Lagoon Nebula – Messier 8

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The Lagoon Nebula, or Messier 8 (M8), is a large interstellar cloud classified as an emission nebula and an H II region. The nebula is located in Sagittarius constellation, within the Milky Way Galaxy. It lies in the direction of the galaxy’s centre. The nebula’s designation in the New General Catalogue is NGC 6523.

The Lagoon Nebula is the brightest, largest nebula in Sagittarius, a constellation that is home to a number of notable nebulous regions. M8 is estimated to lie at a distance between 4,000 and 6,000 light years from Earth. It spans a region 110 by 50 light years in size.

messier 8,m8,ngc 6523

Gas and dust condense, beginning the process of creating new stars in this image of Messier 8, also known as the Lagoon Nebula. Located four to five thousand light-years away, in the constellation of Sagittarius (the Archer), the nebula is a giant interstellar cloud, one hundred light-years across. It boasts many large, hot stars, whose ultraviolet radiation sculpts the gas and dust into unusual shapes. Two of these giant stars illuminate the brightest part of the nebula, known as the Hourglass Nebula, a spiralling, funnel-like shape near its centre. Messier 8 is one of the few star-forming nebulae visible to the unaided eye, and was discovered as long ago as 1747, although the full range of colours wasn’t visible until the advent of more powerful telescopes. The Lagoon Nebula derives its name from the wide lagoon-shaped dark lane located in the middle of the nebula that divides it into two glowing sections.Image: ESO/IDA/Danish 1.5 m/ R. Gendler, U.G. Jørgensen, K. Harpsøe

When observed through a telescope or binoculars, the nebula appears gray, while time-exposure photos reveal a pink colour. The structure of the nebula, resembling that of a tornado or funnel, is a result of ultraviolet light coming from a hot O-type star that heats and ionizes gases on the nebula’s surface.

Messier 8 has an apparent magnitude of 6.0, which makes it barely visibile as a faint patch of light to the naked eye in extremely good conditions. Visually, the object has a diameter about three times that of the full Moon and is the largest and brightest nebula in Sagittarius and the surrounding region.

When observed with binoculars, the Lagoon Nebula has an oblong shape, with the bright central region, known as the Hourglass Nebula, lying on one side, separated by a dark rift from an open cluster of stars that lie on the other side of M8.

The Lagoon Nebula was named for the lagoon-shaped dark lane above the bright Hourglass region. The lane appears to divide the nebula in half.

When seen through a telescope of any size, the cluster is easily resolved and some of the details of the nebula can be seen. Telescopes with a large aperture will also reveal the dark nebula in good viewing conditions. To see the entire Lagoon Nebula, it is best to use low magnification, as it is an exceptionally large object.

The best time of year to observe the Lagoon Nebula is from mid-summer to mid-fall. However, as it is located in the southern sky (-24 degrees declination), it is much easier to observe the nebula from southern latitudes because it appears higher in the sky there. M8 lies to the north of the spout of the Teapot, the asterism Sagittarius is well known for. It is easily seen without binoculars on winter nights in the southern latitudes as it lies in a dark part of the Milky Way.


The Lagoon Nebula was first spotted by the Italian astronomer Giovanni Battista Hodierna in 1654 and then rediscovered by the French astronomer Guillaume Le Gentil in 1747.

The English astronomer John Flamsteed independently observed the object and documented it as a nebula, giving it the designation Number 2446.

In 1746, the Swiss mathematician and astronomer Philippe Loys de Chéseaux was able to resolve some of the stars in the region and classified the object as a star cluster.

When Le Gentil observed the nebula the following year, he noted, “The first [nebula] is between the left heel of Serpentarius and the bow of Sagittarius, to the west of a star cluster which is located in this place in the sky, and which appears the same at eyesight, rather resembling the nebula of Cancer [Messier 44, also known as Praesepe or the Beehive Cluster]: That nebula has exactly the shape of an equilateral triangle, a bit elongated, and the turning point to the south-west. I have observed it with a refractor of 18 to 20 feet [FL], and it always appeared to me nebulous and transparent; it touches with its base a rather beautiful star, seen in the refractor, and which is the brightest of all those which compose the star cluster I have mentioned. The right ascension of this star is for the beginning of 1748, 266d 44′ 22” [17h 46m 57s], its southern declination, 25d 8′ 10”, its [ecliptical] longitude, 26d 45′ 00”, and its southern [ecliptical] latitude 1d 30′ 00”.”

The Lagoon Nebula has a significant number of Bok globules, which are collapsing dark protostellar clouds, consisting of interstellar material, about 10,000 AU (astronomical units) in diameter. The American astronomer E.E. Barnard, who discovered them inside the nebula, documented the three most prominent ones as Barnard 88 (B88), Barnard 89 (B89), and Barnard 296 (B296) in his catalogue of dark nebulae.

messier 8 detail

This close-up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue-white flare at the upper-left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes. Image: ESA, NASA

Charles Messier observed the nebula on May 23 to 24, 1764 and later noted, “I also have determined, in the same night [May 23-24, 1764], the position of a small star cluster which one sees in the form of a nebula, if one views it with an ordinary [non-achromatic] refractor of 3 feet [FL], but when employing a good instrument one notices a large quantity of small stars: near this cluster is a rather brilliant star which is surrounded by a very faint light: this is the ninth star of Sagittarius, of seventh magnitude, according to the catalog of Flamsteed: this cluster appears in an elongated shape which extends from North-East to South-West. I observed its position during its passage of the Meridian, comparing it with the star Delta Sagittarii, and I determined its right ascension as 267d 29′ 30”, and its declination as 24d 21′ 10” south. This star cluster could have an extension, from North-East to South-West, of about 30 minutes of arc.”

The Lagoon Nebula is one of only two star-forming nebulae that can be seen without binoculars from mid-northern latitudes. It is composed mainly of hydrogen, most of it ionized by radiation from the star Herschel 36.

Messier 8 contains the Hourglass Nebula, NGC 6523, and NGC 6530. The Hourglass Nebula, named by John Herschel, who discovered it, lies at the centre of Messier 8. It is not to be confused with the more famous Hourglass Nebula located in the constellation Musca, the Fly. The Hourglass at the core of M8 is the brightest portion of the nebula, and a known star forming region.

lagoon nebula

Messier 8: The Lagoon Nebula. Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.

NGC 6530 is a scattered young open cluster believed to lie just slightly in front of the nebula. The stars in the cluster are less than five million years old, which means that they have been formed only recently by astronomical standards. The cluster itself is classified as of Trumpler type II 2 m n, which means that it is mostly detached, but slightly concentrated towards the centre, moderately rich, with 50 to 100 stars, that the stars scatter in a moderate range of luminosity, and that the cluster is associated with a nebulous region, in this instance the Lagoon Nebula. The brightest star in NGC 6530 is a hot star belonging to the spectral class O5 with an apparent magnitude of 6.9. The star’s estimated age is around two million years.

The Lagoon Nebula contains a region that faintly extends toward the east and has its own IC number, IC 4678.

The two stars emitting strong ultraviolet radiation that is responsible for the nebula’s glow are Herschel 36 and 9 Sagittarii. Herschel 36, a very hot O-type star, is the primary source of the radiation. The star belongs to the spectral class O7 and has an apparent magnitude of 9.5. It illuminates the Hourglass and the neighbouring region. 9 Sagittarii is significantly brighter, with a visual magnitude of 5.97. It belongs to the spectral class O5.

Messier 8 is one of the brightest known regions that are undergoing intense star forming activity, and it has already formed the young star cluster NGC 6530. The nebula will continue forming stars until it runs out of gas, which will take at least hundreds of thousands and maybe even millions of years.

messier 8 location,find lagoon nebula

Lagoon Nebula location, image: Torsten Bronger

The Lagoon Nebula is located a few degrees to the right and slightly above the Teapot asterism. It can be found by following a line from Phi Sagittarii to Lambda Sagittarii and onward. M8 lies about at the same distance down this imaginary line as these two stars are distant from each other.

It can also be located by following the line from Lambda Sagittarii, the Teapot lid star, to Antares, the brightest star in Scorpius constellation and one of the brightest stars in the southern sky. The Lagoon Nebula lies a bit north, about ¼ of the distance between these two stars. It appears as a bright patch resembling a comet about 5 degrees to the west of Lambda Sagittarii.

The neighbouring region is home to other notable deep sky objects, including the Trifid Nebula (Messier 20), which lies about half a degree to the north of Messier 8, and the open cluster Messier 21. Two globular clusters can be seen slightly to the southeast, NGC 6544 and NGC 6553.

Lagoon Nebula – Messier 8 (NGC 6523)
Type: emission nebula
Constellation: Sagittarius
Distance: 5,200 light years
Location: 18h 03m 37s (right ascension), -24°23’12” (declination)
Visual magnitude: 6.0
Size: 110 x 50 light years
Apparent dimensions: 90 x 40 arc minutes
Radius: 55 x 20 light years
Designations: Lagoon Nebula, Messier 8, M8, Sharpless 25, RCW 146, Gum 72, NGC 6523


lagoon nebula,messier 8

An amazing vista of the Lagoon Nebula taken with the 67-million-pixel Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. The image covers more than one and a half square degree— an area eight times larger than that of the Full Moon — with a total of about 370 million pixels. It is based on images acquired using three different broadband filters (B, V, R) and one narrow-band filter (H-alpha). Image: ESO/S. Guisard

messier 8 central region

Central region of the Lagoon Nebula (also known as M8 and NGC 6523) – an H II region in the Sagittarius constellation. The photo was taken by the Southern African Large Telescope (SALT).

messier 8 infrared,m8 infrared

This new infrared view of the star formation region Messier 8, often called the Lagoon Nebula, was captured by the VISTA telescope at ESO’s Paranal Observatory in Chile. This colour picture was created from images taken through J, H and Ks near-infrared filters, and which were acquired as part of a huge survey of the central parts of the Milky Way. The field of view is about 34 by 15 arcminutes. Image: ESO/VVV

messier 8,sagittarius nebula

The VLT Survey Telescope (VST) at ESO’s Paranal Observatory in Chile has captured this richly detailed new image of the Lagoon Nebula. This giant cloud of gas and dust is creating intensely bright young stars, and is home to young stellar clusters. This image is a tiny part of just one of eleven public surveys of the sky now in progress using ESO telescopes. Together these are providing a vast legacy of publicly available data for the global astronomical community. Image: ESO/VPHAS+ team

messier 8 hubble image

This NASA Hubble Space Telescope (HST) image reveals a pair of one-half light-year long interstellar “twisters,” eerie funnels and twisted-rope structures in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 light-years away in the direction of the constellation Sagittarius. The central hot star, O Herschel 36 (lower right), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds, combined with the pressure of starlight, may produce strong horizontal shear to twist the clouds into their tornado-like appearance. Though the spiral shapes suggest the clouds are “twisting,” future observations will be needed, perhaps with Hubble’s next generation instruments, with the spectroscopic capabilities of the Space Telescope Imaging Spectrograph (STIS) or the Near Infrared Camera and Multi-Object Spectrometer (NICMOS), to actually measure velocities. These color-coded images are the combination of individual exposures taken in July and September, 1995 with Hubble’s Wide Field and Planetary Camera 2 (WFPC2) through three narrow-band filters (red light ionized sulphur atoms, blue light, double ionized oxygen atoms, green light, ionized hydrogen). Image: NASA, A.Caulet St-ECF, ESA