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
A stellar cloud, often referred to as a molecular cloud or nebula, is a vast region in space filled with gas and dust, primarily composed of hydrogen molecules. These clouds are the primary sites of star formation, as the dense areas within them can collapse under gravity to form new stars. Stellar clouds can vary in size and density, and they often produce complex structures that can include stellar nurseries, where new stars are birthed, as well as remnants from previous stellar evolution.
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 Nobel Prize in Physics in 1983 was awarded to William A. Fowler for his pioneering work in the understanding of the processes of nuclear reactions in stars, which are crucial for the evolution of stellar structures. His research contributed significantly to the field of astrophysics, particularly in explaining how elements are formed in stars and the role of stellar evolution in the universe.
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