NGC 7027

Click on image for larger version.

The HST image is shown as a tool to identify some of the features of this very complex object. Both images show an inner torus of gas that is glowing very brightly. This inner structure is enshrouded by an obscuring (though translucent) pillow-like cloud of gas and dust. This object is often considered the very initial stage of the expanding planetary nebula within. Soon the tenuous cloud of dust will be blown away- to leave a brilliantly glowing ring-like nebula. Note that the bright green area of the nebula corresponds with the area where the dust is thinnest (see the HST image). Thus, this area is a little window through which we see the OIII emission escaping directly and the baby nebula to come! Be certain to click on our image to see the largest view.

Equipment

20in RC Optical Systems telescope Operating at f/8.4
Paramount ME Robotic Telescope Mount
SBIG ST10XME CCD camera with color filter wheel

L R G B color production was used to create this image.

Luminance = 30 minutes binned 1x1
 Red = 7.5 minutes binned 1x1
 Green = 7.5 minutes binned 1x1
 Blue = 11.5 minutes binned 1x1
  • Many iterations of L-R deconvolution (sharpening) algorithm using CCDsharp were applied to the luminance image.

    • Minimum credit line: Adam Block/NOAO/AURA/NSF

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    Updated: 07/08/2003