M42 & M43 - the Orion Nebula

Description: M42, better known as the Orion Nebula, is a star-forming region located in Orion's 'sword'. Here we can see the central region of the nebula. The 'blob' of stars near the centre of the image is the Trapezium, over-exposed to bring out the surrounding nebula. To the left of them, a dust lane can be seen obscuring the nebula. The protruberance coming out of the star on the bottom-left of the image is a result of the CCD being overexposed.

Image information: RVB combination of stacked, dark-subtracted, registered images. Image comprises of 20 x 4s R-band images, 24 x 3s V-band images, 16 x 6s B-band images. The image has undergone contrast stretching and a deconvolution filter to enhance clarity, and approximate response weightings to try to match colours with reality. Image taken 14/01/2006 20:00-21:00.

Physical information: Magnitude: 4.0, size: 90'x60', aka Orion Nebula.

Description: Here we see the nebula also in the infra-red. Here the 'red' stars have become much more visible through the dusty nebula. Many of these red objects are very young stars that are still in the process of collapsing from the dust cloud.

Image information: IRV combination of stacked, dark-subtracted, registered images. Image comprises of 50 x 1s I-band images, 20 x 4s R-band images, 24 x 3s V-band images. The image has undergone contrast stretching and a deconvolution filter to enhance clarity, and approximate response weightings to try to match colours with reality. Image taken 14/01/2006 20:00-21:00.


Description: Here are two different views of M42's neighbouring nebula, M43, which also forms part of the Orion Nebula complex.

The first image is true colour, which shows the bright star which ionises the nebula, stripping the electrons from the hydrogen atoms. When the electrons recombine, they emit a reddish glow. A dark dust lane runs down the middle of the image - this is interstellar dust, which is roughly similar to coal dust, and forms a barrier through which light doesn't very easily penetrate.

If we look in the second image, we are looking in infrared, which allows us to more readily see through the dust to the stars behind the nebula. Note the bright, red star in the top-right.

Image information: Images are RVB- and IRV-band combinations of 16 x 10s images in each band, plus 56 x 10s images in unfiltered light as a luminosity channel. Images have been stacked, calibrated and registered in AIP4Win, and cropped and compressed in Paint Shop Pro. Images taken 01/11/2006 00:00.

Description: This image shows the whole M42/M43 complex (at centre) along with the rest of Orion's "sword", which includes the open clusters NGC 1977 and 1981 (top), and the iota Orionis group (bottom).

Image information: Sony DSC-H1, piggy-backed onto the back of the Keele 12-inch refractor. Images taken 11/11/2007 22:42.

Physical information:
M42: Magnitude: 4.0, size: 90'x60', aka Orion Nebula.
M43: Magnitude: 9.0, size: 20', part of Orion Nebula.

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