Black Holes Through Einstein’s Lens of Relativity

  1. Black holes are regions where gravity warps spacetime so intensely that nothing can escape.
  2. Einstein’s general relativity predicted black holes as natural outcomes of massive stars collapsing.
  3. At the event horizon, the escape velocity equals the speed of light.
  4. Time slows dramatically near a black hole compared to distant observers.
  5. Light bends around black holes, creating dramatic gravitational lensing effects.
  6. Supermassive black holes sit at the centers of most galaxies, including our Milky Way.
  7. The first image of a black hole’s shadow was captured in 2019 by the Event Horizon Telescope.
  8. Black holes merge and send out gravitational waves—ripples in spacetime detected on Earth.
  9. Relativity shows black holes stretch space and distort time in extreme ways.
  10. Though invisible directly, black holes reveal themselves through their effects on nearby stars and gas.