Astronomy Picture of the Day |
APOD: 2000 August 6 - The Coma Cluster of Galaxies
Explanation:
Almost every object in the above photograph is a galaxy.
The Coma Cluster of Galaxies
pictured above is one of the densest
clusters known - it contains thousands of
galaxies.
Each of these galaxies houses billions of stars -
just as our own Milky Way Galaxy does.
Although nearby when compared to most other
clusters,
light from the Coma Cluster
still takes hundreds of millions of years to reach us.
In fact, the
Coma Cluster is so big it takes light
millions of years just to go from one side to the other!
Most galaxies in Coma and other clusters are
ellipticals,
while most galaxies outside of clusters are
spirals.
The nature of
Coma's X-ray emission is
still being investigated.
APOD: 2000 February 20 - The Virgo Cluster Galaxies
Explanation:
Pictured are several galaxies of the Virgo Cluster,
the closest
cluster of galaxies to our
Milky Way Galaxy.
The
Virgo Cluster spans more than 5 degrees on the sky -
about 10 times the angle made by a
full Moon.
It contains over 100 galaxies of many types - including
spirals,
ellipticals, and
irregular
galaxies.
The
Virgo Cluster is so massive that it is noticeably
pulling our Galaxy toward it.
The cluster contains not only galaxies filled with stars but also
gas so hot it glows in
X-rays.
Motions of galaxies in and around clusters indicate
that they contain more
dark matter than any visible matter we can see.
Notable bright galaxies in the Virgo Cluster include
bright Messier objects such as
M61,
M87,
M90, and
M100.
APOD: 1996 April 19 - The Virgo Cluster: Hot Plasma and Dark Matter
Explanation:
This ROSAT image of the
Virgo cluster of galaxies reveals a
hot X-ray emitting plasma or gas with a
temperature of 10-100 million degrees pervading
the cluster. False colors have been used to represent
the intensity of X-ray emission.
The large area of X-ray emission, just below and left of center,
is about 1 million light-years across.
The giant elliptical galaxy M87,
the biggest member
of the cluster, is centered in that area while
other cluster members
are scattered around it.
By adding up the amount of
X-ray emitting gas astronomers
have found that its total mass is
up to 5 times the total mass of the cluster galaxies themselves -
yet all this
matter still does not produce nearly enough gravity to keep
the cluster from flying apart! Where is the unseen mass?
Because galaxy clusters are the
largest structures in the Universe, this
mysterious Dark Matter must dominate the cosmos
but its nature is still an
open question.
Authors & editors:
Robert
Nemiroff
(MTU)
& Jerry Bonnell (USRA)
NASA Technical Rep.:
Jay Norris.
Specific rights apply.
A service of:
LHEA at
NASA/
GSFC
&
Michigan Tech. U.