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Chapter 14: Stellar Remnants

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High mass stars, after a supernova explosion. Neutron star. Initial ... About the ... Neutrons squish together tighter than carbon atoms. Spin about 1000 ... – PowerPoint PPT presentation

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Title: Chapter 14: Stellar Remnants


1
Chapter 14 Stellar Remnants
  • Dr. Michelle Arnold
  • November 13, 2009

2
What Remains After a Star Dies
  • Low mass stars, after a planetary nebula
  • White dwarf
  • Initial star 0.1-10 M
  • White dwarf lt1.4 M
  • High mass stars, after a supernova explosion
  • Neutron star
  • Initial star 10-25 M
  • White dwarf 1-3 M
  • Black hole
  • Initial star 25-30 M
  • White dwarf gt3 M

3
White Dwarfs
  • About the mass of Sun
  • About the size of the Earth
  • Mostly degenerate carbon, may have a small amount
    of helium and hydrogen on the surface
  • High temperatures remain from previous fusion and
    gravitational collapse
  • Small size means they are very dim
  • Continue to cool

4
Neutron Star
  • Degenerate neutrons
  • Very small
  • About 10 km across
  • MUCH smaller than white dwarfs
  • Neutrons squish together tighter than carbon
    atoms
  • Spin about 1000 times per second!
  • Some are pulsars
  • Axis of rotation is different from magnetic axis
  • Appear as light house lights blinking on and
    off in the radio wave frequency

5
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6
Gravity
  • Newton described gravity in an equation
  • He did not explain the why or how
  • Einstein proposed that any mass will distort or
    bend the space around it
  • 2D world, it bends into the third dimension
  • 3D world, it bends into the fourth dimension!
  • If another mass approaches this dip in space,
    it can fall in, setup a stable orbit or escape
    and fly off (depending on how fast it is going)

7
Distorted 2D Space
8
Evidence that SupportsEinsteins Theory of
Gravity
  • Circumference of Earths orbit 2?r
  • Measured distance (radius) from Earth to Sun is
    bigger!
  • Gravity can effect light which has no mass!

9
Black Hole
  • Large mass (singularity) causes a large
    distortion in space
  • They are not little vacuum cleaners!
  • Event horizon distance from the singularity at
    which the escape velocity equals the speed of
    light
  • Nothing can escape after it passes closer than
    the event horizon
  • Black holes appear black
  • Left on its own a black hole would evaporate!
    (Hawking radiation)

10
  • http//www.dailymotion.com/video/x2enyl_homer-3d_s
    hortfilms

11
Adding Mass to a Star Remnant(Type 1 Supernova
anddetecting a black hole)
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