The Eagle Nebula, also known as the Star Queen Nebula, Messier 16 (M16), IC 4703, and NGC 6611, is an emission nebula surrounding a young open star cluster located in Serpens constellation. The nebula is a well-known star forming region. The cluster with which it is associated consists of a number of young stars belonging to the spectral classes O and B.
Messier 16 is best known for the famous Pillars of Creation, a region where intense star forming activity is taking place. The region was imaged by the Hubble Space Telescope in the 1990s. The Eagle Nebula in fact contains several active starburst regions.
The Eagle Nebula was named for its shape, which resembles that of an eagle. It is part of a larger H II region designated as IC 4703, which is a diffuse emission nebula approximately 7,000 light years from Earth.
Messier 16 can be seen in binoculars and amateur telescopes, which reveal about 20 stars and some of the surrounding nebulosity. The three pillars require extremely good observing conditions.
The Eagle Nebula and the open cluster are best observed with low-powered telescopes.
Three-colour composite mosaic image of the Eagle Nebula (Messier 16, or NGC 6611), based on images obtained with the Wide-Field Imager camera on the MPG/ESO 2.2-metre telescope at the La Silla Observatory. At the centre, the so-called “Pillars of Creation” can be seen. This wide-field image shows not only the central pillars, but also several others in the same star-forming region, as well as a huge number of stars in front of, in, or behind the Eagle Nebula. The cluster of bright stars to the upper right is NGC 6611, home to the massive and hot stars that illuminate the pillars. The “Spire” — another large pillar — is in the middle left of the image. This image is a composite of 3 filters in the visible range: B (blue), V (green) and R (red).Image: ESO
The star cluster associated with the Eagle Nebula was originally discovered by the Swiss astronomer Philippe Loys de Chéseaux in 1745-46. He observed the cluster, but did not see the surrounding nebula.
Charles Messier was the first to discover the nebulosity associated with the open cluster in June 1764.
He noted, “In the same night of June 3 to 4, 1764, I have discovered a cluster of small stars, mixed with a faint light, near the tail of Serpens, at little distance from the parallel of the star Zeta of that constellation: this cluster may have 8 minutes of arc in extension: with a weak refractor, these stars appear in the form of a nebula; but when employing a good instrument one distinguishes these stars, and one remarks in addition a nebulosity which contains three of these stars. I have determined the position of the middle of this cluster; its right ascension was 271d 15′ 3″, and its declination 13d 51′ 44″ south.”
Messier included the nebula in his catalogue as the 16th object on the list, and it remains known as Messier 16.
The nebula was added to the IC II of 1908 as IC 4703, and is often referred to by that designation, while the open cluster is referred to as NGC 6611.
The Eagle Nebula is illuminated by the ultraviolet light of the young stars newly formed in one of the nebula’s star forming regions.
The hot, young stars within the nebula also emit strong X-ray radiation.
The nebula has an estimated mass of more than 12,000 solar masses.
HD 168076, the brightest star in the Eagle Nebula, is a binary system consisting of an O3.5V star and an O7.5V companion. The star system has a visual magnitude of 8.24 and can be seen in good binoculars.
Stellar Spire in the Eagle Nebula. Image: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
The young open cluster associated with Messier 16 consists of about 460 stars.
The brightest members of the cluster belong to the spectral class O. They are extremely massive, luminous stars, and can be up to a million times brighter than the Sun.
The age of the cluster is believed to be 1-2 million years.
The other name for M16, the Star Queen Nebula, was introduced by the American astronomer Robert Burnham, Jr.
Burnham gave it this name because he thought the central pillar in the nebula looked like the Star Queen shown in silhouette.
The Eagle Nebula was first imaged way back in 1895 by the American astronomer Edward Barnard.
Isaac Roberts photographed it in 1897, after which the object was added to the IC catalogue.
LOCATION AND SIZE
The Eagle Nebula stretches across an area about 70 by 55 light years in size. It lies at a distance of 7,000 light years from Earth. The nebula lies in the Sagittarius-Carina Arm, the inner spiral arm of our galaxy, the Milky Way, next to our own arm.
M16 can be found by first locating the Teapot asterism in Sagittarius constellation, and then by following the line from the star Kaus Australis (Epsilon Sagittarii), the brightest star in Sagittarius, to just east of Kaus Media (Delta Sagittarii). Another way to find the nebula is by extending a line from Lambda Scuti in Scutum constellation to Alpha Scuti, and then to the south to Gamma Scuti.
When observed through binoculars, the Eagle Nebula can be seen in the same field as the Omega Nebula (Messier 17) in Sagittarius. This region of the sky contains several other notable deep sky objects, including Messier 22 (Sagittarius Cluster), Messier 28, Messier 8 (Lagoon Nebula), Messier 20 (Trifid Nebula), Messier 21, Messier 23, Messier 25, and Messier 18.
In good viewing conditions, the open cluster in M16 is easy to find, but to see the surrounding nebulosity well, one needs a large aperture telescope.
The best time to observe the Eagle Nebula from the northern hemisphere is summer and early autumn, when the nebula can be found in the southern sky in the evening.
Eagle Nebula – Messier 16 (NGC 6611)
Constellation: Serpens Cauda
Coordinates: 18h18m48s (right ascension), -13°49′ (declination)
Distance: 7,000 light years
Visual magnitude: +6.0
Absolute magnitude: -8.21
Apparent dimensions: 7.0 arc minutes
Radius: 70×55 light years
Estimated age: 5.5 million years
Designations: Eagle Nebula, Star Queen Nebula, Messier 16 (M16), NGC 6611, IC 4703, Gum 83, Sharpless 49, RCW 165
PILLARS OF CREATION
Star forming pillars in the Eagle Nebula, as seen by the Hubble Space Telescope’s WFPC2. The picture is composed of 32 different images from four separate cameras in this instrument. The photograph was made with light emitted by different elements in the cloud and appears as a different colour in the composite image: green for hydrogen, red for singly-ionized sulphur and blue for double-ionized oxygen atoms. Image: NASA, Jeff Hester, and Paul Scowen (Arizona State University)
The region known as the Pillars of Creation became famous in 1995, when it was imaged by Jeff Hester and Paul Scowen using the Hubble Space Telescope. It is one of the star forming regions within the Eagle Nebula. The pillars stretch across an area of approximately four light years and are illuminated by the light of newly formed stars.
The pillars region is similar to the larger Soul Nebula, located in Cassiopeia constellation, which was nicknamed the Pillars of Star Formation.
The region consists of columns of interstellar dust and hydrogen gas within which new stars are formed. The dense pockets of gas seen at the top of the pillars are called EGGs, or evaporating gaseous globules, and last for about 10,000-20,000 years. Those that contain enough gas will eventually collapse to form new stars.
Images obtained from the Spitzer Space Telescope in 2007 indicate that the pillars may have been destroyed as a result of a supernova explosion in the vicinity, but the light showing the result of the supernova will not reach us for another 1,000 years.
The supernova event is believed to have occurred about 8,000 to 9,000 years ago. The shock wave from the explosion would have taken a few millennia to move through the region, and the nebula is 7,000 light years distant from Earth, which means that we are seeing it as it appeared 7,000 years ago. The area where the supernova exploded is full of young, very massive stars that are also ready to explode.
Four Hubble Space Telescope’s images of the Eagle Nebula (Messier 16). Image: NASA, STScI, WikiSky
This set of images from NASA’s Spitzer Space Telescope shows the Eagle nebula in different hues of infrared light. Each view tells a different tale. The left picture shows lots of stars and dusty structures with clarity. Dusty molecules found on Earth called polycyclic aromatic hydrocarbons produce most of the red; gas is green and stars are blue.
The middle view is packed with drama, because it tells astronomers that a star in this region violently erupted, or went supernova, heating surrounding dust (orange). This view also reveals that the hot dust is shell shaped, another indication that a star exploded.
The final picture highlights the contrast between the hot, supernova-heated dust (green) and the cooler dust making up the region’s dusty star-forming clouds and towers (red, blue and purple).
The left image is a composite of infrared light with the following wavelengths: 3.6 microns (blue); 4.5 microns (green); 5.8 microns (orange); and 8 microns (red). The right image includes longer infrared wavelengths, and is a composite of light of 4.5 to 8.0 microns (blue); 24 microns (green); and 70 microns (red). The middle image is made up solely of 24-micron light. Image: NASA/JPL-Caltech/N. Flagey (IAS/SSC) & A. Noriega-Crespo (SSC/Caltech)
North-East part of en:Eagle Nebula by en:Hubble Space Telescope; 3.24′ view. Image: NASA, STScI, WikiSky
The NASA/ESA Hubble Space Telescope has once more turned its attention towards the magnificent Eagle Nebula (Messier 16). This picture shows the northwestern part of the region, well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow.
The star cluster is very bright and was discovered in the mid-eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed “The Pillars of Creation” ever since the Hubble Space Telescope captured an iconic image of dramatic pillars of star-forming gas and dust.
The cluster and nebula are fascinating targets for small and medium-sized telescopes, particularly from a dark site free from light pollution. Messier 16 can be found within the constellation of Serpens Cauda (the Tail of the Serpent), which is sandwiched between Aquila, Sagittarius, and Ophiuchus in the heart of one of the brightest parts of the Milky Way. Small telescopes with low power are useful for observing large, but faint, swathes of the nebula, whereas 30 cm telescopes and larger may reveal the dark pillars under good conditions. But a space telescope in orbit around the Earth, like Hubble — which boasts a 2.4-metre diameter mirror and state-of-the-art instruments — is required for an image as spectacular as this one.
This picture was created from images taken with the Wide Field Channel of Hubble’s Advanced Camera for Surveys. Images through a near-infrared filter (F775W) are coloured red and images through a blue filter (F475W) are blue. The exposures times were one hour and 54 minutes respectively and the field of view is about 3.3 arcminutes across. Image: ESA, Hubble and NASA
This majestic view taken by NASA’s Spitzer Space Telescope tells an untold story of life and death in the Eagle nebula, an industrious star-making factory located 7,000 light-years away in the Serpens constellation. The image shows the region’s entire network of turbulent clouds and newborn stars in infrared light.
The color green denotes cooler towers and fields of dust, including the three famous space pillars, dubbed the “Pillars of Creation,” which were photographed by NASA’s Hubble Space Telescope in 1995.
But it is the color red that speaks of the drama taking place in this region. Red represents hotter dust thought to have been warmed by the explosion of a massive star about 8,000 to 9,000 years ago. Since light from the Eagle nebula takes 7,000 years to reach us, this “supernova” explosion would have appeared as an oddly bright star in our skies about 1,000 to 2,000 years ago.
According to astronomers’ estimations, the explosion’s blast wave would have spread outward and toppled the three pillars about 6,000 years ago (which means we wouldn’t witness the destruction for another 1,000 years or so). The blast wave would have crumbled the mighty towers, exposing newborn stars that were buried inside, and triggering the birth of new ones.
The pillars of the Eagle nebula were originally sculpted by radiation and wind from about 20 or so massive stars hidden from view in the upper left portion of the image. The radiation and wind blew dust away, carving out a hollow cavity (center) and leaving only the densest nuggets of dust and gas (tops of pillars) flanked by columns of lighter dust that lie in shadow (base of pillars). This sculpting process led to the creation of a second generation of stars inside the pillars.
If a star did blow up in this region, it is probably located among the other massive stars in the upper left portion of the image. Its blast wave might have already caused a third generation of stars to spring from the wreckage of the busted pillars.
This image is a composite of infrared light detected by Spitzer’s infrared array camera and multiband imaging photometer. Blue is 4.5-micron light; green is 8-micron light; and red is 24-micron light. Image: NASA/JPL-Caltech/N. Flagey (IAS/SSC & A. Noriega-Crespo (SSC/Caltech)
This infrared picture highlights the contrast between the hot, supernova-heated dust (green) and the cooler dust making up the Eagle Nebula’s dusty star-forming clouds and towers (red, blue and purple).The image includes longer infrared wavelengths, and is a composite of light of 4.5 to 8.0 microns (blue); 24 microns (green); and 70 microns (red). Image: NASA/JPL-Caltech/N. Flagey (IAS/SSC) & A. Noriega-Crespo (SSC/Caltech)
This majestic false-color image from NASA’s Spitzer Space Telescope shows the “mountains” where stars are born. Dubbed “Mountains of Creation” by Spitzer scientists, these towering pillars of cool gas and dust are illuminated at their tips with light from warm, embryonic stars.
The new infrared picture is reminiscent of Hubble’s iconic visible-light image of the Eagle Nebula (inset), which also features a star-forming region, or nebula, that is being sculpted into pillars by radiation and winds from hot, massive stars. The pillars in the Spitzer image are part of a region called W5, in the Cassiopeia constellation 7,000 light-years away and 50 light-years across. They are more than 10 times in the size of those in the Eagle Nebula (shown to scale here).
The Spitzer’s view differs from Hubble’s because infrared light penetrates dust, whereas visible light is blocked by it. In the Spitzer image, hundreds of forming stars (white/yellow) can seen for the first time inside the central pillar, and dozens inside the tall pillar to the left. Scientists believe these star clusters were triggered into existence by radiation and winds from an “initiator” star more than 10 times the mass of our Sun. This star is not pictured, but the finger-like pillars “point” toward its location above the image frame.
The Spitzer picture also reveals stars (blue) a bit older than the ones in the pillar tips in the evacuated areas between the clouds. Scientists believe these stars were born around the same time as the massive initiator star not pictured. A third group of young stars occupies the bright area below the central pillar. It is not known whether these stars formed in a related or separate event. Some of the blue dots are foreground stars that are not members of this nebula.
The red color in the Spitzer image represents organic molecules known as polycyclic aromatic hydrocarbons. These building blocks of life are often found in star-forming clouds of gas and dust. Like small dust grains, they are heated by the light from the young stars, then emit energy in infrared wavelengths.
This image was taken by the Infrared Array Camera (IRAC) on Spitzer. It is a 4-color composite of infrared light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange), and 8.0 microns (red). Image: NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
An infrared view of M16 and its famous ‘Pillars of Creation’. The pillars or columns are numbered 1 to 3 from left to right (east to west). The pillars themselves are less prominent than on the Hubble visible-light image of this region – this because near-infrared light penetrates the thinner parts of the gas and dust clouds and only the heads remain opaque. A number of red objects can be seen associated with the pillars: some of these are just background sources seen through the dust, but some are probably real young stars embedded in the pillars. The purple arc near the bottom of the picture is Herbig-Haro object 216, a fast-moving clump of heated gas emanating from a young star. Image: ESO
Messier 16 (M16), also known as the Eagle Nebula, is located in the southern constellation of Serpens.
Using the infrared multi-mode ISAAC instrument on the 8.2-m VLT ANTU telescope, European astronomers were able to image the Eagle Nebula at near-infrared wavelength. The ISAAC near-infrared images cover a 9 x 9 arcmin region, in three broad-band colours and with sufficient sensitivity to detect young stars of all masses and – most importantly – with an image sharpness as good as 0.35 arcsec.
The wide-field view of M16 shows that there is much happening in the region. The first impression one gets is of an enormous number of stars. Those which are blue in the infrared image are either members of the young NGC 6611 cluster – whose massive stars are concentrated in the upper right (north west) part of the field – or foreground stars which happen to lie along the line of sight towards M16.
Most of the stars are fainter and more yellow. They are ordinary stars behind M16, along the line of sight through the galactic bulge, and are seen through the molecular clouds out of which NGC 6611 formed. Some very red stars are also seen: these are either very young and embedded in gas and dust clouds, or just brighter stars in the background shining through them.
This photo is the result of a three-colour composite mosaic image of the Eagle Nebula (Messier 16), based on 144 individual images obtained with the infrared multi-mode instrument ISAAC on the ESO Very Large Telescope (VLT) at the Paranal Observatory. At the centre, the so-called “Pillars of Creation” can be seen. This wide-field infrared image shows not only the central three pillars but also several others in the same star-forming region, as well as a huge number of stars in front of, in, or behind the Eagle Nebula. The cluster of bright blue stars to the upper right is NGC 6611, home to the massive and hot stars that illuminate the pillars. Image: ESO
X-RAY AND OPTICAL
A new look at the famous “Pillars of Creation” with NASA’s Chandra X-ray Observatory has allowed astronomers to peer inside the dark columns of gas and dust. This penetrating view of the central region of the Eagle Nebula reveals how much star formation is happening inside these iconic structures.
The Chandra data shows bright X-ray sources in this field, most of which are young stars. In this image, red, green, and blue represent low, medium, and high energy X-rays. The Chandra data have been overlaid on the Hubble Space Telescope image to show the context of these X-ray data.
Very few X-ray sources are found in the pillars themselves. This suggests that the Eagle Nebula may be past its star-forming prime, since young stars are usually bright X-ray sources. However, there are two X-ray objects found near the tips of the pillars. One is a young star about 4 or 5 times as massive as the Sun, visible as the blue source near the tip of the pillar on the left. The other is a lower mass star near the top of the other pillar that is so faint it is not visible in the composite image.
The Chandra observations did not detect X-rays from any of the so-called evaporating gaseous globules, or EGGs. The EGGs are dense, compact pockets of interstellar gas where stars are believed to be forming. The lack of X-rays from these objects may mean that most of the EGGs do not contain enshrouded stars. However, infrared observations have shown that 11 of the 73 EGGs contain infant stellar objects and 4 of these are massive enough to form a star. The stars embedded in these 4 EGGs might be so young that they have not generated X-rays yet and one of them (E42) – estimated to have about the mass of the Sun – could represent one of the earliest stages of evolution of our nearest star. The Sun was likely born in a region like the Pillars of Creation.
The pillars and the few stars forming inside them are the last vestiges of star formation in the Eagle Nebula, also known as M16, which peaked several million years earlier. This contrasts strongly with the active star forming regions in other clusters such as NGC 2024, where Chandra sees a dense cluster of embedded young stars.
The results were published in the January 1st issue of The Astrophysical Journal and the research team, led by Jeffrey Linsky of the University of Colorado, includes Marc Gagne and Anna Mytyk (West Chester University), Mark McCaughrean (University of Exeter) and Morten Andersen (University of Arizona). X-ray: NASA/CXC/U.Colorado/Linsky et al.; Optical: NASA/ESA/STScI/ASU/J.Hester & P.Scowen.