What resistance force exerted by the gas itself works to counteract gravitational compression in a nebula?
Answer
Thermal pressure
Thermal pressure is the outward force generated by the internal heat and kinetic energy of the gas particles within the nebula. This pressure actively resists the inward pull of gravity, attempting to keep the cloud stable and expanded. For gravitational collapse to proceed toward star formation, the concentration of mass must be significant enough for self-gravity to overcome this inherent thermal resistance, leading to a state where the kinetic energy conversion results in immense heat associated with the onset of fusion.

Related Questions
What is the main force dictating the eventual fate and change of a massive nebula?What cosmic structures are nebulae described as the fundamental building blocks for?What is the name for the concept central to solar system creation driven by gravitational collapse of a nebula?What resistance force exerted by the gas itself works to counteract gravitational compression in a nebula?What physical law dictates that shrinking clumps of material within a nebula begin to spin faster?During core formation, what energy conversion drives the tremendous heating of the central contracting mass?What type of nebula is characterized by being lit up by nearby energetic, hot stars?What event marks the successful transition of the hot, contracting core mass into a star?What observable phenomenon suggests gravity is the currently prevailing large-scale force organizing a region of gas and dust?During the initial creation of a solar nebula, what force works alongside gravity to shape the structure before collapse dominates?