Hubble image archive

Black Hole-Powered Spiral Galaxy NGC 7742

What may first appear as a sunny side up egg is actually NASA Hubble Space Telescope's face-on snapshot of the small spiral galaxy NGC 7742. But NGC 7742 is not a run-of-the-mill spiral galaxy. In fact, this spiral is known to be a Seyfert 2 active galaxy, a type of galaxy that i...

Date
Jan 1, 1998
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-1998-28-696-image
By

What may first appear as a sunny side up egg is actually NASA Hubble Space Telescope's face-on snapshot of the small spiral galaxy NGC 7742. But NGC 7742 is not a run-of-the-mill spiral galaxy. In fact, this spiral is known to be a Seyfert 2 active galaxy, a type of galaxy that is probably powered by a black hole residing in its core. The core of NGC 7742 is the large yellow "yolk" in the center of the image. The lumpy, thick ring around this core is an area of active starbirth. The ring is about 3,000 light-years from the core. Tightly wound spiral arms also are faintly visible. Surrounding the inner ring is a wispy band of material, which is probably the remains of a once very active stellar breeding ground.

Credits

Image

AURA, STScI, NASA, Hubble Heritage Project (STScI, AURA)

Image Details

About The Object
Object NameNGC 7742
Object DescriptionFace-on Spiral galaxy
R.A. Position23h 44m 15.85s
Dec. Position10° 46' 0.9"
ConstellationPegasus
Distance72 million light-years (22 million parsecs)
DimensionsThe entire visible galaxy is 36,000 light-years (11,000 parsecs) across. The image is approximately 80 arcseconds across.
About The Data
Data DescriptionPrincipal Astronomers: C. R. Lynds (NOAO/KPNO), J. A. Westphal (CalTech), Earl O'Neil Jr. (NOAO/KPNO), and collaborators.
InstrumentHST>WFPC2
Exposure DatesJuly 9, 1995, Exposure Time: 1 hour
FiltersF336W (U), F555W (V), and F675W (R)
About The Image
Color InfoBlue: F336W (U) Green: F555W (V) Red: F675W (R)

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