High and low mass stars evolve differently into red giants primarily due to their core temperatures and pressures. Low mass stars, like our Sun, expand and cool as they burn hydrogen in a shell around an inert helium core, leading to a gradual increase in size. In contrast, high mass stars experience more intense gravitational pressure, allowing them to fuse heavier elements in successive shells, causing rapid and more dramatic expansion. This difference in stellar evolution results in distinct characteristics and lifespans for red giants based on their initial mass.
The type of star an object will evolve into depends on its initial mass. For example, a star like our Sun will eventually become a red giant and then a white dwarf. More massive stars will end their lives as supernovae, neutron stars, or black holes.
The difference is in mass. Low to medium mass stars (up to about 8-10 solar masses) become white dwarfs. Massive stars (10 to 25 solar masses) become neutron stars. Stars above 25 solar masses tend to become black holes.
There are three types of stellar remnants. Low to medium mass stars will become white dwarfs. High mass stars will become neutron stars. Very high mass stars will become black holes.
Not all protostars become true stars. Some protostars may not have enough mass to sustain nuclear fusion in their cores and never become true stars, instead becoming failed stars known as brown dwarfs.
Shooting stars are not stars. They are bits of dirt and dust that burn up in our atmosphere, briefly making them look like stars. Most of that is debris is from comets or others bits of dirt in space, but they are not stars and were not stars. So stars do not become shooting stars.
High mass stars and low mass stars evolve differently due to their distinct physical characteristics and life cycles. High mass stars undergo rapid fusion processes, leading to a brief lifespan and ending in supernova explosions, often forming neutron stars or black holes. In contrast, low mass stars evolve more slowly, transitioning through stages such as red giants and ending as white dwarfs after shedding their outer layers. These differences in evolution result from variations in temperature, pressure, and nuclear fusion rates within the stars.
No. Intermediate mass stars will evolve into Red Giants and then to White Dwarfs. See related questions for more information.
You have to raise its IQ up to four stars, and then you can evolve it.
No, low mass stars do not become neutron stars. Low mass stars like the Sun end their lives as white dwarfs. Medium mass stars can evolve into neutron stars, but they must first go through the supernova stage to shed their outer layers and leave behind a dense core of neutrons.
No, the sun will not become a neutron star. Neutron stars form from the remnants of massive stars that have undergone a supernova explosion. The sun is not massive enough to undergo this process and will instead evolve into a white dwarf.
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Some massive stars will become neutron stars. When massive stars die they will either become neutron stars or black holes depending on how much mass is left behind.
The type of star an object will evolve into depends on its initial mass. For example, a star like our Sun will eventually become a red giant and then a white dwarf. More massive stars will end their lives as supernovae, neutron stars, or black holes.
The difference is in mass. Low to medium mass stars (up to about 8-10 solar masses) become white dwarfs. Massive stars (10 to 25 solar masses) become neutron stars. Stars above 25 solar masses tend to become black holes.
Stars that become white dwarfs die but become black holes . Neutron stars are born from a Super Nova that stored its energy and became a neutron star.
They Collide and become part of another star which causes Stars to be come Parts of other Stars.
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