The Orion Nebula, M42 and M43
AAO image reference AAT 19a.     « Previous || Next »

The Great Orion Nebula, M42 and M43, NGC 1976 m42.jpg, orion_nebula.jpg, ncg1976.jpg)
Top left is NE. Image width is about 46 arc min
Image and text © 2000-2002, Anglo-Australian Observatory, photograph by David Malin.

This image is a slightly wider view than AAT 19. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1350 light years) means that we know more about it than any other star-forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars.

The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five-minute exposures were used to make this picture, which covers a slightly wider field than AAT 19.

Entry from NGC 2000.0 (R.W. Sinnott, Ed.) © Sky Publishing Corporation, 1988:

NGC 1976  Nb 05 35.4  -05 27 s  Ori  66.    4.   !!! theta1 Ori and the great neb; = M42
NGC 1982  Nb 05 35.6  -05 16 s  Ori  20.    9.   ! vB, vL, R with tail, mbM *8-9;  = M43
Related Images
AAT 19.   The Orion nebula
AAT 19b. The Orion nebula (no unsharp mask)
AAT 29.   The Trapezium stars in Orion
UKS 8.    The Great Nebula in Orion
UKS 23.   Faint nebulosity near Orion and Horsehead Nebulae

For details of photographic exposure, search technical table by AAT reference number.

Image availability: Photo Print

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