Abstract

The discovery of excess ^(107)Ag (^(107)Ag*) was made in a IVB iron meteorite ten years ago. The ^(107)Ag* anomaly is inferred to be due to decay of ^(107)pd (t_(1/2)=6.5 10^6 y) and appears to provide a chronometer for the timescale of early planet formation and differentiation.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.