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 1 May 1970:
Vol. 168. no. 3931, pp. 575 - 576
DOI: 10.1126/science.168.3931.575

Articles

Radioactivity Induced in Apollo 11 Lunar Surface Material by Solar Flare Protons

H. R. Heydegger 1 and Anthony Turkevich 2

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

Comparison of values of the specific radioactivities reported for lunar surface material from the Apollo 11 mission with analogous data for stone meteorites suggests that energetic particles from the solar flare of 12 April 1969 may have produced most of the cobalt-56 observed.





To Advertise     Find Products


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