Short-lived radionuclides in the early solar system

Details Short-lived radionuclides in the early solar system Short-lived radionuclides in the early solar system

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003acasn..44..231h&link_type=abstract

Acta Astronomica Sinica, vol. 44, no. 3, p. 231-239

Astronomy and Astrophysics

Astronomy

1

Solar System: Formation, Astrochemistry, Short-Lived Radionuclides

Scientific paper

It reviews the evidence for short-lived radionuclides in the early solar system and evaluates models for their origins. The stellar model requires that some freshly-nucleosynthesized radionuclides were injected into the protosolar cloud shortly before it began to collapse. The spallation model suggests that these isotopes were the products of interaction between energetic particles and gases/dusts in the protosolar cloud or solar nebula. A brief discussion was given to the new theory for the solar system formation---X-wind model.

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