|Pronunciation||//, genitive //|
|Symbolism||The compass box|
|Area||221 sq. deg. (65th)|
|Stars with planets||4|
|Stars brighter than 3.00m||0|
|Stars within 10.00 pc (32.62 ly)||1|
|Brightest star||α Pyx (3.68m)|
|Nearest star||Gliese 318
(30.13 ly, 9.24 pc)
|Visible at latitudes between +50° and −90°.
Best visible at 21:00 (9 p.m.) during the month of March.
Pyxis (//; Greek: box) is a small and faint constellation in the southern sky. Abbreviated from Pyxis Nautica, its name is Latin for a mariner's compass (contrasting with Circinus, which represents a draftsman's compasses). Pyxis was introduced by Nicolas Louis de Lacaille in the 18th century. The constellation is located close to those forming the old constellation of Argo Navis (the ship Argo), and in the 19th century astronomer John Herschel suggested renaming Pyxis to 'Malus, the mast', but the suggestion was not followed. Pyxis is completely visible from latitudes south of 53 degrees north, with its best evening-sky visibility in January through March.
The brightest star is Alpha Pyxidis at magnitude 3.68, a blue-white star around 22,000 times as luminous as the Sun. Near Alpha is T Pyxidis, a recurrent nova that has flared in brightness every few decades. Three star systems have planets, all discovered by doppler spectroscopy.
The French astronomer Nicolas Louis de Lacaille first described the constellation in French as la Boussole (the Marine Compass) in 1751–52, after he had observed and catalogued 10,000 southern stars during a two-year stay at the Cape of Good Hope. He devised fourteen new constellations in uncharted regions of the Southern Celestial Hemisphere not visible from Europe. All but one honoured instruments that symbolised the Age of Enlightenment. Lacaille Latinised the name to Pixis [sic] Nautica on his 1763 chart. The Greeks identified the four main stars of Pyxis as the mast of the great ship.
German astronomer Johann Bode defined the constellation Lochium Funis (the "Log and Line," a nautical device once used for measuring speed and distance traveled at sea) around Pyxis in his 1801 star atlas but this did not survive. In 1844 John Herschel attempted to resurrect the classical configuration by renaming it Malus (the "Mast"), a suggestion followed by Francis Baily, but Benjamin Gould restored Lacaille's nomenclature.
Covering 220.8 square degrees and hence 0.535% of the sky, Pyxis ranks 65th of the 88 modern constellations by area. Its position in the Southern Celestial Hemisphere means that the whole constellation is visible to observers north of 52°N.[a] A small constellation, it is bordered by Hydra to the north, Puppis to the west, Vela to the south, and Antlia to the east. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is 'Pyx'. The official constellation boundaries, as set by Eugène Delporte in 1930, are defined by a polygon of eight segments (illustrated in infobox). In the equatorial coordinate system, the right ascension coordinates of these borders lie between 10h 32.8m and 27h 42.5m, while the declination coordinates are between −17.41° and −37.29°.
Lacaille gave Bayer designations to ten stars now named Alpha to Lambda Pyxidis, skipping the Greek letters iota and kappa. Although a nautical element, the constellation was not an integral part of the old Argo Navis and hence did not share in the original Bayer designations of that constellation, which were split between Carina, Vela and Puppis. Overall, there are 41 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5.[b]
With a visual magnitude of 3.68, Alpha Pyxidis is the brightest star in the constellation. Located 880 ± 30 light-years distant from Earth, it is a blue-white star of spectral type B1.5III that is around 22,000 times as luminous as the Sun and has 9.4 ± 0.7 times its diameter. It began life with a mass 12.1 ± 0.6 times that of the Sun, almost 15 million years ago. Its light is dimmed by 30% due to interstellar dust, so would be a brighter magnitude of 3.31 if not for this. The second brightest star at magnitude 3.97 is Beta Pyxidis, a yellow bright giant or supergiant of spectral type G7Ib-II that is around 435 times as luminous as the Sun, lying 420 ± 10 light-years distant away from Earth. It has a companion star of magnitude 12.5 separated by 9 arcseconds. Gamma Pyxidis is a star of magnitude 4.02 that lies 207 ± 2 light-years distant. It is an orange giant of spectral type K3III that has exhausted its core hydrogen and cooled and swollen to 3.7 times the diameter of the Sun.
Kappa Pyxidis was catalogued but not given a Bayer designation by Lacaille, however Gould felt the star was bright enough to warrant a letter. Kappa has a visual magnitude of 4.62 and is 560 ± 50 light years distant. An orange giant of spectral type K4/K5III, Kappa has a luminosity approximately 965 times that of the Sun and has a surface temperature of 4031 K. It is separated by 2.1 arcseconds from a magnitude 10 star. Theta Pyxidis is a red giant of spectral type M1III and semi-regular variable with two measured periods of 13 and 98.3 days, and an average visual magnitude of 4.71, and is 500 ± 30 light-years distant from Earth. It has swollen to 5.4 times the diameter of the Sun.
Located around 4 degrees northeast of Alpha is T Pyxidis, a binary star system composed of a white dwarf with around 0.8 times the Sun's mass and a red dwarf that orbit each other every 1.8 hours located around 15,500 light-years away from Earth. A recurrent nova, it has brightened to the 7th magnitude in the years 1890, 1902, 1920, 1944, 1966 and 2011 from a baseline of around 14th magnitude. These outbursts are thought to be due to the white dwarf sucking material from its companion and ejecting it in shells.
TY Pyxidis is an eclipsing binary star whose apparent magnitude ranges from 6.85 to 7.5 over 3.2 days. The two components are both of spectral type G5IV with a diameter 2.2 times, and mass 1.2 times that of the Sun, and revolve around each other every 3.2 days. The system is classified as a RS Canum Venaticorum variable, a binary system with prominent starspot activity, and lies 184 ± 5 light years away. RZ Pyxidis is another eclipsing binary system, made up of two young stars less than 200,000 years old. Both are hot blue-white stars of spectral type B7V and are around 2.5 times the size of the Sun. One is around five times as luminous as the sun and the other around four times as luminous. The system is classified as a Beta Lyrae variable, the apparent magnitude varying from 8.83 to 9.72 over 0.66 days. AK Pyxidis is a red giant of spectral type M5III and semi-regular variable that varies between magnitudes 6.09 and 6.51. Its pulsations take place over multiple periods simultaneously of 55.5, 57.9, 86.7, 162.9 and 232.6 days. UZ Pyxidis is another semi-regular variable red giant, this time a carbon star, that is around 3560 times as luminous as the Sun with a surface temperature of 3482 K, located some 2116 light-years away from Earth. It varies between magnitudes 6.99 and 7.83 over 159 days. VY Pyxidis is a BL Herculis variable (type II Cepheid), ranging between apparent magnitudes 7.13 and 7.40 over a period of 1.23995 days. Located around 650 light-years distant, it shines with a luminosity approximately 45 times that of the Sun and has a surface temperature of 5892 K.
The closest star to earth in the constellation is Gliese 318, a white dwarf of spectral class DA5 and visual magnitude 11.85, which is estimated to be 26 or 28.7 ± 0.5 light-years distant from Earth. It has around 45% of the Sun's mass, yet only 0.15% of its luminosity. WISEPC J083641.12-185947.2 is a brown dwarf located around 72 light years from earth which was discovered by infrared astronomy in 2011.
Pyxis is home to three stars with confirmed planetary systems—all discovered by doppler spectroscopy: HD 73256 is a yellow star of spectral type G9V that has 69% of our Sun's luminosity, 89% its diameter and 105% of its mass. Around 119 light years away, it shines with an apparent magnitude of 8.08 and is around a billion years old. A hot Jupiter, HD 73256 b, that orbits it every 2.55 days was discovered using the CORALIE spectrograph in 2003. HD 73267 is a 7 billion year-old star of spectral type G5V that is around 89% as massive as the Sun. Its companion HD 73267 b, orbiting it every 1260 days, was discovered with the High Accuracy Radial Velocity Planet Searcher (HARPS) in 2008. Gliese 317 is a red dwarf of spectral type M2.5V that is has around 42% the Sun's mass and is around 50 light years distant. Orbited by two gas giant planets, it is a good candidate for future searches for more terrestrial rocky planets.
Deep sky objects
Pyxis lies in the plane of the Milky Way, although part of the eastern edge is dark, with material obscuring our galaxy arm there. NGC 2818 is a planetary nebula that lies within a dim open cluster of magnitude 8.2. NGC 2613 is a spiral galaxy of magnitude 10.5 which appears spindle shaped as it is almost edge-on to observers on Earth. Henize 2-10 is a dwarf galaxy which lies some 30 million light years away. It is notable for having a black hole around a million solar masses at its centre. Known as a starburst galaxy due to very high rates of star formation, it has a bluish colour due to the huge numbers of young stars within it.
- While parts of the constellation technically rise above the horizon to observers between the 52°N and 72°N, stars within a few degrees of the horizon are to all intents and purposes unobservable.
- Objects of magnitude 6.5 are among the faintest visible to the unaided eye in suburban-rural transition night skies.
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