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Aquila (constellation)

Aquila is a constellation on the celestial equator. Its name is Latin for 'eagle' and it represents the bird that carried Zeus/Jupiter's thunderbolts in Greek-Roman mythology.

Aquila
Constellation
AbbreviationAql
GenitiveAquilae[1]
Pronunciation/ˈækwɪlə/ Áquila,
occasionally /əˈkwɪlə/;
genitive /ˈækwɪl/
Symbolismthe Eagle[1]
Right ascension18h 41m 18.2958s20h 38m 23.7231s[2]
Declination18.6882229°–−11.8664360°[2]
Area652 sq. deg. (22nd)
Main stars10[1]
Bayer/Flamsteed
stars
65
Stars with planets9
Stars brighter than 3.00m3
Stars within 10.00 pc (32.62 ly)2
Brightest starAltair (α Aql) (0.76m)
Messier objects0
Meteor showers
  • June Aquilids
  • Epsilon Aquilids
Bordering
constellations
Visible at latitudes between +90° and −75°.
Best visible at 21:00 (9 p.m.) during the month of August.

Its brightest star, Altair, is one vertex of the Summer Triangle asterism. The constellation is best seen in the northern summer, as it is located along the Milky Way. Because of this location, many clusters and nebulae are found within its borders, but they are dim and galaxies are few.

History edit

 
The constellation Aquila as it can be seen by the naked eye.

Aquila was one of the 48 constellations described by the second-century astronomer Ptolemy. It had been earlier mentioned by Eudoxus in the fourth century BC and Aratus in the third century BC.[3]

It is now one of the 88 constellations defined by the International Astronomical Union. The constellation was also known as Vultur volans (the flying vulture) to the Romans, not to be confused with Vultur cadens which was their name for Lyra. It is often held to represent the eagle which held Zeus's/Jupiter's thunderbolts in Greco-Roman mythology. Aquila is also associated with the eagle that kidnapped Ganymede, a son of one of the kings of Troy (associated with Aquarius), to Mount Olympus to serve as cup-bearer to the gods.[1]

Ptolemy catalogued 19 stars jointly in this constellation and in the now obsolete constellation of Antinous, which was named in the reign of the emperor Hadrian (AD 117–138), but sometimes erroneously attributed to Tycho Brahe, who catalogued 12 stars in Aquila and seven in Antinous. Hevelius determined 23 stars in the first[4] and 19 in the second.[4][3]

The Greek Aquila is probably based on the Babylonian constellation of the Eagle, but is sometimes mistakenly thought as a seagull which is located in the same area as the Greek constellation.[5]

Notable features edit

Stars edit

Aquila, which lies in the Milky Way, contains many rich starfields and has been the location of many novae.[1]

Animation fading-in of Aquila, Delphinus, Sagitta, and the summer Milky Way as seen in Dark-sky preserve Westhavelland
  • α Aql (Altair) is the brightest star in this constellation and one of the closest naked-eye stars to Earth at a distance of 17 light-years. Its name comes from the Arabic phrase al-nasr al-tair, meaning "the flying eagle". Altair has a magnitude of 0.76.[1] It is one of the three stars of the Summer Triangle, along with Vega and Deneb.[6][7][8] It is an A-type main-sequence star with 1.8 times the mass of the Sun and 11 times its luminosity.[9][10] The star rotates quickly, and this gives the star an oblate shape where it is flattened towards the poles.[9][10][11]
  • β Aql (Alshain) is a yellow-hued star of magnitude 3.7, 45 light-years from Earth. Its name comes from the Arabic phrase shahin-i tarazu, meaning "the balance"; this name referred to Altair, Alshain, and Tarazed.[1] The primary is a G-type subgiant star with a spectral type of G9.5 IV and the secondary is a red dwarf.[12][13] The subgiant primary has three times the radius of the Sun and six times the luminosity.[14]
  • γ Aql (Tarazed) is an orange-hued giant star of around magnitude 2.7,[15] 460 light-years from Earth. Its name, like that of Alshain, comes from the Arabic for "the balance".[1] It is the second-brightest star in the constellation and is an unconfirmed variable star.[16]
  • ζ Aql (Okab[17]) is a binary star[18] of magnitude 3.0, 83 light-years from Earth.[1] The primary is an A-type main sequence star,[19] and the secondary has half the mass of the Sun.[18]
  • η Aql is a yellow-white-hued supergiant star, 1200 light-years from Earth. Among the brightest Cepheid variable stars, it has a minimum magnitude of 4.4 and a maximum magnitude of 3.5 with a period of 7.2 days.[1] The variability was originally observed by Edward Pigott in 1784.[20] There are also two companion stars which orbit the supergiant: a B-type main sequence star[21] and an F-type main sequence star.[22]
  • ρ Aql moved across the border into neighboring Delphinus in 1992,[23][24] and is an A-type star with a lower metallicity than the Sun.[25]
  • 15 Aql is an optical double star. The primary is an orange-hued giant of magnitude 5.41 and a spectral type of K1 III,[26][27] 325 light-years from Earth. The secondary is a purple-hued star of magnitude 7.0, 550 light-years from Earth. The pair is easily resolved in small amateur telescopes.[1]
  • 57 Aql is a binary star. The primary is a blue-hued star of magnitude 5.7 and the secondary is a white star of magnitude 6.5. The system is approximately 350 light-years from Earth; the pair is easily resolved in small amateur telescopes.[1] Both stars in the system rotate rapidly.[28]
  • R Aql is a red-hued giant star 690 light-years from Earth. It is a Mira variable with a minimum magnitude of 12.0, a maximum magnitude of 6.0, and a period around 9 months. It has a diameter of 400 D.[1]
  • V Aql is a typical Cool Carbon Star. It's one of the most red-colored examples of this sort of stars, observable through common amateur telescopes.
  • FF Aql is a yellow-white-hued supergiant star, 2500 light-years from Earth. It is a Cepheid variable star with a minimum magnitude of 5.7, a maximum magnitude of 5.2, and a period of 4.5 days.[1] It is a spectroscopic binary with a spectral type of F6Ib.[29] A third star is also a member of the system,[30] and there is also a fourth star which is probably unconnected with the main system.[31][32]

Novae edit

A bright nova was observed in Aquila in 1918 (Nova Aquilae 1918) and briefly shone brighter than Altair, the brightest star in Aquila. It was first seen by Zygmunt Laskowski[33] and was confirmed on the night of 8 June 1918.[34] Nova Aquilae reached a peak apparent magnitude of −0.5 and was the brightest nova recorded since the invention of the telescope.[35]

Deep-sky objects edit

 
IRAS 19024+0044 is a protoplanetary nebula in Aquila.

Three interesting planetary nebulae lie in Aquila:

More deep-sky objects:

  • NGC 6709 is a loose open cluster containing roughly 40 stars, which range in magnitude from 9 to 11. It is about 3000 light-years from Earth.[1] It has an overall magnitude of 6.7 and is about 9100 light-years from Earth. NGC 6709 appears in a rich Milky Way star field and is classified as a Shapley class d and Trumpler class III 2 m cluster. These designations mean that it does not have many stars, is loose, does not show greater concentration at the center, and has a moderate range of star magnitudes.[38] There are 305 confirmed member stars[39] and one candidate red giant.[40]
  • NGC 6755 is an open cluster of 7.5 m; it is made up of about a dozen stars with magnitudes 12 through 13. It is located approximately 8,060 light-years from the Solar System.[41]
  • NGC 6760 is a globular cluster of 9.1 m. At least two pulsars have been discovered in the globular cluster,[42] and it has a Shapley-Sawyer Concentration Class of IX.[43]
  • NGC 6749 is an open cluster.
  • NGC 6778 is a planetary nebula located about 10,300 light-years away from the Solar System.[44]
  • NGC 6741 is a planetary nebula.
  • NGC 6772 is a planetary nebula.
  • W51 (3C400) is one of the largest stellar nurseries in the Milky Way. Located about 17,000 light-years from Earth, W51 is about 350 light-years – or about 2 quadrillion miles – across. However, it's located in an area so thick with interstellar dust that it's opaque to visible light. Observations by the Chandra X-Ray Observatory and the Spitzer Infrared Telescope reveal W51 would appear about as large as the full Moon in visible light.[45][46]

Aquila also holds some extragalactic objects. One of them is what may be the largest single mass concentration of galaxies in the Universe known, the Hercules–Corona Borealis Great Wall. It was discovered in November 2013, and has the size of 10 billion light years. It is the biggest and the most massive structure in the Universe known.

Other edit

NASA's Pioneer 11 space probe, which flew by Jupiter and Saturn in the 1970s, is expected to pass near the star Lambda (λ) Aquilae in about 4 million years.[47]

Illustrations edit

In illustrations of Aquila that represent it as an eagle, a nearly straight line of three stars symbolizes part of the wings. The center and brightest of these three stars is Altair.[citation needed]

Mythology edit

 
Aquila, with the now-obsolete figure of Antinous, as depicted by Sidney Hall in Urania's Mirror,[48] a set of constellation cards published in London around 1825. At left is Delphinus.

According to Gavin White, the Babylonian Eagle carried the constellation called the Dead Man in its talons. The author also draws a comparison to the classical stories of Antinous and Ganymede.[5]

In classical Greek mythology, Aquila was identified as Αετός Δίας (Aetos Dios), the eagle that carried the thunderbolts of Zeus and was sent by him to carry the shepherd boy Ganymede, whom he desired, to Mount Olympus; the constellation of Aquarius is sometimes identified with Ganymede.[1]

In the Chinese love story of Qi Xi, Niu Lang (Altair) and his two children (β and γ Aquilae) are separated forever from their wife and mother Zhi Nu (Vega), who is on the far side of the river, the Milky Way.[49]

In Hinduism, the constellation Aquila is identified with the half-eagle half-human deity Garuda.[50][51]

In ancient Egypt, Aquila possibly was seen as the falcon of Horus.[52] According to Berio, the identification of Aquila as an Egyptian constellation, and not merely Graeco-Babylonian, is corroborated by the Daressy Zodiac.[53] It depicts an outer ring showing the Sphaera Graeca, the familiar Hellenistic zodiac, while the middle ring depicts the Sphaera Barbarica or foreigner's zodiac with the zodiacal signs of the Egyptian dodekaoros which were also recorded by Teucros of Babylon.[54] Under the sign of Sagittarius is the falcon of Horus, presumably because Aquila rises with Sagittarius.

Equivalents edit

In Chinese astronomy, ζ Aql is located within the Heavenly Market Enclosure (天市垣, Tiān Shì Yuán), and the other stars of the constellation are placed within the Black Tortoise of the North (北方玄武, Běi Fāng Xuán Wǔ).

Several different Polynesian equivalents to Aquila as a whole are known. On the island of Futuna, it was called Kau-amonga, meaning "Suspended Burden". Its name references the Futunan name for Orion's belt and sword, Amonga.[55] In Hawaii, Altair was called Humu, translated to English as "to sew, to bind together parts of a fishhook." "Humu" also refers to the hole by which parts of a hook are bound together.[56] Humu-ma was said to influence the astrologers.[57] Pao-toa was the name for the entire constellation in the Marquesas Islands; the name meant "Fatigued Warrior".[58] Also, Polynesian constellations incorporated the stars of modern Aquila. The Pukapuka constellation Tolu, meaning "three", was made up of Alpha, Beta, and Gamma Aquilae.[59] Altair was commonly named among Polynesian peoples, as well. The people of Hawaii called it Humu, the people of the Tuamotus called it Tukituki ("Pound with a hammer")[60] - they named Beta Aquilae Nga Tangata ("The Men")[61] - and the people of Pukapuka called Altair Turu and used it as a navigational star.[62] The Māori people named Altair Poutu-te-rangi, "Pillar of the Sky", because of its important position in their cosmology. It was used differently in different Māori calendars, being the star of February and March in one version and March and April in the other. Altair was also the star that ruled the annual sweet potato harvest.[63]

See also edit

References edit

Citations
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  50. ^ Raymond L. Langsten; Marc Jason Gilbert (1983), Research on Bengal: proceedings of the 1981 Bengal Studies Conference, Issue 34 of South Asia series, Michigan State University Asian Studies Center, Asian Studies Center, Michigan State University, 1983, ... and the appearance of the constellation Aquila that marks ... As Aquila was an eagle for the Greeks, it is the Garuda kite to Hindus...
  51. ^ V.Chandran (1993), Astronomy Quiz Book, Pustak Mahal, 1993, ISBN 978-81-223-0366-7, ... later spread to other cultures such as Arab, Hindu, Greek and Roman where the names were reinterpreted to suit the local cultures. Hence Aquila/Garuda, Leo/Singha, Hydra/Vasuki and other similarities in names ...
  52. ^ Berio, Alessandro (2014). "The Celestial River: Identifying the Ancient Egyptian Constellations" (PDF). Sino-Platonic Papers. 253: 7. Bibcode:2014SPP...253....1B.
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  55. ^ Makemson 1941, p. 218.
  56. ^ Nā Puke Wehewehe ʻŌlelo Hawaiʻi
  57. ^ Makemson 1941, p. 212.
  58. ^ Makemson 1941, p. 240.
  59. ^ Makemson 1941, p. 262.
  60. ^ Makemson 1941, p. 263.
  61. ^ Makemson 1941, p. 256.
  62. ^ Makemson 1941, p. 264.
  63. ^ Makemson 1941, p. 245.
References
  •   This article incorporates text from a publication now in the public domainChisholm, Hugh, ed. (1911). "Aquila". Encyclopædia Britannica. Vol. 2 (11th ed.). Cambridge University Press. p. 249.
  • Levy, David H. (2005), Deep Sky Objects, Prometheus Books, ISBN 1-59102-361-0
  • Makemson, Maud Worcester (1941). The Morning Star Rises: an account of Polynesian astronomy. Yale University Press. Bibcode:1941msra.book.....M.
  • Ridpath, Ian (2001), Stars and Planets, Illustrated by Wil Tirion (3rd ed.), Princeton University Press, ISBN 0-691-08913-2
  • Ridpath, Ian (2007), Stars and Planets Guide, Wil Tirion (4th ed.), Princeton University Press, ISBN 978-0-691-13556-4
  • White, Gavin (2008), Babylonian Star-lore, Solaria Pubs

External links edit

  • Ian Ridpath's Star Tales – Aquila
  • The Deep Photographic Guide to the Constellations: Aquila
  • WIKISKY.ORG: Aquila constellation
  • Warburg Institute Iconographic Database (medieval and early modern images of Aquila)
  • The clickable Aquila

aquila, constellation, aquila, constellation, celestial, equator, name, latin, eagle, represents, bird, that, carried, zeus, jupiter, thunderbolts, greek, roman, mythology, aquilaconstellationlist, stars, aquilaabbreviationaqlgenitiveaquilae, pronunciation, Áq. Aquila is a constellation on the celestial equator Its name is Latin for eagle and it represents the bird that carried Zeus Jupiter s thunderbolts in Greek Roman mythology AquilaConstellationList of stars in AquilaAbbreviationAqlGenitiveAquilae 1 Pronunciation ˈ ae k w ɪ l e Aquila occasionally e ˈ k w ɪ l e genitive ˈ ae k w ɪ l iː Symbolismthe Eagle 1 Right ascension18h 41m 18 2958s 20h 38m 23 7231s 2 Declination18 6882229 11 8664360 2 Area652 sq deg 22nd Main stars10 1 Bayer Flamsteedstars65Stars with planets9Stars brighter than 3 00m3Stars within 10 00 pc 32 62 ly 2Brightest starAltair a Aql 0 76m Messier objects0Meteor showersJune Aquilids Epsilon AquilidsBorderingconstellationsSagitta Hercules Ophiuchus Serpens Cauda Scutum Sagittarius Capricornus Aquarius DelphinusVisible at latitudes between 90 and 75 Best visible at 21 00 9 p m during the month of August Its brightest star Altair is one vertex of the Summer Triangle asterism The constellation is best seen in the northern summer as it is located along the Milky Way Because of this location many clusters and nebulae are found within its borders but they are dim and galaxies are few Contents 1 History 2 Notable features 2 1 Stars 2 2 Novae 2 3 Deep sky objects 2 4 Other 3 Illustrations 4 Mythology 5 Equivalents 6 See also 7 References 8 External linksHistory edit nbsp The constellation Aquila as it can be seen by the naked eye Aquila was one of the 48 constellations described by the second century astronomer Ptolemy It had been earlier mentioned by Eudoxus in the fourth century BC and Aratus in the third century BC 3 It is now one of the 88 constellations defined by the International Astronomical Union The constellation was also known as Vultur volans the flying vulture to the Romans not to be confused with Vultur cadens which was their name for Lyra It is often held to represent the eagle which held Zeus s Jupiter s thunderbolts in Greco Roman mythology Aquila is also associated with the eagle that kidnapped Ganymede a son of one of the kings of Troy associated with Aquarius to Mount Olympus to serve as cup bearer to the gods 1 Ptolemy catalogued 19 stars jointly in this constellation and in the now obsolete constellation of Antinous which was named in the reign of the emperor Hadrian AD 117 138 but sometimes erroneously attributed to Tycho Brahe who catalogued 12 stars in Aquila and seven in Antinous Hevelius determined 23 stars in the first 4 and 19 in the second 4 3 The Greek Aquila is probably based on the Babylonian constellation of the Eagle but is sometimes mistakenly thought as a seagull which is located in the same area as the Greek constellation 5 Notable features editStars edit See also List of stars in Aquila Aquila which lies in the Milky Way contains many rich starfields and has been the location of many novae 1 source source source source source source source source Animation fading in of Aquila Delphinus Sagitta and the summer Milky Way as seen in Dark sky preserve Westhavellanda Aql Altair is the brightest star in this constellation and one of the closest naked eye stars to Earth at a distance of 17 light years Its name comes from the Arabic phrase al nasr al tair meaning the flying eagle Altair has a magnitude of 0 76 1 It is one of the three stars of the Summer Triangle along with Vega and Deneb 6 7 8 It is an A type main sequence star with 1 8 times the mass of the Sun and 11 times its luminosity 9 10 The star rotates quickly and this gives the star an oblate shape where it is flattened towards the poles 9 10 11 b Aql Alshain is a yellow hued star of magnitude 3 7 45 light years from Earth Its name comes from the Arabic phrase shahin i tarazu meaning the balance this name referred to Altair Alshain and Tarazed 1 The primary is a G type subgiant star with a spectral type of G9 5 IV and the secondary is a red dwarf 12 13 The subgiant primary has three times the radius of the Sun and six times the luminosity 14 g Aql Tarazed is an orange hued giant star of around magnitude 2 7 15 460 light years from Earth Its name like that of Alshain comes from the Arabic for the balance 1 It is the second brightest star in the constellation and is an unconfirmed variable star 16 z Aql Okab 17 is a binary star 18 of magnitude 3 0 83 light years from Earth 1 The primary is an A type main sequence star 19 and the secondary has half the mass of the Sun 18 h Aql is a yellow white hued supergiant star 1200 light years from Earth Among the brightest Cepheid variable stars it has a minimum magnitude of 4 4 and a maximum magnitude of 3 5 with a period of 7 2 days 1 The variability was originally observed by Edward Pigott in 1784 20 There are also two companion stars which orbit the supergiant a B type main sequence star 21 and an F type main sequence star 22 r Aql moved across the border into neighboring Delphinus in 1992 23 24 and is an A type star with a lower metallicity than the Sun 25 15 Aql is an optical double star The primary is an orange hued giant of magnitude 5 41 and a spectral type of K1 III 26 27 325 light years from Earth The secondary is a purple hued star of magnitude 7 0 550 light years from Earth The pair is easily resolved in small amateur telescopes 1 57 Aql is a binary star The primary is a blue hued star of magnitude 5 7 and the secondary is a white star of magnitude 6 5 The system is approximately 350 light years from Earth the pair is easily resolved in small amateur telescopes 1 Both stars in the system rotate rapidly 28 R Aql is a red hued giant star 690 light years from Earth It is a Mira variable with a minimum magnitude of 12 0 a maximum magnitude of 6 0 and a period around 9 months It has a diameter of 400 D 1 V Aql is a typical Cool Carbon Star It s one of the most red colored examples of this sort of stars observable through common amateur telescopes FF Aql is a yellow white hued supergiant star 2500 light years from Earth It is a Cepheid variable star with a minimum magnitude of 5 7 a maximum magnitude of 5 2 and a period of 4 5 days 1 It is a spectroscopic binary with a spectral type of F6Ib 29 A third star is also a member of the system 30 and there is also a fourth star which is probably unconnected with the main system 31 32 Novae edit A bright nova was observed in Aquila in 1918 Nova Aquilae 1918 and briefly shone brighter than Altair the brightest star in Aquila It was first seen by Zygmunt Laskowski 33 and was confirmed on the night of 8 June 1918 34 Nova Aquilae reached a peak apparent magnitude of 0 5 and was the brightest nova recorded since the invention of the telescope 35 Deep sky objects edit nbsp IRAS 19024 0044 is a protoplanetary nebula in Aquila Three interesting planetary nebulae lie in Aquila NGC 6804 shows a small but bright ring NGC 6781 bears some resemblance with the Owl Nebula in Ursa Major It was discovered by William Herschel in 1788 36 NGC 6751 also known as the Glowing Eye is a planetary nebula The nebula is estimated to be roughly 0 8 light years in diameter 37 More deep sky objects NGC 6709 is a loose open cluster containing roughly 40 stars which range in magnitude from 9 to 11 It is about 3000 light years from Earth 1 It has an overall magnitude of 6 7 and is about 9100 light years from Earth NGC 6709 appears in a rich Milky Way star field and is classified as a Shapley class d and Trumpler class III 2 m cluster These designations mean that it does not have many stars is loose does not show greater concentration at the center and has a moderate range of star magnitudes 38 There are 305 confirmed member stars 39 and one candidate red giant 40 NGC 6755 is an open cluster of 7 5 m it is made up of about a dozen stars with magnitudes 12 through 13 It is located approximately 8 060 light years from the Solar System 41 NGC 6760 is a globular cluster of 9 1 m At least two pulsars have been discovered in the globular cluster 42 and it has a Shapley Sawyer Concentration Class of IX 43 NGC 6749 is an open cluster NGC 6778 is a planetary nebula located about 10 300 light years away from the Solar System 44 NGC 6741 is a planetary nebula NGC 6772 is a planetary nebula W51 3C400 is one of the largest stellar nurseries in the Milky Way Located about 17 000 light years from Earth W51 is about 350 light years or about 2 quadrillion miles across However it s located in an area so thick with interstellar dust that it s opaque to visible light Observations by the Chandra X Ray Observatory and the Spitzer Infrared Telescope reveal W51 would appear about as large as the full Moon in visible light 45 46 Aquila also holds some extragalactic objects One of them is what may be the largest single mass concentration of galaxies in the Universe known the Hercules Corona Borealis Great Wall It was discovered in November 2013 and has the size of 10 billion light years It is the biggest and the most massive structure in the Universe known Other edit NASA s Pioneer 11 space probe which flew by Jupiter and Saturn in the 1970s is expected to pass near the star Lambda l Aquilae in about 4 million years 47 Illustrations editIn illustrations of Aquila that represent it as an eagle a nearly straight line of three stars symbolizes part of the wings The center and brightest of these three stars is Altair citation needed Mythology editThis section needs additional citations for verification Please help improve this article by adding citations to reliable sources in this section Unsourced material may be challenged and removed November 2009 Learn how and when to remove this template message nbsp Aquila with the now obsolete figure of Antinous as depicted by Sidney Hall in Urania s Mirror 48 a set of constellation cards published in London around 1825 At left is Delphinus According to Gavin White the Babylonian Eagle carried the constellation called the Dead Man in its talons The author also draws a comparison to the classical stories of Antinous and Ganymede 5 In classical Greek mythology Aquila was identified as Aetos Dias Aetos Dios the eagle that carried the thunderbolts of Zeus and was sent by him to carry the shepherd boy Ganymede whom he desired to Mount Olympus the constellation of Aquarius is sometimes identified with Ganymede 1 In the Chinese love story of Qi Xi Niu Lang Altair and his two children b and g Aquilae are separated forever from their wife and mother Zhi Nu Vega who is on the far side of the river the Milky Way 49 In Hinduism the constellation Aquila is identified with the half eagle half human deity Garuda 50 51 In ancient Egypt Aquila possibly was seen as the falcon of Horus 52 According to Berio the identification of Aquila as an Egyptian constellation and not merely Graeco Babylonian is corroborated by the Daressy Zodiac 53 It depicts an outer ring showing the Sphaera Graeca the familiar Hellenistic zodiac while the middle ring depicts the Sphaera Barbarica or foreigner s zodiac with the zodiacal signs of the Egyptiandodekaoros which were also recorded by Teucros of Babylon 54 Under the sign of Sagittarius is the falcon of Horus presumably because Aquila rises with Sagittarius Equivalents editIn Chinese astronomy z Aql is located within the Heavenly Market Enclosure 天市垣 Tian Shi Yuan and the other stars of the constellation are placed within the Black Tortoise of the North 北方玄武 Bei Fang Xuan Wǔ Several different Polynesian equivalents to Aquila as a whole are known On the island of Futuna it was called Kau amonga meaning Suspended Burden Its name references the Futunan name for Orion s belt and sword Amonga 55 In Hawaii Altair was called Humu translated to English as to sew to bind together parts of a fishhook Humu also refers to the hole by which parts of a hook are bound together 56 Humu ma was said to influence the astrologers 57 Pao toa was the name for the entire constellation in the Marquesas Islands the name meant Fatigued Warrior 58 Also Polynesian constellations incorporated the stars of modern Aquila The Pukapuka constellation Tolu meaning three was made up of Alpha Beta and Gamma Aquilae 59 Altair was commonly named among Polynesian peoples as well The people of Hawaii called it Humu the people of the Tuamotus called it Tukituki Pound with a hammer 60 they named Beta Aquilae Nga Tangata The Men 61 and the people of Pukapuka called Altair Turu and used it as a navigational star 62 The Maori people named Altair Poutu te rangi Pillar of the Sky because of its important position in their cosmology It was used differently in different Maori calendars being the star of February and March in one version and March and April in the other Altair was also the star that ruled the annual sweet potato harvest 63 See also editAquila Chinese astronomy References editCitations a b c d e f g h i j k l m n o p Ridpath 2001 pp 80 82 a b Aquila constellation boundary The Constellations International Astronomical Union Retrieved 14 February 2014 a b Chisholm 1911 a b Prodromus astronomiae 1690 pp 272 273 Archived from the original on 2011 07 27 a b White 2008 p 95 NAME ALTAIR Variable Star of delta Sct type database entry SIMBAD Accessed on line November 25 2008 Altair entry The Internet Encyclopedia of Science David Darling Accessed on line November 25 2008 Summer Triangle entry The Internet Encyclopedia of Science David Darling Accessed on line November 26 2008 a b Monnier J D Zhao M Pedretti E Thureau N Ireland M Muirhead P Berger J P Millan Gabet R Van Belle G Ten Brummelaar T McAlister H Ridgway S Turner N Sturmann L Sturmann J Berger D 2007 Imaging the surface of Altair Science 317 5836 342 345 arXiv 0706 0867 Bibcode 2007Sci 317 342M doi 10 1126 science 1143205 PMID 17540860 S2CID 4615273 See second column of Table 1 for stellar parameters a href Template Cite journal html title Template Cite journal cite journal a CS1 maint postscript link a b Peterson D M Hummel C A Pauls T A et al 2006 Resolving the Effects of Rotation in Altair with Long Baseline Interferometry The Astrophysical Journal 636 2 1087 1097 arXiv astro ph 0509236 Bibcode 2006ApJ 636 1087P doi 10 1086 497981 S2CID 18683397 See Table 2 for stellar parameters Belle Gerard T van Ciardi David R Thompson Robert R Akeson Rachel L Lada Elizabeth A 2001 Altair s Oblateness and Rotation Velocity from Long Baseline Interferometry The Astrophysical Journal 559 2 1155 1164 Bibcode 2001ApJ 559 1155V doi 10 1086 322340 ISSN 0004 637X S2CID 13969695 Gray R O et al July 2006 Contributions to the Nearby Stars NStars Project spectroscopy of stars earlier than M0 within 40 pc The Southern Sample The Astronomical Journal 132 1 161 170 arXiv astro ph 0603770 Bibcode 2006AJ 132 161G doi 10 1086 504637 S2CID 119476992 Montes D et al September 2018 Calibrating the metallicity of M dwarfs in wide physical binaries with F G and K primaries I High resolution spectroscopy with HERMES stellar parameters abundances and kinematics Monthly Notices of the Royal Astronomical Society 479 1 1332 1382 arXiv 1805 05394 Bibcode 2018MNRAS 479 1332M doi 10 1093 mnras sty1295 Rains Adam D et al April 2020 Precision angular diameters for 16 southern stars with VLTI PIONIER Monthly Notices of the Royal Astronomical Society 493 2 2377 2394 arXiv 2004 02343 Bibcode 2020MNRAS 493 2377R doi 10 1093 mnras staa282 S2CID 214802418 Cousins A W J 1984 Standardization of Broadband Photometry of Equatorial Standards South African Astronomical Observatory Circulars 8 59 Bibcode 1984SAAOC 8 59C Kornilov V G Volkov I M Zakharov A I Kozyreva V S Kornilova L N Krutyakov A N Krylov A V Kusakin A V Leont Ev S E Mironov A V Moshkalev V G Pogrosheva T M Sementsov V N Khaliullin Kh F 1991 Catalogue of WBVR magnitudes of bright stars of the northern sky Trudy Gosudarstvennogo Astronomicheskogo Instituta 63 1 Bibcode 1991TrSht 63 1K Naming Stars IAU org Retrieved 30 July 2018 a b De Rosa R J et al 2014 The VAST Survey III The multiplicity of A type stars within 75 pc Monthly Notices of the Royal Astronomical Society 437 2 1216 1240 arXiv 1311 7141 Bibcode 2014MNRAS 437 1216D doi 10 1093 mnras stt1932 Cowley A et al April 1969 A study of the bright A stars I A catalogue of spectral classifications Astronomical Journal 74 375 406 Bibcode 1969AJ 74 375C doi 10 1086 110819 Pigott Edward 1785 Observations of a New Variable Star In a Letter from Edward Pigott Esq to Sir H C Englefield Bart F R S and A S Philosophical Transactions of the Royal Society of London 75 127 136 Bibcode 1785RSPT 75 127P doi 10 1098 rstl 1785 0007 S2CID 186212958 Remage Evans Nancy Bond Howard E Schaefer Gail H Mason Brian D Karovska Margarita Tingle Evan 2013 Binary Cepheids Separations and Mass Ratios in 5 M Binaries The Astronomical Journal 146 4 93 arXiv 1307 7123 Bibcode 2013AJ 146 93E doi 10 1088 0004 6256 146 4 93 S2CID 34133110 Gallenne A Kervella P Merand A Evans N R Girard J H V Gieren W Pietrzynski G 2014 Searching for visual companions of close Cepheids Astronomy amp Astrophysics 567 A60 arXiv 1406 0493 Bibcode 2014A amp A 567A 60G doi 10 1051 0004 6361 201423872 S2CID 55702630 Patrick Moore 29 June 2013 The Observer s Year 366 Nights of the Universe Springer Science amp Business Media pp 132 ISBN 978 1 4471 3613 2 Hirshfeld A et al August 1992 Book Review Sky Catalogue 2000 0 V 1 Stars to Magnitude 8 0 ED 2 Journal of the Royal Astronomical Society of Canada 86 4 221 Bibcode 1992JRASC 86 221L Anders F Khalatyan A Chiappini C Queiroz A B Santiago B X Jordi C Girardi L Brown A G A Matijevic G Monari G Cantat Gaudin T Weiler M Khan S Miglio A Carrillo I Romero Gomez M Minchev I de Jong R S Antoja T Ramos P Steinmetz M Enke H 1 August 2019 Photo astrometric distances extinctions and astrophysical parameters for Gaia DR2 stars brighter than G 18 Astronomy and Astrophysics 628 A94 arXiv 1904 11302 Bibcode 2019A amp A 628A 94A doi 10 1051 0004 6361 201935765 ISSN 0004 6361 S2CID 131780028 Frasca A et al December 2009 REM near IR and optical photometric monitoring of pre main sequence stars in Orion Rotation periods and starspot parameters Astronomy and Astrophysics 508 3 1313 1330 arXiv 0911 0760 Bibcode 2009A amp A 508 1313F doi 10 1051 0004 6361 200913327 S2CID 118361131 Cousins A W J 1964 Photometric Data for Stars in the Equatorial Zone Seventh List Monthly Notes of the Astronomical Society of Southern Africa 23 175 Bibcode 1964MNSSA 23 175C Abt Helmut A Levato Hugo Grosso Monica July 2002 Rotational Velocities of B Stars The Astrophysical Journal 573 1 359 365 Bibcode 2002ApJ 573 359A doi 10 1086 340590 Abt Helmut A 2009 MK Classifications of Spectroscopic Binaries The Astrophysical Journal Supplement 180 1 117 118 Bibcode 2009ApJS 180 117A doi 10 1088 0067 0049 180 1 117 S2CID 122811461 Evans Nancy Remage Welch Douglas L Scarfe Colin D Teays Terry J 1990 The orbit and companions of the classical Cepheid FF AQL Astronomical Journal 99 1598 1611 arXiv astro ph 9706292 Bibcode 1990AJ 99 1598E doi 10 1086 115442 ISSN 0004 6256 Gallenne A Kervella P Merand A Evans N R Girard J H V Gieren W Pietrzynski G 2014 Searching for visual companions of close Cepheids Astronomy amp Astrophysics 567 A60 arXiv 1406 0493 Bibcode 2014A amp A 567A 60G doi 10 1051 0004 6361 201423872 S2CID 55702630 Udalski A Evans Nancy R 1993 The visual companion of the classical Cepheid FF AQL Astronomical Journal 106 1 348 51 Bibcode 1993AJ 106 348U doi 10 1086 116643 ISSN 0004 6256 The Contribution of Amateurs to Astronomy Proceedings of Colloquium 98 of the International Astronomical Union June 20 24 1987 page 41 Mobberley Martin 2009 Cataclysmic Cosmic Events and How to Observe Them Springer p 46 ISBN 978 0 387 79946 9 Johnson Christopher B Schaefer Bradley E Kroll Peter Henden Arne A 2013 Nova Aquilae 1918 V603 Aql Faded by 0 44 mag century from 1938 2013 The Astrophysical Journal 780 2 L25 arXiv 1310 6802 Bibcode 2014ApJ 780L 25J doi 10 1088 2041 8205 780 2 L25 S2CID 118403602 Seligman Courtney NGC Objects NGC 6750 6799 Celestial Atlas Retrieved 2021 01 07 The Glowing Eye of Planetary Nebula NGC 6751 HubbleSite 2000 04 06 Retrieved 2021 04 12 Levy 2005 pp 79 80 Cole Kodikara Elizabeth M et al March 2021 NGC 6709 A Faint Zero Age Main Sequence Open Cluster The 20 5th Cambridge Workshop on Cool Stars Stellar Systems and the Sun CS20 5 virtually anywhere March 2 4 2021 Bibcode 2021csss confE 175C doi 10 5281 zenodo 4565515 175 Subramaniam Annapurni Sagar Ram February 1999 Multicolor CCD Photometry and Stellar Evolutionary Analysis of NGC 1907 NGC 1912 NGC 2383 NGC 2384 and NGC 6709 Using Synthetic Color Magnitude Diagrams The Astronomical Journal 117 2 937 961 Bibcode 1999AJ 117 937S doi 10 1086 300716 S2CID 34294008 Cantat Gaudin T Anders F January 2020 Clusters and mirages cataloguing stellar aggregates in the Milky Way Astronomy amp Astrophysics 633 22 arXiv 1911 07075 Bibcode 2020A amp A 633A 99C doi 10 1051 0004 6361 201936691 S2CID 208138247 A99 Freire Paulo C C Hessels Jason W T Nice David J Ransom Scott M Lorimer Duncan R Stairs Ingrid H 2005 03 10 The Millisecond Pulsars in NGC 6760 The Astrophysical Journal 621 2 959 965 arXiv astro ph 0411160 Bibcode 2005ApJ 621 959F doi 10 1086 427748 ISSN 0004 637X S2CID 119342837 Shapley Harlow Sawyer Helen B August 1927 A Classification of Globular Clusters Harvard College Observatory Bulletin 849 849 11 14 Bibcode 1927BHarO 849 11S Paturel G et al December 2003 HYPERLEDA I Identification and designation of galaxies Astronomy and Astrophysics 412 45 55 Bibcode 2003A amp A 412 45P doi 10 1051 0004 6361 20031411 Spitzer Image of Star Factory W51 Jet Propulsion Laboratory Chandra Photo Album W51 July 12 2017 Hardware Leaving the Solar System Where are they now DK Eyewitness Space Encyclopedia Urania s Mirror c 1825 Ian Ridpath s Antique Star Atlases Ianridpath com Retrieved 2012 10 21 Star Tales Lyra Ianridpath com Retrieved 2021 07 05 Raymond L Langsten Marc Jason Gilbert 1983 Research on Bengal proceedings of the 1981 Bengal Studies Conference Issue 34 of South Asia series Michigan State University Asian Studies Center Asian Studies Center Michigan State University 1983 and the appearance of the constellation Aquila that marks As Aquila was an eagle for the Greeks it is the Garuda kite to Hindus V Chandran 1993 Astronomy Quiz Book Pustak Mahal 1993 ISBN 978 81 223 0366 7 later spread to other cultures such as Arab Hindu Greek and Roman where the names were reinterpreted to suit the local cultures Hence Aquila Garuda Leo Singha Hydra Vasuki and other similarities in names Berio Alessandro 2014 The Celestial River Identifying the Ancient Egyptian Constellations PDF Sino Platonic Papers 253 7 Bibcode 2014SPP 253 1B Daressy Georges 1916 L Egypte celeste Bulletin de l Institut Francais d Archeologie Orientale 12 1 37 Boll Franz Sphaera neue griechische Texte und Untersuchungen zur Geschichte der Sternbilder Leipzig 1903 digi ub uni heidelberg de Retrieved 2016 10 21 Makemson 1941 p 218 Na Puke Wehewehe ʻŌlelo Hawaiʻi Makemson 1941 p 212 Makemson 1941 p 240 Makemson 1941 p 262 Makemson 1941 p 263 Makemson 1941 p 256 Makemson 1941 p 264 Makemson 1941 p 245 References nbsp This article incorporates text from a publication now in the public domain Chisholm Hugh ed 1911 Aquila Encyclopaedia Britannica Vol 2 11th ed Cambridge University Press p 249 Levy David H 2005 Deep Sky Objects Prometheus Books ISBN 1 59102 361 0 Makemson Maud Worcester 1941 The Morning Star Rises an account of Polynesian astronomy Yale University Press Bibcode 1941msra book M Ridpath Ian 2001 Stars and Planets Illustrated by Wil Tirion 3rd ed Princeton University Press ISBN 0 691 08913 2 Ridpath Ian 2007 Stars and Planets Guide Wil Tirion 4th ed Princeton University Press ISBN 978 0 691 13556 4 White Gavin 2008 Babylonian Star lore Solaria PubsExternal links edit nbsp Wikimedia Commons has media related to Aquila category Ian Ridpath s Star Tales Aquila The Deep Photographic Guide to the Constellations Aquila WIKISKY ORG Aquila constellation Warburg Institute Iconographic Database medieval and early modern images of Aquila The clickable Aquila Portals nbsp Astronomy nbsp Stars nbsp Spaceflight nbsp Outer space nbsp Solar System Retrieved from https en wikipedia org w index php title Aquila constellation amp oldid 1197127810, wikipedia, wiki, book, books, library,

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