The origin of short-lived radionuclides in the solar system
โ Scribed by Matthieu Gounelle
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 127 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1387-6473
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๐ SIMILAR VOLUMES
Model calculations for the production of the short-lived nuclides 10 Be, 26 Al, 41 Ca and 53 Mn by solar energetic particles (SEP) in the asteroidal region during the early evolution of the solar system are presented. Based on the results of these calculations and the initial solar system abundances
The first results from the STARDUST mission revealed that refractory phases formed at a close distance from the nascent Sun have been transported to the comet forming region. Such refractory phases from meteorites (that originate from the asteroid belt), hold the ashes of Short-Lived Radionuclei (SL
The observational astronomer generally feels only an indirect interest in the problem of how our earth and its companion planets came into being; his telescope can give him no direct information on the subject, since such planets as other suns may possess are too small and too distant to be observed