Saturday, July 9, 2016

Blackholes are the evolution of natural stages in physics

-  1891  -  Blackholes are the evolution of natural stages in physics and astronomy.  They are inevitable outcomes of interactions of mass and energy in the Universe.  The mystery remains, what happens after the Blackhole?
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------------------------  1891 -  Blackholes are the evolution of natural events.
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-  Blackholes are easy to explain and are the expected result of natural happenings.  Happenings that occur all over the Universe all the time.  So, how many Blackholes are out there?
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-  Mass and energy are the same thing.  Mass is simply concentrated energy according to E=mc^2.  Energy  =  mass  times  90,000,000,000,000,000.
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-  Mass bends , or warps, space-time.  Motion in space shrinks space and slows time, up to the limit of the speed of light.  Mass creates a gravity well that more mass falls in to.  Once enough mass is collected the gravity well is so steep, the gravity “ force” so strong, that not even the motion of photons can escape.  “c”  the speed of light, is not fast enough to climb the steep gravity well before falling back into the Blackhole.  “Black” because not even light can escape.
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-  Massive stars end their lives as supernovae explosions.  If the stars are large enough they leave behind a 3 to 20 Solar mass cinder with a radius small enough that a Blackhole forms.  There are super massive Blackholes at the center of most galaxies.  These Galactic Blackholes range in size from 1 million to 10 billion Solar Mass.
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-  Blackholes are a simple reality of evolution as gravity collects mass.  Enough mass and a Blackhole forms.  As a cluster of stars, or galaxies, grows denser, more mass lives at the center of the cluster.  Gravitational attraction between stars becomes stronger.  Stars orbit at faster rates.  Friction and temperatures rise.  The core gets denser and hotter and the outer regions expand.
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-  In the case of a single star the hydrogen to helium fusion produces gas pressure that holds the star up against the compression of gravity.  Heat is lost at the surface but nuclear reactions replace it.  Our Sun will do this for 10 billion years.  Our star is an intermediate mass and it will evolve into a Red Giant star ( a planetary nebula) with a White Dwarf star at its core.
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-  If the Sun were a larger star the greater mass and gravitational pressure would overcome electron degeneracy pressure ( collapsing atoms ) and even neutron degeneracy pressure collapsing into a Blackhole.  The Blackhole is inescapable for stars greater than 20 Solar Mass.
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-  When these natural processes go through enough stages in building compact cores the formation of a Blackhole is an inevitable outcome of general physics.  What happens next?  Where do Blackholes go from there?  Stay tuned as announcement will be made shortly.
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-  Request these Reviews to learn more about Blackholes:
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-  #1882  -  Could Blackholes explain Dark Matter?  The Universe expands into time, so, is there an edge to time?
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-  #1869  -  Blackhole mysteries,  how big can they get? NGC1600 is a Blackhole that is 2,700,000,000  Solar Mass.
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-  #1843  -  Great walls in space with Blackholes.
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-  #1819  -  New discoveries that may close the gap between stellar and galaxy center Blackholes.
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-  #1819  -  Lists 4 more reviews and there still remains 17 more on the subject.  Mysteries need lots of explanations.  Which ones will turn out to be right?
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