The Omega Nebula, M17

[Omega] The Omega Nebula, Messier object 17 (M17), NGC6618, in the constellation Sagittarius, as seen by the Kitt Peak 4-meter Mayall telescope in 1973. North is at the top.

Downloadable versions (see NOAO Conditions of Use):
250 x 200 11 kb B&W JPEG(on this page)
500 x 400 41 kb B&W JPEG
2500 x 2000 680 kb B&W JPEG
2500 x 2000 4.8 Mb B&W TIFF

The Omega Nebula, Messier object 17 (M17), NGC 6618, in the constellation Sagittarius, as seen by the Kitt Peak 4-meter Mayall telescope in 1973. This bright nebula, criss-crossed by clouds and lanes of opaque dust and gas, is also known as the Swan Nebula and the Horseshoe Nebula. M17 is estimated to contain over 800 times as much material as the Sun within its 17 light-year diameter. At a distance of 5700 light-years, M17 is also a source of radio noise. North is at the top. We also have an interesting infrared image, a newer 0.9-meter optical image, and a deeper Schmidt image.

Minimum credit line: NOAO/AURA/NSF (for details see Conditions of Use)

Return to: nebulae page, emission nebulae page.
NOAO is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under cooperative agreement with the National Science Foundation

Comments by e-mail to images@noao.edu