Short-lived radionuclides in the early solar system - A meteoritic perspective of the solar system formation

Details Short-lived radionuclides in the early solar system - A meteoritic perspective of the solar system formation Short-lived radionuclides in the early solar system - A meteoritic perspective of the solar system formation

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cha%26a..27..365h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 27, Issue 4, p. 365-373.

Astronomy and Astrophysics

Astrophysics

1

Cosmochemistry-Solar System, Formation-Nuclear Reactions, Nucleosynthesis, Abundances

Scientific paper

This paper reviews the evidence for short-lived radionuclides in the early solar system and evaluates the models of their origin. The stellar model requires that some freshly-nucleosynthesized radionuclides were injected into the proto-solar cloud shortly before it began to collapse. The spallation theory suggests that these nuclides were the products of interaction between energetic particles and gas/dust in the proto-solar cloud or solar nebula. A brief discussion is given to a new theory for the X-wind model of solar system formation.

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