M81: Bode's Galaxy
M81 is one of the brightest galaxies in the northern sky. It can
easily be seen in a pair of binoculars under a relatively dark sky. However,
it is only with a sensitive detector (like a CCD camera) that the spectacular
nature of this Sb spiral galaxy can be appreciated. The nearby starburst
galaxy,
M82, recently
(in galactic terms) interacted with M81 by making a close pass in their
mutual orbits. Unlike the seemingly unaffected M81 shown here-
M82
is undergoing
incredible starforming and energy production throughout the galaxy.
Like most spiral galaxies, the starformation in M81 is taking place in the
defined arms of the galaxy. Small pink balls of light show the location
of a myriad of HII regions (the emission nebulae of M81). Bluish clumps
hint at the uncountable numbers of new stars in the spiral arms.
Interestingly, astronomers can learn a great deal about galaxies like this
by observing them various wavelengths of light. Recently the
Spitzer (formerly SIRTIF), space telescope imaged M81 in the micron
wavelengths of light which highlight the dust that is heated by these energetic
new stars.
M81 and M82 are around 12 million light years away.
Please click on the image below to see a larger image size.
Also be certain to check out this widefield image
of M81 and M82. |
Click on image for larger version.
Equipment
20in
RC Optical Systems telescope Operating at f/8.4
Paramount ME Robotic Telescope Mount
SBIG STL11000 CCD camera with color filter wheel
|
L
R
G
B
color production was used to create this image.
Luminance = 120 minutes
binned 1x1
Red = 30 minutes
binned 2x2
Green = 30 minutes
binned 2x2
Blue = 30 minutes
binned 2x2
|
Two iterations of L-R deconvolution (sharpening) algorithm using
CCDsharp were applied to the luminance image.
Digital Development (DDP) via Maxim/DL was also used in order to
display the the very dim and very bright details of the image simultaneously.
|
Minimum credit line: Stefan Seip/Adam Block/NOAO/AURA/NSF
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Updated: 02/08/2005