Swawel-32: Verskil tussen weergawes

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Lyn 18:
 
== Nukleosintese ==
Swawel-32 is die isotoop wat die volopste voorkom en die rede daarvoor dat is dit volop gevorm word gedurende die suurstofverbrandings fase van 'n [[supernova]]-ontploffing.<ref>[https://history.nasa.gov/CP-2156/ch1.3.htm NASA]</ref> Hierdie proses word ook die alfa-proses genoem. Dit word saam met [[kalsium-40|{{sub sup|40|}}Ca]], [[argon-36|{{sub sup|36|}}Ar]], [[chroom-48|{{sub sup|48|}}Cr]], [[yster-52|{{sub sup|52|}}Fe]] en [[nikkel-56|{{sub sup|56|}}Ni]]as een van die alfa-kerne beskou.<ref>[https://pubs.geoscienceworld.org/msa/rimg/article/81/1/107/141046/nucleosynthetic-isotope-variations-of-siderophile Nucleosynthetic Isotope Variations of Siderophile and Chalcophile Elements in the Solar System {{Outeur|Tetsuya Yokoyama, Richard J. Walker}} Reviews in Minralogy and Geochemistry (2016) 81(1): 107-160]</ref>
 
==KMR==