Cosmogenic C-14 in Antarctic and non-Antarctic meteorites and lunar samples

• Main Authors: Donahue, D. J., Jull, A. J. Timothy, Burr, G. S.
• Format: Other/Unknown Material
• Language: unknown
• Published: 1994
• Subjects: ASTROPHYSICS; Antarctic; Antarc*
• Online Access: http://hdl.handle.net/2060/19940025400

We were able to develop measurements of C-14 in meteorites as a useful tool for estimates of terrestrial age. Prior to this accomplishment, only a few measurements of C-14 terrestrial ages had been made. The sample sizes were larger, and there had been no systematic study of the various parameters affecting production of C-14, such as depth dependence, and the production cross sections for C-14 from spallation amounted to a few data points. Presently, C-14 ages are an accepted terrestrial age estimate in the meteorite community, whereas before this work the few data available were difficult to interpret. We have obtained terrestrial ages not only on groups of meteorites from different geographic areas but also information on unique meteorites from particularly interesting groups, such as meteorites originating from the Moon, or SNC meteorites, which many researchers believe are derived from Mars.