Astrophysics - Stellar Evolution Flashcards
1
Q
how are stars classified?
A
according to their colours
2
Q
what does a star’s colour relate to?
A
the star’s surface temperature: blue as the hottest and red as the coldest
3
Q
what is the evolution of a star with a similar mass to the sun?
A
- nebula
- main sequence
- red giant
- white dwarf
4
Q
what happens when a star is a nebula?
A
- stars form from large clouds of dust and gas particles (nebulae) that are drawn together by gravitational forces over millions of years
- as the particles get closer the temperature and pressure becomes so large that nuclear fusion of hydrogen nuclei to helium nuclei occurs
- this releases enormous amounts of energy in the form of heat and light.
5
Q
what happens when a star is a main sequence?
A
- fusion produces forces that make the star expand outwards, but the gravitational force is always pulling the particles within the star inwards
- when these two opposing forces become balanced a star is stable and called a main sequence star
- it should stay this way for millions of years, at a constant size and temperature
6
Q
what happens when a star is a red giant?
A
- eventually, hydrogen fusion stops as the star runs out of fuel
- gravitational force is now bigger than the outward fusion force which causes the star to collapse inwards and compress
- this causes it to heat up to even higher temperatures so that fusion of helium nuclei begins
- the increased power output causes the star to expand greatly
- the surface area is so large that it is cooler than before, so its colour changes to red and the star is called a red giant
7
Q
what happens when a star is a white dwarf?
A
- eventually, fusion stops when the star runs out of helium nuclei and the gravitational force causes the star to collapse inwards and compress again
- this heats it so it changes colour to emit white light
- the star is squashed so greatly by the gravitational force to become a small and very dense white dwarf
- a white dwarf eventually cools down and changes colour as it does so, eventually becoming black
8
Q
what is the evolution of a star with a larger mass to the sun?
A
- nebula
- main sequence
- red supergiant
- supernova
- neutron star/black hole
9
Q
what happens when a red supergiant becomes a supernova?
A
- after the stable period, a giant star expands into a red supergiant (it produces all the elements up to iron during nuclear fusion)
- when it finally runs out of nuclei to fuse it collapses due to the gravitational force, and then explodes into a supernova
10
Q
what happens when a supernova becomes a neutron star?
A
- the supernova throws dust and gas back into space and so another nebula is formed
- a dense core remains (a neutron star)
- if its mass is large enough it can compress further to become a black hole