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Historically, Aries has been depicted as a crouched, wingless ram with its head turned towards Taurus. Ptolemy asserted in his "Almagest" that Hipparchus depicted Alpha Arietis as the ram's muzzle, though Ptolemy did not include it in his constellation figure. Instead, it was listed as an "unformed star", and denoted as "the star over the head". John Flamsteed, in his "Atlas Coelestis", followed Ptolemy's description by mapping it above the figure's head. Flamsteed followed the general convention of maps by depicting Aries lying down. Astrologically, Aries has been associated with the head and its humors. It was strongly associated with Mars, both the planet and the god. It was considered to govern Western Europe and Syria and to indicate a strong temper in a person.
The First Point of Aries, the location of the vernal equinox, is named for the constellation. This is because the Sun crossed the celestial equator from south to north in Aries more than two millennia ago. Hipparchus defined it in 130 BC. as a point south of Gamma Arietis. Because of the precession of the equinoxes, the First Point of Aries has since moved into Pisces and will move into Aquarius by around 2600 AD. The Sun now appears in Aries from late April through mid-May, though the constellation is still associated with the beginning of spring.
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Medieval Muslim astronomers depicted Aries in various ways. Astronomers like al-Sufi saw the constellation as a ram, modelled on the precedent of Ptolemy. However, some Islamic celestial globes depicted Aries as a nondescript four-legged animal with what may be antlers instead of horns. Some early Bedouin observers saw a ram elsewhere in the sky; this constellation featured the Pleiades as the ram's tail. The generally accepted Arabic formation of Aries consisted of thirteen stars in a figure along with five "unformed" stars, four of which were over the animal's hindquarters and one of which was the disputed star over Aries's head. Al-Sufi's depiction differed from both other Arab astronomers' and Flamsteed's, in that his Aries was running and looking behind itself.
The obsolete constellations Apes, Vespa, Lilium, and Musca Borealis all centred on the same four stars, now known as 33, 35, 39, and 41 Arietis. In 1612, Petrus Plancius introduced Apes, a constellation representing a bee. In 1624, the same stars were used by Jakob Bartsch for Vespa, representing a wasp. In 1679, Augustin Royer used these stars for his constellation Lilium, representing the fleur-de-lis. None of these constellations became widely accepted. Johann Hevelius renamed the constellation "Musca" in 1690 in his "Firmamentum Sobiescianum". To differentiate it from Musca, the southern fly, it was later renamed Musca Borealis but it did not gain acceptance and its stars were ultimately officially reabsorbed into Aries.
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In 1922, the International Astronomical Union defined its recommended three-letter abbreviation, "Ari". The official boundaries of Aries were defined in 1930 by Eugène Delporte as a polygon of 12 segments. Its right ascension is between 1h 46.4m and 3h 29.4m and its declination is between 10.36° and 31.22° in the equatorial coordinate system.
In non-Western astronomy.
In traditional Chinese astronomy, stars from Aries were used in several constellations. The brightest stars—Alpha, Beta, and Gamma Arietis—formed a constellation called 'Lou',variously translated as "bond" or "lasso" also "sickle", which was associated with the ritual sacrifice of cattle. This name was shared by the 16th lunar mansion, the location of the full moon closest to the autumnal equinox. This constellation has also been associated with harvest-time as it could represent a woman carrying a basket of food on her head. 35, 39, and 41 Arietis were part of a constellation called "Wei" (胃), which represented a fat abdomen and was the namesake of the 17th lunar mansion, which represented granaries. Delta and Zeta Arietis were a part of the constellation "Tianyin" (天陰), thought to represent the Emperor's hunting partner. "Zuogeng" (左更), a constellation depicting a marsh and pond inspector, was composed of Mu, Nu, Omicron, Pi, and Sigma Arietis. He was accompanied by "Yeou-kang", a constellation depicting an official in charge of pasture distribution.
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In a similar system to the Chinese, the first lunar mansion in Hindu astronomy was called "Aswini", after the traditional names for Beta and Gamma Arietis, the Aswins. Because the Hindu new year began with the vernal equinox, the Rig Veda contains over 50 new-year's related hymns to the twins, making them some of the most prominent characters in the work. Aries itself was known as ""Aja" and "Mesha". In Hebrew astronomy Aries was named "Taleh""; it signified either Simeon or Gad, and generally symbolizes the "Lamb of the World". The neighboring Syrians named the constellation "Amru", and the bordering Turks named it "Kuzi". Half a world away, in the Marshall Islands, several stars from Aries were incorporated into a constellation depicting a porpoise, along with stars from Cassiopeia, Andromeda, and Triangulum. Alpha, Beta, and Gamma Arietis formed the head of the porpoise, while stars from Andromeda formed the body and the bright stars of Cassiopeia formed the tail. Other Polynesian peoples recognized Aries as a constellation. The Marquesas islanders called it "Na-pai-ka"; the Māori constellation "Pipiri" may correspond to modern Aries as well. In indigenous Peruvian astronomy, a constellation with most of the same stars as Aries existed. It was called the "Market Moon" and the "Kneeling Terrace", as a reminder of when to hold the annual harvest festival, Ayri Huay.
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Features.
Stars.
Bright stars.
Aries has three prominent stars forming an asterism, designated Alpha, Beta, and Gamma Arietis by Johann Bayer. Alpha (Hamal) and Beta (Sheratan) are commonly used for navigation. There is also one other star above the fourth magnitude, 41 Arietis (Bharani). α Arietis, called Hamal, is the brightest star in Aries. Its traditional name is derived from the Arabic word for "lamb" or "head of the ram" ("ras al-hamal"), which references Aries's mythological background. With a spectral class of K2 and a luminosity class of III, it is an orange giant with an apparent visual magnitude of 2.00, which lies 66 light-years from Earth. Hamal has a luminosity of and its absolute magnitude is −0.1.
β Arietis, also known as Sheratan, is a blue-white star with an apparent visual magnitude of 2.64. Its traditional name is derived from "sharatayn", the Arabic word for "the two signs", referring to both Beta and Gamma Arietis in their position as heralds of the vernal equinox. The two stars were known to the Bedouin as "qarna al-hamal", "horns of the ram". It is 59 light-years from Earth. It has a luminosity of and its absolute magnitude is 2.1. It is a spectroscopic binary star, one in which the companion star is only known through analysis of the spectra. The spectral class of the primary is A5. Hermann Carl Vogel determined that Sheratan was a spectroscopic binary in 1903; its orbit was determined by Hans Ludendorff in 1907. It has since been studied for its eccentric orbit.
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γ Arietis, with a common name of Mesarthim, is a binary star with two white-hued components, located in a rich field of magnitude 8–12 stars. Its traditional name has conflicting derivations. It may be derived from a corruption of "al-sharatan", the Arabic word meaning "pair" or a word for "fat ram". However, it may also come from the Sanskrit for "first star of Aries" or the Hebrew for "ministerial servants", both of which are unusual languages of origin for star names. Along with Beta Arietis, it was known to the Bedouin as "qarna al-hamal". The primary is of magnitude 4.59 and the secondary is of magnitude 4.68. The system is 164 light-years from Earth. The two components are separated by 7.8 arcseconds, and the system as a whole has an apparent magnitude of 3.9. The primary has a luminosity of and the secondary has a luminosity of ; the primary is an A-type star with an absolute magnitude of 0.2 and the secondary is a B9-type star with an absolute magnitude of 0.4. The angle between the two components is 1°. Mesarthim was discovered to be a double star by Robert Hooke in 1664, one of the earliest such telescopic discoveries. The primary, γ1 Arietis, is an Alpha² Canum Venaticorum variable star that has a range of 0.02 magnitudes and a period of 2.607 days. It is unusual because of its strong silicon emission lines.
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The constellation is home to several double stars, including Epsilon, Lambda, and Pi Arietis. ε Arietis is a binary star with two white components. The primary is of magnitude 5.2 and the secondary is of magnitude 5.5. The system is 290 light-years from Earth. Its overall magnitude is 4.63, and the primary has an absolute magnitude of 1.4. Its spectral class is A2. The two components are separated by 1.5 arcseconds. λ Arietis is a wide double star with a white-hued primary and a yellow-hued secondary. The primary is of magnitude 4.8 and the secondary is of magnitude 7.3. The primary is 129 light-years from Earth. It has an absolute magnitude of 1.7 and a spectral class of F0. The two components are separated by 36 arcseconds at an angle of 50°; the two stars are located 0.5° east of 7 Arietis. π Arietis is a close binary star with a blue-white primary and a white secondary. The primary is of magnitude 5.3 and the secondary is of magnitude 8.5. The primary is 776 light-years from Earth. The primary itself is a wide double star with a separation of 25.2 arcseconds; the tertiary has a magnitude of 10.8. The primary and secondary are separated by 3.2 arcseconds.
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Most of the other stars in Aries visible to the naked eye have magnitudes between 3 and 5. δ Ari, called Boteïn, is a star of magnitude 4.35, 170 light-years away. It has an absolute magnitude of −0.1 and a spectral class of K2. ζ Arietis is a star of magnitude 4.89, 263 light-years away. Its spectral class is A0 and its absolute magnitude is 0.0. 14 Arietis is a star of magnitude 4.98, 288 light-years away. Its spectral class is F2 and its absolute magnitude is 0.6. 39 Arietis (Lilii Borea) is a similar star of magnitude 4.51, 172 light-years away. Its spectral class is K1 and its absolute magnitude is 0.0. 35 Arietis is a dim star of magnitude 4.55, 343 light-years away. Its spectral class is B3 and its absolute magnitude is −1.7. 41 Arietis, known both as c Arietis and Nair al Butain, is a brighter star of magnitude 3.63, 165 light-years away. Its spectral class is B8 and it has a luminosity of . Its absolute magnitude is −0.2. 53 Arietis is a runaway star of magnitude 6.09, 815 light-years away. Its spectral class is B2. It was likely ejected from the Orion Nebula approximately five million years ago, possibly due to supernovae. Finally, Teegarden's Star is the closest star to Earth in Aries. It is a red dwarf of magnitude 15.14 and spectral class M6.5V. With a proper motion of 5.1 arcseconds per year, it is the 24th closest star to Earth overall.
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Variable stars.
Aries has its share of variable stars, including R and U Arietis, Mira-type variable stars, and T Arietis, a semi-regular variable star. R Arietis is a Mira variable star that ranges in magnitude from a minimum of 13.7 to a maximum of 7.4 with a period of 186.8 days. It is 4,080 light-years away. U Arietis is another Mira variable star that ranges in magnitude from a minimum of 15.2 to a maximum of 7.2 with a period of 371.1 days. T Arietis is a semiregular variable star that ranges in magnitude from a minimum of 11.3 to a maximum of 7.5 with a period of 317 days. It is 1,630 light-years away. One particularly interesting variable in Aries is SX Arietis, a rotating variable star considered to be the prototype of its class, helium variable stars. SX Arietis stars have very prominent emission lines of Helium I and Silicon III. They are normally main-sequence B0p—B9p stars, and their variations are not usually visible to the naked eye. Therefore, they are observed photometrically, usually having periods that fit in the course of one night. Similar to α2s, SX Arietis stars have periodic changes in their light and magnetic field, which correspond to the periodic rotation; they differ from the α2 Canum Venaticorum variables in their higher temperature. There are between 39 and 49 SX Arietis variable stars currently known; ten are noted as being "uncertain" in the General Catalog of Variable Stars.
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Deep sky objects.
NGC 772 is a spiral galaxy with an integrated magnitude of 10.3, located southeast of β Arietis and 15 arcminutes west of 15 Arietis. It is a relatively bright galaxy and shows obvious nebulosity and ellipticity in an amateur telescope. It is 7.2 by 4.2 arcminutes, meaning that its surface brightness, magnitude 13.6, is significantly lower than its integrated magnitude. NGC 772 is a class SA(s)b galaxy, which means that it is an unbarred spiral galaxy without a ring that possesses a somewhat prominent bulge and spiral arms that are wound somewhat tightly. The main arm, on the northwest side of the galaxy, is home to many star forming regions; this is due to previous gravitational interactions with other galaxies. NGC 772 has a small companion galaxy, NGC 770, that is about 113,000 light-years away from the larger galaxy. The two galaxies together are also classified as Arp 78 in the Arp peculiar galaxy catalog. NGC 772 has a diameter of 240,000 light-years and the system is 114 million light-years from Earth. Another spiral galaxy in Aries is NGC 673, a face-on class SAB(s)c galaxy. It is a weakly barred spiral galaxy with loosely wound arms. It has no ring and a faint bulge and is 2.5 by 1.9 arcminutes. It has two primary arms with fragments located farther from the core. 171,000 light-years in diameter, NGC 673 is 235 million light-years from Earth.
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NGC 678 and NGC 680 are a pair of galaxies in Aries that are only about 200,000 light-years apart. Part of the NGC 691 group of galaxies, both are at a distance of approximately 130 million light-years. NGC 678 is an edge-on spiral galaxy that is 4.5 by 0.8 arcminutes. NGC 680, an elliptical galaxy with an asymmetrical boundary, is the brighter of the two at magnitude 12.9; NGC 678 has a magnitude of 13.35. Both galaxies have bright cores, but NGC 678 is the larger galaxy at a diameter of 171,000 light-years; NGC 680 has a diameter of 72,000 light-years. NGC 678 is further distinguished by its prominent dust lane. NGC 691 itself is a spiral galaxy slightly inclined to our line of sight. It has multiple spiral arms and a bright core. Because it is so diffuse, it has a low surface brightness. It has a diameter of 126,000 light-years and is 124 million light-years away. NGC 877 is the brightest member of an 8-galaxy group that also includes NGC 870, NGC 871, and NGC 876, with a magnitude of 12.53. It is 2.4 by 1.8 arcminutes and is 178 million light-years away with a diameter of 124,000 light-years. Its companion is NGC 876, which is about 103,000 light-years from the core of NGC 877. They are interacting gravitationally, as they are connected by a faint stream of gas and dust. Arp 276 is a different pair of interacting galaxies in Aries, consisting of NGC 935 and IC 1801.
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NGC 821 is an E6 elliptical galaxy. It is unusual because it has hints of an early spiral structure, which is normally only found in lenticular and spiral galaxies. NGC 821 is 2.6 by 2.0 arcminutes and has a visual magnitude of 11.3. Its diameter is 61,000 light-years and it is 80 million light-years away. Another unusual galaxy in Aries is Segue 2, a dwarf and satellite galaxy of the Milky Way, recently discovered to be a potential relic of the epoch of reionization.
Meteor showers.
Aries is home to several meteor showers. The Daytime Arietid meteor shower is one of the strongest meteor showers that occurs during the day, lasting from 22 May to 2 July. It is an annual shower associated with the Marsden group of comets that peaks on 7 June with a maximum zenithal hourly rate of 54 meteors. Its parent body may be the asteroid Icarus. The meteors are sometimes visible before dawn, because the radiant is 32 degrees away from the Sun. They usually appear at a rate of 1–2 per hour as "earthgrazers", meteors that last several seconds and often begin at the horizon. Because most of the Daytime Arietids are not visible to the naked eye, they are observed in the radio spectrum. This is possible because of the ionized gas they leave in their wake. Other meteor showers radiate from Aries during the day; these include the Daytime Epsilon Arietids and the Northern and Southern Daytime May Arietids. The Jodrell Bank Observatory discovered the Daytime Arietids in 1947 when James Hey and G. S. Stewart adapted the World War II-era radar systems for meteor observations.
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The Delta Arietids are another meteor shower radiating from Aries. Peaking on 9 December with a low peak rate, the shower lasts from 8 December to 14 January, with the highest rates visible from 8 to 14 December. The average Delta Arietid meteor is very slow, with an average velocity of per second. However, this shower sometimes produces bright fireballs. This meteor shower has northern and southern components, both of which are likely associated with 1990 HA, a near-Earth asteroid.
The Autumn Arietids also radiate from Aries. The shower lasts from 7 September to 27 October and peaks on 9 October. Its peak rate is low. The Epsilon Arietids appear from 12 to 23 October. Other meteor showers radiating from Aries include the October Delta Arietids, Daytime Epsilon Arietids, Daytime May Arietids, Sigma Arietids, Nu Arietids, and Beta Arietids. The Sigma Arietids, a class IV meteor shower, are visible from 12 to 19 October, with a maximum zenithal hourly rate of less than two meteors per hour on 19 October.
Planetary systems.
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Aries contains several stars with extrasolar planets. HIP 14810, a G5 type star, is orbited by three giant planets (those more than ten times the mass of Earth). HD 12661, like HIP 14810, is a G-type main sequence star, slightly larger than the Sun, with two orbiting planets. One planet is 2.3 times the mass of Jupiter, and the other is 1.57 times the mass of Jupiter. HD 20367 is a G0 type star, approximately the size of the Sun, with one orbiting planet. The planet, discovered in 2002, has a mass 1.07 times that of Jupiter and orbits every 500 days. In 2019, scientists conducting the CARMENES survey at the Calar Alto Observatory announced evidence of two Earth-mass exoplanets orbiting Teegarden's star, located in Aries, within its habitable zone. The star is a small red dwarf with only around a tenth of the mass and radius of the Sun. It has a large radial velocity.
References.
Online sources.
"SIMBAD"
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Aquarius (constellation)
Aquarius is an equatorial constellation of the zodiac, between Capricornus and Pisces. Its name is Latin for "water-carrier" or "cup-carrier", and its old astronomical symbol is (♒︎), a representation of water. Aquarius is one of the oldest of the recognized constellations along the zodiac (the Sun's apparent path). It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
At apparent magnitude 2.9, Beta Aquarii is the brightest star in the constellation.
History and mythology.
Aquarius is identified as "The Great One" in the Babylonian star catalogues and represents the god Ea himself, who is commonly depicted holding an overflowing vase. The Babylonian star-figure appears on entitlement stones and cylinder seals from the second millennium. It contained the winter solstice in the Early Bronze Age. In Old Babylonian astronomy, Ea was the ruler of the southernmost quarter of the Sun's path, the "Way of Ea", corresponding to the period of 45 days on either side of winter solstice. Aquarius was also associated with the destructive floods that the Babylonians regularly experienced, and thus was negatively connoted. In Ancient Egypt astronomy, Aquarius was associated with the annual flood of the Nile; the banks were said to flood when Aquarius put his jar into the river, beginning spring.
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In the Greek tradition, the constellation came to be represented simply as a single vase from which a stream poured down to Piscis Austrinus. The name in the Hindu zodiac is likewise "kumbha" "water-pitcher".
In Greek mythology, Aquarius is sometimes associated with Deucalion, the son of Prometheus who built a ship with his wife Pyrrha to survive an imminent flood. They sailed for nine days before washing ashore on Mount Parnassus. Aquarius is also sometimes identified with beautiful Ganymede, a youth in Greek mythology and the son of Trojan king Tros, who was taken to Mount Olympus by Zeus to act as cup-carrier to the gods. Neighboring Aquila represents the eagle, under Zeus' command, that snatched the young boy; some versions of the myth indicate that the eagle was in fact Zeus transformed. One tradition, stated that he was carried off by Eos. Yet another figure associated with the water bearer is Cecrops I, a king of Athens who sacrificed water instead of wine to the gods.
Depictions.
In the first century, Ptolemy's "Almagest" established the common Western depiction of Aquarius. His water jar, an asterism itself, consists of Gamma, Pi, Eta, and Zeta Aquarii; it pours water in a stream of more than 20 stars terminating with Fomalhaut, now assigned solely to Piscis Austrinus. The water bearer's head is represented by 5th magnitude 25 Aquarii while his left shoulder is Beta Aquarii; his right shoulder and forearm are represented by Alpha and Gamma Aquarii respectively.
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In Eastern astronomy.
In Chinese astronomy, the stream of water flowing from the Water Jar was depicted as the "Army of Yu-Lin" ("Yu-lim-kiun" or "Yulinjun", Hanzi: 羽林君). The name "Yu-lin" means "feathers and forests", referring to the numerous light-footed soldiers from the northern reaches of the empire represented by these faint stars. The constellation's stars were the most numerous of any Chinese constellation, numbering 45, the majority of which were located in modern Aquarius. The celestial army was protected by the wall "Leibizhen" (垒壁阵), which counted Iota, Lambda, Phi, and Sigma Aquarii among its 12 stars. 88, 89, and 98 Aquarii represent "Fou-youe", the axes used as weapons and for hostage executions. Also in Aquarius is "Loui-pi-tchin", the ramparts that stretch from 29 and 27 Piscium and 33 and 30 Aquarii through Phi, Lambda, Sigma, and Iota Aquarii to Delta, Gamma, Kappa, and Epsilon Capricorni. Similarly in the Hindu calendar Aquarius is depicted as Kumbha, and Kumbha, which means a pot or a jug, stands for the zodiac sign of Aquarius.
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Near the border with Cetus, the axe "Fuyue" was represented by three stars; its position is disputed and may have instead been located in Sculptor. "Tienliecheng" also has a disputed position; the 13-star castle replete with ramparts may have possessed Nu and Xi Aquarii but may instead have been located south in Piscis Austrinus. The Water Jar asterism was seen to the ancient Chinese as the tomb, "Fenmu". Nearby, the emperors' mausoleum "Xiuliang" stood, demarcated by Kappa Aquarii and three other collinear stars. "Ku" ("crying") and "Qi" ("weeping"), each composed of two stars, were located in the same region.
Three of the Chinese lunar mansions shared their name with constellations. "Nu", also the name for the 10th lunar mansion, was a handmaiden represented by Epsilon, Mu, 3, and 4 Aquarii. The 11th lunar mansion shared its name with the constellation "Xu" ("emptiness"), formed by Beta Aquarii and Alpha Equulei; it represented a bleak place associated with death and funerals. "Wei", the rooftop and 12th lunar mansion, was a V-shaped constellation formed by Alpha Aquarii, Theta Pegasi, and Epsilon Pegasi; it shared its name with two other Chinese constellations, in modern-day Scorpius and Aries.
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Features.
Stars.
Despite both its prominent position on the zodiac and its large size, Aquarius has no particularly bright stars, its four brightest stars being less bright than (The Apparent Magnitude scale is reverse logarithmic, with increasingly bright objects having lower and lower (more negative) magnitudes.) Recent research has shown that there are several stars lying within its borders that possess planetary systems.
The two brightest stars, α Aquarii and β Aquarii, are luminous yellow supergiants, of spectral types G0Ib and G2Ib respectively, that were once hot blue-white B-class main sequence stars 5 to 9 times as massive as the Sun. The two are also moving through space perpendicular to the plane of the Milky Way. β Aquarii is the brightest star in Aquarius with apparent – only slightly brighter than α Aquarii. It also has the proper name of Sadalsuud. Having cooled and swollen to around 50 times the Sun's diameter, it is around 2200 times as luminous as the Sun. It is around 6.4 times as massive as the Sun and around 56 million years old. Sadalsuud is from Earth. α Aquarii, also known as "Sadalmelik", has apparent It is distant from Earth, and is around 6.5 times as massive as the Sun, and 3000 times as luminous. It is 53 million years old.
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γ Aquarii, also called "Sadachbia", is a white main sequence star of spectral type star of spectral type A0V that is between 158 and 315 million years old and is around 2.5 times the Sun's mass (), and double its radius. Its magnitude is 3.85, and it is away, hence its luminosity is . The name "Sadachbia" comes from the Arabic for "lucky stars of the tents", "sa'd al-akhbiya".
δ Aquarii, also known as "Skat" or "Scheat" is a blue-white spectral type A2 star with apparent magnitude 3.27 and luminosity .
ε Aquarii, also known as "Albali", is a blue-white spectral type A1 star with apparent magnitude 3.77, absolute magnitude 1.2, and a luminosity of .
ζ Aquarii is a spectral type F2 double star; both stars are white. In combination, they appear to be magnitude 3.6 with luminosity . The primary has magnitude 4.53 and the secondary's magnitude is 4.31, but both have absolute The system's orbital period is 760 years; currently the two components are moving farther apart.
θ Aquarii, sometimes called "Ancha", is spectral type G8 with apparent magnitude 4.16 and an absolute
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κ Aquarii, also called "Situla", has an apparent
λ Aquarii, also called "Hudoor" or "Ekchusis", is spectral type M2 with magnitude 3.74 and luminosity .
ξ Aquarii, also called "Bunda", is spectral type A7 with an apparent magnitude 4.69 and an absolute
π Aquarii, also called "Seat", is spectral type B0 with apparent magnitude 4.66 and absolute
Planetary systems.
Twelve exoplanet systems have been found in Aquarius as of 2013. Gliese 876, one of the nearest stars to Earth at a distance of 15 light-years, was the first red dwarf star to be found to possess a planetary system. It is orbited by four planets, including one terrestrial planet 6.6 times the mass of Earth. The planets vary in orbital period from 2 days to 124 days. 91 Aquarii is an orange giant star orbited by one planet, 91 Aquarii b. The planet's mass is 2.9 times the mass of Jupiter, and its orbital period is 182 days. Gliese 849 is a red dwarf star orbited by the first known long-period Jupiter-like planet, Gliese 849 b. The planet's mass is 0.99 times that of Jupiter and its orbital period is 1,852 days.
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There are also less-prominent systems in Aquarius. WASP-6, a type G8 star of magnitude 12.4, is host to one exoplanet, WASP-6 b. The star is 307 parsecs from Earth and has a mass of 0.888 solar masses and a radius of 0.87 solar radii. WASP-6 b was discovered in 2008 by the transit method. It orbits its parent star every 3.36 days at a distance of 0.042 astronomical units (AU). It is 0.503 Jupiter masses but has a proportionally larger radius of 1.224 Jupiter radii. HD 206610, a K0 star located 194 parsecs from Earth, is host to one planet, HD 206610 b. The host star is larger than the Sun; more massive at 1.56 solar masses and larger at 6.1 solar radii. The planet was discovered by the radial velocity method in 2010 and has a mass of 2.2 Jupiter masses. It orbits every 610 days at a distance of 1.68 AU. Much closer to its sun is WASP-47 b, which orbits every 4.15 days only 0.052 AU from its sun, yellow dwarf (G9V) WASP-47. WASP-47 is close in size to the Sun, having a radius of 1.15 solar radii and a mass even closer at 1.08 solar masses. WASP-47 b was discovered in 2011 by the transit method, like WASP-6 b. It is slightly larger than Jupiter with a mass of 1.14 Jupiter masses and a radius of 1.15 Jupiter masses.
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There are several more single-planet systems in Aquarius. HD 210277, a magnitude 6.63 yellow star located 21.29 parsecs from Earth, is host to one known planet: HD 210277 b. The 1.23 Jupiter mass planet orbits at nearly the same distance as Earth orbits the Sun1.1 AU, though its orbital period is significantly longer at around 442 days. HD 210277 b was discovered earlier than most of the other planets in Aquarius, detected by the radial velocity method in 1998. The star it orbits resembles the Sun beyond their similar spectral class; it has a radius of 1.1 solar radii and a mass of 1.09 solar masses. HD 212771 b, a larger planet at 2.3 Jupiter masses, orbits host star HD 212771 at a distance of 1.22 AU. The star itself, barely below the threshold of naked-eye visibility at magnitude 7.6, is a G8IV (yellow subgiant) star located 131 parsecs from Earth. Though it has a similar mass to the Sun1.15 solar massesit is significantly less dense with its radius of 5 solar radii. Its lone planet was discovered in 2010 by the radial velocity method, like several other exoplanets in the constellation.
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As of 2013, there were only two known multiple-planet systems within the bounds of Aquarius: the Gliese 876 and HD 215152 systems. The former is quite prominent; the latter has only two planets and has a host star farther away at 21.5 parsecs. The HD 215152 system consists of the planets HD 215152 b and HD 215152 c orbiting their K0-type, magnitude 8.13 sun. Both discovered in 2011 by the radial velocity method, the two tiny planets orbit very close to their host star. HD 215152 c is the larger at 0.0097 Jupiter masses (still significantly larger than the Earth, which weighs in at 0.00315 Jupiter masses); its smaller sibling is barely smaller at 0.0087 Jupiter masses. The error in the mass measurements (0.0032 and respectively) is large enough to make this discrepancy statistically insignificant. HD 215152 c also orbits further from the star than HD 215152 b, 0.0852 AU compared to 0.0652.
On 23 February 2017, NASA announced that ultracool dwarf star TRAPPIST-1 in Aquarius has seven Earth-like rocky planets. Of these, as many as four may lie within the system's habitable zone, and may have liquid water on their surfaces. The discovery of the TRAPPIST-1 system is seen by astronomers as a significant step toward finding life beyond Earth.
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Deep sky objects.
Because of its position away from the galactic plane, the majority of deep-sky objects in Aquarius are galaxies, globular clusters, and planetary nebulae. Aquarius contains three deep sky objects that are in the Messier catalog: the globular clusters Messier 2, Messier 72, and the asterism Messier 73. While M73 was originally catalogued as a sparsely populated open cluster, modern analysis indicates the 6 main stars are not close enough together to fit this definition, reclassifying M73 as an asterism. Two well-known planetary nebulae are also located in Aquarius: the Saturn Nebula (NGC 7009), to the southeast of μ Aquarii; and the famous Helix Nebula (NGC 7293), southwest of δ Aquarii.
M2, also catalogued as NGC 7089, is a rich globular cluster located approximately 37,000 light-years from Earth. At magnitude 6.5, it is viewable in small-aperture instruments, but a 100 mm aperture telescope is needed to resolve any stars. M72, also catalogued as NGC 6981, is a small 9th magnitude globular cluster located approximately 56,000 light-years from Earth. M73, also catalogued as NGC 6994, is an open cluster with highly disputed status.
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Aquarius is also home to several planetary nebulae. NGC 7009, also known as the Saturn Nebula, is an 8th magnitude planetary nebula located 3,000 light-years from Earth. It was given its moniker by the 19th century astronomer Lord Rosse for its resemblance to the planet Saturn in a telescope; it has faint protrusions on either side that resemble Saturn's rings. It appears blue-green in a telescope and has a central star of magnitude 11.3. Compared to the Helix Nebula, another planetary nebula in Aquarius, it is quite small. NGC 7293, also known as the Helix Nebula, is the closest planetary nebula to Earth at a distance of 650 light-years. It covers 0.25 square degrees, making it also the largest planetary nebula as seen from Earth. However, because it is so large, it is only viewable as a very faint object, though it has a fairly high integrated magnitude of 6.0.
One of the visible galaxies in Aquarius is NGC 7727, of particular interest for amateur astronomers who wish to discover or observe supernovae. A spiral galaxy (type S), it has an integrated magnitude of 10.7 and is 3 by 3 arcseconds. NGC 7252 is a tangle of stars resulting from the collision of two large galaxies and is known as the Atoms-for-Peace galaxy because of its resemblance to a cartoon atom.
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Meteor showers.
There are three major meteor showers with radiants in Aquarius: the Eta Aquariids, the Delta Aquariids, and the Iota Aquariids.
The Eta Aquariids are the strongest meteor shower radiating from Aquarius. It peaks between 5 and 6 May with a rate of approximately 35 meteors per hour. Originally discovered by Chinese astronomers in 401, Eta Aquariids can be seen coming from the Water Jar beginning on 21 April and as late as 12 May. The parent body of the shower is Halley's Comet, a periodic comet. Fireballs are common shortly after the peak, approximately between 9 May and 11 May. The normal meteors appear to have yellow trails.
The Delta Aquariids is a double radiant meteor shower that peaks first on 29 July and second on 6 August. The first radiant is located in the south of the constellation, while the second radiant is located in the northern circlet of Pisces asterism. The southern radiant's peak rate is about 20 meteors per hour, while the northern radiant's peak rate is about 10 meteors per hour.
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The Iota Aquariids is a fairly weak meteor shower that peaks on 6 August, with a rate of approximately 8 meteors per hour.
Astrology.
, the Sun appears in the constellation Aquarius from 16 February to 12 March. In tropical astrology, the Sun is considered to be in the sign Aquarius from 20 January to 19 February, and in sidereal astrology, from 15 February to 14 March.
Aquarius is also associated with the Age of Aquarius, a concept popular in 1960s counterculture and Medieval Alchemy. The date of the start of The Age of Aquarius is a topic of much debate.
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Anime
is hand-drawn and computer-generated animation originating from Japan. Outside Japan and in English, "anime" refers specifically to animation produced in Japan. However, , in Japan and in Japanese, describes all animated works, regardless of style or origin. Many works of animation with a similar style to Japanese animation are also produced outside Japan. Video games sometimes also feature themes and art styles that are sometimes labelled as anime.
The earliest commercial Japanese animation dates to 1917. A characteristic art style emerged in the 1960s with the works of cartoonist Osamu Tezuka and spread in the following decades, developing a large domestic audience. Anime is distributed theatrically, through television broadcasts, directly to home media, and over the Internet. In addition to original works, anime are often adaptations of Japanese comics (manga), light novels, or video games. It is classified into numerous genres targeting various broad and niche audiences.
Anime is a diverse medium with distinctive production methods that have adapted in response to emergent technologies. It combines graphic art, characterization, cinematography, and other forms of imaginative and individualistic techniques. Compared to Western animation, anime production generally focuses less on movement, and more on the detail of settings and use of "camera effects", such as panning, zooming, and angle shots. Diverse art styles are used, and character proportions and features can be quite varied, with a common characteristic feature being large and emotive eyes.
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The anime industry consists of over 430 production companies, including major studios such as Studio Ghibli, Kyoto Animation, Sunrise, Bones, Ufotable, MAPPA, Wit Studio, CoMix Wave Films, Madhouse, Inc., TMS Entertainment, Pierrot, Production I.G, Nippon Animation and Toei Animation. Since the 1980s, the medium has also seen widespread international success with the rise of foreign dubbed, subtitled programming, and since the 2010s due to the rise of streaming services and a widening demographic embrace of anime culture, both within Japan and worldwide. Japanese animation accounted for 60% of the world's animated television shows.
Etymology.
As a type of animation, anime is an art form that comprises many genres found in other mediums; it is sometimes mistakenly classified as a genre itself. In Japanese, the term "anime" is used to refer to all animated works, regardless of style or origin. English-language dictionaries typically define "anime" () as "a style of Japanese animation" or as "a style of animation originating in Japan". Other definitions are based on origin, making production in Japan a requisite for a work to be considered "anime".
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The etymology of the term "anime" is disputed. The English word "animation" is written in Japanese "katakana" as () and as (, ) in its shortened form. Some sources claim that the term is derived from the French term for animation ("cartoon", literally 'animated drawing'), but others believe this to be a myth derived from the popularity of anime in France in the late 1970s and 1980s.
In English, "anime"—when used as a common noun—normally functions as a mass noun. (For example: "Do you watch anime?" or "How much anime have you watched?") As with a few other Japanese words, such as "saké" and "Pokémon", English texts sometimes spell "anime" as "animé" (as in French), with an acute accent over the final "e", to cue the reader to pronounce the letter, not to leave it silent as English orthography may suggest. Prior to the widespread use of "anime", the term "Japanimation", a portmanteau of Japan and animation, was prevalent throughout the 1970s and 1980s. In the mid-1980s, the term "anime" began to supplant "Japanimation"; in general, the latter term now only appears in period works where it is used to distinguish and identify Japanese animation.
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History.
Precursors.
and shadow plays ("kage-e") are considered precursors of Japanese animation. was common in the eleventh century. Traveling storytellers narrated legends and anecdotes while the was unrolled from the right to left in chronological order, as a moving panorama. "Kage-e" was popular during the Edo period and originated from the shadow plays of China. Magic lanterns from the Netherlands were also popular in the eighteenth century. The paper play called "kamishibai" surged in the twelfth century and remained popular in the street theater until the 1930s. Puppets of the Bunraku theater and "ukiyo-e" prints are considered ancestors of characters of most Japanese animation. Finally, manga were a heavy inspiration for anime. Cartoonists Kitzawa Rakuten and Okamoto Ippei used film elements in their strips.
Pioneers.
Animation in Japan began in the early 20th century, when filmmakers started to experiment with techniques pioneered in France, Germany, the United States, and Russia. A claim for the earliest Japanese animation is "Katsudō Shashin" (), a private work by an unknown creator. In 1917, the first professional and publicly displayed works began to appear; animators such as Ōten Shimokawa, Seitarō Kitayama, and Jun'ichi Kōuchi (considered the "fathers of anime") produced numerous films, the oldest surviving of which is Kōuchi's "Namakura Gatana". Many early works were lost with the destruction of Shimokawa's warehouse in the 1923 Great Kantō earthquake.
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By the mid-1930s, animation was well-established in Japan as an alternative format to the live-action industry. It suffered competition from foreign producers, such as Disney, and many animators, including Noburō Ōfuji and Yasuji Murata, continued to work with cheaper cutout animation rather than cel animation. Other creators, including Kenzō Masaoka and Mitsuyo Seo, nevertheless made great strides in technique, benefiting from the patronage of the government, which employed animators to produce educational shorts and propaganda. In 1940, the government dissolved several artists' organizations to form the The first talkie anime was "Chikara to Onna no Yo no Naka" (1933), a short film produced by Masaoka. The first feature-length anime film was "" (1945), produced by Seo with a sponsorship from the Imperial Japanese Navy. The 1950s saw a proliferation of short, animated advertisements created for television.
Modern era.
In the 1960s, manga artist and animator Osamu Tezuka adapted and simplified Disney animation techniques to reduce costs and limit frame counts in his productions. Originally intended as temporary measures to allow him to produce material on a tight schedule with inexperienced staff, many of his limited animation practices came to define the medium's style. "Three Tales" (1960) was the first anime film broadcast on television; the first anime television series was "Instant History" (1961–64). An early and influential success was "Astro Boy" (1963–66), a television series directed by Tezuka based on his manga of the same name. Many animators at Tezuka's Mushi Production later established major anime studios (including Madhouse, Sunrise, and Pierrot).
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The 1970s saw growth in the popularity of manga, many of which were later animated. Tezuka's work—and that of other pioneers in the field—inspired characteristics and genres that remain fundamental elements of anime today. The giant robot genre (also known as "mecha"), for instance, took shape under Tezuka, developed into the super robot genre under Go Nagai and others, and was revolutionized at the end of the decade by Yoshiyuki Tomino, who developed the real robot genre. Robot anime series such as "Gundam" and "Super Dimension Fortress Macross" became instant classics in the 1980s, and the genre remained one of the most popular in the following decades. The bubble economy of the 1980s spurred a new era of high-budget and experimental anime films, including "Nausicaä of the Valley of the Wind" (1984), "" (1987), and "Akira" (1988).
"Neon Genesis Evangelion" (1995), a television series produced by Gainax and directed by Hideaki Anno, began another era of experimental anime titles, such as "Ghost in the Shell" (1995) and "Cowboy Bebop" (1998). In the 1990s, anime also began attracting greater interest in Western countries; major international successes include "Sailor Moon" and "Dragon Ball Z", both of which were dubbed into more than a dozen languages worldwide. In 2003, "Spirited Away", a Studio Ghibli feature film directed by Hayao Miyazaki, won the Academy Award for Best Animated Feature at the 75th Academy Awards. It later became the highest-grossing anime film, earning more than $355 million. Since the 2000s, an increased number of anime works have been adaptations of light novels and visual novels; successful examples include "The Melancholy of Haruhi Suzumiya" and "Fate/stay night" (both 2006). "" became the highest-grossing Japanese film and one of the world's highest-grossing films of 2020. It also became the fastest grossing film in Japanese cinema, because in 10 days it made 10 billion yen ($95.3m; £72m). It beat the previous record of "Spirited Away" which took 25 days.
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In 2021, the anime adaptations of "Jujutsu Kaisen", "" and "Tokyo Revengers" were among the top 10 most discussed TV shows worldwide on Twitter. In 2022, "Attack on Titan" won the award of "Most In-Demand TV Series in the World 2021" in the Global TV Demand Awards. "Attack on Titan" became the first ever non-English language series to earn the title of World's Most In-Demand TV Show, previously held by only "The Walking Dead" and "Game of Thrones". In 2024, "Jujutsu Kaisen" broke the Guinness World Record for the "Most in-demand animated TV show" with a global demand rating 71.2 times than that of the average TV show, previously held by "Attack on Titan".
Attributes.
Anime differs from other forms of animation by its art styles, methods of animation, its production, and its process. Visually, anime works exhibit a wide variety of art styles, differing between creators, artists, and studios. While no single art style predominates anime as a whole, they do share some similar attributes in terms of animation technique and character design.
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Anime is fundamentally characterized by the use of limited animation, flat expression, the suspension of time, its thematic range, the presence of historical figures, its complex narrative line and, above all, a peculiar drawing style, with characters characterized by large and oval eyes, with very defined lines, bright colors and reduced movement of the lips.
Technique.
Modern anime follows a typical animation production process, involving storyboarding, voice acting, character design, and cel production. Since the 1990s, animators have increasingly used computer animation to improve the efficiency of the production process. Early anime works were experimental, and consisted of images drawn on blackboards, stop motion animation of paper cutouts, and silhouette animation. Cel animation grew in popularity until it came to dominate the medium. In the 21st century, the use of other animation techniques is mostly limited to independent short films, including the stop motion puppet animation work produced by Tadahito Mochinaga, Kihachirō Kawamoto and Tomoyasu Murata. Computers were integrated into the animation process in the 1990s, with works such as "Ghost in the Shell" and "Princess Mononoke" mixing cel animation with computer-generated images. Fuji Film, a major cel production company, announced it would stop cel production, producing an industry panic to procure cel imports and hastening the switch to digital processes.
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Prior to the digital era, anime was produced with traditional animation methods using a pose to pose approach. The majority of mainstream anime uses fewer expressive key frames and more in-between animation.
Japanese animation studios were pioneers of many limited animation techniques, and have given anime a distinct set of conventions. Unlike Disney animation, where the emphasis is on the movement, anime emphasizes the art quality and let limited animation techniques make up for the lack of time spent on movement. Such techniques are often used not only to meet deadlines but also as artistic devices. Anime scenes place emphasis on achieving three-dimensional views, and backgrounds are instrumental in creating the atmosphere of the work. The backgrounds are not always invented and are occasionally based on real locations, as exemplified in "Howl's Moving Castle" and "The Melancholy of Haruhi Suzumiya". Oppliger stated that anime is one of the rare mediums where putting together an all-star cast usually comes out looking "tremendously impressive".
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The cinematic effects of anime differentiates itself from the stage plays found in American animation. Anime is cinematically shot as if by camera, including panning, zooming, distance and angle shots to more complex dynamic shots that would be difficult to produce in reality. In anime, the animation is produced before the voice acting, contrary to American animation which does the voice acting first.
Characters.
The body proportions of human anime characters tend to accurately reflect the proportions of the human body in reality. The height of the head is considered by the artist as the base unit of proportion. Head to height ratios vary drastically by art style, with most anime characters falling between 5 and 8 heads tall. Anime artists occasionally make deliberate modifications to body proportions to produce chibi characters that feature a disproportionately small body compared to the head; many chibi characters are two to four heads tall. Some anime works like "Crayon Shin-chan" completely disregard these proportions, in such a way that they resemble caricatured Western cartoons.
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A common anime character design convention is exaggerated eye size. The animation of characters with large eyes in anime can be traced back to Osamu Tezuka, who was deeply influenced by such early animation characters as Betty Boop, who was drawn with disproportionately large eyes. Tezuka is a central figure in anime and manga history, whose iconic art style and character designs allowed for the entire range of human emotions to be depicted solely through the eyes. The artist adds variable color shading to the eyes and particularly to the cornea to give them greater depth. Generally, a mixture of a light shade, the tone color, and a dark shade is used. However, not all anime characters have large eyes. For example, the works of Hayao Miyazaki are known for having realistically proportioned eyes, as well as realistic hair colors on their characters.
Hair in anime is often unnaturally lively and colorful or uniquely styled. The movement of hair in anime is exaggerated and "hair actions" is used to emphasize the action and emotions of characters for added visual effect. Gilles Poitras traces hairstyle color to cover illustrations on manga, where eye-catching artwork and colorful tones are attractive for children's manga. Some anime will depict non-Japanese characters with specific ethnic features, such as a pronounced nose and jutting jaw for European characters. In other cases, anime feature characters whose race or nationality is not always defined, and this is often a deliberate decision, such as in the "Pokémon" animated series.
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Anime and manga artists often draw from a common canon of iconic facial expression illustrations to denote particular moods and thoughts. These techniques are often different in form than their counterparts in Western animation, and they include a fixed iconography that is used as shorthand for certain emotions and moods. For example, a male character may develop a nosebleed when aroused. A variety of visual symbols are employed, including sweat drops to depict nervousness, visible blushing for embarrassment, or glowing eyes for an intense glare. Another recurring sight gag is the use of chibi (deformed, simplified character designs) figures to comedically punctuate emotions like confusion or embarrassment.
Music.
The opening and credits sequences of most anime television series are accompanied by J-pop or J-rock songs, often by reputed bands—as written with the series in mind—but are also aimed at the general music market, therefore they often allude only vaguely or not at all, to the thematic settings or plot of the series. Also, they are often used as incidental music ("insert songs") in an episode, in order to highlight particularly important scenes.
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Future funk, a musical microgenre that evolved in the early 2010s from Vaporwave with a French house Euro disco influence, heavily uses anime visuals and samples along with Japanese City pop to build an aesthetic.
Since the 2020s anime songs have experienced a rapid growth in global online popularity due to their widened availability on music streaming services like Spotify and promotion by fans and artists on social media. In 2023, the opening theme "Idol" by Yoasobi of the anime series "Oshi no Ko" topped the Billboard Global 200 Excl. U.S. charts with 45.7 million streams and 24,000 copies sold outside the U.S. "Idol" has become the first Japanese song and anime song to top the Billboard Global chart as well as taking the first spot on the Apple Music's Top 100: Global chart.
Genres.
Anime are often classified by target demographic, including , , , , and a diverse range of genres targeting an adult audience. Shōjo and shōnen anime sometimes contain elements popular with children of all genders in an attempt to gain crossover appeal. Adult anime may feature a slower pace or greater plot complexity that younger audiences may typically find unappealing, as well as adult themes and situations. A subset of adult anime works featuring pornographic elements are labeled "R18" in Japan, and are internationally known as "hentai" (originating from ). By contrast, some anime subgenres incorporate "ecchi", sexual themes or undertones without depictions of sexual intercourse, as typified in the comedic or harem genres; due to its popularity among adolescent and adult anime enthusiasts, the inclusion of such elements is considered a form of fan service. Some genres explore homosexual romances, such as "yaoi" (male homosexuality) and "yuri" (female homosexuality). While often used in a pornographic context, the terms "yaoi" and "yuri" can also be used broadly in a wider context to describe or focus on the themes or the development of the relationships themselves.
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Anime's genre classification differs from other types of animation and does not lend itself to simple classification. Gilles Poitras compared the labeling of "Gundam 0080" and its complex depiction of war as a "giant robot" anime akin to simply labeling "War and Peace" a "war novel". Science fiction is a major anime genre and includes important historical works like Tezuka's "Astro Boy" and Yokoyama's "Tetsujin 28-go". A major subgenre of science fiction is mecha, with the "Gundam" metaseries being iconic. The diverse fantasy genre includes works based on Asian and Western traditions and folklore; examples include the Japanese feudal fairytale "InuYasha", and the depiction of Scandinavian goddesses who move to Japan to maintain a computer called Yggdrasil in "Ah! My Goddess". Genre crossing in anime is also prevalent, such as the blend of fantasy and comedy in "Dragon Half", and the incorporation of slapstick humor in the crime anime film "Castle of Cagliostro". Other subgenres found in anime include magical girl, harem, sports, martial arts, literary adaptations, medievalism, and war.
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Formats.
Early anime works were made for theatrical viewing, and required played musical components before sound and vocal components were added to the production. In 1958, Nippon Television aired "Mogura no Abanchūru" ("Mole's Adventure"), both the first televised and first color anime to debut. It was not until the 1960s when the first televised series were broadcast and it has remained a popular medium since. Works released in a direct-to-video format are called "original video animation" (OVA) or "original animation video" (OAV); and are typically not released theatrically or televised prior to home media release. The emergence of the Internet has led some animators to distribute works online in a format called "original net animation" (ONA).
The home distribution of anime releases was popularized in the 1980s with the VHS and LaserDisc formats. The VHS NTSC video format used in both Japan and the United States is credited with aiding the rising popularity of anime in the 1990s. The LaserDisc and VHS formats were transcended by the DVD format which offered the unique advantages; including multiple subtitling and dubbing tracks on the same disc. The DVD format also has its drawbacks in its usage of region coding; adopted by the industry to solve licensing, piracy and export problems and restricted region indicated on the DVD player. The Video CD (VCD) format was popular in Hong Kong and Taiwan, but became only a minor format in the United States that was closely associated with bootleg copies.
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A key characteristic of many anime television shows is serialization, where a continuous story arc stretches over multiple episodes or seasons. Traditional American television had an episodic format, with each episode typically consisting of a self-contained story. In contrast, anime shows such as "Dragon Ball Z" had a serialization format, where continuous story arcs stretch over multiple episodes or seasons, which distinguished them from traditional American television shows; serialization has since also become a common characteristic of American streaming television shows during the "Peak TV" era.
Industry.
The animation industry consists of more than 430 production companies with some of the major studios including Toei Animation, Gainax, Madhouse, Gonzo, Sunrise, Bones, TMS Entertainment, Nippon Animation, P.A.Works, Studio Pierrot, Production I.G, Ufotable and Studio Ghibli. Many of the studios are organized into a trade association, The Association of Japanese Animations. There is also a labor union for workers in the industry, the Japanese Animation Creators Association.
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Many of the studios are organized into a trade association, The Association of Japanese Animations. There is also a labor union for workers in the industry, the Japanese Animation Creators Association. Studios will often work together to produce more complex and costly projects, as done with Studio Ghibli's "Spirited Away". An anime episode can cost between US$100,000 and US$300,000 to produce. In 2001, animation accounted for 7% of the Japanese film market, above the 4.6% market share for live-action works. The popularity and success of anime is seen through the profitability of the DVD market, contributing nearly 70% of total sales. According to a 2016 article on "Nikkei Asian Review", Japanese television stations have bought over worth of anime from production companies "over the past few years", compared with under from overseas. There has been a rise in sales of shows to television stations in Japan, caused by late night anime with adults as the target demographic.
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Anime has to be licensed by companies in other countries in order to be legally released. While anime has been licensed by its Japanese owners for use outside Japan since at least the 1960s, the practice became well-established in the United States in the late 1970s to early 1980s, when such TV series as "Gatchaman" and "Captain Harlock" were licensed from their Japanese parent companies for distribution in the US market. The trend towards American distribution of anime continued into the 1980s with the licensing of titles such as "Voltron" and the 'creation' of new series such as "Robotech" through the use of source material from several original series.
In the early 1990s, several companies began to experiment with the licensing of less child-oriented material. Some, such as A.D. Vision, and Central Park Media and its imprints, achieved fairly substantial commercial success and went on to become major players in the now very lucrative American anime market. Others, such as AnimEigo, achieved limited success. Many companies created directly by Japanese parent companies did not do as well, most releasing only one or two titles before completing their American operations.
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Licenses are expensive, often hundreds of thousands of dollars for one series and tens of thousands for one movie. The prices vary widely; for example, "" cost only $91,000 to license while "Kurau Phantom Memory" cost $960,000. Simulcast Internet streaming rights can be cheaper, with prices around $1,000–2,000 an episode, but can also be more expensive, with some series costing more than per episode.
The anime market for the United States was worth approximately $2.74 billion in 2009. Dubbed animation began airing in the United States in 2000 on networks like The WB and Cartoon Network's Adult Swim. In 2005, this resulted in five of the top ten anime titles having previously aired on Cartoon Network. As a part of localization, some editing of cultural references may occur to better follow the references of the non-Japanese culture. The cost of English localization averages US$10,000 per episode.
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Since the 2010s, anime has become a global multibillion industry setting a sales record in 2017 of ¥2.15 trillion ($19.8 billion), driven largely by demand from overseas audiences. In 2019, Japan's anime industry was valued at $24 billion a year with 48% of that revenue coming from overseas (which is now its largest industry sector). By 2025 the anime industry is expected to reach a value of $30 billion with over 60% of that revenue coming from
overseas.
Markets.
Japan External Trade Organization (JETRO) valued the domestic anime market in Japan at (), including from licensed products, in 2005. JETRO reported sales of overseas anime exports in 2004 to be (). JETRO valued the anime market in the United States at (), including in home video sales and over from licensed products, in 2005. JETRO projected in 2005 that the worldwide anime market, including sales of licensed products, would grow to (). The anime market in China was valued at in 2017, and is projected to reach by 2020. In Europe the anime merchandising market was valued at about $950 million with the figurine segment accounting for most of the share and is expected to reach a value of over $2 billion by 2030. The global anime market size was valued at $26.055 billion in 2021 with 29% of the revenue coming from merchandise. It is expected that the global anime market will reach a value of $47.14 billion by 2028. In 2023 the anime industry generated a $19.8 billion in total global revenue, including $5.5 billion from streaming and $14.3 billion from merchandising sales. North America and Asia contributed a combined $14.3 billion in total revenue, accounting for over 72% of anime's global impact. By 2030 the global anime market is expected to reach a value of $48.3 Billion with the largest contributors to this growth being North America, Europe, Asia–Pacific and The Middle East. The global anime market size was valued at $25.8 Billion in 2022 and is expected to have a market size of $62.7 Billion by 2032 with a CAGR of 9.4%.
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In 2019, the annual overseas exports of Japanese animation exceeded $10 billion for the first time in history.
Awards.
The anime industry has several annual awards that honor the year's best works. Major annual awards in Japan include the Ōfuji Noburō Award, the Mainichi Film Award for Best Animation Film, the Animation Kobe Awards, the Japan Media Arts Festival animation awards, the Seiyu Awards for voice actors, the Tokyo Anime Award and the Japan Academy Prize for Animation of the Year. Internationally, anime TV series and films compete in the Crunchyroll Anime Awards. There were also the American Anime Awards, which were designed to recognize excellence in anime titles nominated by the industry, and were held only once in 2006. Anime productions have also been nominated and won awards not exclusively for anime, like the Academy Award for Best Animated Feature or the Golden Bear.
Working conditions.
In recent years, the anime industry has been accused by both Japanese and foreign media of underpaying and overworking its animators. In response the Japanese Prime Minister Fumio Kishida promised to improve the working conditions and salary of all animators and creators working in the industry. A few anime studios such as MAPPA have taken actions to improve the working conditions of their employees. There has also been a slight increase in production costs and animator pays during the COVID-19 pandemic. Throughout 2020 and 2021 the American streaming service Netflix announced that it will greatly invest and fund the anime industry as well as support training programs for new animators. On April 27, 2023, Nippon Anime Film Culture Association (NAFCA) was officially founded. The association aims to solve problems in the industry, including the improvement of conditions of the workers.
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Global popularity and cultural impact.
Anime has become commercially profitable in the Western world, as demonstrated by early commercially successful Western adaptations of anime, such as "Astro Boy" and "Speed Racer". Early American adaptions in the 1960s made Japan expand into the continental European market, first with productions aimed at European and Japanese children, such as "Heidi", "Vicky the Viking" and "Barbapapa", which aired in various countries. Italy, Spain, and France grew a particular interest in Japan's output, due to its cheap selling price and productive output. As of 2014, Italy imported the most anime outside Japan. Anime and manga were introduced to France in the late 1970s and became massively popular in spite of a moral panic led by French politicians in the 1980s and 1990s. These mass imports influenced anime popularity in East Asian, Southeast Asian, South Asian, Latin American, Arabic and German markets.
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Netflix reported that, between October 2019 and September 2020, more than member households worldwide had watched at least one anime title on the platform. Anime titles appeared on the streaming platform's top-ten lists in almost 100 countries within the one-year period.
As of 2021, anime series are the most demanded foreign-language television shows in the United States accounting for 30.5% of the market share. (In comparison, Spanish-language and Korean-language shows account for 21% and 11% of the market share, respectively.) In 2021 more than half of Netflix's global members watched anime.
In 2022, the anime series "Attack on Titan" won the award of "Most In-Demand TV Series in the World 2021" in the Global TV Demand Awards. "Attack on Titan" became the first ever non-English language series to earn the title of "World's Most In-Demand TV Show", previously held by only "The Walking Dead" and "Game of Thrones". In 2024, the anime series "Jujutsu Kaisen" won the award of "Most In-Demand TV Series in the World 2023" in the Global TV Demand Awards.
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Rising interest in anime as well as Japanese video games has led to an increase of university students in the United Kingdom wanting to get a degree in the Japanese language. The word "anime" alongside other Japanese pop cultural terms like "shonen", "shojo" and "isekai" have been added to the Oxford English Dictionary.
Various anime and manga series have influenced Hollywood in the making of numerous famous movies and characters. Hollywood itself has produced live-action adaptations of various anime series such as "Ghost in the Shell", "Death Note", "Dragon Ball Evolution" and "Cowboy Bebop". However most of these adaptations have been reviewed negatively by both the critics and the audience and have become box-office flops. The main reasons for the unsuccessfulness of Hollywood's adaptions of anime being the often change of plot and characters from the original source material and the limited capabilities a live-action movie or series can do in comparison to an animated counterpart. One of the few particular exceptions to this includes "", which has become a moderate commercial success, receiving generally positive reviews from both the critics and the audience for its visual effects and following the source material. The movie grossed $404 million worldwide, making it director Robert Rodriguez's highest-grossing film.
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Anime and manga alongside many other imports of Japanese pop culture have helped Japan to gain a positive worldwide image and improve its relations with other countries. In 2015, during remarks welcoming Japanese Prime Minister Shinzo Abe to the White House, President Barack Obama thanked Japan for its cultural contributions to the United States by saying:
In July 2020, after the approval of a Chilean government project in which citizens of Chile would be allowed to withdraw up to 10% of their privately held retirement savings, journalist Pamela Jiles celebrated by running through Congress with her arms spread out behind her, imitating the move of many characters of the anime and manga series "Naruto". In April 2021, Peruvian politicians Jorge Hugo Romero of the PPC and Milagros Juárez of the UPP cosplayed as anime characters to get the "otaku" vote. On October 28, 2024, The Vatican unveiled its own anime-styled mascot, "Luce", in order to connect with Catholic youth through pop culture.
In April 2023, the Japan Business Federation laid out a proposal aiming to spur the economic growth of Japan by further promoting the contents industry abroad, primarily anime, manga and video games, for measures to invite industry experts from abroad to come to Japan to work, and to link with the tourism sector to help foreign fans of manga and anime visit sites across the country associated with particular manga stories. The federation seeks on quadrupling the sales of Japanese content in overseas markets within the upcoming 10 years.
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A 2018 survey conducted in 20 countries and territories using a sample consisting of 6,600 respondents held by Dentsu revealed that 34% of all surveyed people found excellency in anime and manga more than other Japanese cultural or technological aspects, which makes this mass Japanese media the third most-liked "Japanese thing", below Japanese cuisine (34.6%) and Japanese robotics (35.1%). The advertisement company views anime as a profitable tool for marketing campaigns in foreign countries due to its popularity and high reception.
Anime plays a role in driving tourism to Japan. In surveys held by Statista between 2019 and 2020, 24.2% of tourists from the United States, 7.7% of tourists from China and 6.1% of tourists from South Korea said they were motivated to visit Japan because of Japanese popular culture. In a 2021 survey held by Crunchyroll market research, 94% of Gen-Z's and 73% of the general population said that they are familiar with anime.
Fan response.
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Anime enthusiasts have produced fan fiction and fan art, including computer wallpapers, and anime music videos (AMVs).
Many fans visit sites depicted in anime, games, manga and other forms of otaku culture. This behavior is known as "Anime pilgrimage".
As of the 2020s, many anime fans and followers use social media platforms and other sites like YouTube, Bilibili, Twitch, Fandom, Facebook, Instagram, Reddit, Discord, Tumblr, 4chan, TikTok and Twitter with online communities and databases such as IMDb, MyAnimeList to discuss anime, manga and track their progress watching respective series as well as using news outlets such as Anime News Network.
According to Crunchyroll's research data from 2023 to 2024 provided by its President Rahul Parini, revealed that there are approximately 800 million people globally (outside of China and Japan) who are either highly aware of anime, show interest in anime or currently watch anime and identify as fans.
According to a 2024 survey conducted on anime fans by Polygon, 65% of the surveyed anime fans said that they find anime more emotionally compelling than other forms of media and more than 3 in 4 of Millennial and Gen-Z fans use the medium as a form of escapism. Almost two-thirds of the anime-watching Gen Z audience said they emotionally connect better with anime than they do with traditional media. Over 50% of surveyed Gen-Z anime fans said that anime influences their identity, fashion and social understanding.
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Due to anime's increased popularity in recent years, a large number of celebrities such as Elon Musk, BTS and Ariana Grande have come out as anime fans.
Anime style.
One of the key points that differentiated anime from a handful of Western cartoons is the potential for visceral content. Once the expectation that the aspects of visual intrigue or animation are just for children is put aside, the audience can realize that themes involving violence, suffering, sexuality, pain, and death can all be storytelling elements utilized in anime just as much as other media.
However, as anime itself became increasingly popular, its styling has been inevitably the subject of both satire and serious creative productions. "South Park"s "Chinpokomon" and "Good Times with Weapons" episodes, Adult Swim's "Perfect Hair Forever", and Nickelodeon's "Kappa Mikey" are examples of Western satirical depictions of Japanese culture and anime, but anime tropes have also been satirized by some anime such as "KonoSuba."
Traditionally only Japanese works have been considered anime, but some works have sparked debate about blurring the lines between anime and cartoons, such as the American anime-style productions ' and '. These anime-styled works have become defined as anime-influenced animation, in an attempt to classify all anime styled works of non-Japanese origin. Some creators of these works cite anime as a source of inspiration, for example the French production team for "Ōban Star-Racers" that moved to Tokyo to collaborate with a Japanese production team. When anime is defined as a "style" rather than as a national product, it leaves open the possibility of anime being produced in other countries, but this has been contentious amongst fans, with John Oppliger stating, "The insistence on referring to original American art as Japanese "anime" or "manga" robs the work of its cultural identity."
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While some anime will depict non-Japanese characters with specific ethnic features, such as a pronounced nose and jutting jaw for European characters, there are some styles that deliberately forgo any identification of its characters with real-world ethnicities or nationalities, termed in criticism as "mukokuseki" (statelessness). "Mukokuseki" characters can significantly impact the reception of a property outside of Japan.
A U.A.E.-Filipino produced TV series called "Torkaizer" is dubbed as the "Middle East's First Anime Show", and is currently in production and looking for funding. Netflix has produced multiple anime series in collaboration with Japanese animation studios, and in doing so, has offered a more accessible channel for distribution to Western markets. Similar initiatives have been enacted by the US-based streaming service Crunchyroll, producing titles such as "High Guardian Spice" and an adaptation of "Tower of God".
The web-based series "RWBY", produced by Texas-based company Rooster Teeth, is produced using an anime art style, and the series has been described as "anime" by multiple sources. For example, "Adweek", in the headline to one of its articles, described the series as "American-made anime", and in another headline, "The Huffington Post" described it as simply "anime", without referencing its country of origin. In 2013, Monty Oum, the creator of "RWBY", said "Some believe just like Scotch needs to be made in Scotland, an American company can't make anime. I think that's a narrow way of seeing it. Anime is an art form, and to say only one country can make this art is wrong." "RWBY" has been released in Japan with a Japanese language dub; the CEO of Rooster Teeth, Matt Hullum, commented "This is the first time any American-made anime has been marketed to Japan. It definitely usually works the other way around, and we're really pleased about that."
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Media franchises.
In Japanese culture and entertainment, media mix is a strategy to disperse content across multiple representations: different broadcast media, gaming technologies, cell phones, toys, amusement parks, and other methods. It is the Japanese term for a transmedia franchise. The term gained its circulation in late 1980s, but the origins of the strategy can be traced back to the 1960s with the proliferation of anime, with its interconnection of media and commodity goods.
A number of anime and manga media franchises such as "", "Dragon Ball", "Fate/stay night", "Yu-Gi-Oh!", "Neon Genesis Evangelion" and "Gundam" have gained considerable global popularity, and are among the world's highest-grossing media franchises. "Pokémon" in particular is estimated to be the highest-grossing media franchise of all time.
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Asterism
Asterism may refer to:
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Ankara
Ankara is the capital city of Turkey. Located in the central part of Anatolia, the city has a population of about 5.2 million in its urban center and about 5.8 million in Ankara Province. Ankara is Turkey's second-largest city by population after Istanbul, first by urban land area, and third by metro land area after Konya and Sivas.
Ankara was historically known as Ancyra and Angora. Serving as the capital of the ancient Celtic state of Galatia (280–64 BC), and later of the Roman province with the same name (25 BC–7th century), Ankara has various Hattian, Hittite, Lydian, Phrygian, Galatian, Greek, Persian, Roman, Byzantine, and Ottoman archeological sites. The Ottomans made the city the capital first of the Anatolia Eyalet (1393 – late 15th century) and then the Angora Eyalet (1827–1864) and the Angora Vilayet (1867–1922). On 23 April 1920, the Grand National Assembly of Turkey was established in Ankara, which became the headquarters of the Turkish National Movement during the Turkish War of Independence. Ankara became the new Turkish capital upon the establishment of the Republic on 29 October 1923, succeeding in this role as the former Turkish capital Istanbul following the fall of the Ottoman Empire.
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The historical center of Ankara is a rocky hill rising over the left bank of the Ankara River, a tributary of the Sakarya River. The hill remains crowned by the ruins of Ankara Castle. Although few of its outworks have survived, there are well-preserved examples of Roman and Ottoman architecture throughout the city.
The government is a prominent employer, but Ankara is also an important commercial and industrial city located at the center of Turkey's road and railway networks. The city gave its name to the Angora wool shorn from Angora rabbits, the long-haired Angora goat (the source of mohair), and the Angora cat. The area is also known for its pears, honey and Muscat grapes. Although situated in one of the driest regions of Turkey and surrounded mostly by steppe vegetation (except for the forested areas on the southern periphery), Ankara can be considered a green city in terms of green areas per inhabitant, at per head. Ankara is among the top 100 science and technology clusters in the world.
Etymology.
The orthography of the name "Ankara" has varied over the ages. It has been identified with the Hittite cult center , although this remains a matter of debate. In classical antiquity and during the medieval period, the city was known as (, ) in Greek and in Latin; the Galatian Celtic name was probably a similar variant. Following its annexation by the Seljuk Turks in 1073, the city became known in many European languages as "Angora"; it was also known in Ottoman Turkish as (). The form "Angora" is preserved in the names of breeds of many different kinds of animals, and in the names of several locations in the US (see Angora).
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History.
The region's history can be traced back to the Bronze Age Hattic civilization, which was succeeded in the 2nd millennium BC by the Hittites, in the 10th century BC by the Phrygians, and later by the Lydians, Persians, Greeks, Galatians, Romans, Byzantines, and Turks (the Seljuk Sultanate of Rûm, the Ottoman Empire and finally republican Türkiye).
Ancient history.
The oldest settlements in and around the city center of Ankara belonged to the Hattic civilization which existed during the Bronze Age and was gradually absorbed c. 2000 – 1700 BC by the Indo-European Hittites. The city grew significantly in size and importance under the Phrygians starting around 1000 BC, and experienced a large expansion following the mass migration from Gordion, (the capital of Phrygia), after an earthquake which severely damaged that city around that time. In Phrygian tradition, King Midas was venerated as the founder of Ancyra, but Pausanias mentions that the city was actually far older, which accords with present archeological knowledge.
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Phrygian rule was succeeded first by Lydian and later by Persian rule, though the strongly Phrygian character of the peasantry remained, as evidenced by the gravestones of the much later Roman period. Persian sovereignty lasted until the Persians' defeat at the hands of Alexander the Great who conquered the city in 333 BC. Alexander came from Gordion to Ankara and stayed in the city for a short period. After his death at Babylon in 323 BC and the subsequent division of his empire among his generals, Ankara, and its environs fell into the share of Antigonus.
Another important expansion took place under the Greeks of Pontos who came there around 300 BC and developed the city as a trading center for the commerce of goods between the Black Sea ports and Crimea to the north; Assyria, Cyprus, and Lebanon to the south; and Georgia, Armenia and Persia to the east. By that time, the city also took its name Ἄγκυρα ("Ánkyra", meaning "anchor" in Greek) which, in slightly modified form, provides the modern name of "Ankara".
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Celtic history.
In 278 BC, the city, along with the rest of central Anatolia, was occupied by a Celtic group, the Galatians, who were the first to make Ankara one of their main tribal centers, the headquarters of the Tectosages tribe. Other centers were Pessinus, today's Ballıhisar, for the Trocmi tribe, and Tavium, to the east of Ankara, for the Tolistobogii tribe. The city was then known as "Ancyra". The Celtic element was probably relatively small in numbers; a warrior aristocracy which ruled over Phrygian-speaking peasants. However, the Celtic language continued to be spoken in Galatia for many centuries. At the end of the 4th century, St. Jerome, a native of Dalmatia, observed that the language spoken around Ankara was very similar to that being spoken in the northwest of the Roman world near Trier.
Roman history.
The city was subsequently passed under the control of the Roman Empire. In 25 BC, Emperor Augustus raised it to the status of a "polis" and made it the capital city of the Roman province of Galatia. Ankara is famous for the "Monumentum Ancyranum" ("Temple of Augustus and Rome") which contains the official record of the "Acts of Augustus", known as the "Res Gestae Divi Augusti", an inscription cut in marble on the walls of this temple. The ruins of Ancyra still furnish today valuable bas-reliefs, inscriptions and other architectural fragments. Two other Galatian tribal centers, Tavium near Yozgat, and Pessinus (Balhisar) to the west, near Sivrihisar, continued to be reasonably important settlements in the Roman period, but it was Ancyra that grew into a grand metropolis.
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An estimated 200,000 people lived in Ancyra in good times during the Roman Empire, a far greater number than was to be the case from after the fall of the Roman Empire until the early 20th century. The small Ankara River ran through the center of the Roman town. It has now been covered and diverted, but it formed the northern boundary of the old town during the Roman, Byzantine and Ottoman periods. Çankaya, the rim of the majestic hill to the south of the present city center, stood well outside the Roman city, but may have been a summer resort. In the 19th century, the remains of at least one Roman villa or large house were still standing not far from where the Çankaya Presidential Residence stands today. To the west, the Roman city extended until the area of the Gençlik Park and Railway Station, while on the southern side of the hill, it may have extended downward as far as the site presently occupied by Hacettepe University. It was thus a sizeable city by any standards and much larger than the Roman towns of Gaul or Britannia.
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Ancyra's importance rested on the fact that it was the junction point where the roads in northern Anatolia running north–south and east–west intersected, giving it major strategic importance for Rome's eastern frontier. The great imperial road running east passed through Ankara and a succession of emperors and their armies came this way. They were not the only ones to use the Roman highway network, which was equally convenient for invaders. In the second half of the 3rd century, Ancyra was invaded in rapid succession by the Goths coming from the west (who rode far into the heart of Cappadocia, taking slaves and pillaging) and later by the Arabs. For about a decade, the town was one of the western outposts of one of Palmyrean empress Zenobia in the Syrian Desert, who took advantage of a period of weakness and disorder in the Roman Empire to set up a short-lived state of her own.
The town was reincorporated into the Roman Empire under Emperor Aurelian in 272. The tetrarchy, a system of multiple (up to four) emperors introduced by Diocletian (284–305), seems to have engaged in a substantial program of rebuilding and of road construction from Ancyra westwards to Germe and Dorylaeum (now Eskişehir).
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In its heyday, Roman Ancyra was a large market and trading center but it also functioned as a major administrative capital, where a high official ruled from the city's Praetorium, a large administrative palace or office. During the 3rd century, life in Ancyra, as in other Anatolian towns, seems to have become somewhat militarized in response to the invasions and instability of the town.
Byzantine history.
The city is well known during the 4th century as a center of Christian activity (see also below), due to frequent imperial visits, and through the letters of the pagan scholar Libanius. Bishop Marcellus of Ancyra and Basil of Ancyra were active in the theological controversies of their day, and the city was the site of no fewer than three church synods in 314, 358 and 375, the latter two in favor of Arianism.
The city was visited by Emperor Constans I (r. 337–350) in 347 and 350, Julian (r. 361–363) during his Persian campaign in 362, and Julian's successor Jovian (r. 363–364) in winter 363/364 (he entered his consulship while in the city). After Jovian's death soon after, Valentinian I (r. 364–375) was acclaimed emperor at Ancyra, and in the next year his brother Valens (r. 364–378) used Ancyra as his base against the usurper Procopius. When the province of Galatia was divided sometime in 396/99, Ancyra remained the civil capital of Galatia I, as well as its ecclesiastical center (metropolitan see). Emperor Arcadius (r. 383–408) frequently used the city as his summer residence, and some information about the ecclesiastical affairs of the city during the early 5th century is found in the works of Palladius of Galatia and Nilus of Ancyra.
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In 479, the rebel Marcian attacked the city, without being able to capture it. In 610/11, Comentiolus, brother of Emperor Phocas (r. 602–610), launched his own unsuccessful rebellion in the city against Heraclius (r. 610–641). Ten years later, in 620 or more likely 622, it was captured by the Sassanid Persians during the Byzantine–Sassanid War of 602–628. Although the city returned to Byzantine hands after the end of the war, the Persian presence left traces in the city's archeology, and likely began the process of its transformation from a late antique city to a medieval fortified settlement.
In 654, the city, also known in Arabic sources as "Qalat as-Salasil" ("fortress of the chains"), was captured for the first time by the Arabs of the Rashidun Caliphate, under Muawiyah, the future founder of the Umayyad Caliphate. At about the same time, the themes were established in Anatolia, and Ancyra became capital of the Opsician Theme, which was the largest and most important theme until it was split up under Emperor Constantine V (r.
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At about the same time, the themes were established in Anatolia, and Ancyra became capital of the Opsician Theme, which was the largest and most important theme until it was split up under Emperor Constantine V (r. 741–775); Ancyra then became the capital of the new Bucellarian Theme. The city was captured at least temporarily by the Umayyad prince Maslama ibn Hisham in 739/40, the last of the Umayyads' territorial gains from the Byzantine Empire. Ancyra was attacked without success by Abbasid forces in 776 and in 798/99. In 805, Emperor Nikephoros I (r. 802–811) strengthened its fortifications, a fact which probably saved it from sack during the large-scale invasion of Anatolia by Caliph Harun al-Rashid in the next year. Arab sources report that Harun and his successor al-Ma'mun (r. 813–833) took the city, but this information is later invention. In 838, however, during the Amorium campaign, the armies of Caliph al-Mu'tasim (r. 833–842) converged and met at the city; abandoned by its inhabitants, Ancara was razed to the ground, before the Arab armies went on to besiege and destroy Amorium reaching as far as Smyrna.
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833–842) converged and met at the city; abandoned by its inhabitants, Ancara was razed to the ground, before the Arab armies went on to besiege and destroy Amorium reaching as far as Smyrna. In 859, Emperor Michael III (r. 842–867) came to the city during a campaign against the Arabs, and ordered its fortifications restored. In 872, the city was menaced, but not taken, by the Paulicians under Chrysocheir. The last Arab raid to reach the city was undertaken in 931, by the Abbasid governor of Tarsus, Thamal al-Dulafi, but the city again was not captured.
Ecclesiastical history.
Early Christian martyrs of Ancyra, about whom little is known, included Proklos and Hilarios who were natives of the otherwise unknown nearby village of Kallippi, and suffered repression under the emperor Trajan (98–117). In the 280s we hear of Philumenos, a Christian corn merchant from southern Anatolia, being captured and martyred in Ankara, and Eustathius.
As in other Roman towns, the reign of Diocletian marked the culmination of the persecution of the Christians. In 303, Ancyra was one of the towns where the co-emperors Diocletian and his deputy Galerius launched their anti-Christian persecution. In Ancyra, their first target was the 38-year-old Bishop of the town, whose name was Clement. Clement's life describes how he was taken to Rome, then sent back, and forced to undergo many interrogations and hardship before he, and his brother, and various companions were put to death. The remains of the church of St. Clement can be found today in a building just off Işıklar Caddesi in the Ulus district. Quite possibly this marks the site where Clement was originally buried. Four years later, a doctor of the town named Plato and his brother Antiochus also became celebrated martyrs under Galerius. Theodotus of Ancyra is also venerated as a saint.
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However, the persecution proved unsuccessful and in 314 Ancyra was the center of an important council of the early church; its 25 disciplinary canons constitute one of the most important documents in the early history of the administration of the Sacrament of Penance. The synod also considered ecclesiastical policy for the reconstruction of the Christian Church after the persecutions, and in particular the treatment of "lapsi"—Christians who had given in to forced paganism (sacrifices) to avoid martyrdom during these persecutions.
Though paganism was probably tottering in Ancyra in Clement's day, it may still have been the majority religion. Twenty years later, Christianity and monotheism had taken its place. Ancyra quickly turned into a Christian city, with a life dominated by monks and priests and theological disputes. The town council or senate gave way to the bishop as the main local figurehead. During the middle of the 4th century, Ancyra was involved in the complex theological disputes over the nature of Christ, and a form of Arianism seems to have originated there.
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In 362–363, Emperor Julian passed through Ancyra on his way to an ill-fated campaign against the Persians, and according to Christian sources, engaged in a persecution of various holy men. The stone base for a statue, with an inscription describing Julian as "Lord of the whole world from the British Ocean to the barbarian nations", can still be seen, built into the eastern side of the inner circuit of the walls of Ankara Castle. The Column of Julian which was erected in honor of the emperor's visit to the city in 362 still stands today. In 375, Arian bishops met at Ancyra and deposed several bishops, among them St. Gregory of Nyssa.
In the late 4th century, Ancyra became something of an imperial holiday resort. After Constantinople became the East Roman capital, emperors in the 4th and 5th centuries would retire from the humid summer weather on the Bosporus to the drier mountain atmosphere of Ancyra. Theodosius II (408–450) kept his court in Ancyra in the summers. Laws issued in Ancyra testify to the time they spent there.
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The Metropolis of Ancyra continued to be a residential see of the Eastern Orthodox Church until the 20th century, with about 40,000 faithful, mostly Turkish-speaking, but that situation ended as a result of the 1923 Convention Concerning the Exchange of Greek and Turkish Populations. The earlier Armenian genocide put an end to the residential eparchy of Ancyra of the Armenian Catholic Church, which had been established in 1850. It is also a titular metropolis of the Ecumenical Patriarchate of Constantinople.
Both the Ancient Byzantine Metropolitan archbishopric and the 'modern' Armenian eparchy are now listed by the Catholic Church as titular sees, with separate apostolic successions.
Seljuk and Ottoman history.
After the Battle of Manzikert in 1071, the Seljuk Turks overran much of Anatolia. By 1073, the Turkish settlers had reached the vicinity of Ancyra, and the city was captured shortly after, at the latest by the time of the rebellion of Nikephoros Melissenos in 1081. In 1101, when the Crusade under Raymond IV of Toulouse arrived, the city had been under Danishmend control for some time. The Crusaders captured the city, and handed it over to the Byzantine emperor Alexios I Komnenos (r. 1081–1118). Byzantine rule did not last long, and the city was captured by the Seljuk Sultanate of Rum at some unknown point; in 1127, it returned to Danishmend control until 1143, when the Seljuks of Rum retook it.
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After the Battle of Köse Dağ in 1243, in which the Mongols defeated the Seljuks, most of Anatolia became part of the dominion of the Mongols. Taking advantage of Seljuk decline, a semi-religious cast of craftsmen and trade people named "Ahiler" chose Angora as their independent city-state in 1290. Orhan, the second Bey of the Ottoman Empire, captured the city in 1356. Timur defeated Bayezid I at the Battle of Ankara in 1402 and took the city, but in 1403 Angora was again under Ottoman control.
The Levant Company maintained a factory in the town from 1639 to 1768. In the 19th century, its population was estimated at 20,000 to 60,000. It was sacked by Egyptians under Ibrahim Pasha in 1832.
From 1867 to 1922, the city served as the capital of the Angora Vilayet, which included most of ancient Galatia.
Prior to World War I, the town had a British consulate and a population of around 28,000, roughly of whom were Christian.
Turkish republican capital.
Following the Ottoman defeat in World War I, the Ottoman capital Constantinople (modern Istanbul) and much of Anatolia was occupied by the Allies, who planned to share these lands between Armenia, France, Greece, Italy and the United Kingdom, leaving for the Turks the core piece of land in central Anatolia. In response, the leader of the Turkish nationalist movement, Mustafa Kemal Atatürk, established the headquarters of his resistance movement in Angora in 1920. After the Turkish War of Independence was won and the Treaty of Sèvres was superseded by the Treaty of Lausanne (1923), the Turkish nationalists replaced the Ottoman Empire with the Republic of Turkey on 29 October 1923. A few days earlier, Angora had officially replaced Constantinople as the new Turkish capital city, on 13 October 1923, and Republican officials declared that the city's name is Ankara.
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After Ankara became the capital of the newly founded Republic of Turkey, new development divided the city into an old section, called "Ulus", and a new section, called "Yenişehir". Ancient buildings reflecting Roman, Byzantine, and Ottoman history and narrow winding streets mark the old section. The new section, now centered on Kızılay Square, has the trappings of a more modern city: wide streets, hotels, theaters, shopping malls, and high-rises.
Government offices and foreign embassies are also located in the new section. Ankara has experienced a phenomenal growth since it was made Turkey's capital in 1923, when it was "a small town of no importance". In 1924, the year after the government had moved there, Ankara had about 35,000 residents. By 1927 there were 44,553 residents and by 1950 the population had grown to 286,781. After 1930, the city officially became known in Western languages as Ankara. By the late 1930s, the English name "Angora" was no longer in popular use.
Ankara continued to grow rapidly during the latter half of the 20th century and eventually outranked İzmir as Turkey's second-largest city, after Istanbul. Ankara's urban population reached 4,587,558 in 2014, while the population of Ankara Province reached 5,150,072 in 2015.
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The Presidential Palace of Türkiye is situated in Ankara. This building serves as the main residence of the president.
Geography.
Geographically, Ankara is located in between the Kızılırmak and Sakarya rivers, and the Sakarya River forms its border with Eskişehir in the west. Ankara shares its borders with Bolu and Çankırı in the north; Konya in the south and Kırıkkale in the east.
Ankara and its province are located in the Central Anatolia Region of Turkey. The Çubuk Brook flows through the city center of Ankara. It is connected in the western suburbs of the city to the Ankara River, which is a tributary of the Sakarya River.
Climate.
Ankara has a cold semi-arid climate under the Köppen climate classification ("BSk"), while under the Trewartha climate classification, the city is classified as humid continental ("Dc"). Due to its elevation and inland location, Ankara has cold and snowy winters, and hot and dry summers. Rainfall occurs mostly during the spring and autumn. The city lies in USDA Hardiness zone 7b, and its annual average precipitation is fairly low at , nevertheless precipitation can be observed throughout the year. Monthly mean temperatures range from in January to in July, with an annual mean of . Ankara's overall temperature regime is very similar to New York City.
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Demographics.
Ankara had a population of 75,000 in 1927. There were 74,632 male residents and 48,882 female residents in Ankara according to the 1935 census. As of 2022, the population of the Ankara Province was 5,782,285. When Ankara became the capital of the Republic of Turkey in 1923, it was designated as a planned city for 500,000 future inhabitants. During the 1920s, 1930s and 1940s, the city grew in a planned and orderly pace. However, from the 1950s onward, the city grew much faster than envisioned, because unemployment and poverty forced people to migrate from the countryside into the city to seek a better standard of living. As a result, many illegal houses called gecekondu were built around the city, causing the unplanned and uncontrolled urban landscape of Ankara, as not enough planned housing could be built fast enough. Although precariously built, the vast majority of them have electricity, running water and modern household amenities.
Nevertheless, many of these gecekondus have been replaced by huge public housing projects in the form of tower blocks such as Elvankent, Eryaman and Güzelkent; and also as mass housing compounds for military and civil service accommodation. Although many gecekondus still remain, they too are gradually being replaced by mass housing compounds, as empty land plots in the city of Ankara for new construction projects are becoming impossible to find.
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Çorum and Yozgat, which are located in Central Anatolia and whose population is decreasing, are the provinces with the highest net migration to Ankara. About one third of the Central Anatolia population of 15,608,868 people resides in Ankara.
The literacy rate in the whole province for people who are 15 years old or older is 98.18% according to 2020 TÜİK data. Ankara Province also has the highest percentage of tertiary education graduates in Turkey with 29.08% of the population having either an undergraduate, master's or doctor's degree.
Economy and infrastructure.
Ankara has long been a productive agricultural region in Anatolia. In the Ottoman period, Ankara was well known for producing grain, cotton, and fruits.
The city has exported mohair (from the Angora goat) and Angora wool (from the Angora rabbit) internationally for centuries. In the 19th century, the city also exported substantial amounts of goat and cat skins, gum, wax, honey, berries, and madder root. It was connected to Istanbul by railway before the First World War, continuing to export mohair, wool, berries, and grain.
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The Central Anatolia Region is one of the primary locations of grape and wine production in Turkey, and Ankara is particularly famous for its Kalecik Karası and Muscat grapes; and its Kavaklıdere wine, which is produced in the Kavaklıdere neighborhood within the Çankaya district of the city. Ankara is also famous for its pears. Another natural product of Ankara is its indigenous type of honey ("Ankara Balı") which is known for its light color and is mostly produced by the Atatürk Forest Farm and Zoo in the Gazi district, and by other facilities in the Elmadağ, Çubuk and Beypazarı districts. Çubuk-1 and Çubuk-2 dams on the Çubuk Brook in Ankara were among the first dams constructed in the Turkish Republic.
Ankara is the center of the state-owned and private Turkish defence and aerospace companies, where the industrial plants and headquarters of the Turkish Aerospace Industries, MKE, ASELSAN, HAVELSAN, ROKETSAN, FNSS, Nurol Makina, and numerous other firms are located. Exports to foreign countries from these defense and aerospace firms have steadily increased in the past decades. The IDEF in Ankara is one of the largest international expositions of the global arms industry. A number of the global automotive companies also have production facilities in Ankara, such as the German bus and truck manufacturer MAN SE. Ankara hosts the OSTIM Industrial Zone, Turkey's largest industrial park.
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A large percentage of the complicated employment in Ankara is provided by the state institutions; such as the ministries, subministries, and other administrative bodies of the Turkish government. There are also many foreign citizens working as diplomats or clerks in the embassies of their respective countries.
Transportation.
The "Electricity, Gas, Bus General Directorate" (EGO) operates the Ankara Metro and other forms of public transportation. Ankara is served by a suburban rail named Başkentray (B1) and five Metro lines (A1, M1, M2, M3, M4) of the Ankara Metro with about 400,000 total daily commuters, while additional subway lines (A2 and M2a/b) are planned. A long gondola lift with four stations connects the district of Şentepe to the Yenimahalle metro station.
Ankara Central Station is a major rail hub in Turkey. The Turkish State Railways operates passenger train service from Ankara to other major cities, such as: Istanbul, Eskişehir, Balıkesir, Kütahya, İzmir, Kayseri, Adana, Kars, Elazığ, Malatya, Diyarbakır, Karabük, Zonguldak and Sivas. Commuter rail also runs between the stations of Sincan and Kayaş. On 13 March 2009, the new Yüksek Hızlı Tren (YHT) high-speed rail service began operation between Ankara and Eskişehir. On 23 August 2011, another YHT high-speed line commercially started its service between Ankara and Konya. On 25 July 2014, the Ankara–Istanbul high-speed line of YHT entered service.
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Ankara Esenboğa Airport, located in the north-east of the city, is Ankara's main airport. Whilst the AŞTİ is the main coach terminal.
Ankara public transportation statistics.
The average amount of time people spend commuting on public transit in Ankara on a weekday is 71 minutes. 17% of public transit passengers, ride for more than two hours every day. The average amount of time people wait at a stop or station for public transit is sixteen minutes, while 28% of users wait for over twenty minutes on average every day. The average distance people usually ride in a single trip with public transit is , while 27% travel for over in a single direction.
Politics.
Since 8 April 2019, the mayor of Ankara is Mansur Yavaş from the Republican People's Party (CHP), who won the mayoral election in 2019 and 2024.
Ankara is politically a triple battleground between the ruling conservative AK Party, the opposition Kemalist center-left Republican People's Party (CHP) and the nationalist far-right MHP. The province of Ankara is divided into 25 districts. Historically, the CHP's key and almost only political stronghold in Ankara lied within the central area of Çankaya, which is the city's most populous district. While the CHP has always gained between 60 and 70% of the vote in Çankaya since 2002, political support elsewhere throughout Ankara was minimal. The high population within Çankaya, as well as Yenimahalle to an extent, has allowed the CHP to take overall second place behind the AK Party in both local and general elections, with the MHP a close third, despite the fact that the MHP was politically stronger than the CHP in almost every other district. Overall, the AK Party enjoyed the most support throughout the city. The electorate of Ankara thus tended to vote in favor of the political right, far more so than the other main cities of Istanbul and İzmir. In retrospect, the 2013–14 protests against the AK Party government were particularly strong in Ankara, proving to be fatal on multiple occasions.
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The city suffered from a series of terrorist attacks in 2015 and 2016, most notably on 10 October 2015; 17 February 2016; and 13 March 2016. The city was also one of the sites of the coup attempt on 15 July 2016.
Melih Gökçek was the Metropolitan Mayor of Ankara between 1994 and 2017. Initially elected in the 1994 local elections, he was re-elected in 1999, 2004 and 2009. In the 2014 local elections, Gökçek stood for a fifth term. The MHP's metropolitan mayoral candidate for the 2009 local elections, Mansur Yavaş, stood as the CHP's candidate against Gökçek in 2014. In a heavily controversial election, Gökçek was declared the winner by just 1% ahead of Yavaş amid allegations of systematic electoral fraud. With the Supreme Electoral Council and courts rejecting his appeals, Yavaş declared his intention to take the irregularities to the European Court of Human Rights. Although Gökçek was inaugurated for a fifth term, most election observers believe that Yavaş was the winner of the election. Gökçek resigned on 28 October 2017 and was replaced by the former mayor of Sincan district, Mustafa Tuna; who was succeeded by Mansur Yavaş of the CHP, the current mayor of Ankara, elected in 2019.
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Main sights.
Ancient/archeological sites.
Ankara Citadel.
The foundations of the Ankara castle and citadel were laid by the Galatians on a prominent lava outcrop (), and the rest was completed by the Romans. The Byzantines and Seljuks further made restorations and additions. The area around and inside the citadel, being the oldest part of Ankara, contains many fine examples of traditional architecture. There are also recreational areas to relax. Many restored traditional Turkish houses inside the citadel area have found new life as restaurants, serving local cuisine.
The citadel was depicted in various Turkish banknotes during 1927–1952 and 1983–1989.
Roman Theater.
The remains, the stage, and the backstage of the Antique Rome theatre of Ankara can be seen outside the castle. Roman statues that were found here are exhibited in the Museum of Anatolian Civilizations. The seating area is still under excavation.
Temple of Augustus and Rome.
The Augusteum, now known as the Temple of Augustus and Rome, was built 25 20 BC following the conquest of Central Anatolia by the Roman Empire. Ancyra then formed the capital of the new province of Galatia. After the death of Augustus in AD 14, a copy of the text of the "Res Gestae Divi Augusti" (the "Monumentum Ancyranum") was inscribed on the interior of the temple's ' in Latin and a Greek translation on an exterior wall of the '. The temple on the ancient acropolis of Ancyra was enlarged in the 2nd century and converted into a church in the 5th century. It is located in the Ulus quarter of the city. It was subsequently publicized by the Austrian ambassador Ogier Ghiselin de Busbecq in the 16th century.
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Roman Baths.
The Roman Baths of Ankara have all the typical features of a classical Roman bath complex: a "frigidarium" (cold room), a "tepidarium" (warm room) and a "caldarium" (hot room). The baths were built during the reign of the Roman emperor Caracalla in the early 3rd century to honor Asclepios, the God of Medicine. Today, only the basement and first floors remain. It is situated in the Ulus quarter.
Roman Road.
The Roman Road of Ankara or "Cardo Maximus" was found in 1995 by Turkish archeologist Cevdet Bayburtluoğlu. It is long and wide. Many ancient artifacts were discovered during the excavations along the road and most of them are displayed at the Museum of Anatolian Civilizations.
Column of Julian.
The Column of Julian or Julianus, now in the Ulus district, was erected in honor of the Roman emperor Julian the Apostate's visit to Ancyra in 362.
Mosques.
Kocatepe Mosque.
Kocatepe Mosque is the largest mosque in the city. Located in the Kocatepe quarter, it was constructed between 1967 and 1987 in classical Ottoman style with four minarets. Its size and prominent location have made it a landmark for the city.
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Ahmet Hamdi Akseki Mosque.
Ahmet Hamdi Akseki Mosque is located near the Presidency of Religious Affairs on the Eskişehir Road. Built in the Turkish neoclassical style, it is one of the largest new mosques in the city, completed and opened in 2013. It can accommodate 6 thousand people during general prayers, and up to 30 thousand people during funeral prayers. The mosque was decorated with Anatolian Seljuk style patterns.
Yeni (Cenab Ahmet) Mosque.
It is the largest Ottoman mosque in Ankara and was built by the famous architect Sinan in the 16th century. The mimber (pulpit) and mihrap (prayer niche) are of white marble, and the mosque itself is of Ankara stone, an example of very fine workmanship.
Hacı Bayram Mosque.
This mosque, in the Ulus quarter next to the Temple of Augustus, was built in the early 15th century in Seljuk style by an unknown architect. It was subsequently restored by architect Mimar Sinan in the 16th century, with Kütahya tiles being added in the 18th century. The mosque was built in honor of Hacı Bayram-ı Veli, whose tomb is next to the mosque, two years before his death (1427–28). The usable space inside this mosque is on the first floor and on the second floor.
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Ahi Elvan Mosque.
It was founded in the Ulus quarter near the Ankara Citadel and was constructed by the Ahi fraternity during the late 14th and early 15th centuries. The finely carved walnut mimber (pulpit) is of particular interest.
Alâeddin Mosque.
The Alâeddin Mosque is the oldest mosque in Ankara. It has a carved walnut mimber, the inscription on which records that the mosque was completed in early AH 574 (which corresponds to the summer of 1178 AD) and was built by the Seljuk prince Muhiddin Mesud Şah (died 1204), the Bey of Ankara, who was the son of the Anatolian Seljuk sultan Kılıç Arslan II (reigned 1156–1192.)
Modern monuments.
There are at least 50 monuments and reliefs throughout the city. Some notables are;
Victory Monument.
The Victory Monument (Turkish: "") was crafted by Austrian sculptor Heinrich Krippel in 1925 and was erected in 1927 at Ulus Square. The monument is made of marble and bronze and features an equestrian statue of Mustafa Kemal Atatürk, who wears a Republic era modern military uniform, with the rank Field Marshal.
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Statue of Atatürk.
Located at Zafer(Victory) Square (Turkish: "Zafer Meydanı"), the marble and bronze statue was crafted by the Italian sculptor Pietro Canonica in 1927 and depicts a standing Atatürk who wears a Republic era modern military uniform, with the rank Field Marshal.
Monument of Security.
The Security Monument, located in Güvenpark near Kızılay Square, was erected in 1935 and bears Atatürk's advice to his people: "Turk! Be proud, work hard, and believe in yourself." (There is debate on whether or not Atatürk actually said "Use your mind"(Turkish: öğün) instead of "Be proud"(Turkish: övün))
The monument was depicted on the reverse of the Turkish 5 lira banknote of 1937–1952 and of the 1000 lira banknotes of 1939–1946.
Hatti Monument.
Erected in 1978 at Sıhhiye Square, this impressive monument symbolizes the Hatti Sun Disc (which was later adopted by the Hittites) and commemorates Anatolia's earliest known civilization. The Hatti Sun Disc has been used in the previous logo of Ankara Metropolitan Municipality. It was also used in the previous logo of the Ministry of Culture & Tourism.
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Korean War Monument.
The Monument to Turkish Soldiers Fighting in Korea opened in 1973 to commemorate the veterans and martyrs of the Turkish Brigade.
Inns.
Suluhan.
Suluhan is a historical Inn in Ankara. It is also called the "Hasanpaşa Han". It is about southeast of Ulus Square and situated in the Hacıdoğan neighborhood. According to the "vakfiye" (inscription) of the building, the Ottoman era "han" was commissioned by Hasan Pasha, a regional beylerbey, and was constructed between 1508 and 1511, during the final years of the reign of Sultan Bayezid II.
There are 102 rooms (now shops) which face the two yards. In each room there is a window, a niche and a chimney.
Çengelhan Rahmi M. Koç Museum.
Çengelhan Rahmi M. Koç Museum is a museum of industrial technology situated in , an Ottoman era Inn which was completed in 1523, during the early years of the reign of Sultan Suleiman the Magnificent. The exhibits include industrial/technological artifacts from the 1850s onwards. There are also sections about Mustafa Kemal Atatürk, the founder of modern Turkey; Vehbi Koç, Rahmi Koç's father and one of the first industrialists of Turkey, and Ankara city.
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Shopping.
Foreign visitors to Ankara usually like to visit the old shops in "Çıkrıkçılar Yokuşu" (Weavers' Road) near Ulus, where myriad things ranging from traditional fabrics, hand-woven carpets and leather products can be found at bargain prices. "Bakırcılar Çarşısı" (Bazaar of Coppersmiths) is particularly popular, and many interesting items, not just of copper, can be found here like jewelry, carpets, costumes, antiques and embroidery. Up the hill to the castle gate, there are many shops selling a huge and fresh collection of spices, dried fruits, nuts, and other produce.
Modern shopping areas are mostly found in Kızılay, or on Tunalı Hilmi Avenue, including the modern mall of Karum (named after the ancient Assyrian merchant colonies called "Kârum" that were established in central Anatolia at the beginning of the 2nd millennium BC) which is located towards the end of the Avenue; and in Çankaya, the quarter with the highest elevation in the city. Atakule Tower next to Atrium Mall in Çankaya has views over Ankara and also has a revolving restaurant at the top. The symbol of the Armada Shopping Mall is an anchor, and there's a large anchor monument at its entrance, as a reference to the ancient Greek name of the city, Ἄγκυρα (Ánkyra), which means anchor. Likewise, the anchor monument is also related with the Spanish name of the mall, Armada, which means naval fleet.
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As Ankara started expanding westward in the 1970s, several modern, suburbia-style developments, mini-cities and business districts such as Söğütözü began to rise along the western highway, also known as the Eskişehir Road. The "Armada", "CEPA" and "Kentpark" malls on the highway, the "Galleria", "Arcadium" and "Gordion" in Ümitköy, and a huge mall, "Real" in Bilkent Center, offer North American and European style shopping opportunities (these places can be reached through the Eskişehir Highway.) There is also the newly expanded "ANKAmall" at the outskirts, on the Istanbul Highway, which houses most of the well-known international brands. This mall is the largest throughout the Ankara region. In 2014, a few more shopping malls were open in Ankara. They are "Next Level" and "Taurus" on the Boulevard of Mevlana (also known as Konya Road).
Culture.
The arts.
Turkish State Opera and Ballet, the national directorate of opera and ballet companies of Turkey, has its headquarters in Ankara, and serves the city with three venues:
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Music.
Ankara is host to five classical music orchestras:
There are four concert halls in the city:
The city has been host to several well-established, annual theater, music, film festivals:
Ankara also has a number of concert venues such as "Eskiyeni", "IF Performance Hall", "Jolly Joker", "Kite", "Nefes Bar", and "Route", which host the live performances and events of popular musicians.
Theater.
The Turkish State Theatres also has its head office in Ankara and runs the following stages in the city:
In addition, the city is served by several private theater companies, among which , who have their own stage in the city center, is a notable example.
Museums.
There are about 50 museums in the city. Some notables include;
Museum of Anatolian Civilizations.
The Museum of Anatolian Civilizations ("Anadolu Medeniyetleri Müzesi") is situated at the entrance of the Ankara Castle. It is an old 15th century bedesten (covered bazaar) that has been restored and now houses a collection of Paleolithic, Neolithic, Hatti, Hittite, Phrygian, Urartian and Roman works as well as a major section dedicated to Lydian treasures.
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Anıtkabir.
Anıtkabir is located on an imposing hill, which forms the "Anıttepe" quarter of the city, where the mausoleum of Mustafa Kemal Atatürk, founder of the Republic of Turkey, stands. Completed in 1953, it is a fusion of ancient and modern architectural styles. An adjacent museum houses a wax statue of Atatürk, his writings, letters and personal items, as well as an exhibition of photographs recording important moments in his life and during the establishment of the Republic. Anıtkabir is open every day, while the adjacent museum is open every day except Mondays.
Ankara Aviation Museum.
Ankara Aviation Museum ("Hava Kuvvetleri Müzesi Komutanlığı") is located near the Istanbul Road in Etimesgut. The museum opened to the public in September 1998. It is home to various missiles, avionics, aviation materials and aircraft that have served in the Turkish Air Force (e.g. combat aircraft such as the F-86 Sabre, F-100 Super Sabre, F-102 Delta Dagger, F-104 Starfighter, F-5 Freedom Fighter, F-4 Phantom; and cargo planes such as the Transall C-160.) Also a Hungarian MiG-21, a Pakistani MiG-19, and a Bulgarian MiG-17 are on display at the museum.
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Cer Modern.
Cer Modern is the modern-arts museum of Ankara, inaugurated on 1 April 2010. It is situated in the renovated building of the historic TCDD Cer Atölyeleri, formerly a workshop of the Turkish State Railways. The museum incorporates the largest exhibition hall in Turkey. The museum holds periodic exhibitions of modern and contemporary art as well as hosting other contemporary arts events.
Ankara Ethnography Museum.
Ankara Ethnography Museum ("Etnoğrafya Müzesi") is located opposite to the Ankara Opera House on Talat Paşa Boulevard, in the Ulus district. There is a fine collection of folkloric items, as well as artifacts from the Seljuk and Ottoman periods. In front of the museum building, there is a marble and bronze equestrian statue of Mustafa Kemal Atatürk (who wears a Republic era modern military uniform, with the rank Field Marshal) which was crafted in 1927 by the Italian sculptor Pietro Canonica.
Mehmet Akif Literature Museum Library.
The Mehmet Akif Literature Museum Library is an important literary museum and archive opened in 2011 and dedicated to Mehmet Akif Ersoy (1873–1936), the poet of the Turkish National Anthem.
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METU Science and Technology Museum / Archaeology Museum.
Both the METU Science and Technology Museum ("ODTÜ Bilim ve Teknoloji Müzesi") and the Archaeology Museum ("ODTÜ Arkeoloji Müzesi") are located inside the Middle East Technical University campus.
Republic & War of Independence Museum.
Both the Republic Museum and War of Independence Museum are located on Ulus Square. They were originally the first and second Parliament building (TBMM) of the Republic of Turkey, respectively. The War of Independence was planned and directed here as recorded in various photographs and items presently on exhibition. In another display, wax figures of former presidents of the Republic of Turkey are on exhibit.
State Art and Sculpture Museum.
The State Art and Sculpture Museum ("Resim-Heykel Müzesi") which opened to the public in 1980 is close to the Ethnography Museum and houses a rich collection of Turkish art from the late 19th century to the present day. There are also galleries which host guest exhibitions.
TCDD Open Air Steam Locomotive Museum.
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The TCDD Open Air Steam Locomotive Museum is an open-air museum which traces the history of steam locomotives.
Sports.
As with all other cities of Turkey, football is the most popular sport in Ankara. The city currently has three football clubs competing in the second tier of Turkish football, the TFF First League: Ankaragücü, Gençlerbirliği and Ankara Keçiörengücü. Ankaragücü, founded in 1910, is the oldest club in Ankara and is associated with Ankara's military arsenal manufacturing company MKE. They were the Turkish Cup winners in 1972 and 1981. Gençlerbirliği, founded in 1923, are known as the "Ankara Gale" or the "Poppies" because of their colors: red and black. They were the Turkish Cup winners in 1987 and 2001. Ankara Keçiörengücü also compete in this tier. They were founded in 1987, and bear purple and white colours on their home kit. Büyükşehir Belediye Ankaraspor also played in the Süper Lig until 2010, when they were expelled. The club was reconstituted in 2014 as Osmanlıspor but have since returned to their old identity as Ankaraspor. Ankaraspor currently play in the TFF Second League at the Etimesgut Belediyesi Atatürk Stadium. Gençlerbirliği's B team, Hacettepe S.K. (formerly known as Gençlerbirliği OFTAŞ) played in the Süper Lig but folded in 2023. Ankara Demirspor and Etimesgut Belediyespor also play in the TFF Second League. Ankara has a large number of minor teams, playing at regional levels, including Çankaya FK, Altındağspor, Mamak FK, Çubukspor, and Bağlumspor.
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In the Turkish Basketball Super League, Ankara is represented by Türk Telekom B.K., who play at the Ankara Arena. TED Ankara Kolejliler, MKE Ankaragücü, and OGM Ormanspor play in the second-tier Turkish First League. Türk Telekom became the fourth team in the country's history to participate in EuroCup finals (22-23).
Halkbank Ankara is the leading domestic powerhouse in men's volleyball, having won many championships and cups in the Turkish Men's Volleyball League and even the CEV Cup in 2013.
Ankara Buz Pateni Sarayı is where the ice skating and ice hockey competitions take place in the city.
There are many popular spots for skateboarding which is active in the city since the 1980s. Skaters in Ankara usually meet in the park near the Grand National Assembly of Turkey.
The 2012-built THF Sport Hall hosts the Handball Super League and Women's Handball Super League matches scheduled in Ankara.
Parks.
Ankara has many parks and open spaces mainly established in the early years of the Republic and well maintained and expanded thereafter. The most important of these parks are: Gençlik Parkı (houses an amusement park with a large pond for rowing), the Botanical garden, Seğmenler Park, Anayasa Park, Kuğulu Park (famous for the swans received as a gift from the Chinese government), Abdi İpekçi Park, Esertepe Parkı, Güven Park (see above for the monument), Kurtuluş Park (has an ice-skating rink), Altınpark (also a prominent exposition/fair area), Harikalar Diyarı (claimed to be Biggest Park of Europe inside city borders) and Göksu Park. Dikmen Vadisi (Dikmen Valley) is a park and recreation area situated in Çankaya district.
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Gençlik Park was depicted on the reverse of the Turkish 100 lira banknotes of 1952–1976.
Atatürk Forest Farm and Zoo ("Atatürk Orman Çiftliği") is an expansive recreational farming area which houses a zoo, several small agricultural farms, greenhouses, restaurants, a dairy farm and a brewery. It is a pleasant place to spend a day with family, be it for having picnics, hiking, biking or simply enjoying good food and nature. There is also an exact replica of the house where Atatürk was born in 1881, in Thessaloniki, Greece. Visitors to the "Çiftlik" (farm) as it is affectionately called by Ankarans, can sample such famous products of the farm such as old-fashioned beer and ice cream, fresh dairy products and meat rolls/kebabs made on charcoal, at a traditional restaurant ("Merkez Lokantası", Central Restaurant), cafés and other establishments scattered around the farm.
Education.
Universities.
Ankara is noted, within Turkey, for the multitude of universities it is home to. These include the following, several of them being among the most reputable in the country:
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Fauna.
Angora cat.
Ankara is home to a world-famous domestic cat breed – the Turkish Angora, called "Ankara kedisi" (Ankara cat) in Turkish. Turkish Angoras are one of the ancient, naturally occurring cat breeds, having originated in Ankara and its surrounding region in central Anatolia.
They mostly have a white, silky, medium to long length coat, no undercoat and a fine bone structure. There seems to be a connection between the Angora Cats and Persians, and the Turkish Angora is also a distant cousin of the Turkish Van. Although they are known for their shimmery white coat, there are more than twenty varieties including black, blue and reddish fur. They come in tabby and tabby-white, along with smoke varieties, and are in every color other than pointed, lavender, and cinnamon (all of which would indicate breeding to an outcross.)
Eyes may be blue, green, or amber, or even one blue and one amber or green. The W gene which is responsible for the white coat and blue eye is closely related to the hearing ability, and the presence of a blue eye can indicate that the cat is deaf to the side the blue eye is located. However, a great many blue and odd-eyed white cats have normal hearing, and even deaf cats lead a very normal life if kept indoors.
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Ears are pointed and large, eyes are almond shaped and the head is massive with a two plane profile. Another characteristic is the tail, which is often kept parallel to the back.
Angora goat.
The Angora goat () is a breed of domestic goat that originated in Ankara and its surrounding region in central Anatolia.
This breed was first mentioned in the time of Moses, roughly in 1500 BC. The first Angora goats were brought to Europe by Charles V, Holy Roman Emperor, about 1554, but, like later imports, were not very successful. Angora goats were first introduced in the United States in 1849 by James P. Davis. Seven adult goats were a gift from Sultan Abdülmecid I in appreciation for his services and advice on the raising of cotton.
The fleece taken from an Angora goat is called mohair. A single goat produces between of hair per year. Angoras are shorn twice a year, unlike sheep, which are shorn only once. Angoras have high nutritional requirements due to their rapid hair growth. A poor quality diet will curtail mohair development. The United States, Turkey, and South Africa are the top producers of mohair.
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For a long period of time, Angora goats were bred for their white coat. In 1998, the Colored Angora Goat Breeders Association was set up to promote breeding of colored Angoras. Today, Angora goats produce white, black (deep black to greys and silver), red (the color fades significantly as the goat gets older), and brownish fiber.
Angora goats were depicted on the reverse of the Turkish 50 lira banknotes of 1938–1952.
Angora rabbit.
The Angora rabbit () is a variety of domestic rabbit bred for its long, soft hair. The Angora is one of the oldest types of domestic rabbit, originating in Ankara and its surrounding region in central Anatolia, along with the Angora cat and Angora goat. The rabbits were popular pets with French royalty in the mid-18th century, and spread to other parts of Europe by the end of the century. They first appeared in the United States in the early 20th century. They are bred largely for their long Angora wool, which may be removed by shearing, combing, or plucking (gently pulling loose wool).
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