Dark Matter Halos: Invisible Skeletons of Galaxies

  1. Dark matter halos are invisible cocoons of matter that surround galaxies.
  2. They act as the “skeletons” holding galaxies together with their unseen gravity.
  3. Without halos, galaxies would fly apart—their visible mass isn’t enough to bind them.
  4. Halos are far larger than the galaxies they host, stretching hundreds of thousands of light-years.
  5. We can’t see dark matter, but we detect halos through their gravitational effects.
  6. Galaxy rotation curves—stars moving too fast at the edges—first revealed their presence.
  7. Halos also bend light from distant galaxies, a phenomenon called gravitational lensing.
  8. Computer simulations show halos as the backbone of the cosmic web.
  9. They are thought to contain 80–90% of a galaxy’s total mass.
  10. Unlocking the mystery of halos could solve one of the biggest puzzles in modern physics.