The Great Nebula in Orion - M42

Orion RRGB

M42 - The Great Nebula in Orion
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From SEDS.ORG:

The Orion Nebula M42 is the brightest diffuse nebula in the sky, and one of the brightest deepsky objects of all. It is visible to the naked eye under moderately good conditions, and rewarding in telescopes of every size, from the smallest glasses to the greatest Earth-bound observatories as well as outer-space observatories like the Hubble Space Telescope. It is also a big object in the sky, extending to over 1 degree in diameter, thus covering more than four times the area of the Full Moon.

As it is so well visible to the naked eye, one may wonder that its nebulous nature was apparently not documented before the invention of the telescope. However, the brightest stars within the nebula were noted early and cataloged as one bright star of about fifth magnitude: In about 130 AD, Ptolemy included it in his catalog, as did Tycho Brahe in the late 16th century, and Johann Bayer in 1603 - the latter cataloging it as Theta Orion in his Uranometria. In 1610, Galileo detected a number of faint stars when first looking at this region with his telescope, but didn't note the nebula. Some years later, on February 4, 1617, Galileo took a closer look at the main star, Theta1, and found it to be triple, at his magnification of 27 or 28x, again not perceiving the nebula.

See the rest of the massive write-up on this object here: http://www.seds.org/messier/m/m042.html
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ST-10XME and CFW8a with Astrodon RGB
Takahashi FSQ self-guided on AP900GTO
12 x 2 min Red and 4 x 2 min Green and Blue
Image acquisition, darks and flats done with CCDSoft5
All images debloomed, aligned and combined in Maxim using Russ Croman's sigma reject plug-in for the combines
Colour assembly, Levels, Curves and selective sharpening using Layer Masking in PS CS2
I took extra red data and used a sharpened version of the red chanel layered in at 50% as luminance layer for the RGB.

Click on the image above to see a larger version of the image.

Flesherton, Ontario
Nov 25th 2006

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