There is no general name. How a star ends depends on its mass.
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.
The protostellar stage for a star like our Sun typically lasts for about 100,000 years. During this stage, the star is accumulating mass from its surrounding disk of gas and dust, contracting and heating up until nuclear fusion ignites in its core.
The third stage in the life cycle of a star is the main sequence stage, where a star fuses hydrogen into helium in its core. During this stage, stars like our Sun are stable and shine steadily due to the balance between gravitational forces pulling inward and nuclear fusion pushing outward. This stage can last for billions of years, depending on the mass of the star.
The main sequence, where the star combines hydrogen atoms to form helium atoms and produce energy, through the process of nuclear fusion. And it also the beginning of a new planet called farshinia
A star is called a protostar before it begins nuclear fusion in its core and officially becomes a star. During this stage, a protostar is formed from a collapsing cloud of gas and dust, as gravity pulls material together and heats up the core.
The middle part of a star's life is called the main sequence stage. During this stage, a star fuses hydrogen into helium in its core, releasing energy that allows it to shine steadily. The Sun is currently in the main sequence stage.
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.
Yes black hole is last stage of a star
The protostellar stage for a star like our Sun typically lasts for about 100,000 years. During this stage, the star is accumulating mass from its surrounding disk of gas and dust, contracting and heating up until nuclear fusion ignites in its core.
The third stage in the life cycle of a star is the main sequence stage, where a star fuses hydrogen into helium in its core. During this stage, stars like our Sun are stable and shine steadily due to the balance between gravitational forces pulling inward and nuclear fusion pushing outward. This stage can last for billions of years, depending on the mass of the star.
similarly black hole is the last stage of star....
The main sequence, where the star combines hydrogen atoms to form helium atoms and produce energy, through the process of nuclear fusion. And it also the beginning of a new planet called farshinia
A Pulsar.
The portion of a star's life cycle when it uses hydrogen for fuel is called the main sequence stage. During this stage, the star fuses hydrogen to form helium in its core, releasing energy in the process. This is the longest and most stable stage in a star's life.
rynhety
A star is called a protostar before it begins nuclear fusion in its core and officially becomes a star. During this stage, a protostar is formed from a collapsing cloud of gas and dust, as gravity pulls material together and heats up the core.
The main sequence stage of a sunlike star typically lasts for about 10 billion years. It is during this stage that the star fuses hydrogen into helium in its core, maintaining a balance between the force of gravity pulling in and the energy produced by nuclear fusion pushing out.