Credit & Copyright: NASA /
X-ray: Y. Chu (UIUC) et al.,
Optical: J. P. Harrington, K. J. Borkowski
(UMD),
Composite: Z. Levay (STScI)
Explanation:
Haunting patterns within planetary nebula
NGC 6543
readily suggest its popular moniker -- the Cat's Eye nebula.
In 1995, a stunning false-color optical image
from the Hubble
Space Telescope detailed the swirls of this
glowing nebula, known to
be the gaseous shroud expelled from a dying
sun-like
star about 3,000 light-years from Earth.
This composite picture combines the famous Hubble image
with new x-ray data from the
orbiting
Chandra Observatory and reveals
surprisingly intense x-ray emission indicating the presence
of extremely hot gas.
X-ray emission is shown as blue-purple hues superimposed on red and
green optical emission.
The nebula's central star itself is clearly immersed in
the multimillion degree, x-ray emitting gas.
Other pockets of x-ray hot gas seem to be bordered by cooler
gas emitting strongly at optical wavelengths, a clear indication
that expanding hot gas is sculpting the
visible Cat's Eye
filaments and structures.
Gazing into the Cat's Eye, astronomers see
the fate of our sun,
destined to enter its own
planetary nebula phase
of evolution ... in about
5 billion
years.
Composite: Z. Levay (STScI)
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Publikacii s klyuchevymi slovami:
Planetarnaya tumannost' - planetary nebula - Cat's Eye Nebula - NGC 6543 - rentgenovskoe izluchenie - tumannost' Koshachii glaz
Publikacii so slovami: Planetarnaya tumannost' - planetary nebula - Cat's Eye Nebula - NGC 6543 - rentgenovskoe izluchenie - tumannost' Koshachii glaz | |
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