it starts with nebula
Life Cycle of a Star
The endpoints of stellar evolution are: White Dwarf Neutron Star Black Hole The endpoint is dependent upon birth 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 total mass. That will determine the life cycle of the star, the nature of its death and of the remnants after its death.
Darude Sandstorm
A white dwarf is the death of a medium sized star - similar to our own Sun.
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.
After a death of a Giant Star, a corpse of a star will be the remaining of it, right in the center of the aftermath, you will find one of the strangest objects in the Universe, the Pulsar and the Neutron Star.
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.
Evolution of the Red Star - 1973 was released on: USA: 1973
Stellar evolution is the term for the changes a star undergoes during its lifetime.
There are several theories about how stars are formed, such as the nebular hypothesis which suggests that stars form from collapsing clouds of gas and dust. Stellar evolution theory describes the life cycle of a star from birth to death. There are also theories about star classification based on their temperature, color, and size, such as the Hertzsprung-Russell diagram.