Depending on the mass a star may live 10million to 200billion years!
A supernova (plural: supernovae or supernovas) is a stellar explosion that creates an extremely luminous object.Check the link given for more information.
The remains of a star after a supernova can be classified primarily as either a neutron star or a black hole, depending on the mass of the original star. If the core's mass is below a certain threshold, it may collapse into a neutron star, which is incredibly dense and composed mostly of neutrons. If the core's mass exceeds this limit, it may collapse further into a black hole, where gravity is so strong that not even light can escape. Additionally, the explosion disperses the outer layers of the star into space, creating a supernova remnant.
When the outer layers of a star cool, it typically becomes a red giant or a supergiant, depending on its initial mass. As the star expands and its temperature decreases, it emits light primarily in the red spectrum. Eventually, it may shed its outer layers, leaving behind a hot core that can become a white dwarf, neutron star, or even a black hole, depending on the star's mass. The cooling process marks the later stages of stellar evolution, ultimately leading to the star's death.
Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.
Juvenile star is typically classified as a low mass star, as it is in the early stage of its life cycle. These stars have a mass similar to that of the Sun or less. They are characterized by their long lifespan and relatively stable nature.
Usually a neutron star, or a black hole, depending on the remaining mass.
A high-mass star will use up its fuel faster than a low-mass one. Depending on the amount of mass that remains at the end of its life, it may convert to a neutron star, or to a black hole.
A supergiant star can explode into a supernova, where the outer layers are ejected into space. What remains may collapse into a neutron star or black hole, depending on the mass of the original star.
When a supergiant star exhausts its nuclear fuel and dies, it may explode in a supernova event. Depending on its mass, the remnants can either collapse into a neutron star or form a black hole. The outcome is determined by the star's initial mass and the processes occurring during the supernova explosion.
A supernova (plural: supernovae or supernovas) is a stellar explosion that creates an extremely luminous object.Check the link given for more information.
The remains of a star after a supernova can be classified primarily as either a neutron star or a black hole, depending on the mass of the original star. If the core's mass is below a certain threshold, it may collapse into a neutron star, which is incredibly dense and composed mostly of neutrons. If the core's mass exceeds this limit, it may collapse further into a black hole, where gravity is so strong that not even light can escape. Additionally, the explosion disperses the outer layers of the star into space, creating a supernova remnant.
When the outer layers of a star cool, it typically becomes a red giant or a supergiant, depending on its initial mass. As the star expands and its temperature decreases, it emits light primarily in the red spectrum. Eventually, it may shed its outer layers, leaving behind a hot core that can become a white dwarf, neutron star, or even a black hole, depending on the star's mass. The cooling process marks the later stages of stellar evolution, ultimately leading to the star's death.
Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.Because of their previous history. The star that converted to a black hole may have had more or less mass for a start. Also, a black hole can increase in mass when matter falls into it, so depending on the amount of matter available for the black hole, the results may vary.However, it is not yet known how the galactic black holes achieved the enormous mass they have.
the life san of stars is like if you had everyone bring in candles into the class,some would be round,some would be tall and skinney,and they all would go ot at different times.the round candles may take a lung time to go out, while tea lights may last only a short period of time.just like stars
Juvenile star is typically classified as a low mass star, as it is in the early stage of its life cycle. These stars have a mass similar to that of the Sun or less. They are characterized by their long lifespan and relatively stable nature.
Yes it does to a certain extent.The colour of a star depends almost exclusively on its initial mass.The initial mass determines the evolution of the star. Depending on the initial mass it may become a neutron star,a black hole, a supernova, a nova, a white dwarf, a red giant. Ultimately it will be a burned out cinder, a black dwarf or nothing at all except Hawking radiation
Star grass plants typically have a lifespan of 2-3 years, but this can vary depending on growing conditions and care. With proper maintenance and ideal growing conditions, they may live longer. Regular pruning and dividing can also help prolong the lifespan of star grass plants.