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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 | ![]() |
Next helium burning: helium flash Up: helium burning