Abstract
The extinct p-process nuclide 146Sm serves as an astrophysical and geochemical chronometer through measurements of isotopic anomalies of its α-decay daughter 142Nd. Based on analyses of 146Sm/147Sm α-activity and atom ratios, we determined the half-life of 146Sm to be 68 ± 7 (1σ) million years, which is shorter than the currently used value of 103 ± 5 million years. This half-life value implies a higher initial 146Sm abundance in the early solar system, (146Sm/144Sm)0 = 0.0094 ± 0.0005 (2σ), than previously estimated. Terrestrial, lunar, and martian planetary silicate mantle differentiation events dated with 146Sm-142Nd converge to a shorter time span and in general to earlier times, due to the combined effect of the new 146Sm half-life and (146Sm/144Sm)0 values.
| Original language | English |
|---|---|
| Pages (from-to) | 1614-1617 |
| Number of pages | 4 |
| Journal | Science |
| Volume | 335 |
| Issue number | 6076 |
| DOIs | |
| State | Published - 30 Mar 2012 |
Fingerprint
Dive into the research topics of 'A shorter 146Sm half-life measured and implications for 146Sm-142Nd chronology in the solar system'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver