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Click the image for a 70%
size, 4.95
arcsec/pixel display (1800 x 1200)
Instrument |
Takahashi FSQ-106ED @
f/5.0 (530 mm F.L.) Captured at 3.5 arcsec/pixel. Shown
resampled to 11.9 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
Acquisition Data |
1/11/2009
to 1/28/2009 Chino Valley... with CCDAutoPilot3 |
Exposure |
SII:Ha:OIII
45 min. (15 x 1 min. each filter, bin 1x1)
SII:Ha:OIII 225
min. (15 x 5 min. each filter, bin 1x1)
SII:Ha:OIII 675
min. (15 x 15 min. each filter, bin 1x1)
SII,Ha & OIII are mapped
to RGB respectivly. An RGB overlay was added for the star
colors.
Click
here for the natural colored image.
Click here for the B & W Ha filtered
image. |
Software |
CCDSoft,
CCDStack, Photoshop CS w/ the Fits Liberator plugin and Noel Carboni's actions.
CCDStack to calibrate, register,
normalize, data reject & combine sub exposures.
PhotoShop for
non-linear stretching and color combine. |
Comment |
North is to the top.
This image was created
using the Hubble color palette. The colors
follow the spirit of the palette and the hydrogen (green), sulfur
(red) and oxygen (blue) areas can easy be identified.
The Orion Nebula (also
known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated
south of Orion's Belt. It is one of the brightest nebulae, and is
visible to the naked eye. M42 is located at a distance of 1,270±76
light years and is the closest region of massive star formation to
Earth. The M42 nebula is estimated to be 24 light years across.
Source:
Wikipedia
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