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Life Cycle of Stars

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Life Cycle of Stars Stars are born in Nebulae Vast clouds of gas and dust Composed mostly of hydrogen and helium Some cosmic event triggers the collapse of a portion ... – PowerPoint PPT presentation

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Title: Life Cycle of Stars


1
Life Cycle of Stars
2
Stars are born in Nebulae
  • Vast clouds of gas and dust
  • Composed mostly of hydrogen and helium
  • Some cosmic event triggers the collapse of a
    portion of the nebula
  • Gravity condenses the matter into a central area
  • Heat and pressure build in the core
  • Protostar is formed

3
Eagle Nebula
Helix Nebula
4
Protostar
5
A Star is Born
  • When fusion of hydrogen begins in the core, the
    protostar becomes a star
  • High Mass Star a star whose mass is gt3 solar
    masses (gt3 times the mass of our sun)
  • Low Mass Star A star whose mass is lt3 solar
    masses

6
Nuclear Fusion
7
Hertzsprung-Russell Diagram
8
A Stars Balancing Act
  • A star stays on the Main Sequence as long as
    there is a balance of inward and outward forces
  • Inward Force Gravity
  • Outward Force Heat Pressure generated by
  • nuclear fusion

9
Nuclear fusion
Star Equilibrium Balance of Forces
10
Life Span Low Mass Star
  • Hydrogen fusion in the core continues for
    billions of years, forming helium
  • Once the hydrogen in the core is used up, the
    star begins to collapse and moves to the next
    stage in its life.
  • Heat and pressure in the core cause the helium to
    fuses rapidly, causing a helium flash.
  • Outer layers of the star begin to expand

11
Final Stages Low Mass Star
  • Outer layers expand and star becomes a Red Giant
  • Eventually the outer layers disperse, leaving a
    very hot, dense core (maybe the size of Earth)
    called a White Dwarf

12
Red Giant
Red Giant
White Dwarf
13
Life Span High Mass Star
  • Hydrogen fuses to helium in the core but is used
    up much faster may last only 100 million years
  • Once the hydrogen in the core is used up, the
    star begins to fuse heavier elements.
  • Heavier elements continue to fuse until iron
    (element 26) is formed.
  • Iron cannot be fused in the core of a star
    fusion stops and gravity takes over, collapsing
    the star

14
Final Stages High Mass Star
  • With decreasing outward pressure, gravity causes
    the star to collapse.
  • The collision of atoms in the core causes a
    Supernova explosion.
  • All the elements heavier than iron are formed in
    a supernova explosion.
  • Remnants of a supernova depends on the stars
    mass
  • Neutron Star a dense star body made of neutrons
  • Black Hole an object so dense even light cannot
    escape.

15
Black Hole
High Mass Star
Supernova
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