Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 2 December 1977:
Vol. 198. no. 4320, pp. 927 - 930
DOI: 10.1126/science.198.4320.927

Articles

Primordial Noble Gases in Chondrites: The Abundance Pattern Was Established in the Solar Nebula

LEO ALAERTS 1, ROY S. LEWIS 1, and EDWARD ANDERS 1

1 Enrico Fermi Institute and Department of Chemistry, University of Chicago, Chicago, Illinois 60637

Ordinary chondrites, like carbonaceous chondrites, contain primordial noble gases mainly in a minor phase comprising le0.05 percent of the meteorite, probably an iron-chromium sulfide. The neon-20/argon-36 ratios decrease with increasing argon-36 concentration, as expected if the gas pattern was established by condensation from the solar nebula, and was negligibly altered by metamorphism in the meteorite parent bodies. Meteoritic and planetary matter apparently condensed over a substantial range of temperatures.

Submitted on August 2, 1977
Revised on September 7, 1977





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)