The Helix Nebula by ESO (European Southern Observatory) at the La Silla observatory in Chile.
The blue-green glow in the centre of the Helix comes from oxygen atoms shining under effects of the intense ultraviolet radiation of the 120 000 degree Celsius central star and the hot gas. Further out from the star and beyond the ring of knots, the red colour from hydrogen and nitrogen is more prominent. A careful look at the central part of this object reveals not only the knots, but also many remote galaxies seen right through the thinly spread glowing gas.

The Helix Nebula by ESO (European Southern Observatory) at the La Silla observatory in Chile.

The blue-green glow in the centre of the Helix comes from oxygen atoms shining under effects of the intense ultraviolet radiation of the 120 000 degree Celsius central star and the hot gas. Further out from the star and beyond the ring of knots, the red colour from hydrogen and nitrogen is more prominent. A careful look at the central part of this object reveals not only the knots, but also many remote galaxies seen right through the thinly spread glowing gas.

  1. craftytrickyjellyjam reblogged this from sixeyesfromhell
  2. aloneindaastros reblogged this from atomic-astronaut
  3. polymath4ever reblogged this from sixeyesfromhell
  4. skinnyjeansandconverse reblogged this from sixeyesfromhell
  5. sixeyesfromhell posted this