What physical element contributes to the steep temperature gradient and immense pressure at the star's center?
Answer
The sheer physical weight of the star's material above the core
The extreme conditions required for nuclear fusion, namely high pressure and temperature, are not uniform throughout the stellar structure; they are concentrated intensely at the core. This concentration arises directly from the weight of all the stellar material lying above the core region. This accumulated mass generates crushing pressure, effectively acting as an infinite compressor powered by gravity, forcing the hydrogen fuel into an incredibly dense state. This severe compression is directly linked to the high internal energy, or temperature, required to keep the protons colliding violently enough to initiate and sustain fusion reactions.

Related Questions
What energy source drives the initial heating of the collapsing mass forming a protostar?What critical temperature threshold must the protostar core exceed for nuclear fusion to commence?What state describes the balance between opposing forces within a star during its main sequence phase?What is the specific conversion process powering the star during the Hydrogen Burning phase?What physical element contributes to the steep temperature gradient and immense pressure at the star's center?How does the lifespan of a Sun-like star compare to a star ten times its mass on the main sequence?What process allows a star to ignite heavier elements after the core hydrogen supply is depleted?What is the immediate result of converting gravitational potential energy during the initial collapse of the molecular cloud?What relationship links the star's mass to the required core temperature for maintaining stability?Which famous equation describes the energy generation far exceeding gravitational heating during ongoing fusion?