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| SUPERNOVAS! |
Supernova
1987A, in the LMC |
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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...
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:
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One of 2 things may
be left behind...
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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. |
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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:

[Clicking on image will begin download of an MPEG animation
from Cambridge University in the UK]
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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
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Visit: The Web Nebulae and find
stellar
remnants. |
Click on one of these links to get a
plug-in that plays MPEG movies.
UPDATED:
11/04/07 |