Ara Constellation

Ara is a small constellation located in the southern sky. Its name means “the altar” in Latin.

The constellation represents the altar used by Zeus and other Greek gods to swear a vow of allegiance before they went to war against Cronus and the Titans. In another Greek myth, Ara represents the altar of King Lycaon of Arcadia.

Ara was one of the 88 constellations listed by the Greek astronomer Ptolemy in the 2nd century.


Ara is among the smaller constellations (63rd in size), occupying an area of 237 square degrees. It lies in the third quadrant of the southern hemisphere (SQ3) and can be seen at latitudes between +25° and -90°.

The neighboring constellations are Apus, Corona Australis, Norma, Pavo, Scorpius, Telescopium, and Triangulum Australe.

The constellation Ara has seven stars with known exoplanets: Mu Arae (four planets), Gliese 676 (binary system with four planets), HD 154857 (one confirmed and one suspected planet), Gliese 674, HD 152079, HD 154672 and HD 156411

Ara contains two stars brighter than magnitude 3.00 and three stars located within 10 parsecs (32.6 light years) of Earth. The brightest star in the constellation is Beta Arae. The nearest star, Gliese 674 (spectral class M3V), lies at a distance of 14.80 light years from Earth. There are no meteor showers linked to Ara. The constellation does not contain any Messier objects.

Ara belongs to the Hercules family of constellations, together with Aquila, Centaurus, Corona Australis, Corvus, Crater, Crux, Cygnus, Hercules, Hydra, Lupus, Lyra, Ophiuchus, Sagitta, Scutum, Serpens, Sextans, Triangulum Australe, and Vulpecula.

The constellation contains several notable deep sky objects: the Stingray Nebula, the open clusters Westerlund 1 (Ara Cluster) and NGC 6193, the globular clusters NGC 6397, NGC 6352 and NGC 6362, the barred spiral galaxy NGC 6300, the planetary nebula NGC 6326 and the pre-planetary Water Lily Nebula.

ara constellation,star chart,star map

Ara Constellation Map, by IAU and Sky&Telescope magazine


There are several myths associated with the constellation. In one of them, Ara represents the altar on which Zeus and other gods vowed to defeat the Titans and overthrow Cronus, who ruled the universe. Cronus was one of the 12 Titans who had deposed his father Uranus, the previous ruler.

When a prophecy said that the same fate would befall Cronus and he would be defeated by one of his own children, to prevent it from happening, he swallowed all his children – Hestia, Demeter, Hera, Hades, and Poseidon – all of them future gods and goddesses. When the youngest child, Zeus, was born, his mother Rhea hid him in Crete and gave Cronus a stone to swallow, telling him the stone was Zeus.

When Zeus grew up, he made Cronus vomit his brothers and sisters. Once freed, they swore to overthrow Cronus and the Titans. The war between the gods and the Titans lasted a decade and the gods won in the end. Zeus became the god of the sky, ruling from Olympus, Poseidon became the god of the sea, and Hades the ruler of the underworld. Zeus placed the altar among the stars to commemorate the gods’ victory.

In another story, Ara represents the altar of Lycaon, the king of Arcadia who decided to test Zeus by serving him a meal of a dismembered child, and later tried to kill the god while he slept. Zeus, enraged, transformed Lycaon into a wolf and killed his 50 sons with lightning bolts. In one version of the tale, the sacrificed child was Arcas, the son of Zeus and Lycaon’s daughter Callisto.


β Arae (Beta Arae)

Beta Arae is an orange K-type bright giant (possibly supergiant), approximately 603 light years distant. With an apparent magnitude of 2.84, it is the brightest star in the Ara constellation.

α Arae (Alpha Arae)

Alpha Arae, the second brightest star in Ara, is a variable Be star, a B-type star with prominent emission lines of hydrogen in its spectrum. Its apparent magnitude varies between 2.76 and 2.90.

Alpha Arae is approximately 240 light years from Earth.

It rotates very quickly (estimated speed at the equator is 470 km/s) and, as a result of this, the star is surrounded by an equatorial disk of ejected material.

γ Arae (Gamma Arae)

Gamma Arae is a blue-white B-type supergiant, approximately 1140 light years distant. It has a visual companion 17.9 arcseconds away. The companion is a white A-type main sequence dwarf. Gamma Arae has an apparent magnitude of 3.5.

ζ Arae (Zeta Arae)

Zeta Arae is another orange K-type giant, about 574 light years distant. It has an apparent magnitude of 3.12.

μ Arae (Mu Arae)

Mu Arae (HD 160691) is a main sequence G-type star that has four known planets in its orbit. It is approximately 50 light years distant and has an apparent magnitude of 5.12. Three of the four planets in the star’s orbit have masses similar to that of Jupiter.

ε Arae (Epsilon Arae)

Epsilon Arae is a binary star system. Epsilon-1 Arae has an apparent magnitude of 4.06 and is about 300 light years distant. It is an orange K-type giant.

Epsilon-2 Arae is a binary star, 85.9 light years away, with an apparent magnitude of 5.27. The primary component is a yellow-white F-type main sequence dwarf. The closer companion star is only 0.6 arcseconds away and has an apparent magnitude of 8.6. The system has a third component, a 13th magnitude star that lies 25 arcseconds away from the primary star.


NGC 6193

ngc 6193

NGC 6193. Photo by Rbarba. Three-colors image of NGC 6193 and NGC 6188 obtained with the Curtis-Schmidt telescope at Cerro Tololo Inter-American Observatory (Chile).

NGC 6193 is a large open cluster that contains 27 stars, many of them binaries. The cluster lies eight degrees west and one degree north of Alpha Arae. Its estimated age is 3 million years.

The two hottest stars in the cluster are responsible for the illumination of NGC 6188, an emission nebula also located in Ara constellation.

NGC 6193 has a visual magnitude of 5.2, is 15′ in diameter, and lies approximately 4,300 light years from Earth.

NGC 6397

globular cluster,ara constellation

NGC 6397, photo: NASA/ESA and the Hubble Heritage Team (AURA/STScI)

NGC 6379 is a bright globular star cluster located three degrees to the northeast of Beta Arae. It contains about 400,000 stars.

The cluster is approximately 7,200 light years distant, which makes it one of the nearest globular clusters to us.

It was first discovered in the mid-18th century by the French astronomer Nicolas Lacaille.

The cluster is notable for the number of blue stragglers it contains. (Blue stragglers are main sequence stars that are bluer, two to three times more massive, and a few magnitudes above the stars at the main sequence turn-off point for the cluster.)

The Stingray Nebula (Hen 3-1357)

hen 1357,stingray nebula

The Singray Nebula, photo: NASA, Matt Bobrowsky, Orbital Sciences Corporation

The Stingray Nebula is a planetary nebula approximately 18,000 light years from Earth. It is the youngest planetary nebula known.

The central star is a white dwarf that has a companion 0.3 arcseconds away. The nebula has an apparent magnitude of 10.75.

Even though it is significantly smaller than most other planetary nebulae discovered so far, the Stingray Nebula is 130 times larger than our solar system.

NGC 6362

globular cluster

This colourful view of the globular star cluster NGC 6362 was captured by the Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile in 2012. Image: European Southern Astronomy (ESO)

The globular cluster NGC 6362 has an apparent magnitude of 8.3 and lies at a distance of about 24,800 light years from Earth. It is located near the border with the constellation Apus.

NGC 6362 was discovered by the British astronomer James Dunlop on June 30, 1826.

The cluster is estimated to be 13.57 billion years old and composed mostly of evolved red giant stars. It also contains a number of blue stragglers, stars that appear younger than they really are. These stars are bluer and more luminous than their neighbours either because they were formed in collisions of two old stars or because they have stolen mass from their companions.

NGC 6326

NGC 6326 is an irregular planetary nebula in Ara. It has a visual magnitude of 12.2 and lies at an approximate distance of 11,000 light years from Earth. The nebula was discovered by the Scottish astronomer James Dunlop on August 26, 1826. It occupies an area 0.32′ in size.

planetary nebula

The Hubble Space Telescope captured this beautiful image of NGC 6326, a planetary nebula with glowing wisps of outpouring gas that are lit up by a central star nearing the end of its life. When a star ages and the red giant phase of its life comes to an end, it starts to eject layers of gas from its surface leaving behind a hot and compact white dwarf. Sometimes this ejection results in elegantly symmetric patterns of glowing gas, but NGC 6326 is much less structured. This object is located in the constellation of Ara, the Altar, about 11 000 light-years from Earth. This picture was created from images taken using the Hubble Space Telescope’s Wide Field Planetary Camera 2. The red light was captured through a filter letting through the glow from hydrogen gas (F658N). The blue glow comes from ionised oxygen and was recorded through a green filter (F502N). The green layer of the image, which shows the stars well, was taken through a broader yellow filter (F555W). The total exposure times were 1400 s, 360 s and 260 s respectively. The field of view is about 30 arcseconds across. Image: ESA/Hubble and NASA

NGC 6300

NGC 6300 is a barred spiral galaxy classified as a Seyfert galaxy. It has a visual magnitude of 8.78 and lies at a distance of 50.9 million light years from Earth. The galaxy was discovered by James Dunlop on June 30, 1826. It is suspected to contain a black hole with a mass 300,000 times that of the Sun.

spiral galaxy in ara

This image shows the bright centre and swirling arms of the spiral galaxy NGC 6300. NGC 6300 is located in a starry patch of sky in the southern constellation of Ara (The Altar) which contains a variety of intriguing deep-sky objects. NGC 6300 has beautiful pinwheeling arms connected by a straight bar that cuts through the middle of the galaxy. While it may look like a standard spiral galaxy in visible-light images like this one, it is actually a Seyfert II galaxy. Such galaxies have unusually luminous centres that emit very energetic radiation, meaning that they are often intensely bright in part of the spectrum either side of the visible. NGC 6300 is thought to contain a massive black hole at its heart some 300 000 times more massive than the Sun. This black hole is emitting high energy X-rays as it is fed by the material that is pulled into it. This image of NGC 6300 was taken by the ESO Faint Object Spectrograph and Camera (EFOSC2) on the 3.58-metre New Technology Telescope (NTT). Image: ESO/C. Snodgrass

NGC 6352

NGC 6352 is a globular cluster with an apparent magnitude of 7.8. It occupies an area 7.1′ in size and lies at a distance of 19,570 light years from Earth. Also known as Caldwell 93, the cluster is a relatively loose one. Individual stars can be resolved in 6-inch and larger telescopes.

globular cluster in ara

NGC 6352. Image: NASA (Hubble Space Telescope)

Ara Cluster (Westerlund 1)

The Ara Cluster is a compact young open cluster located approximately 12,100 light years from Earth. It was named Westerlund 1 after Bengt Westerlund, the Swedish astronomer who discovered it in 1961.

Westerlund 1 is one of the most massive young clusters in our galaxy. It contains an unusually high number of rare high-mass stars, including the red supergiant Westerlund 1-26. Westerlund 1-26 is one of the largest stars known, with a radius approximately 1,530 times that of the Sun.

The Ara Cluster is also home to 6 yellow hypergiants, 3 other red supergiants, 24 Wolf-Rayet stars, a considerable number of OB supergiants, and a luminous blue variable.

westerlund 1

Ara Cluster (Westerlund 1). This exceptionally bright cluster lies about 16 000 light-years from Earth in the southern constellation of Ara (The Altar). It contains hundreds of very massive and brilliant stars, all of which are just a few million years old — babies by stellar standards. But our view of this cluster is hampered by gas and dust that prevents most of the visible light from the cluster’s stars from getting to Earth. Now, astronomers studying images of Westerlund 1 from a new survey of the southern skies have spotted something unexpected in this cluster. Around one of the stars — known as W26, a red supergiant and possibly the biggest star known— they have discovered clouds of glowing hydrogen gas, shown as green features in this new image. Such glowing clouds around massive stars are very rare, and are even rarer around a red supergiant— this is the first ionised nebula discovered around such a star. W26 itself would be too cool to make the gas glow; the astronomers speculate that the source of the ionising radiation may be either hot blue stars elsewhere in the cluster, or possibly a fainter, but much hotter, companion star to W26. W26 will eventually explode as a supernova. The nebula that surrounds it is very similar to the nebula surrounding SN1987A, the remnants of a star that went supernova in 1987. SN1987A was the closest observed supernova to Earth since 1604, and as such it gave astronomers a chance to explore the properties of these explosions. Studying objects like this new nebula around W26 will help astronomers to understand the mass loss processes around these massive stars, which eventually lead to their explosive demise. Image: ESO/VPHAS+ Survey/N. Wright

Water Lily Nebula

The Water Lily Nebula, catalogued as IRAS 16594-4656, is a pre-planetary nebula found in Ara. It is in the process of evolving into a planetary nebula. The nebula was discovered and imaged by the Hubble Space Telescope.

pre-planetary nebula,protoplanetary nebula

The Water Lily Nebula in Ara constellation. Image: Judy Schmidt

Other deep sky objects in Ara include the intermediate spiral galaxy NGC 6328, the barred spiral galaxy NGC 6221, the young open cluster NGC 6250, the spiral galaxies NGC 6215 and NGC 6221, the open clusters IC 4651, NGC 6200, NGC 6204, and NGC 6208, and the globular cluster ESO 280-SC06.