Celestial hemisphere:  Southern  ·  Constellation: Sagittarius (Sgr)  ·  Contains:  Checkmark Nebula  ·  HD167281  ·  HD167283  ·  HD167313  ·  HD167332  ·  HD167333  ·  HD167334  ·  HD167335  ·  HD167396  ·  HD167431  ·  HD167452  ·  HD167474  ·  HD167499  ·  HD167545  ·  HD167546  ·  HD167567  ·  HD167593  ·  HD167608  ·  HD167632  ·  HD167633  ·  HD167655  ·  HD167656  ·  HD167657  ·  HD167697  ·  HD167743  ·  HD167744  ·  HD167745  ·  HD167769  ·  HD167791  ·  HD167792  ·  And 64 more.
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The Omega Nebula (M17) in SHO with surrounding nebula, Cfosterstars
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The Omega Nebula (M17) in SHO with surrounding nebula

Getting plate-solving status, please wait...
The Omega Nebula (M17) in SHO with surrounding nebula, Cfosterstars
Powered byPixInsight

The Omega Nebula (M17) in SHO with surrounding nebula

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I have image M17 previously with my older camera and as the season was running short, I decided to go for M17 even though I might now finish this year. I got 15 hours and since its a bright target, I felt that its enough. This is a wider FOV than I have previously taken so I got some of the surrounding nebulosity. Please comment and let me know what you thing.

The Omega Nebula, also known as the Swan NebulaCheckmark NebulaLobster Nebula, and the Horseshoe Nebula[ (catalogued as Messier 17 or M17 or NGC 6618) is an H II region in the constellationSagittarius. It was discovered by Philippe Loys de Chéseaux in 1745. Charles Messier catalogued it in 1764. It is by some of the richest starfields of the Milky Way, figuring in the northern two-thirds of Sagittarius.

The Omega Nebula is between 5,000 and 6,000 light-years from Earth and it spans some 15 light-years in diameter. The cloud of interstellar matter of which this nebula is a part is roughly 40 light-years in diameter and has a mass of 30,000 solar masses. The total mass of the Omega Nebula is an estimated 800 solar masses. t is considered one of the brightest and most massive star-forming regions of our galaxy. Its local geometry is similar to the Orion Nebula except that it is viewed edge-on rather than face-on.

The open cluster NGC 6618 lies embedded in the nebulosity and causes the gases of the nebula to shine due to radiation from these hot, young stars; however, the actual number of stars in the nebula is much higher – up to 800, 100 of spectral type earlier than B9, and 9 of spectral type O, ]citation needed ] plus over a thousand stars in formation on its outer regions. It is also one of the youngest clusters known, with an age of just 1 million years.  The luminous blue variableHD 168607, in the south-east part of the nebula, is generally assumed to be associated with it; its close neighbor, the blue hypergiantHD 168625, may be too.  The Swan portion of M17, the Omega Nebula in the Sagittariusnebulosity is said to resemble a barber's pole.

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The Omega Nebula (M17) in SHO with surrounding nebula, Cfosterstars