What is the single most important factor determining a star’s future path and lifetime?
Answer
The final mass locked into the core during formation
The evolutionary destiny, lifespan, and characteristics of any star are almost entirely dictated by one parameter established during its birth: its final mass. The total amount of material accreted into the core before hydrostatic equilibrium is achieved sets the maximum temperature and pressure the core can sustain, thereby governing the rate at which nuclear fuel will be consumed. Low-mass stars, being frugal with their fuel, can survive for trillions of years. Conversely, the most massive stars burn their fuel with extraordinary intensity due to extremely hot cores, resulting in extremely short main sequence lifetimes, sometimes only lasting a few million years.

Related Questions
What are the initial reservoirs of gas and dust for star birth called?What commonly triggers the gravitational collapse within a diffuse molecular cloud?Where does the heat of a protostar originate before fusion begins?What object results if a core fails to accumulate mass greater than 8% of the Sun's mass?Approximately what core temperature must a protostar reach to ignite sustained nuclear fusion?What state is achieved when outward energy pressure counteracts the inward crush of gravity?What physical process characterizes the pre-main-sequence stage of stellar evolution?How long does the pre-main sequence contraction phase last for a star with the mass of our Sun?What is the single most important factor determining a star’s future path and lifetime?Compared to low-mass red dwarfs, what is the approximate main sequence lifetime for high-mass stars (> 8 M☉)?