What temperature does the helium-burning core of a solar-mass star reach when it ignites the triple-alpha process as a red giant?
Answer
Around 100 million Kelvin
When a star like the Sun evolves into a red giant, its core contracts and heats up to approximately 100 million Kelvin to ignite helium fusion via the triple-alpha process.

#Videos
How Hot and Dense Must a Star's Core Be? - YouTube
Related Questions
What is the approximate core temperature of an average star like our Sun?What state describes the perfect balance between a star's immense gravity and its outward thermal pressure?What is the primary fusion reaction sustained by the Sun's core temperature?At approximately what mass threshold does the core temperature favor the CNO cycle over the proton-proton chain?What range are the core temperatures of Wolf-Rayet stars often estimated to be?What temperature does the helium-burning core of a solar-mass star reach when it ignites the triple-alpha process as a red giant?What temperature range can the core spike to during the final, catastrophic implosion of the most massive stars?What process occurs during the final implosion when the core temperature is so high that photons break apart atomic nuclei?How do scientists gain a verifiable check on the computed temperature profiles of the Sun's core?What is the fundamental trade-off highlighted by comparing the Sun's lifespan to that of a massive star?