Stephan's Quintet is a group of five galaxies in the constellation Pegasus.
Downloadable versions (see
NOAO Conditions of Use):
Note that this picture includes a sixth nearby galaxy with similar
redshift to the four high-redshift members of the group.
The components are identified in this picture by their NGC number,
with their redshift in kilometers per second given underneath
each name.
This picture was taken at the Kitt Peak National Observatory's 0.9-meter
telescope in October of 1998 by Nigel Sharp.
North is up, east is to the left.
Minimum credit line: N.A.Sharp/NOAO/AURA/NSF
(for details see Conditions of Use)
400 x 400 16 kb color JPEG
1600 x 1600 264 kb color JPEG
1600 x 1600 2.5 Mb 8-bit color TIFF
1600 x 1600 7.5 Mb 24-bit color TIFF
Stephan's Quintet, as its name implies, is a group of five galaxies
(NGC7317, 7318A, 7318B, 7319 and 7320) in the constellation Pegasus.
This unusual system has often been used as proof that the redshift
is not truly a distance indicator, which would completely overturn current
cosmology, because although four of the galaxies have similar, large
redshifts, the fifth (NGC7320), although apparently a member of the group,
shows a much smaller redshift. Conventional theory states that the
low-redshift galaxy is in a nearby group (the NGC7331 group) and by
coincidence appears on the sky projected against a distant background group.
Opponents point to debris and tails around the low-redshift galaxy,
suggesting that it is interacting with the high-redshift systems, which would
require that all five galaxies be at the same physical location in space.
Component labels and redshifts.
Return to:
galaxies page.
Comments by e-mail to images@noao.edu