Research page:Black holes

From eagle-rock.org

Introductory notes

  1. A black hole is an infinitely dense region that contains the mass of millions or billions of Suns and from which no light can escape
  2. Probably each elliptical galaxy, the largest in the cosmos, contains a supermassive black hole when about 3.5 billion years old - these are called high-energy quasars
  3. The biggest black hole discovered as of 2009 weighs 18 billion suns and is about the size of an entire galaxy
  4. The event horizon is the sphere around a black hole within which nothing can escape because all light and info is pulled in and because nothing can go quicker than the speed of light, the event horizon can also be seen as the edge of the universe. The universe looks like a kind of Swiss cheese.
  5. 'The properties of time and space are reversed'
  6. Celestial bodies can orbit around a black hole as long as they are outside the event horizon. The mass is still there.
  7. The heaviest black hole observed in 2008 was 3 billion x sun mass, which is about the mass of an ordinary galaxy = supermassive black holes
  8. An ordinary black hole has about the mass of 10 suns
  9. Light cannot escape a black hole because it loses energy trying to escape, just like light that moves away from a heavy object loses energy because it red-shifts to lower frequencies of life.
  10. It isn't clear where the super-massive black holes at the centers of galaxies came from. They have a mass of billions of suns. It may be that at the beginning of the cosmos there existed super-massive stars whose collapse caused the super-massive black holes.
  11. Black holes don't have a surface but neutron stars do. This means that all gas that approaches a black hole gets sucked in and doesn't radiate light while neutron stars emit light when this happens.

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