Hydrogen, helium, and carbon fuel are found in more massive stars. The diameter of more massive stars is bigger. Helium is found in greater abundance in more massive stars. The weight of more massive stars is greater.
It is the mass of the star.
The total mass. That will determine the life cycle of the star, the nature of its death and of the remnants after its death.
The mass of a star affects the lifespan of the star. The less the mass, the longer life span of the star. More massive stars burn up their fuel more quickly than the smaller stars. As the massive stars begin to burn the fuel and become smaller, the life span increases.
It's initial mass.
Determining wither it is a high or low mass star.
It is the mass of the star.
Its mass.
The main factor is its mass.
If a star has more mass, there will be more gravitational attraction. The star's material will get closer together, and the star will have more temperature and more pressure.
The total mass. That will determine the life cycle of the star, the nature of its death and of the remnants after its death.
The total mass. That will determine the life cycle of the star, the nature of its death and of the remnants after its death.
The mass of the star affects the evolution of the star. It helps to determine how long evolution will take and what kinds of changes will happen.
They weigh each star with a scale
The mass of a star affects the lifespan of the star. The less the mass, the longer life span of the star. More massive stars burn up their fuel more quickly than the smaller stars. As the massive stars begin to burn the fuel and become smaller, the life span increases.
It forms a "neutron star".
The endpoints of stellar evolution are: White Dwarf Neutron Star Black Hole The endpoint is dependent upon birth mass of the star.
It's initial mass.