DOOMSDAY
Theories on the Destruction of Earth

SUN:
SUPERNOVA
NASA/Gates Version
Supernova
for Dummies Version
Conclusion
NASA/Gates version:
As the mass
of the star's iron core approaches 1.4 solar masses (due to continued silicon
and sulfur burning in a thin shell adjacent to the iron core), a dramatic
sequence of events is being triggered: Gravity, which up to now was balanced
by the outward force of the pressure, decisively gains the upper hand and
.In less than a second, the core collapses from a size of about 5,000 miles
to one of about a dozen miles, and an enormous amount of energy is released.
This collapse happens so fast that the star's outer layers have no time
to react and participate in it. What is released during core collapse is
truly gigantic. It is equivalent to the energy produced by 100 stars like
the Sun, during their entire lifetimes of more than 10 billion years! Most
of the energy released during the collapse of the iron core is carried
off into space by elusive particles. A small fraction of the energy is
deposited into the lower layers of the envelope surrounding the core and
triggers the supernova explosion.
The
energy deposited in the lower layers of the envelope creates a super strong
shock wave that runs outward through the envelope toward the star's surface.
As the shock wave runs outward, it heats the envelope, induces explosive
nuclear burning, and ejects the envelope at speeds of thousands of miles
per second (i.e., in excess of 10 million miles/hour). It is during this
phase that elements heavier than iron are being manufactured. When the
shock wave reaches the star's surface, it very quickly heats the surface
layers and brightens them. Within a day or two the exploding star becomes
brighter than a billion Suns. This is the moment when distant observers
first learn that a supernova is exploding (unless they have been lucky
enough to detect some of the neutrinos that were emitted earlier during
core collapse). A star appears where, as viewed over the great distances
of interstellar or intergalactic space, none was seen before -- hence,
the term nova, which means "new." The result of these events is a compact
stellar remnant and a rapidly expanding gaseous shell. The stellar remnant
is a neutron star or a black hole. The expanding gaseous shell plows into
the surrounding interstellar medium, and pushes, compresses, and intermingles
with it. Such regions of the interstellar medium are known as After
some
weeks, the brightness of the explosion diminishes, although the supernova
may remain visible for many months or years, even across intergalactic
distances. About 20 to 30 supernovae are discovered each year in galaxies
beyond the Milky Way. Most are too faint to be seen without a telescope
due to their great distances.

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Supernova
for Dummies version:
Scientists
say that a star's lifetime is around 10 billion years old, and right now
the Sun is about 5 billion years old, so it should be (you can do the statistical
math). When the Sun goes supernova, be ready to say bye bye to mommy.
After
10 billion years is up the Sun will start to expand and swell up like a
fat man at an all you can eat bar. As it increases in size, it will devour
Mercury, Venus and com a little too close to home. As the temperature increases
we will be toasted beings, actually dead ones. The crust of the sun would
remain rather cool than normal, only about 3,000 kelvin. Its normal temperature
is about 6,000 kelvin. Within a quick time the star's core collapses and
then explodes, leaving a black hole, matter and some heat from the
sun being blown out into space. The explosion can be seen from many galaxies
away due to the bright light it emits. Strong gravitational pulling occurs
as the black hole sucks everything into oblivion. Now on your merry little
journey to oblivion, planets, comets and mass objects may collide creating
catastrophes within a catastrophe.
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Conclusion:
In conclusion,
a supernova will come and there is nothing we can do about it but experience
the massive pain it will inflict. Whenever it comes GOD HELP US ALL.
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