M8, also known as the Lagoon Nebula or NGC 6523, Sharpless 25, RCW 146, Gum 72, is a large, bright emission nebula located in the constellation Sagittarius. Classified as an H II region, the star-forming nebula has an apparent magnitude of 6.0 and lies at a distance of 4,100 light-years from Earth; right ascension 18h 03m 37s and declination -24°23’12”, with a radius of 110 x 50 light-years. The cluster is only about 2 million years old. The hot young stars in it are responsible for the nebula’s glow. The brightest star in the cluster belongs to the spectral class O5 and has an apparent magnitude of 6.9. Messier 8 never rises very high above the horizon for observers north of the equator, but can be seen in the summer months, when Sagittarius is prominent on the southern horizon when observed from northern latitudes. M8 is located just above and to the right of the Teapot asterism in Sagittarius. It can be found about 5 degrees west of Lambda Sagittarii, the star that marks the top of the Teapot. It is currently undergoing a period of active star formation and has already formed a sizable cluster of stars. The large, lagoon-shaped band of dust seen to the left of the cluster’s centre is what earned the Lagoon Nebula its name. The faint extension of the nebula to the east, spanning about 25 light-years, has its own designation in the Index Catalogue of Nebulae and Clusters of Stars: IC 4678. The nebula’s apparent size is about three times the size of the full Moon. The surrounding region contains a number of notable deep-sky objects, starting with the Trifid Nebula (Messier 20), which lies only half a degree north of the Lagoon. The open cluster Messier 21 and the globular cluster Messier 28 also lie in the vicinity. The globular cluster NGC 6544 is located a degree to the southeast of M8, and NGC 6553, yet another globular, lies another degree to the southeast.
M8 was discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. Hodierna listed the nebula as No. II.6 in his catalogue. English astronomer John Flamsteed discovered the object independently around 1680 and added it as No. 2446 to his catalogue. In 1746, Swiss astronomer Jean-Philippe Loys de Chéseaux resolved some of the stars in M8 and classified it as a cluster. The following year, French astronomer Guillaume Le Gentil observed both the Lagoon Nebula and the associated cluster. Nicolas Louis de Lacaille listed the nebula in his 1751-52 catalogue as Lacaille III.13 and described it as “three stars enclosed in a drag of a nebula parallel to the Equator.” The category III in Lacaille’s catalogue was reserved for “nebulous stars.” Charles Messier added the object to his catalogue as Messier 8 on May 23, 1764. The German-British astronomer William Herschel catalogued two objects within M8 separately: H V.9 (GC 4363, NGC 6526) and H V.13 (GC 4368, NGC 6533). His son John Herschel listed the cluster NGC 6530 separately as h 3725 (GC 4366) and catalogued the Lagoon Nebula as h 3723 (NGC 6523, GC 4361).
Messier 8 is one of two star-forming nebulae that can be seen without binoculars from mid-northern latitudes. The other one is the Orion Nebula, or Messier 42 (NGC 1976), the famous diffuse nebula located in Orion constellation. The Nebula contains many Bok globules, or dark clouds of dense dust, in which new stars are being formed. These dark nebulae are collapsing proto-stellar clouds of material about 10,000 astronomical units in diameter. The most prominent Bok globules in the Lagoon Nebula were catalogued by the American astronomer Edward Emerson Barnard as Barnard 88 (B88), Barnard 89 (B89) and Barnard 296 (B296). B88 is comet-shaped and 0.5′ wide, and it extends from north to south for 2.7′ just above the star 9 Sagittarii. B296 is long and narrow and can be seen at the nebula’s south edge, while B89 is found in the region of the open cluster.
Messier 8 also contains a region known as the Hourglass Nebula, a bright knot of dust and gas, located in the nebula’s bright central region. The Hourglass Nebula was named by the English astronomer John Herschel, who discovered it. It should not be confused with the more famous Engraved Hourglass Nebula (MyCn 18), which lies in the constellation Musca, the Fly. The brightest region of M8 is a site of ongoing star formation. The Hourglass is illuminated by the extremely hot, young stars. It lies near 9 Sagittarii, one of the brightest stars associated with Messier 8. 9 Sagittariii belongs to the spectral class O5 and has an apparent magnitude of 5.97. The Lagoon Nebula also contains funnel-like structures, created by an O-type star emitting ultraviolet light that heats up and ionizes the gases on the surface of M8. There are at least two such structures in the nebula’s central region, each spanning about half a light-year. The area is illuminated by Herschel 36, an extremely bright star with the stellar classification of O7 V and a visual magnitude of 9.5. The first direct proof of star-forming activity by accretion within M8 was discovered in 2006 when scientists found the first four Herbig-Haro objects within the Hourglass structure. Herbig-Haro objects are small patches of nebulosity that are formed when jets of gas ejected by newly formed stars from their poles collide with nearby dust and gas at high speeds. They are frequently found near very young stars. Credits: Messier Objects, Wikipedia.