids, In Situ Measurement, Nonequilibrium Conditions, Low Temperature, Solar System Evolution

Scientific paper

To better understand the formation of magnetite and low-temperature processes in the solar nebula and in the parent asteroids of the chondrites, the authors performed in situ measurements of O-isotopic compositions of magnetite in the Semarkona and Ngawi ordinary chondrites. The compositions of magnetite are cvlearly distinguished by larger Delta O-17 values (average = 5.3 per mil) from those of bulk chondrites.

Affiliated with

Also associated with

No associations

Rating

Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula 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 Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetite in unequilibrated ordinary chondrites - Evidence for an O-17-rich reservoir in the solar nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-871479