Which energy-generating stage immediately precedes the catastrophic collapse triggered by the iron core?
Answer
Silicon Burning
The progression of fusion in a massive star accelerates dramatically as heavier elements form. Following the fusion of oxygen, which creates silicon and sulfur, the star enters the Silicon Burning stage. This is explicitly stated as the final energy-generating stage before the core composition shifts entirely to iron and nickel. Once silicon is fused, the resulting product is a dense mix centered around iron. The creation of iron signals the end of energy generation via fusion, causing the outward thermal pressure to vanish and initiating the core collapse that leads to the supernova event.

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?