The Great Nebula in Orion (Messier 42 . NGC 1976 . Sharpless 2-281)

Perhaps the most well known celestial object in the night sky is The Great Nebula in the belt of the constellation Orion, the Hunter. Visible to the naked eye, this massive nebula is a relatively close 1500 light-years distance, and busily in the process of forming new stars. The Great Nebula is in-fact the brightest part of a far larger and much fainter nebula that covers more than 10 degrees of our night sky.

The Great Nebula is mostly illuminated from star light produced by the four young stars at the crux of the nebula just above centre image. These four stars, collectively known as the Trapezium, appear to the naked-eye as a single star named Theta-1 Orionis. The Trapezium stars are young stars which have formed from the nebula. Since birth their stellar winds have blown the nebula into the partial bubble shape we see today. The Great Nebula was first discovered by Peiresc, 159 years before it become the 42nd object (M42) in the famous Messier list.

Paul Mayo

Image Details Messier 42 - 20060319
Image Field of View approx. 48 arc-minutes wide.
Telescope 12-inch f/5 newtonian telescope.
Guiding hand guided with 4.5-inch guide-scope.
Camera

Canon EOS 300D Digital - Hα enabled.

Exposures Main Image;
6 x 180 second exposures @ ISO200 with
dark frame subtraction, bias and flat-fielded.
Image used to mask core;
3 x 15 second exposures @ ISO200
Total Exposure time 18-minutes.
Filter/equipment Used Baader Multi-purpose Coma Corrector.
Sky Conditions Seeing: 7.5/10. Wind: 3/10. Moisture: 3/10
Ambient Temperature 23°C
Notes Moon Rising ends imaging session.
Processing Iris, Photoshop, Noiseware CE.

(C) Copyright 2006 Paul Mayo.
paulm@skylab.com.au

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