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black holes

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PRESENTATION OUTLINE

BLACK HOLES

KATE HACKERSON

BLACK HOLE THEORY

  • Nothing can escape Black holes
  • Scientists can’t see black holes
  • Black holes absorb dust to expand in mass

Types Of Black Holes

STELLAR

  • Smallest size of black hole
  • 3x and more of the sun’s mass
  • Forms when a supernova happens

INTERMEDIATE

  • Mid-size black hole
  • Fairly recently discovered, not easily found
  • Forms when stars in a cluster collides in a chain reaction
Photo by theqspeaks

SUPERMASSIVE

  • The biggest black hole, Billions-millions times greater than the sun’s mass
  • They lie at the center of every galaxy
  • Potentially formed by merging black holes, large gas clouds collapsing on themselves, or a stellar cluster collasping

BINARY BLACK HOLES

  • 2 black holes progressively getting closer to each other
  • May be formed from two black holes falling together, or two stars born together and die together
  • Categorized like regular black holes

Parts of a Black Hole

EGROSPHERE

  • Where the gravitational pull starts
  • Objects can’t be stationary anymore
  • Outside the event horizon

EVENT HORIZON

  • “Black” part of the Black hole
  • Speed of light gravitational pull
  • Once a particle crosses the event horizon, it cannot escape

SINGULARITY

  • The center-most region of the Black hole
  • Where all the mass lies
  • A single point in space time

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QUANTUM MECHANICS

  • Each particle has an antiparticle
  • If an antiparticle-particle pair forms just after the event horizon, one of the pair will be ejected
  • The event horizon is reduced and the black hole can decay if this happens
Photo by rawpixel.com

LAST THINGS TO THINK ABOUT

  • No black hole is close enough to destroy earth
  • The sun is not big enough to create a black hole
  • If you fell into a black hole, you would die before you reached the singularity
  • Nothing would happen if a black hole the same mass as the sun replaced the sun
Photo by Kevin M. Gill