The stellar origins of presolar silicates discovered in Antarctic micrometeorites

Yada T., Stadermann F.J., Floss C., Zinner E., Olinger C.T., Graham G.A., Bradley J.P., Dai Z.R., Nakamura T. and Noguchi T. (2005) 29th Symposium on Antarctic Meteorites, NIPR.


ABSTRACT

Presolar grains, which formed in the stars existed before the solar system, have given us valuable information about stellar nucleosynthesis and the origin of the solar system. In these years, presolar silicates have been discovered in interplanetary dust particles (IDPs) and chondrites, which indicates that presolar grains existed more ubiquitously in the early solar nebula than previously considered. As reported before, presolar silicates were discovered also in Antarctic micrometeorites (AMMs), using NanoSIMS. This discovery tells us that parent bodies of the AMMs preserve a primary feature since their accretions in the early solar nebula. Here we review the discovered presolar silicates and discuss about their stellar origins.


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