Pyxis Constellation

Pyxis constellation lies in the southern sky. It represents a mariner’s compass. It was one of the constellations created by the French astronomer Nicolas Louis de Lacaille in the 18th century.

Lacaille originally named the constellation Pyxis Nautica, but the name was later simplified to just Pyxis.

Pyxis lies near the former constellation Argo Navis, which represented the Argonauts’ ship, but was eventually broken into several smaller constellations.


pyxis stars,pyxis constellation,pyxis star map,pyxis location

Pyxis Constellation Map, by IAU and Sky&Telescope magazine

Pyxis is the 65th constellation in size, occupying an area of 221 square degrees.

It is located in the second quadrant of the southern hemisphere (SQ2) and can be seen at latitudes between +50° and -90°.

The neighboring constellations are Antlia, Hydra, Puppis and Vela.

Pyxis contains three stars with known planets and has no Messier objects.

The brightest star in the constellation is Alpha Pyxidis, with an apparent visual magnitude of 3.68.

There are no meteor showers associated with the constellation.

Pyxis belongs to the Heavenly Waters family of constellations, along with Carina, Columba, Delphinus, Equuleus, Eridanus, Piscis Austrinus, Puppis and Vela.


The constellation Pyxis was created by the French astronomer Nicolas Louis de Lacaille in 1751-52 during his exploration of the southern skies. He named the constellation la Boussole and later Latinized the name to Pixis Nautica. The constellation appeared under this name in the second edition of Lacaille’s chart in 1763. The name was eventually shortened to Pyxis.

The constellation represents the magnetic compass used by navigators and seamen and should not be confused with Circinus, which was named after a draftsman’s compasses. Pyxis lies in the vicinity of the three constellations that were once known as Argo Navis, a single large constellation that represented the ship of the Argonauts. Lacaille was the one who divided the constellation into three smaller ones – Carina, Puppis and Vela – and this might be the reason why Pyxis is sometimes mentioned as the fourth constellation that was part of Argo Navis, even though it wasn’t. The Greek astronomer Ptolemy had catalogued the stars from Alpha to Delta Pyxidis, but not as part of Argo Navis, but as stars located on or around the ship’s mast.

In 1844, the English astronomer John Herschel suggested that the name Pyxis be replaced with Malus, the mast, which would have made the constellation a subdivision of Argo Navis if Herschel’s suggestion had been accepted, but it wasn’t. The International Astronomical Union (IAU) eventually adopted Pyxis as one of the 88 modern constellations.


α Pyxidis (Alpha Pyxidis)

Alpha Pyxidis is a giant star belonging to the spectral class B1.5III. It has an apparent visual magnitude of 3.67 and is approximately 880 light years distant. The star is classified as a Beta Cephei variable, which means that variations in its brightness are a result of pulsations of the star’s surface.

Alpha Pyxidis has more than 10 solar masses and a radius six times that of the Sun. It is about 10,000 times more luminous than the Sun and will eventually end its life in a supernova explosion.

β Pyxidis (Beta Pyxidis)

Beta Pyxidis is a binary star with a combined apparent magnitude of 3.954, about 420 light years distant from the Sun. It is the second brightest star in Pyxis.

The star has a spectral classification G7Ib-II, which means that it is either a bright giant or supergiant, yellowish in colour. It has 28 times the Sun’s radius. It has a magnitude 12.5 visual companion located 12.7 arc seconds away.

γ Pyxidis (Gamma Pyxidis)

Gamma Pyxidis is an orange giant of the spectral type K3III. It has a visual magnitude of 4.026 and is approximately 209 light years distant. It is the third brightest star in the constellation.

recurrent nova

T Pyxidis, image: NASA, Hubble Space Telescope

T Pyxidis

T Pyxidis is a binary star composed of a star similar to the Sun and a white dwarf. It usually has a visual magnitude of 15.5, but being a recurrent nova, when it erupts, the magnitude can go up to 6.4. There are currently only ten recurrent novae known. T Pyxidis was observed erupting in 1890, 1902, 1920, 1944, 1966 and 2011.

The two stars in the T Pyxidis system lie close together and the white dwarf draws mass off the Sun-like star, which causes the periodic eruptions.

T Pyxidis is 3260 light years distant from Earth. Evidence suggests that the star has increased in mass despite the eruptions and that it might soon explode as a Type 1a supernova, the kind of supernova that results from a violent explosion of a white dwarf. When this happens, and soon does not mean tomorrow but some time in the next 10 million years, the explosion and the resulting thermonuclear blast will destroy the ozone layer and make our planet uninhabitable.

κ Pyxidis (Kappa Pyxidis)

Kappa Pyxidis is a multiple star with the spectral classification K4/K5III. The brightest component in the system is an orange giant. The system has a combined apparent magnitude of 4.62 and is 487 light years distant. It will come within 306 light years of the Sun in about 2.6 million years, and brighten to magnitude 3.34.

θ Pyxidis (Theta Pyxidis)

Theta Pyxidis is a red giant of the spectral type M0III. It has a visual amgnitude of 4.71 and is about 522 light years distant. Some 5.8 million years ago, the star came within 241 light years of the Sun and had an apparent magnitude of 3.12.

ζ Pyxidis (Zeta Pyxidis)

Zeta Pyxidis is another multiple star in Pyxis. The brightest component is a yellow giant star of the spectral type G5III, about 236 light years distant from the Sun.

δ Pyxidis (Delta Pyxidis)

Delta Pyxidis is also a multiple star. It has an apparent magnitude of 4.87 and is 226 light years distant. The primary component in the system is a white subgiant of the spectral type A3IV.


planetary nebula

A Hubble Space Telescope photo of the planetary nebula NGC 2818, one of few planetary nebulae in the Milky Way residing inside a star cluster. Image: NASA, ESA, and the Hubble Heritage Team

NGC 2818

NGC 2818 is a planetary nebula in Pyxis, created when a dying star ejected its outer layers, which now appear as glowing gases.

The remnant of the central star’s core remains as a white dwarf.

The nebula is 3.25 light years in radius and lies about 10,400 light years from the solar system.

NGC 2627

NGC 2627 is an open cluster in Pyxis. It contains about 40 stars with magnitudes ranging from 11 to 13.

barred spiral galaxy,spiral galaxy in pyxis

NGC 2613, image: ESO, IDA, Danish 1.5 m, R. Gendler, J.-E. Ovaldsen, C. Thöne and C. Féron

The cluster has a visual magnitude of 8.4 and is about 8000 light years distant. The cluster is located to the south-west of Zeta Pyxidis.

NGC 2613

NGC 2613 is a barred spiral galaxy, seen almost edge-on. It is believed to resemble our galaxy, the Milky Way.

It has an apparent magnitude of 10.6 and is approximately 60 million light years distant.