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Coordinates: Sky map 06h 23m 57.1099s, −52° 41′ 44.378″
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In 2014, astronomer Eric Mamajek reported that an extremely magnetically active M dwarf (having strong coronal X-ray emission), 1.16 degrees south of Canopus, appears to share common proper motion with Canopus. The projected separation of the M dwarf 2MASS J06234738-5351131 ("Canopus B") is approximately 1.9 parsecs, however, despite this large separation, it is still within the estimated tidal radius (2.9 parsecs) for the massive star Canopus.<ref name="mamajek"/> Canopus is bright at [[microwave]] wavelengths, one of the few F-class stars to be detected by radio.<ref name=gudel2002>{{cite journal |bibcode=2002ARA&A..40..217G |title=Stellar Radio Astronomy: Probing Stellar Atmospheres from Protostars to Giants |last1=Güdel |first1=Manuel |journal=Annual Review of Astronomy and Astrophysics |year=2002 |volume=40 |pages=217–261 |doi=10.1146/annurev.astro.40.060401.093806 |arxiv=astro-ph/0206436 }}</ref>
In 2014, astronomer Eric Mamajek reported that an extremely magnetically active M dwarf (having strong coronal X-ray emission), 1.16 degrees south of Canopus, appears to share common proper motion with Canopus. The projected separation of the M dwarf 2MASS J06234738-5351131 ("Canopus B") is approximately 1.9 parsecs, however, despite this large separation, it is still within the estimated tidal radius (2.9 parsecs) for the massive star Canopus.<ref name="mamajek"/> Canopus is bright at [[microwave]] wavelengths, one of the few F-class stars to be detected by radio.<ref name=gudel2002>{{cite journal |bibcode=2002ARA&A..40..217G |title=Stellar Radio Astronomy: Probing Stellar Atmospheres from Protostars to Giants |last1=Güdel |first1=Manuel |journal=Annual Review of Astronomy and Astrophysics |year=2002 |volume=40 |pages=217–261 |doi=10.1146/annurev.astro.40.060401.093806 |arxiv=astro-ph/0206436 }}</ref>

==Distance==
Before the launch of the [[Hipparcos]] satellite telescope, distance estimates for Canopus varied widely, from 96 [[light-year]]s to 1200 light-years. The closer distance was derived from parallax measurements of around {{val|33|ul=mas}}.<ref name=vandekamp1943>{{cite journal |bibcode=1943PA.....51..172V }}</ref> The larger distance derives from the assumption of a very bright [[absolute magnitude]] for Canopus.<ref name=vanzyl>{{cite book|author=J.E. van Zyl|title=Unveiling the Universe: An Introduction to Astronomy|url=https://books.google.com/books?id=Cj7uBwAAQBAJ&pg=PA184|date=6 December 2012|publisher=Springer Science & Business Media|isbn=978-1-4471-1037-8|pages=184–}}</ref>

⚫
Hipparcos established Canopus as being {{val|310|u=light-years}} ({{val|95|ul=parsecs}}) from the [[Solar System]]; this is based on its 2007 [[parallax]] measurement of {{Val|10.43|0.53|ul=mas}}.<ref name="van Leeuwen2007"/> At 96 parsecs, the [[interstellar extinction]] for Canopus is very low at 0.08 magnitudes.<ref name="detail"/>


==Physical characteristics==
==Physical characteristics==
Line 80: Line 85:


Canopus pulsates slightly with a period of {{val|6.9|u=days}}. This was first detected in 1906 and the [[doppler effect|doppler]] variations were interpreted as orbital motion.<ref name=curtis1907>{{cite journal |bibcode=1907PASP...19R.259C |title=The orbits of the spectroscopic binaries alpha Carinae, kappa Velorum, and alpha Pavonis |last1=Curtis |first1=H. D. |journal=Publications of the Astronomical Society of the Pacific |year=1907 |volume=19 |page=259 }}</ref> An orbit was even calculated, but no such companion exists and the small radial velocity changes are due to movements in the atmosphere of the star. The maximum observed [[radial velocities]] are only 0.7 to {{val|1.6|ul=km/s}}. Canopus also has a magnetic field that varies with the same period, detected by the [[Zeeman splitting]] of its spectral lines.<ref name=weiss1986>{{cite journal |bibcode=1986A&A...160..243W }}</ref>
Canopus pulsates slightly with a period of {{val|6.9|u=days}}. This was first detected in 1906 and the [[doppler effect|doppler]] variations were interpreted as orbital motion.<ref name=curtis1907>{{cite journal |bibcode=1907PASP...19R.259C |title=The orbits of the spectroscopic binaries alpha Carinae, kappa Velorum, and alpha Pavonis |last1=Curtis |first1=H. D. |journal=Publications of the Astronomical Society of the Pacific |year=1907 |volume=19 |page=259 }}</ref> An orbit was even calculated, but no such companion exists and the small radial velocity changes are due to movements in the atmosphere of the star. The maximum observed [[radial velocities]] are only 0.7 to {{val|1.6|ul=km/s}}. Canopus also has a magnetic field that varies with the same period, detected by the [[Zeeman splitting]] of its spectral lines.<ref name=weiss1986>{{cite journal |bibcode=1986A&A...160..243W }}</ref>

⚫
Before the launch of the [[Hipparcos]] satellite telescope, distance estimates for Canopus varied widely, from 96 [[light-year]]s to 1200 light-years. Had the latter distance been correct, Canopus would have been one of the most luminous stars in the [[Milky Way]] galaxy. Hipparcos established Canopus as being {{val|310|u=light-years}} ({{val|96|ul=parsecs}}) from the [[Solar System]]; this is based on its 2007 [[parallax]] measurement of {{Val|10.43|0.53|ul=mas}}.<ref name="van Leeuwen2007"/> At 96 parsecs, the [[interstellar extinction]] for Canopus is very low at 0.08 magnitudes.<ref name="detail"/>


[[Very-long-baseline interferometry]] has been used to calculate Canopus' angular diameter at {{val|6.9|ul=mas}}. Combined with distance calculated by Hipparcos, this gives it a radius of 71 times [[Solar radius|that of the Sun]].<ref name=vlti/> If it were at the centre of the Solar System, it would extend 90% of the way to the orbit of [[Mercury (planet)|Mercury]].<ref name=Kalerstars>{{cite web|url=http://stars.astro.illinois.edu/sow/canopus.html|title=Canopus|last=Kaler|first=Jim|work=Stars|publisher=University of Illinois|accessdate=8 July 2012|date=26 June 2009}}</ref> It is over ten thousand times more luminous than the Sun.<ref name=vlti/> Measurements of its shape find a 1.1° departure from spherical symmetry.<ref name=cruzalebes2015>{{cite journal |bibcode=2015MNRAS.446.3277C |title=Departure from centrosymmetry of red giants and supergiants measured with VLTI/AMBER |last1=Cruzalèbes |first1=P. |last2=Jorissen |first2=A. |last3=Chiavassa |first3=A. |last4=Paladini |first4=C. |last5=Rabbia |first5=Y. |last6=Spang |first6=A. |journal=Monthly Notices of the Royal Astronomical Society |year=2015 |volume=446 |issue=4 |page=3277 |doi=10.1093/mnras/stu2382 }}</ref>
[[Very-long-baseline interferometry]] has been used to calculate Canopus' angular diameter at {{val|6.9|ul=mas}}. Combined with distance calculated by Hipparcos, this gives it a radius of 71 times [[Solar radius|that of the Sun]].<ref name=vlti/> If it were at the centre of the Solar System, it would extend 90% of the way to the orbit of [[Mercury (planet)|Mercury]].<ref name=Kalerstars>{{cite web|url=http://stars.astro.illinois.edu/sow/canopus.html|title=Canopus|last=Kaler|first=Jim|work=Stars|publisher=University of Illinois|accessdate=8 July 2012|date=26 June 2009}}</ref> It is over ten thousand times more luminous than the Sun.<ref name=vlti/> Measurements of its shape find a 1.1° departure from spherical symmetry.<ref name=cruzalebes2015>{{cite journal |bibcode=2015MNRAS.446.3277C |title=Departure from centrosymmetry of red giants and supergiants measured with VLTI/AMBER |last1=Cruzalèbes |first1=P. |last2=Jorissen |first2=A. |last3=Chiavassa |first3=A. |last4=Paladini |first4=C. |last5=Rabbia |first5=Y. |last6=Spang |first6=A. |journal=Monthly Notices of the Royal Astronomical Society |year=2015 |volume=446 |issue=4 |page=3277 |doi=10.1093/mnras/stu2382 }}</ref>

Revision as of 16:25, 13 May 2020

For other uses, see Canopus (disambiguation).
Canopus

An image of Canopus by Expedition 6
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Pronunciation /kəˈnoʊpəs/
Right ascension 06h 23m 57.10988s[1]
Declination −52° 41′ 44.3810″[1]
Apparent magnitude (V) −0.74[2]
Characteristics
Spectral type A9 II[3][4]
U−B color index +0.10[2]
B−V color index +0.15[2]
Astrometry
Radial velocity (Rv)20.3[5] km/s
Proper motion (μ) RA: 19.93[1] mas/yr
Dec.: 23.24[1] mas/yr
Parallax (π)10.55 ± 0.56 mas[1]
Distance310 ± 20 ly
(95 ± 5 pc)
Absolute magnitude (MV)–5.71[6]
Details
Mass8.0±0.3[7] M☉
Radius71±4[7] R☉
Luminosity10,700[7] L☉
Surface gravity (log g)1.64±0.05[7] cgs
Temperature7,400[8] K
Metallicity [Fe/H]–0.07[6] dex
Rotational velocity (v sin i)9[8] km/s
Other designations
Suhayl, Suhel, Suhail, α Carinae, CPD−52°1941, FK5 245, GC 8302, HD 45348, HIP 30438, HR 2326, SAO 234480[9]
Database references
SIMBADdata

Canopus /kəˈnoʊpəs/[10] is the brightest star in the southern constellation of Carina. It is around 310 light-years from the Sun. With a visual apparent magnitude of −0.74, it is the second-brightest star in the night sky, after Sirius. Its proper name is generally considered to originate from the mythological Canopus, who was a navigator for Menelaus, king of Sparta. Canopus has the Bayer designation α Carinae, which is Latinised to Alpha Carinae and abbreviated Alpha Car or α Car.

Canopus is an aging bright giant of spectral type A9 or F0, so it is essentially white when seen with the naked eye. Canopus is undergoing core helium burning and is currently in the so-called blue loop phase of its evolution, having already passed through the red-giant branch after exhausting the hydrogen in its core. Canopus has eight times the mass of the Sun and has expanded to 71 times the Sun's radius. It has a luminosity of over 10,000 times that of the luminosity of the Sun It's enlarged photosphere has an effective temperature of around 7,400 K. Canopus is an X-ray source, which is likely being emitted from its corona.

The prominent appearance of Canopus means it has been the subject of mythological lore among many ancient peoples. The acronychal rising marked the date of the Ptolemaia festival in Egypt. In Hinduism, it was named Agastya after the revered Vedic sage. For Chinese astronomers, it was known as the Old Man of the South Pole.

Nomenclature

In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[11] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[12] included a table of the first two batches of names approved by the WGSN; which included Canopus for this star. It is now so entered in the IAU Catalog of Star Names.[13]

α Carinae (Latinised to Alpha Carinae) is the star's Bayer designation. It is also listed in the Bright Star Catalogue as HR 2326, the Henry Draper Catalogue as HD 45348, and the Hipparcos catalogue as HIP 30438. Flamsteed did not number this southern star, but Gould gave it the number 7 (7 G. Carinae) in his Uranometria Argentina.

Observation

In the Southern Hemisphere, Canopus and Sirius are both visible high in the sky simultaneously, and reach a meridian just 21 min apart. Brighter than first magnitude, Canopus can be seen by naked eye in the early twilight. Most visible in summer in the Southern Hemisphere, Canopus culminates at midnight on December 27,[14] and at 9 PM on February 11.[15]

It is a circumpolar star when seen from points with latitude south of 37° 18′ S; for example, Victoria and Tasmania, Australia; Auckland and south of it, New Zealand; Bahía Blanca, Argentina; and Valdivia, Chile, and south of these cities in South America. Since Canopus is so far south in the sky, it never rises in mid- to far-northern latitudes; in theory the northern limit of visibility is latitude 37° 18′ north. This is just south of Athens, Richmond, Virginia (USA), and San Francisco, and very close to Seville and Agrigento. It is almost exactly the latitude of Lick Observatory on Mt. Hamilton, California, from which it is readily visible because of the effects of elevation and atmospheric refraction, which add another degree to its apparent altitude. Under ideal conditions, it can be spotted as far north as latitude 37° 31′ from the Pacific coast.[16] Another northernmost record of visibility came from Mount Nemrut in Turkey, latitude 37° 59′.[17] It is more easily visible in places such as the Gulf Coast and Florida, and the island of Crete (Greece) where the best season for viewing it around 9 p.m. is during late January and early February.[14] Canopus is also visible from India, but in North India (36° 13′) can be seen near the horizon, while in Southern India it can be seen without difficulty high above the horizon (08° 04′).

Canopus has a B–V color index of +0.15 where 0 is a blue-white, indicating it is essentially white, although it has been described as yellow-white. Canopus' spectral type has been given as F0 and more recently A9. It is less yellow than Altair or Procyon, with indices measured as 0.22 and 0.42, respectively. It may be that some observers have perceived Canopus as yellow-tinged because it is low in the sky and hence subject to atmospheric effects.[18] Patrick Moore said that it never appeared anything but white to him.[19]

Canopus was previously proposed to be a member of the Scorpius–Centaurus Association, however it is not located near the subgroups of that association, and has not been included as a Sco-Cen member in kinematic studies that used Hipparcos astrometric data.[20] At present, Canopus is not thought to be a member of any nearby young stellar groups.[21]

No star closer than Canopus is more luminous than it, and it has been the brightest star in Earth's night sky during three epochs over the past four million years.[22] Other stars appear brighter only during relatively temporary periods, during which they are passing the Solar System much closer than Canopus. About 90,000 years ago, Sirius moved close enough that it became brighter than Canopus, and that will remain so for another 210,000 years. But in 480,000 years, as Sirius moves further away and appears fainter, Canopus will once again be the brightest, and will remain so for a period of about 510,000 years.

Canopus was little-studied by western scientists before the 20th century. It was given a spectral class of F in 1897,[23] and given as the standard for F0 in the Henry Draper Catalogue with a class of F0I.[24] An early interferometric measurement of its angular diameter in 1968 gave a limb-darkened value of 6.86 mas, close to the accepted modern value.[25] It was studied in the ultraviolet by an early astronomical satellite, Gemini XI. The UV spectra were considered to be consistent with an F0 supergiant having a temperature of 6,900 K, the accepted parameters for Canopus at the time.[26]

In 2014, astronomer Eric Mamajek reported that an extremely magnetically active M dwarf (having strong coronal X-ray emission), 1.16 degrees south of Canopus, appears to share common proper motion with Canopus. The projected separation of the M dwarf 2MASS J06234738-5351131 ("Canopus B") is approximately 1.9 parsecs, however, despite this large separation, it is still within the estimated tidal radius (2.9 parsecs) for the massive star Canopus.[21] Canopus is bright at microwave wavelengths, one of the few F-class stars to be detected by radio.[27]

Distance

Before the launch of the Hipparcos satellite telescope, distance estimates for Canopus varied widely, from 96 light-years to 1200 light-years. The closer distance was derived from parallax measurements of around 33 mas.[28] The larger distance derives from the assumption of a very bright absolute magnitude for Canopus.[29]

Hipparcos established Canopus as being 310 light-years (95 parsecs) from the Solar System; this is based on its 2007 parallax measurement of 10.43±0.53 mas.[1] At 96 parsecs, the interstellar extinction for Canopus is very low at 0.08 magnitudes.[6]

Physical characteristics

Canopus is the brightest star in the constellation of Carina (top).

Canopus has an MK spectral type of A9 II (II indicating a bright giant), although it has also been classified as F0Ib (Ib indicating a less luminous supergiant),[30] or F0II.[7] The spectrum is dominated by strong broad hydrogen lines. There are also absorption lines of carbon, nitrogen, oxygen, sulphur, iron, and many ionised metals.[31] Balmer line profiles and oxygen line strengths indicate the size and luminosity of Canopus.[32] The spectrum consists mostly of absorption lines on a visible continuum, but some emission has been detected. For example, the calcium K line have weak emission wings on each side of the strong central absorption line, first observed in 1966. The emission line profiles are usually correlated with the luminosity of the star as described by the Wilson-Bappu effect, but in the case of Canopus they indicate a luminosity much lower than that calculated by other methods.[33] More detailed observations have shown that the emission line profiles are variable and may be due to plage areas on the surface of the star. Emission can also be found in other lines such as the h and k lines of ionised magnesium.[34]

Canopus pulsates slightly with a period of 6.9 d. This was first detected in 1906 and the doppler variations were interpreted as orbital motion.[35] An orbit was even calculated, but no such companion exists and the small radial velocity changes are due to movements in the atmosphere of the star. The maximum observed radial velocities are only 0.7 to 1.6 km/s. Canopus also has a magnetic field that varies with the same period, detected by the Zeeman splitting of its spectral lines.[36]

Very-long-baseline interferometry has been used to calculate Canopus' angular diameter at 6.9 mas. Combined with distance calculated by Hipparcos, this gives it a radius of 71 times that of the Sun.[7] If it were at the centre of the Solar System, it would extend 90% of the way to the orbit of Mercury.[37] It is over ten thousand times more luminous than the Sun.[7] Measurements of its shape find a 1.1° departure from spherical symmetry.[38]

Canopus is a source of X-rays, which are probably produced by its corona, magnetically heated to several million Kelvin. The temperature has likely been stimulated by fast rotation combined with strong convection percolating through the star's outer layers.[39] The soft X-ray sub-coronal X-ray emission is much weaker than the hard X-ray coronal emission. The same behaviour has been measured in other F-class supergiants such as α Persei and is now believed to be a normal property of such stars.[8]

Evolution

The position of Canopus in the H–R diagram indicates that it is a massive giant star currently in the core-helium burning phase.[7] This is an intermediate mass star that has left the red-giant branch and has entered a blue loop with a significantly increased effective temperature,[30] which has been measured to be 7,400 K.

Observational history

In Indian Vedic literature, Canopus is associated with the sage Agastya, one of the ancient siddhars and rishis (the others are associated with the stars of the Big Dipper).[40] To Agastya, the star is said to be the 'cleanser of waters', and its rising coincides with the calming of the waters of the Indian Ocean. It is thus considered the son of Pulastya, son of Brahma. Canopus is described by Pliny the Elder and Gaius Julius Solinus as the largest, brightest and only source of starlight for navigators near Tamraparni island (ancient Sri Lanka) during many nights.[41][40][42]

Canopus was not visible to the mainland ancient Greeks and Romans; it was, however, visible to the ancient Egyptians.[43] Hence Aratus did not write of the star as it remained below the horizon, while Eratosthenes and Ptolemy—observing from Alexandria—did, calling it Kanōbos.[44]

Averroes, who used his 1153 observation of Canopus in Marrakesh while the star was invisible in his native Spain as an argument that the earth is round.[45]

The Bedouin people of the Negev and Sinai also knew Canopus as Suhayl, and used it and Polaris as the two principal stars for navigation at night. Because it disappears below the horizon in those regions, it became associated with a changeable nature, as opposed to always-visible Polaris, which was circumpolar and hence 'steadfast'.[46] It is also referred to by its Arabic name: سهيل (Suhayl, Soheil in Persian), given by Islamic scientists in the 7th century AD. The Spanish Muslim astronomer Ibn Rushd went to Marrakesh (in Morocco) to observe the star in 1153, which is invisible in his native Córdoba, Al-Andalus. He used the different visibility in different latitudes to argue that the earth is round, following Aristotle's argument which held that such an observation was only possible if the earth was a relatively small sphere.[45]

Called the Old Man of the South Pole (in Chinese: 南极老人; pinyin: Nanji Lǎorén) in Chinese, Canopus appears (albeit misplaced northwards) on the medieval Chinese manuscript the Dunhuang Star Chart, although it cannot be seen from the Chinese capital of Chang'an.[47] The Chinese astronomer Yi Xing had journeyed south to chart Canopus and other far southern stars in 724 AD.[48] However, it was already mentioned by Sima Qian in the second century BC, drawing on sources from the Warring States period, as the southern counterpart of Sirius.[47]

Bright stars were important to the ancient Polynesians for navigation between the many islands and atolls of the Pacific Ocean. Low on the horizon, they acted as stellar compasses to assist mariners in charting courses to particular destinations. Canopus served as the southern wingtip of a "Great Bird" constellation called Manu, with Sirius as the body and Procyon the northern wingtip, which divided the Polynesian night sky into two hemispheres.[49] The Hawaiian people called Canopus Ke Alii-o-kona-i-ka-lewa, "The chief of the southern expanse"; it was one of the stars used by Hawaiʻiloa and Ki when they traveled to the Southern Ocean.[50]

The Māori people of New Zealand/Aotearoa had several names for Canopus. Ariki ("High-born"), was known as a solitary star that appeared in the east, prompting people to weep and chant.[51] They also named it Atutahi, Aotahi or Atuatahi, "Stand Alone".[52] Its solitary nature indicates it is a tapu star, as tapu people are often solitary. Its appearance at the beginning of the Maruaroa season foretells the coming winter; light rays to the south indicate a cold wet winter, and to the north foretell a mild winter. Food was offered to the star on its appearance.[53] This name has several mythologies attached to it. One story tells of how Atutahi was left outside the basket representing the Milky Way when Tāne wove it. Another related myth about the star says that Atutahi was the first-born child of Rangi, who refused to enter the Milky Way and so turned it sideways and rose before it. The same name is used for other stars and constellations throughout Polynesia.[54] Kapae-poto, "Short horizon", referred to it rarely setting as seen in New Zealand;[55] Kauanga ("Solitary") was the name for Canopus only when it was the last star visible before sunrise.[56]

The Tswana people of Botswana knew Canopus as Naka. Appearing late in winter skies, it heralded increasing winds and a time when trees lose their leaves. Stock owners knew it was time to put their sheep with rams.[57] In southern Africa, the Sotho, Tswana and Venda people called Canopus Naka or Nanga, “the Horn Star”, while the Zulu and Swazi called it inKhwenkwezi "Brilliant star". It appears in the predawn sky in the third week of May. According to the Venda, the first person to see Canopus would blow a phalaphala horn from the top of a hill, getting a cow for a reward. The Sotho chiefs also awarded a cow, and ordered their medicine men to roll bone dice and read the fortune for the coming year.[58] To the ǀXam-speaking Bushmen of South Africa, Canopus and Sirius signalled the appearance of termites and flying ants. They also believed that stars had the power to cause death and misfortune, and they would pray to Sirius and Canopus in particular to impart good fortune or skill.[59]

The Kalapalo people of Mato Grosso state in Brazil saw Canopus and Procyon as Kofongo "Duck", with Castor and Pollux representing his hands. The asterism's appearance signified the coming of the rainy season and increase in manioc, a food staple fed to guests at feasts.[60]

Canopus traditionally marked the rudder of the ship Argo Navis.[61] English explorer Robert Hues brought it to the attention of European observers in his 1592 work Tractatus de Globis, along with Achernar and Alpha Centauri, noting:

"Now, therefore, there are but three Stars of the first magnitude that I could perceive in all those parts which are never seene here in England. The first of these is that bright Star in the sterne of Argo which they call Canobus. The second is in the end of Eridanus. The third is in the right foote of the Centaure."[62]

Etymology and cultural significance

The name Canopus is a Latinisation of the Ancient Greek name Κάνωβος/Kanôbos, recorded in Claudius Ptolemy's Almagest (c.150 AD). Eratosthenes used the same spelling.[44] Hipparchos wrote it as Κάνωπος. John Flamsteed wrote Canobus,[63] as did Edmond Halley in his 1679 Catalogus Stellarum Australium.[64] The name has two possible derivations, both listed in Richard Hinckley Allen's seminal Star Names: Their Lore and Meaning.[65]

  • One from the legend of the Trojan War, where the constellation Carina was once part of the now-obsolete constellation of Argo Navis, which represented the ship used by Jason and the Argonauts. The brightest star in the constellation was given the name of a ship's pilot from another Greek legend: Canopus, pilot of Menelaus' ship on his quest to retrieve Helen of Troy after she was taken by Paris.
  • A second from the Egyptian Coptic Kahi Nub ("Golden Earth"), which refers how Canopus would have appeared near the horizon in ancient Egypt, reddened by atmospheric extinction from that position.[65] A ruined ancient Egyptian port named Canopus lies near the mouth of the Nile, site of the Battle of the Nile.

Other names

Africa

An Egyptian priestly poet in the time of Thutmose III mentions the star as Karbana, "the star which pours his light in a glance of fire, When he disperses the morning dew."[65]

Under the Ptolemies, the star was known as Ptolemaion (Greek: Πτολεμαῖον) and its acronychal rising marked the date of the Ptolemaia festival, which was held every four years, from 262 to 145 BC.[66]

In the Guanche mythology of the island of Tenerife (Spain), the star Canopus was linked with the goddess Chaxiraxi.[67]

Americas

The Navajo observed the star and named it Maʼii Bizòʼ, the “Coyote Star”. According to legend, Maʼii (Coyote) took part in the naming and placing of the star constellations during the creation of the universe. He placed Canopus directly south, naming it after himself.[68]

Asia

It is also personified as the Shou star.

In Japan, Canopus is known as Mera-boshi and Roujin-sei (the old man star).[69]

In Ancient Hindu astronomy and astrology, Canopus is named Agasti or Agastya.[65]

In traditional Tibetan astronomy and astrology, Canopus is named Karma Rishi སྐར་མ་རི་ཥི།

Kalīla o Damna, an influential Pahlavi (Middle Persian) book of animal fables was later known as Anvar-i-Suhayli (The Lights of Canopus).

Australia

Canopus was identified as the moiety ancestor Waa "Crow" to some Koori people in southeastern Australia.[70] The Boorong people of northwestern Victoria recalled that War (Canopus) was the brother of Warepil (Sirius), and that he brought fire from the heavens and introduced it to mankind. His wife was Collowgullouric War (Eta Carinae).[71] The Pirt-Kopan-noot people of western Victoria told of Waa "Crow" falling in love with a queen, Gneeanggar "Wedge-tailed Eagle" (Sirius) and her six attendants (the Pleiades). His advances spurned, he hears that the women are foraging for grubs and so transforms himself into a grub. When the women dig him out, he changes into a giant and carries her off.[72]

The Kulin people knew Canopus as Lo-an-tuka.[71] Objects in the sky were also associated with states of being for some tribes; the Wailwun of northern New South Wales knew Canopus as Wumba "deaf", alongside Mars as Gumba "fat" and Venus as Ngindigindoer "you are laughing".[73] Tasmanian aboriginal lore held that Canopus was Dromerdene, the brother of Moinee; the two fought and fell out of the sky, with Dromerdene falling into Louisa Bay in southwest Tasmania.[74]

Middle East

Canopus was known to the ancient Mesopotamians and given the name NUN-ki and represented the city of Eridu in the Three Stars Each Babylonian star catalogues and later MUL.APIN around 1100 BC.[75] Today, the star Sigma Sagittarii is known by the common name Nunki.[76]

An occasional name seen in English is Soheil, or the feminine Soheila; in Turkish is Süheyl, or the feminine Süheyla, from the Arabic name for several bright stars, سهيل suhayl,[65] and Canopus was known as Suhel /ˈsuːhɛl/ in medieval times.[77] Alternative spellings include Suhail, Souhail, Suhilon, Suheyl, Sohayl, Suhayil, Shoel, Sohil, Soheil, Sahil, Suhayeel, Sohayil, Sihel, and Sihil.[65] (See also Lambda Velorum.) An alternative name was Wazn "weight" or Haḍar "ground", possibly related to its low position near the horizon.[65] Hence comes its name in the Alphonsine Tables, Suhel ponderosus, a Latinization of Al Suhayl al Wazn.[65] Its Greek name was revived during the Renaissance.[77]

The southeastern wall of the Kaaba in Mecca is aligned with the rising point of Canopus, and is also named Janūb.[78]

Polynesia

The people of the Society Islands had two names for Canopus, as did the Tuamotu people. The Society Islanders called Canopus Taurua-e-tupu-tai-nanu, "Festivity-whence-comes-the-flux-of-the-sea", and Taurua-nui-o-te-hiti-apatoa "Great-festivity-of-the-border-of-the-south",[79] and the Tuamotu people called the star Te Tau-rari and Marere-te-tavahi, the latter said to be the true name for the former, "He-who-stands-alone".[80]

Among New Zealand Maori Canopus is a circumpolar star called Atutahi (variants include Autahi and Aotahi). Atutahi was considered so sacred that he stood alone outside the Milky Way, it was an important weather predictor and indicated when soils were ready for planting. Te Taki o Atutahi referred to the stars role in leading Te Punga (the anchor) i.e. the Southern Cross.

Role in navigation

To anyone living in the Northern Hemisphere, but far enough south to see the star, it served as a southern pole star. This lasted only until magnetic compasses became common.

In modern times, Canopus serves another navigational use. Canopus's brightness and location well off the ecliptic make it popular for space navigation. Many spacecraft carry a special camera known as a "Canopus Star Tracker" plus a Sun sensor for attitude determination.

The effects of precession will take Canopus within 10° of the south celestial pole around the year 14,000 CE.[81]

Legacy

Canopus-class battleship HMS Glory

Canopus appears on the flag of Brazil, symbolising the state of Goiás.[82]

Two U.S. Navy submarine tenders have been named after Canopus, the first serving from 1922 to 1942 and the second serving from 1965 to 1994.

The Royal Navy built six Template:Sclass-s which entered services between 1899 and 1902, and nine Canopus-class ships of the line in the early 19th century.

There are at least two mountains named after the star: Mount Canopus in Antarctica; and Mount Canopus or Canopus Hill in Tasmania, the location of the Canopus Hill astronomical observatory.

See also

References

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External links

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