Galaxy NGC 474: Shells and Star Streams
Explanation:
What's happening to galaxy NGC 474?
The multiple layers of emission appear strangely complex and unexpected given the
relatively featureless appearance of the
elliptical galaxy in
less deep images.
The cause of the shells is currently unknown, but possibly
tidal tails related to debris left over from absorbing
numerous small galaxies in the past billion years.
Alternatively the
shells
may be like ripples in a pond,
where the ongoing collision with the spiral galaxy just above
NGC 474
is causing
density
waves to ripple through the galactic giant.
Regardless of the actual cause, the
featured
image
dramatically highlights the increasing consensus that at least some elliptical
galaxies
have formed in the recent past, and that the outer halos of most
large galaxies are not really smooth
but have complexities induced by frequent
interactions with --
and accretions of --
smaller nearby galaxies.
The halo of our own
Milky Way Galaxy
is
one example of such
unexpected
complexity.
NGC 474 spans about 250,000
light years and lies about 100 million light years distant toward the constellation
of the Fish
(
Pisces).
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
