AAO image reference AAT 18a. « Previous || Next »
Top left is NE. Image width is about 47.5 arc min
Image and text © 2000-2002, Anglo-Australian Observatory, photograph by David Malin.
Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo-ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 6000 light years distant.
Entry from NGC 2000.0 (R.W. Sinnott, Ed.) © Sky Publishing Corporation, 1988:
NGC 6611 C+N 18 18.8 -13 47 s Ser 35. 6.0 Cl, at least 100 st L & S; = M16 IC 4703 OC 18 18.9 -13 47 x Ser B, eL, Cl M16 invRelated Images
AAT 18. The dust lanes in Messier 16
AAT 47. The dust lanes in Messier 16
For details of photographic exposure, search technical table by AAT reference number.
Image availability: Photo Print