Called the Veil Nebula, the debris is one of the best-known supernova remnants, deriving its name from its delicate, draped filamentary structures … This close-up look unveils wisps of gas … The nebula lies along the edge of a large bubble of low-density gas … In this image, red corresponds to the glow of hydrogen, green from sulfur, and blue from oxygen
A few thin, crisp-looking, red filaments arise after gas is swept into the shock wave at speeds of nearly 1 million miles an hour, so fast that it could travel from Earth to the moon in 15 minutes.
Veil Nebula Supernova Remnant | Hubble NASA
Gravity or Kristian Birkeland plasmoids?
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Despite the nebula’s complexity and distance from us, the movement of some of its delicate structures is clearly visible – particularly the faint red hydrogen filaments. In this image, one such filament can be seen as it meanders through the middle of the brighter features that dominate the image
… Hidden amongst these bright, chaotic structures lie a few thin, sharply edged, red coloured filaments. These faint hydrogen emission features are created through a totally different mechanism than that which generates their fluffy red companions
Revisiting the Veil Nebula | Space Telescope
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Electric plasma power lines or 30,000 light years length of gas powered by some theoretically impossible event 1000's of years ago as the only possible explanation?
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