Gum Nebula, Supernova Remnant

Gum Nebula



One of the closest supernova remnants in the sky is the Gum Nebula. It appears as a giant bubble of gas across the rich starfields of the Milky Way. The objects in the image are below the horizon for most northern hemisphere observers. (Probably visible from the Florida Keys and Hawaii) Even from the most transparent night sky locations it is difficult if not impossible to see any portion of the Gum nebula with the naked eye. However, modern films and digital processing techniques can record much of its extensive sky coverage. This image covers an area of sky through the constellation's Canis Major (top), Puppis & Vela (center), and Carina (bottom). Angular size of the nebula is 75 x 40 degrees. Its distance is roughly 1400 light years from the Earth, with the nearest edge of the nebula only 450 light years away. It was discovered in 1952 by Australian astronomer Colin Gum.

Technical Details:

  • Subject: Gum Nebula Super Nova Remnant
  • Instrument: Pentax 67, 105mm f/4 lens
  • Platform: Losmandy Gll
  • Exposure: 2 x 35 minutes
  • Film: Kodak PPF 400 (unhypersensitized)
  • Location: American-Australian Imaging Station, Coonabarabran, New South Wales, Australia
  • Photographer(s): John Gleason
  • Notes: This image is part of a 180 degree panoramic sequence on the southern Milky Way. Two 35 minute exposures were "added" in Picture Window software and were later enhanced in PhotoShop to bring out the faint nebula details.
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    Last updated: 04/22/00