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M87: Chandra Reviews Black Hole Musical: Epic But Off-Key
A striking example of the power and effervescence of supermassive black
holes is shown in this composite image of the elliptical galaxy M87 in
the Virgo Cluster. The features in this image imply that outbursts and
deep sounds have been generated by the black hole for eons.
The black hole located in the center of M87 is one of the most massive
in the universe. The huge reservoir of hot gas in this cluster is shown
in this low energy X-ray image from the Chandra X-ray Observatory (red).
An optical image from the Digitized Sky Survey shows stars in M87 in blue.
A series of unevenly spaced loops and bubbles are visible in the hot gas
below and to the left of the center of M87. These features are produced
by small outbursts from close to the black hole about once every 6
million years. The sound waves generated by these outbursts, not visible
in this image, will be incredibly deep, about 56 octaves below middle C.
Because the outbursts are unevenly spaced the sound will be more like
noise from the black hole rather than a harmonious musical performance.
A shock wave -- similar to a sonic boom -- is detected in a separate
Chandra image of M87 that shows high energy X-rays. This shock was produced
by a powerful outburst from the black hole about 20 million years ago. The
properties of the shock, including the change in temperature and density in
the gas, are consistent with classical physics. A large bubble in the
X-ray gas shows another powerful outburst occurred about 50 million years
earlier. The long interval between these two outbursts provides evidence
for even deeper sounds, 58 or 59 octaves below middle C.
Other remarkable features are seen in M87 for the first time including
narrow filaments of X-ray emission, which may be due to hot gas trapped
to magnetic fields. One of these filaments is over 100,000 light years
long, and extends below and to the right of the center of M87 in almost
a straight line.
| Fast Facts for M87: |
| Credit |
X-ray: NASA/CXC/CfA/W.Forman et al.; Optical: DSS |
| Scale |
Image is 14.4 arcmin per side |
| Category |
Quasars & Active Galaxies, Groups & Clusters of Galaxies
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| Coordinates (J2000) |
RA 12h 30m 49.50s | Dec +12º 23' 28.00 |
| Constellation |
Virgo |
| Observation Dates |
9 observations between July 2002-Nov 2005
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| Observation Time |
146 hours |
| Obs. IDs |
2707, 3717, 5826-28, 6186, 7210-12
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| Color Code |
Energy (X-ray: Red; Optical: Blue) |
| Instrument |
ACIS |
| Also Known As | NGC 4486 |
| Distance Estimate |
About 50 million light years |
| Release Date |
October 05, 2006 |
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