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stages of a stars life the same size as the sun
protostar
main sequence star
red giant
white dwarf
black dwarf
stages of a stars life much bigger than the sun
protostar
main sequence star
red super giant
syupernova
neutron star or black hole
protostar
cloud or dust and gas pulled together by gravitational attraction
temperature is too low for fusion to take place
protostar to main sequence star
as the cloud becomes denser nuclei of hydrogen atoms and other light elements fuse together
energy is released
main sequence star
the stable period of a star → the forces within it are balanced
can maintain energy output for millions of years until the star runs out of hydrogen nuclei to fuse together
main sequence star to red supergiant
star runs out of hydrogen nuclei to fuse together
stars much bigger than the sun swell out to become a red supergiant
red supergiant
helium and other light elements fuse to form heavier elements
iron is heaviest elements element that can be formed
supernova to neutron star
explosion compresses the core of the star into a neutron star
supernova
the star explodes
conditions extreme enough for iron to fuse and produce heavy elements
elements distributed throughout the universe
neutron star
a star believed to largely consist of neutrons
supernova to black hole
star collapses and keeps collapsing until it is no more than a point in space
black hole
an infinitely dense point in space (escape velocity is greater than the speed of light)
main sequence star to red giant
star runs out of hydrogen nuclei to fuse together
stars about the same size as the sun swell, cool down and turn red
red giant
helium and other light elements fuse to form heavier elements
red giant to white dwarf
forces are insufficient for further fusion reactions
the star collapses under the force of gravity
it heats up and turns from red to yellow to white
white dwarf
a hot dense white star
white dwarf to black dwarf
no further fuel available
the star fades and goes cold
black dwarf
an inert lump in space