Life cycle of stars Flashcards
1
Q
How is a main sequence star formed?
A
- Begins with a cloud of dust and gas, known as a nebula
- Overtime, the force of gravity pulls the dust and gas of the nebula together, forming a protostar
- Protostar continues to grow, which causes the force of gravity to continue to increase
- Gravity squeezes the protostar, making it more dense
- This also causes particles to collide and increase the temperature of the protostar
- When the temperature is high enough, hydrogen nuclei start fusing and forming helium nuclei (binary fusion)
- Binary fusion gives out lots of energ. At this point, the protostar has become a mains sequence star
2
Q
Why is the main sequence star considered stable?
A
- The outward pressure due to binary fusion is prefectly balanced by the inward pressure of gravity
3
Q
What happens to the main sequence star after a long stable period?
A
- After a long stable period, the star runs out of hydrogen and can no longer undergo nuclear fusion
- At this point, the force of gravity makes the star contract into a small ball
- The small ball is so hot and dense that nuclear fusion starts again, causing the star to expand
- Nucear fusion forms heavier elements than helium (up to iron)
4
Q
What happens to the main sequence star if it is a small / medium star?
A
- The main sequence star expands to form a red giant
- After a while, the red giant becomes unstable and expels its outer layers of dust and gas
- This leaves behind a hot, dense and solid core that doesn’t do anymore nuclear fusion. We call this a white dwarf
- Over time, the white dwarf emits all of its energy and can no longer emit light. This is now called a black dwarf
5
Q
What happens to the main sequence star if it is a really big star?
A
- The main sequence star expands to form a red super giant
- The red super giant undergoes more nuclear fusion and passes through several cycles of contraction and expansion
- After a while, the red super giant explodes in a supernova, creating elements even heavier than iron
- If the star was big, it will condense into a neutron star
- If the star was massive, it might collapse in on itself and form a black hole