A star whilst being luminous, will spend most of it's life - about 90% - on the main sequence.
However, when a star "dies" they are still refereed to, by many, as stars so one could argue that a star will spend more time "dead" than "alive".
So you could say that a star spends most of it's life as a stellar remnant.
If this is a homework question, the answer is Main Sequence.
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.
The main sequence stage is the most stable stage in a star's life cycle. During this stage, a star fuses hydrogen into helium in its core, maintaining a stable balance between gravity pulling inward and the energy produced by nuclear fusion pushing outward. This equilibrium allows the star to shine steadily for billions of years.
MAIN-SEQUENCE The average star spends 90% of its life as a hydrogen burning MS 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.
The longest stage in a star's life cycle is the main sequence stage, where the star fuses hydrogen into helium in its core. This stage can last for billions of years for stars like the Sun.
A Star spends most of its life on the "main sequence" of the Hertzsprung-Russell diagram (see related link below). While here it is called a "main sequence" star and its source of energy during this phase of its life is the fusion of hydrogen into helium in its core.
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.
Yes, it is true that an average star spends about 90 percent of its life on the main sequence burning hydrogen into helium through nuclear fusion. This is the longest and most stable phase in a star's life cycle before it transitions into the next phase.
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.
yes, it is the stage where a star dies and turns into a blackhole
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 main sequence stage is the most stable stage in a star's life cycle. During this stage, a star fuses hydrogen into helium in its core, maintaining a stable balance between gravity pulling inward and the energy produced by nuclear fusion pushing outward. This equilibrium allows the star to shine steadily for billions of years.
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.
MAIN-SEQUENCE The average star spends 90% of its life as a hydrogen burning MS star.
dust
the stage on the star is me not you because newton is black in forest
For a star like ours, the black dwarf stage For an immensely massive star, a back hole.