WIENER weiner WIENER weiner PENIS weiner WIENER weiner PEEPEE weiner HOTDOG weiner BRATWURST weiner SAUSAGE weiner MEATSTICK weiner WIENER weiner SCHADENFREUDE B^U buckley
Many people do not understand why it is so important for astronomers to understand the importance of knowing the difference between a regular nova and a Type I supernova. While it may appear, at the outset, that such information is unimportant for the average person, its worth immediately becomes apparent when one knows the repercussions of a Type I supernova.
WIENER weiner WIENER weiner PENIS weiner WIENER weiner PEEPEE weiner HOTDOG weiner LIVERWURST weiner SAUSAGE weiner MEATSTICK weiner WIENER weiner SCHADENFREUDE B^U buckley
While a typical nova merely releases a great deal of its mass and energy into the infinite blackness of space in a brilliant cascade of light, a Type I supernova explodes because it begins fusing carbon. This carbon fusion in a binary star system can be caused by two major factors, as far as we currently know.
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The first possibility, of course, when dealing with a binary star system such as could produce a Type I supernova, is a simple nova. In a simple nova, a white dwarf–whose electrons, at the atomic level, are so close that they are nearly touching each other–begins feeding off a larger star nearby, forming an “accretion disk”.
WOMB uterus WOMB uterus VAGINA vagina VAGINA vagina CORD vagina CORD vagina
The gas compresses and eventually becomes so hot that the the hydroges ignites and fuses into helium furiously.
QUEEF vagina BOOM vagina VAGINA vagina BABY vagina EXPLOSION vagina BOOM boom BOOM boom BOOM boom BOOM boom
The star becomes extremely luminous for a short time and eventually resolves into its original state.
Unfortunately for the white dwarf, this nova process is often not enough, as matter continues to compress on the surface. The star, unfortunately for its fate, cannot rid itself of all its gases. In this case, it becomes so heavy that even its electrons cannot stop an implosion. In this case, the star begins fusing carbon, and it reaches supernova level.
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hk;ahsdgoi;h;eie;gheihgthh;dhgck;hhiegutyyq
[uuzk.,h;haihgdyeuwoil;knci;hegiegrgr
? nac uoy llet tahw i ma gniyas
won ti si lla revo
pu si nwod
nd ıs poʍu
? dluohs siht eb eht dne ro eht gninnigeb
? rettam ti seod
ti si woh ti si
lla si tsol
hk;ahsdgoi;h;eie;gheihgthh;dhgck;hhiegutyyq
[uuzk.,h;haihgdyeuwoil;knci;hegiegrgr
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In another, similar event, a white dwarf hits another white dwarf, which creates a massive star and begins carbon fusion. In any case, the result is the same: the core collapses, and the star violently explodes.
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two lights here
two lights lost
one shattered
one broken
one pained
one frustrated
one hurt
one dejected
os ynam sevil
uʍop ǝpısdn pǝuɹnʇ
an instant in space
has begun
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and ended
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In spite of a supernova’s violence, it is a thing of gorgeous beauty, releasing into space a large amount of the heavy materials we know of on Earth. It is formed throughout the star, whereas a nova is an explosion of the outside of a star. A nova contains mainly hydrogen; a supernova creates nearly none.
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a birth
a beginning
like nobody has ever seen
a love
a life
so cruelly taken
given back
A thousand fold
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The Type I supernova is an integral part of the cosmos. It nearly always occurs with the same results and key properties. It is highly luminous. As such, its brilliant flash serves as a tool for those enterprising astronomers who wish to map the structure of the whole of the tapestry of the universe.
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mother
god
love
son
life
world
child
man
death
cross
rebirth
December 13, 2008 at 11:27 pm
Dude, I’m AFRAID to look at the video, now.