Less massive stars end up as white dwarfs. More massive stars end up as a supernova or a neutron star or for the really massive stars...as a black hole.
As a star ends its time in the main sequence it either becomes a Red Giant and end its life as a White Dwarf or becomes a White Super Giant and ends its life in an explosion (supernova) and if it's really dense it becomes a neutron star or a black hole as mentioned above.
The most massive stars will end up as black holes. Those are the stars that have more than approximately 3 solar masses at the end of their life - i.e., AFTER the supernova explosion.
The most massive ones. The exact amount of mass requires varies, depending on the type of supernova, and on the element mix of the initial star.
Yes, most massive stars (at least eight times the mass of our Sun) will end their life cycle by collapsing into a black hole. This happens after they have gone through the stages of supernova explosion and core collapse.
Massive stars may undergo a supernova explosion at the end of their cycle, leading to the formation of neutron stars or black holes. This explosive event releases a vast amount of energy and is responsible for seeding the surrounding space with heavy elements.
No, stars less massive than the Sun do not have enough mass to undergo a supernova explosion. Instead, they may end their lives as a white dwarf or, if they are even less massive, a planetary nebula. Supernovae are events associated with more massive stars.
The massive stars turn into gas
No. Supernovas are cataclysmic eruptions from massive stars that have come to the end of their lives. See related questions
The most massive stars will end up as black holes. Those are the stars that have more than approximately 3 solar masses at the end of their life - i.e., AFTER the supernova explosion.
False. Medium-sized stars become white dwarfs. Only the most massive stars form black holes.
The most massive stars become black holes.
The most massive ones. The exact amount of mass requires varies, depending on the type of supernova, and on the element mix of the initial star.
The most important factor in determining a star's life cycle is its mass. The mass of a star determines its size, temperature, and how it will evolve over time. More massive stars have shorter lives and end in a violent supernova explosion, while less massive stars like the Sun will eventually become a white dwarf.
Massive stars that are at least eight times more massive than the Sun end their life as a supernova. During the explosion, these stars release a tremendous amount of energy and can briefly outshine an entire galaxy.
Massive stars with at least eight times the mass of the Sun end their lives as supernovae. During their final stages, they undergo a rapid collapse and explosion, releasing an immense amount of energy and forming a bright supernova.
Yes, most massive stars (at least eight times the mass of our Sun) will end their life cycle by collapsing into a black hole. This happens after they have gone through the stages of supernova explosion and core collapse.
Massive stars may undergo a supernova explosion at the end of their cycle, leading to the formation of neutron stars or black holes. This explosive event releases a vast amount of energy and is responsible for seeding the surrounding space with heavy elements.
No, stars less massive than the Sun do not have enough mass to undergo a supernova explosion. Instead, they may end their lives as a white dwarf or, if they are even less massive, a planetary nebula. Supernovae are events associated with more massive stars.