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2016 Fiscal Year Final Research Report

Dating of presolar grains by nuclear cosmochronology

Research Project

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Project/Area Number 15K13602
Research Category

Grant-in-Aid for Challenging Exploratory Research

Allocation TypeMulti-year Fund
Research Field Geochemistry/Cosmochemistry
Research InstitutionTokyo Institute of Technology

Principal Investigator

Yokoyama Tetsuya  東京工業大学, 理学院, 准教授 (00467028)

Project Period (FY) 2015-04-01 – 2017-03-31
KeywordsU-Th核年代法 / プレソーラー粒子 / TIMS / r-process
Outline of Final Research Achievements

High precision analysis of U and Th abundances is key for dating presolar grains by U-Th nuclear cosmochronology. In this study, we have developed an isotope dilution TIMS method that enables the determination of 1 pg U and Th with analytical reproducibilities of 0.45% and 1.3%, respectively. The U-Th cosmochronology with this method would provide a 0.7 Gyr of uncertainty for the age of presolar grains determined.
On the other hand, we constrained the origin and evolution of r-process nuclides in the solar vicinity by a new theoretical study that combined the chemical composition of meteorites with galactic chemical evolution models and astronomical observations. Consequently, the timing of last r-process nucleosynthesis that contributed the solar system was determined to be 0.13-0.14 Gyr before the onset of solar system formation.

Free Research Field

宇宙化学

URL: 

Published: 2018-03-22  

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