Gravity effects stellar evolution by pulling down force on the stars while they are forming. Mass will determine how long the star stays alive and burning.
Life Cycle of a Star
When the outward force of pressure wins over gravity in an old star, the star will expand and cool, becoming a red giant. This process occurs as the star exhausts its nuclear fuel and transitions to a different phase of stellar evolution.
Gravity played a crucial role in shaping our universe by bringing matter together to form stars, galaxies, and other structures. It continues to govern the motion of celestial bodies, shaping the evolution and dynamics of the universe on a cosmic scale. Without gravity, the universe as we know it would look vastly different.
The fact that each star starts out with all the hydrogen that its ever going to have.
If there were no gravity, period, there would be no stars. If gravity ceased to work, there would be a whole lot of violent explosions as the nuclear, mechanical and other forces within the stars popped the stellar balloons, so to speak.
The first stage of stellar evolution is nebula.
You can find an overview of stelar evolution in the Wikipedia article entitled "Stellar evolution".
The longest stage of stellar evolution is the main sequence phase.
Helium burning is most durable stage in stellar evolution.
Stellar evolution is the term for the changes a star undergoes during its lifetime.
Nuclear fusion affects stellar evolution by essentially halting all mitosis and miosis that any cells in a stellar evolution could experience, and they stunt the growth of the object.
W. Sutantyo has written: 'The effect of stellar evolution on the synchronous rotation of components of massive close binaries' -- subject(s): Double stars, Evolution, Stars
The endpoints of stellar evolution are: White Dwarf Neutron Star Black Hole The endpoint is dependent upon birth mass of the star.
Scientist believe that stellar evolution contained only hydrogen and then helium.
Life Cycle of a Star
Main Sequence
it is the cycle of stellar evolution