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| As the Sun expands, its temperature
will be slightly cooler, so it will be red, rather than yellow.
It will be known as a red giant star. At this point, it will be
using helium as fuel. When the helium is used up, the core will
shrink to about the size of Earth and the remaining layers of
gas will float off into space. The core will become a white dwarf
star. A white dwarf has no fuel to convert to radiant energy,
only the leftover thermal energy from its energy-producing days
keeps the star hot for a long time. Over a period of several million
years, a white dwarf cools down and becomes a cold object called
a black dwarf. |
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| Massive
stars go out in a blaze of glory. When a massive star's core runs
out of fuel, it starts shrinking in on itself until it can shrink
no farther. Powerful shock waves from this sudden stop fan outward,
and particles of matter spin off into space carrying huge amounts
of energy with them. A gigantic explosion occurs that is millions
or billions of times as bright as the star ever was. This explosion
is known as a supernova.
It hurls matter and energy
far out into space. Usually, all that will be left behind is a
ball of neutrons that is about 20 km (12 mi) across. This city-sized
object is called a neutron star. |
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| If the
core was quite massive—more massive than three Suns—the
core's own gravity will keep causing it to shrink in on itself
until it becomes a black hole. A black
hole is a point
in space that has such a strong force of gravity that nothing
within a certain distance of it can escape getting pulled into
the black hole—not even light. |
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1. |
What
is the Sun? |
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2. |
Where does a new
star form? |
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3. |
Summarize
the three
ways a star
might die. |
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In this photograph,
stars are seen
forming and dying. |
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| onmouseover="this.T_STATIC=true; return escape('This star is about to have a supernova. The ring and nearby clouds are debris ejected from the star\'s poles and equator.')" /> |
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This star
is about to have a supernova.
The ring
and nearby clouds are debris ejected from the star’s poles
and equator. |
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Stars are forming
in these clouds. |
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At the center of this nebula,
two stars orbit each other. One of the stars is dying and has
thrown off most of its gas layers, creating this butterfly-shaped
cloud of gas and dust. |
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