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.

Créditos:

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

About the Image

Id:noao-n6894block
Tipo:Observation
Release date:22 de Junio de 2014 a las 06:22
Size:1318 x 1318 px

Sobre el Objeto

Nombre:NGC 6894
Constellation:Cygnus
Categoría:Nebulae

Formatos de Imágenes

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459,1 KB
Screensize JPEGScreensize JPEG
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Coordenadas

ObjectValue
Posición (AR):20 16 23.81
Posición (Dec):30° 35' 18.07"
Campo visual:7.49 x 7.50 arcminutes
Orientación:North is 1.0° right of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
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