Black Holes: The Ultimate Stellar Collapse

  1. Black holes form when massive stars collapse under their own gravity after a supernova.
  2. Their gravity is so strong that not even light can escape once it crosses the event horizon.
  3. Black holes come in different sizes, from stellar-mass to supermassive giants at galaxy centers.
  4. The Milky Way’s supermassive black hole, Sagittarius A*, is about 4 million times the Sun’s mass.
  5. Time and space warp dramatically near a black hole, creating extreme gravitational effects.
  6. Matter falling into black holes can heat up and emit powerful X-rays before crossing the horizon.
  7. Some black holes power quasars—brilliant cosmic beacons visible across the universe.
  8. Black hole mergers produce gravitational waves, ripples in spacetime detected on Earth.
  9. Despite their name, black holes can be indirectly observed through their influence on nearby stars and gas.
  10. Over unimaginable timescales, black holes may slowly evaporate through Hawking radiation.