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SUPERNOVAS!

Supernova 1987A, in the LMC

 

    If a star is large enough, it has enough mass to cause the fusion of carbon into
       magnesium and other elements (because the temperature is 600 million K)
       until iron is formed...

        -And iron won't burn-

à     So the star continues to collapse until iron nuclei are touching one another...

    At this point, the mass of the star "bounces" off its core in a tremendous explosion called a supernova...

à That sends most of the star's mass into space at great speed:
 

One of 2 things may be left behind...

A Neutron Star

OR

A Black Hole

At the center, the remains of the iron core collapses to force electrons and protons together to form neutrons resulting in a
neutron star.
  A sufficiently more massive star may collapse beyond the bounds of the neutrons and become a
Black Hole.

If this neutron star emits energy in a particular direction, and we can detect it, it "pulses" a radio wave - called a Pulsar: Download an animation of a pulsar.

[Clicking on image will begin download of an MPEG animation from Cambridge University in the UK]

 

Gravity becomes so great, not even light can escape; In effect, a "hole" in space-time is formed:

Check out the
 Bijou Black Hole Page
APOD: Planet Near a Galaxy Core

  Visit: The Web Nebulae and find stellar remnants.

 

 

From all these processes, matter is strewn about space.

 
 

When it gathers in enough abundance, another nebula is formed...a star-forming nebula.

 

......Here is an Accretion Disk Simulation

à  

 The process of star formation can begin again.

 
 

Many consider that we, therefore, are all made of "star stuff."

   
 

Back to ASTRONOMY Class Outline


Click on one of these links to get a plug-in that plays MPEG movies.

 MPEG sites: 
  MPEG players
  InterVU: Free MPEG player
  Sparkle - An FTP file for The Mac

UPDATED: 11/04/07