life cycle of a star Flashcards
what does the life cycle depend on?
the size of the star
life cycle for sun size star
nebula -> protostar -> main sequence -> red giant -> white dwarf -> black dwarf
life cycle for bigger than sun size star
nebula -> protostar -> main sequence -> red super giant -> supernova -> neutron star OR black hole
describe how the life cycle works for similar size to sun after mains sequence
- eventually hydrogen begins to run out
- star then swells into a red giant
- becomes red as the surface cools
- fusion of helium (and other elements) occur
- heavier elements (up to iron) are created in the core
- then becomes unstable and ejects its outer layer of dust and gas
- leaves behind a hot, dense, solid core (white dwarf)
- as a white dwarf cools down, it emits less and less energy
- when it no longer emits a lot of energy, it is a black dwarf
describe how the life cycle works for stars bigger than the sun after main sequence
- eventually hydrogen begins to run out
- star then swells into a red super giant
- becomes red as the surface cools
- fusion of helium (and other elements) occur
- heavier elements (up to iron) are created in the core
- star starts to glow brightly again as it undergoes more fusion and expands and contract several times, forming elements as heavy as iron
- eventually they explode in a supernova, forming elements heavier than iron and ejecting them into the universe to form new planets and stars
- exploding supernova throws outer layers of dust and has into space, leaving a dense core called a neutron star
- if it is large enough it will become a black hole
what is a black hole?
a dense point in space
how are elements found over the universe?
explosion of a supernova distributes them
how do elements occur?
through fusion in stars
where are elements heavier than iron produced?
in a supernova
where are heavy elements produce, but not heavier than iron?
in the core of a red/red super giant
how do fusion processes lead to the formation of elements?
- fusion in stars starts with hydrogen atoms fusing to form helium
- as stars age and run out of hydrogen, they fuse helium into heavier elements like carbon and oxygen.
- in the most massive stars, fusion continues to create elements all the way up to iron.
- when these stars explode in a supernova, they can create even heavier elements, which are then spread throughout space.