Understanding the Life Cycle of Stars

Sep 24, 2024

Lecture Notes: Life Cycle of Stars and Formation of Elements

Introduction

  • Understanding the first billion years of the universe leads to understanding stars and galaxies.
  • Need to explore the creation of elements beyond hydrogen and helium.
  • Stars play a crucial role from birth to death in creating new elements and celestial bodies.

The Life Cycle of Stars

Birth of a Star

  • Stars form from clouds of gas and dust, primarily hydrogen and helium.
  • Gravity causes the cloud to contract, heating up over millions of years.
  • Nuclear fusion begins when sufficient heat is achieved, forming a main sequence star.

Low-Mass Stars

  • Range from 13 Jupiter masses to around our Sun's mass.
  • Main sequence stars fuse hydrogen into helium, maintaining size and luminosity for billions of years.

Red Giant Phase

  • Occurs once hydrogen is depleted.
  • The core shrinks and heats up, outer layers expand and cool.
  • Star becomes a red giant.

Helium Flash and Beyond

  • Helium burning in the core through the triple alpha process.
  • Formation of elements like carbon and oxygen.
  • Final stages include the horizontal branch and asymptotic giant branch.
  • Ends as a white dwarf surrounded by a planetary nebula.

High-Mass Stars

  • Form from larger gas clouds with more mass.
  • Main sequence stars that are hotter, brighter, and burn fuel faster.

Supernova and Element Formation

  • High-mass stars end in supernovae, ejecting heavy elements into space.
  • Supernovae enable formation of elements heavier than iron.
  • Supernovae are extremely bright and visible across galaxies.

Remnants

  • White Dwarfs: Stars below 1.4 solar masses.
  • Neutron Stars: Stars with core mass between 1.4 and 3 solar masses.
  • Black Holes: Stars with core mass above 3 solar masses.

Black Holes

  • Form from stars whose core mass exceeds the neutron degeneracy pressure limit.
  • Infinite density where even light cannot escape, creating a singularity.
  • Black holes significantly warp spacetime.

Conclusion

  • The mass of a star determines its life cycle and the remnants it leaves behind.
  • Understanding stars is crucial to understanding elemental formation and the universe's development over billions of years.

Upcoming Topics

  • Detailed exploration of black holes.