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      Nucleosynthetic Signatures in Presolar SiC and Graphite Grains

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          Abstract

          Presolar SiC and graphite grains are the grain types whose isotopic signatures have been extensively studied. Isotopic compositions of light and intermediate elements in single grains have been analyzed mostly using secondary ion mass spectrometry. Detailed information about nucleosynthetic conditions can be obtained from isotopic compositions of heavy elements. Isotopic compositions of heavy elements in SiC and graphite grains have been analyzed using resonant ionization mass spectrometry. Analyses of heavy elements and noble gases are likely to produce new insights into presolar grains using newly-developed instruments.

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          Author and article information

          Journal
          101715666
          47003
          JPS Conf Proc
          JPS conference proceedings
          19 January 2019
          17 September 2016
          2017
          06 February 2019
          : 14
          : 010303
          Affiliations
          McDonnell Center for the Space Sciences and Physics Department, Washington University St. Louis, MO 63130, USA
          Article
          PMC6364310 PMC6364310 6364310 nasapa1005142
          10.7566/JPSCP.14.010303
          6364310
          30740603
          ff5918c7-b1e1-4400-a960-9393d0144252
          History
          Categories
          Article

          meteorites,asymptotic giant branch (AGB) stars,supernovae,nucleosynthesis,isotopic anomalies,presolar grains

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