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What is the earliest stage of the life cycle of a star?

dust


What is the middle part of a star's life called?

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.


What is the earliest stages of a star's life?

protostar


What is the name for the portion of a star's life cycle when it uses hydrogen for fuel?

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.


The supernova is the stage in the life of a star?

yes, it is the stage where a star dies and turns into a blackhole


How does a protostar differ from a star?

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.


What is the early stage of life for a star called before it starts to have fusion?

please help me I need answers


What is the longest stage in the life cycle of a 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


What is a star's second 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.


What stage of a stars life is the sun in?

the stage on the star is me not you because newton is black in forest


What will be the final stage in the suns life?

For a star like ours, the black dwarf stage For an immensely massive star, a back hole.


The third stage in the life cycle of a star?

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.