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Two ways for the Sun to become a Black hole



 
 
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  #1  
Old July 14th 05, 02:01 PM
G=EMC^2 Glazier
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Default Two ways for the Sun to become a Black hole

Having its mass squeezed down to the size that its density has created a
black hole(few miles in size). Next way the Sun keeps its mass density
the same(almost twice that as water and is the size of the solar system.
It is possible a quasar fits as a black hole the size of our solar
system. This shows big is equivalent to small. Big falls at the same
rate as small. Does small have a minimum size? Does big have a maximum
size? Are micro objects obeying the same laws as macro objects(I think
not) Accelerating motion can make objects weigh more than the same
object at rest(That means it gained a greater force of gravity) Cern has
given us the weight measurements. Bert

  #2  
Old July 14th 05, 02:35 PM
Double-A
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G=EMC^2 Glazier wrote:
Having its mass squeezed down to the size that its density has created a
black hole(few miles in size). Next way the Sun keeps its mass density
the same(almost twice that as water and is the size of the solar system.



But that takes a hell of a lot more Sun!


It is possible a quasar fits as a black hole the size of our solar
system. This shows big is equivalent to small. Big falls at the same
rate as small. Does small have a minimum size? Does big have a maximum
size? Are micro objects obeying the same laws as macro objects(I think
not) Accelerating motion can make objects weigh more than the same
object at rest(That means it gained a greater force of gravity) Cern has
given us the weight measurements. Bert



It is said that if you crossed the event horizon of a solar system
sized black hole, you would not even notice that anything significant
had happened. There would just be no return ticket!

Double-A

  #3  
Old July 14th 05, 02:54 PM
G=EMC^2 Glazier
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Hi Double-A It is also said "That if you are very close to the event
horizon going in feet first your feet would stretch out miles from your
head(like spaghetti is made) and that you are right you would never
notice this because you are dead.No return ticket for sure Bert

  #4  
Old July 14th 05, 04:06 PM
Luigi Caselli
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"G=EMC^2 Glazier" ha scritto nel messaggio
...
Hi Double-A It is also said "That if you are very close to the event
horizon going in feet first your feet would stretch out miles from your
head(like spaghetti is made) and that you are right you would never
notice this because you are dead.No return ticket for sure Bert


Good news, I prefer spaghetti to italian meat balls... :-)

Luigi Caselli


  #5  
Old July 14th 05, 06:44 PM
G=EMC^2 Glazier
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Hi luigi I had an Italian meat ball fall of my table,and when it hit
the floor it still was in great shape. I had a miniature shuttle fall
off my desk,and hitting the floor it broke its left wing. That
leads me to believe its better to be inside an Italian meat ball than
the shuttle. Beert

  #6  
Old July 15th 05, 04:19 AM
Double-A
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G=EMC^2 Glazier wrote:
Hi Double-A It is also said "That if you are very close to the event
horizon going in feet first your feet would stretch out miles from your
head(like spaghetti is made) and that you are right you would never
notice this because you are dead.No return ticket for sure Bert



No Bert, that's for a much smaller theoretical black hole, where one
would be close enough to the singularity that the tidal forces would be
great. For a solar system sized theoretical black hole, the tidal
forces at the event horizon would be small, and one would have many
minutes left to live inside the black hole. But one would be across
that event horizon in much less than the blink of an eye!

The spaghetti stretching would come later.

Double-A

 




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