m17, the Omega Nebula, (horseshoe)

Horseshoe Nebula, M17. In the depths of the dark clouds of dust and molecular gas known as M17, stars continue to form. The nebula is also known as the Omega Nebula, the Swan Nebula, and M17.

The darkness of these molecular clouds results from background starlight being absorbed by thick carbon-based smoke-sized dust. As bright massive stars form, they produce intense and energetic light that slowly boils away the dark shroud. M17, pictured above, is visible with binoculars towards the constellation of Sagittarius, lies 5000 light-years away, and spans 20 light-years across.

(notes from S.A.C. member) - the Horseshoe (omega) nebula, i first really observed in my 13.1" dobsonian mounted newtonian reflector, back in 2007, the spring i believe. I've seen it before, but through a 13 inch telescope.. it is really defined. looks more like a sickle through my telescope. I enjoyed this as much as the lagoon or trifid because of it's unique shape.

Messier Object 7

Messier 7 (M7, NGC 6475) is a large and brilliant group, easily detected with the naked eye. As Burnham describes it, "the cluster is seen projected on a background of numerous faint and distant Milky Way stars."

This splendid cluster was known to Ptolemy, who mentioned it about 130 AD and described it as the "nebula following the sting of Scorpius." The description may also include M6, but this is uncertain. Because of this presumable discovery, the present author [hf] has proposed the name "Ptolemy's Cluster" for M7 some years ago, a proposition which has found some acceptance meanwhile.

M7 was observed by Hodierna before 1654, who counted 30 stars. Edmond Halley listed it as No. 29 in his catalog of southern stars of 1678, and Abbe Lacaille added it to his catalog of southern objects as Lac II.14. Charles Messier included it as No. 7 in his catalog on May 23, 1764.

M7 consists of about 80 stars brighter mag 10 in a field of about 1.3 degrees apparent diameter which at its distance of perhaps 800 light years corresponds to a linear extension of 18 or 20 light years. It was classified as of Trumpler type I,3,m or I,3,r. This group is approaching us at 14 km/sec. The brightest star is a yellow giant (spectral type gG8, mag 5.6), the hottest main sequence star is of spectral type B6 (mag 5.89). M7's age was estimated at 220 million years, both according to the Sky Catalog 2000 and the new calculation of the Geneva Group of G. Meynet. Recent work suggests a slightly larger distance of 1000 light-years, which would increase the size to 25 light-years but would not affect the age.

Ake Wallenquist found that this is one of the clusters with the highest degree of concentration toward the center. Modern sources agree on M7's integrated apparent visual brightness at magnitude 3.3, while older estimates, mostly from northern observers, had this southern cluster significantly underestimated at mag 4.1 to 5.0.

(notes: S.A.C. member - M7 is an awesome object, just one of the many objects you'll find near Scorpius and Sagittarius - it's not the most profound, but one definitely to observe - check out all the M objects in this region... the heart of the milky way is near!!!)