NGC 6894

NGC 6894 is a seemingly typical planetary nebula. It has a diffuse spherical outer shell with a more convoluted inner structure. The overall pinkish color to this nebula may be due to the reddening of light caused by intervening clouds of gas and dust in this direction. This nebula also has a unique attribute: in deep images (not shown here) this nebula may be interacting with the local interstellar medium (latent galactic gas clouds). Notice that the top left quadrant of the nebula has an oval bright area. This could be a symptom of this interaction. Furthermore, these deep images reveal that the gas released from this nebula has aligned itself with the local magnetic field of the galaxy. These observations help to probe the nature of our galaxy 4000 light years away!

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.

Credit:

KPNO/NOIRLab/NSF/AURA/Dale Niksch/Adam Block

About the Image

Id:noao-n6894block
Type:Observation
Release date:June 22, 2014, 6:22 a.m.
Size:1318 x 1318 px

About the Object

Name:NGC 6894
Constellation:Cygnus
Category:Nebulae

Image Formats

Large JPEGLarge JPEG
459.2 KB
Screensize JPEGScreensize JPEG
291.4 KB

Zoomable


Wallpapers

1024x7681024x768
239.9 KB
1280x10241280x1024
361.9 KB
1600x12001600x1200
437.5 KB
1920x12001920x1200
473.7 KB
2048x15362048x1536
2.2 MB

Coordinates

ObjectValue
Position (RA):20 16 23.81
Position (Dec):30° 35' 18.07"
Field of view:7.49 x 7.50 arcminutes
Orientation:North is 1.0° right of vertical


Colors & filters

BandWave-lengthTele-scope
Optical
B
438 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
G
475 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
R
625 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
Broad Band
555 nmVisitor Center 0.5-meter Telescope
Other CCD