|
Instrument |
12.5" RCOS @ ~f/9
(2880 mm fl) 0.64 arcsec / pixel. The Zoomify image scale is
0.85 to 3.22 arcsec / pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Gen I Filters |
Acquisition Data |
4/17/2008 to 6/7/2008
Chino Valley... with CCDAutoPilot3 |
Exposure |
Lum |
440
min. (44 x 10 min. bin 1x1) |
RGB |
300 min. (10 x 10 min. bin 2x2) each |
Ha |
300 min. (10 x
30 min. bin 1x1) |
|
Software |
-
CCDSoft, CCDStack,
Photoshop CS6, PixInsight and Noel Carboni's actions.
-
eXcalibrator v4.01 for
(g:r) color balancing, using 32 stars from the SDSS-DR9
database.
-
CCDStack to calibrate, register,
normalize, data reject, combine the sub exposures and create the RGB
image.
-
PixInsight for gradient removal and
initial non-linear stretching.
-
PhotoShop for the LRGB combine & final
touch-up.
-
Noiseware 5, a PhotoShop plug-in.
|
Comment |
North is to the top.
M101 was discovered by Pierre Méchain on March 27, 1781, and he
subsequently communicated his discovery to Charles Messier who
verified its position and added it to the Messier Catalogue. AT a
distance of about 27 million light-years, M101 is a relatively large
galaxy compared to the Milky Way. With a diameter of 170,000
light-years it is nearly twice as large.
A remarkable property of this galaxy are its huge and extremely
bright HII regions, of which a total of about 3000. HII regions are
places in galaxies that contain enormous clouds of high density
hydrogen gas contracting under its own gravitational force.
Eventually, when the localized hydrogen contracts enough for fusion
processes to begin, stars are born.
Source:
Wikipedia
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