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physical phenomena > energy source > exothermic fusion process > helium burning > helium shell flash |
helium shell flash | ||||
subject | fact |
helium shell flash | has definition It has been shown that helium shell burning outside a degenerate core is unstable; the helium-burning shell does not generate energy at a constant rate but instead produces energy primarily during short flashes. During a flash, the region just outside the helium-burning shell becomes unstable to convection. The resultant mixing probably leads to the s-process as well as to the upward movement of carbon produced by helium burning. | |
is a kind of helium burning | ||
helium burning | has duration 5 × 105 years | |
has optimum density 700 g/cm3 | ||
requires minimum mass at star birth 0.5 solar masses | ||
has optimum temperature 2 × 108 K | ||
has part product carbon | ||
has next higher temperature reaction carbon burning | ||
has product carbon, oxygen | ||
has reactant helium | ||
exothermic fusion process | liberates energy | |
fusion | has antonym fission | |
produces energy | ||
has reaction probability | ||
has catalyst | ||
has minimum temperature | ||
physical process | has domain physics |
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