Exhausting its hydrogen supply. Main Sequence stars fuse hydrogen to make helium. Eventually, they run out of fuel and then start to fuse helium to make carbon, nitrogen and oxygen, with slightly higher atomic numbers than helium,
The nucleo-chemistry of these reactions involves the generation of more energy and greater loss of mass than hydrogen fusion did which is why after 100 million years or so stars then leave the red giant phase and cool. shrink and turn into white dwarfs.
A red giant is a large non-main sequence star of stellar classification K or M; so-named because of the reddish appearance of the cooler giant stars.
THE SUN
The Sun is expected to become a red giant in about five billion years. It is calculated that the Sun will become sufficiently large to engulf the current orbits of some of the solar system's inner planets, including Earth.
However, the gravitational pull of the Sun will have weakened by then due to its loss of mass, and all planets but Mercury will escape to a wider orbit. That said, Earth's biosphere will be destroyed as the Sun gets brighter while its hydrogen supply becomes depleted.
The extra solar energy will cause the oceans to evaporate to space, causing Earth's atmosphere to become temporarily similar to that of Venus, before the atmosphere is also lost.
Exhausting its hydrogen supply. Main Sequence stars fuse hydrogen to make helium. Eventually, they run out of fuel and then start to fuse helium to make carbon, nitrogen and oxygen, with slightly higher atomic numbers than helium,
The nucleo-chemistry of these reactions involves the generation of more energy and greater loss of mass than hydrogen fusion did which is why after 100 million years or so stars then leave the red giant phase and cool. shrink and turn into white dwarfs.
A red giant is a large non-main sequence star of stellar classification K or M; so-named because of the reddish appearance of the cooler giant stars.
THE SUN
The Sun is expected to become a red giant in about five billion years. It is calculated that the Sun will become sufficiently large to engulf the current orbits of some of the solar system's inner planets, including Earth.
However, the gravitational pull of the Sun will have weakened by then due to its loss of mass, and all planets but Mercury will escape to a wider orbit. That said, Earth's biosphere will be destroyed as the Sun gets brighter while its hydrogen supply becomes depleted.
The extra solar energy will cause the oceans to evaporate to space, causing Earth's atmosphere to become temporarily similar to that of Venus, before the atmosphere is also lost.
As a giant star expands, its surface area increases, allowing more energy to escape from its core. This increased surface area results in the star appearing more luminous. Additionally, the expansion causes the outer layers of the star to become less dense, which allows more light to escape and contribute to its overall brightness.
I am pretty sure it becomes a giant if I'm not mistaken.
A star that is in it's teenage years(medium star) isn't a red giant until it's last years.
A dwarf star is denser than a giant star. Dwarf stars have a higher density due to their smaller size and higher mass compared to giant stars. Giant stars have larger volumes and lower densities as they have expanded and become less dense towards the end of their life cycle.
The red giant star is located in the constellation Orion. Scientists are studying the red giant to understand more about the end stages of a star's life cycle.
That would mainly depend on the star's mass.
A giant star would experience a supernova explosion, in order to become a white dwarf.
After a star burns up all it's hydrogen, it becomes a red giant.
it doesn't because the star may be already dead before its ready to become a giant.
As a giant star expands, its surface area increases, allowing more energy to escape from its core. This increased surface area results in the star appearing more luminous. Additionally, the expansion causes the outer layers of the star to become less dense, which allows more light to escape and contribute to its overall brightness.
A star's entire fate is tied into its initial mass. Nothing else matters.
a super giant.
Just once.
red giant
I am pretty sure it becomes a giant if I'm not mistaken.
yes. in about five billion years the sun will become a red giant.
The Sun will still be "the Sun", but the next type of star it will become is a "red giant" star.