Understanding the Life Cycle of Stars

Apr 16, 2025

Life Cycle of Stars

Nebula

  • Begins with a cloud of dust and gas known as a nebula.
  • Gravity pulls these materials together to form a protostar.

Protostar

  • As particles collide and join:
    • Protostar gets larger.
    • Gravity strengthens, attracting more dust and gas.
    • Increased density leads to more frequent particle collisions and raises temperature.
  • High temperature and pressure cause:
    • Nuclear fusion: Hydrogen nuclei fuse to form helium, releasing energy.
    • Forms a main sequence star.

Main Sequence Star

  • Balance:
    • Outward pressure from energy release via nuclear fusion.
    • Inward pressure from gravity.
  • Sustains a long stable period, can last billions of years.
  • Example: Our Sun is in this stage.

Exhaustion of Hydrogen

  • Once hydrogen runs out, nuclear fusion ceases.
  • Gravity contracts the star into a small ball:
    • Temperature and density increase.
    • Nuclear fusion resumes, forming heavier elements (up to iron).

Evolution of the Star

  • Red Giant:

    • If the star is small to medium-sized (like the Sun), it becomes a red giant.
    • Becomes unstable and expels outer layers of dust and gas.
    • Leaves a hot, dense core called a white dwarf.
    • White dwarf cools and darkens, eventually becoming a black dwarf.
  • Red Supergiant:

    • If the star is very large, it becomes a red supergiant.
    • Undergoes cycles of expansion and contraction.
    • Supernova: Explodes, creating heavier elements than iron.
      • Distributes these elements across the universe.

Outcomes Post-Supernova

  • Neutron Star:
    • Forms if the initial star was very big.
    • Extremely dense core.
  • Black Hole:
    • Forms if the initial star was truly massive.
    • Gravity is so strong that even light cannot escape.

Recap

  • Stars form from nebulae.
  • Transition from protostar to main sequence star with nuclear fusion.
  • Hydrogen depletion leads to either red giant or red supergiant phase.
  • Red giants become white dwarfs, then black dwarfs.
  • Red supergiants result in supernovae, followed by neutron stars or black holes.