What primary elements result from the Helium Burning stage following the exhaustion of core hydrogen?
Answer
Carbon and oxygen
After the central hydrogen fuel is entirely consumed, the core of the massive star contracts and heats up intensely under the unrelenting force of gravity. Once the core reaches the necessary, higher temperature threshold, helium nuclei begin to fuse. This Helium Burning stage converts helium into the next set of stable, heavier elements, which are identified as carbon and oxygen. This newly formed carbon and oxygen then becomes the fuel source for the subsequent fusion shell once the central helium supply is depleted.

Related Questions
What architectural pattern describes a massive star's internal elemental makeup during later life stages?Why does the fusion process halt when the core becomes predominantly iron ($^{56} ext{Fe}$) or nickel?What elements are primarily created during the Carbon Burning stage following helium exhaustion?Which energy-generating stage immediately precedes the catastrophic collapse triggered by the iron core?How are elements heavier than iron, such as gold and uranium, synthesized in massive stars?How does the hydrogen-burning phase duration of a massive star compare to that of our Sun?What mechanism is the primary driver for creating the most neutron-rich elements during a core-collapse supernova?What materials are continuously replenished into the interstellar medium by massive stars via stellar winds before they explode?What determines the general definition of a massive star concerning its initial heft?What primary elements result from the Helium Burning stage following the exhaustion of core hydrogen?What factor sensitively affects the presence of trace elements like sodium or phosphorus in the outer shells during carbon fusion?