Stars are expected to end up as white dwarves, neutron stars, or black holes. If you are interested in the stages before that (when the star still produces power), that include red giants, and supernovae.
It varies, depending on the stage of the star's development.
White dwarf stage. Its shrinks to a lot extent in this stage. Edit: A high mass star is usually one that becomes a supergiant then a supernova. Eventually this should leave either a neutron star or a black hole, depending on the mass of the star. The previous answer is for low mass stars.
On the contrary, "protostar" is the name of an early stage in the development of a star.
The stage that comes first in the life cycle of a high-mass star is the main sequence stage. During this stage, the star fuses hydrogen into helium in its core, maintaining a balance between radiation pressure and gravity.
The Sun is a medium mass star in main sequence.
The Neutron stage follows the White Dwarf stage of star development.
It varies, depending on the stage of the star's development.
White dwarf stage. Its shrinks to a lot extent in this stage. Edit: A high mass star is usually one that becomes a supergiant then a supernova. Eventually this should leave either a neutron star or a black hole, depending on the mass of the star. The previous answer is for low mass stars.
On the contrary, "protostar" is the name of an early stage in the development of a star.
the fourth stage of a star is "supergiant" and its also the hottest stage
It doesn't differ from a star, it is a star and it is the second stage in a stars life after the nebula stage.
The first stage in a star's life is as a nebula. As the gravitational forces spin faster, the star enters it's second stage, that of a prostar.
yes, it is the stage where a star dies and turns into a blackhole
Yes black hole is last stage of a star
A star spends most of its life in the main sequence stage, which is often considered its "happy state." During this phase, it fuses hydrogen into helium in its core, generating stable energy and maintaining gravitational equilibrium. This stage can last for billions of years, depending on the star's mass. It's characterized by a steady output of energy and a relatively stable size and temperature.
Stage 2 of a star refers to the phase when hydrogen fusion begins in the star's core, leading to a stable period of energy production. This stage can last tens of millions to billions of years, depending on the star's size and mass. During this stage, the star is considered a main sequence star, like our Sun.
Star Stage - 1955 was released on: USA: 9 September 1955