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Asteroid | Organic compounds | Organic compounds
Asteroids contain traces of amino acids and other organic compounds, and some speculate that asteroid impacts may have seeded the early Earth with the chemicals necessary to initiate life, or may have even brought life itself to Earth (an event called "panspermia"). In August 2011, a report, based on NASA studies with meteorites found on Earth, was published suggesting DNA and RNA components (adenine, guanine and related organic molecules) may have been formed on asteroids and comets in outer space.
In November 2019, scientists reported detecting, for the first time, sugar molecules, including ribose, in meteorites, suggesting that chemical processes on asteroids can produce some fundamentally essential bio-ingredients important to life, and supporting the notion of an RNA world prior to a DNA-based origin of life on Earth, and possibly, as well, the notion of panspermia. |
Asteroid | Classification | Classification
Asteroids are commonly categorized according to two criteria: the characteristics of their orbits, and features of their reflectance spectrum. |
Asteroid | Orbital classification | Orbital classification
thumb|A complex horseshoe orbit (the vertical looping is due to inclination of the smaller body's orbit to that of the Earth, and would be absent if both orbited in the same plane)
Many asteroids have been placed in groups and families based on their orbital characteristics. Apart from the broadest divisions, it is customary to name a group of asteroids after the first member of that group to be discovered. Groups are relatively loose dynamical associations, whereas families are tighter and result from the catastrophic break-up of a large parent asteroid sometime in the past. Families are more common and easier to identify within the main asteroid belt, but several small families have been reported among the Jupiter trojans. Main belt families were first recognized by Kiyotsugu Hirayama in 1918 and are often called Hirayama families in his honor.
About 30–35% of the bodies in the asteroid belt belong to dynamical families, each thought to have a common origin in a past collision between asteroids. A family has also been associated with the plutoid dwarf planet .
Some asteroids have unusual horseshoe orbits that are co-orbital with Earth or another planet. Examples are 3753 Cruithne and . The first instance of this type of orbital arrangement was discovered between Saturn's moons Epimetheus and Janus. Sometimes these horseshoe objects temporarily become quasi-satellites for a few decades or a few hundred years, before returning to their earlier status. Both Earth and Venus are known to have quasi-satellites.
Such objects, if associated with Earth or Venus or even hypothetically Mercury, are a special class of Aten asteroids. However, such objects could be associated with the outer planets as well. |
Asteroid | Spectral classification | Spectral classification
In 1975, an asteroid taxonomic system based on color, albedo, and spectral shape was developed by Chapman, Morrison, and Zellner. These properties are thought to correspond to the composition of the asteroid's surface material. The original classification system had three categories: C-types for dark carbonaceous objects (75% of known asteroids), S-types for stony (silicaceous) objects (17% of known asteroids) and U for those that did not fit into either C or S. This classification has since been expanded to include many other asteroid types. The number of types continues to grow as more asteroids are studied.
The two most widely used taxonomies now used are the Tholen classification and SMASS classification. The former was proposed in 1984 by David J. Tholen, and was based on data collected from an eight-color asteroid survey performed in the 1980s. This resulted in 14 asteroid categories. In 2002, the Small Main-Belt Asteroid Spectroscopic Survey resulted in a modified version of the Tholen taxonomy with 24 different types. Both systems have three broad categories of C, S, and X asteroids, where X consists of mostly metallic asteroids, such as the M-type. There are also several smaller classes.
The proportion of known asteroids falling into the various spectral types does not necessarily reflect the proportion of all asteroids that are of that type; some types are easier to detect than others, biasing the totals. |
Asteroid | Problems | Problems
Originally, spectral designations were based on inferences of an asteroid's composition. However, the correspondence between spectral class and composition is not always very good, and a variety of classifications are in use. This has led to significant confusion. Although asteroids of different spectral classifications are likely to be composed of different materials, there are no assurances that asteroids within the same taxonomic class are composed of the same (or similar) materials. |
Asteroid | Active asteroids | Active asteroids
thumb|Asteroid seen ejecting particles by the OSIRIS-REx
Active asteroids are objects that have asteroid-like orbits but show comet-like visual characteristics. That is, they show comae, tails, or other visual evidence of mass-loss (like a comet), but their orbit remains within Jupiter's orbit (like an asteroid). These bodies were originally designated main-belt comets (MBCs) in 2006 by astronomers David Jewitt and Henry Hsieh, but this name implies they are necessarily icy in composition like a comet and that they only exist within the main-belt, whereas the growing population of active asteroids shows that this is not always the case.
The first active asteroid discovered is 7968 Elst–Pizarro. It was discovered (as an asteroid) in 1979 but then was found to have a tail by Eric Elst and Guido Pizarro in 1996 and given the cometary designation 133P/Elst-Pizarro. Another notable object is 311P/PanSTARRS: observations made by the Hubble Space Telescope revealed that it had six comet-like tails. The tails are suspected to be streams of material ejected by the asteroid as a result of a rubble pile asteroid spinning fast enough to remove material from it.
thumb|Dimorphos and the tail created after the DART impact, photo by the Hubble Space Telescope
By smashing into the asteroid Dimorphos, NASA's Double Asteroid Redirection Test spacecraft made it an active asteroid. Scientists had proposed that some active asteroids are the result of impact events, but no one had ever observed the activation of an asteroid. The DART mission activated Dimorphos under precisely known and carefully observed impact conditions, enabling the detailed study of the formation of an active asteroid for the first time. Observations show that Dimorphos lost approximately 1 million kilograms after the collision. Impact produced a dust plume that temporarily brightened the Didymos system and developed a -long dust tail that persisted for several months. |
Asteroid | Observation and exploration | Observation and exploration
Until the age of space travel, objects in the asteroid belt could only be observed with large telescopes, their shapes and terrain remaining a mystery. The best modern ground-based telescopes and the Earth-orbiting Hubble Space Telescope can only resolve a small amount of detail on the surfaces of the largest asteroids. Limited information about the shapes and compositions of asteroids can be inferred from their light curves (variation in brightness during rotation) and their spectral properties. Sizes can be estimated by timing the lengths of star occultations (when an asteroid passes directly in front of a star). Radar imaging can yield good information about asteroid shapes and orbital and rotational parameters, especially for near-Earth asteroids. Spacecraft flybys can provide much more data than any ground or space-based observations; sample-return missions gives insights about regolith composition. |
Asteroid | Ground-based observations | Ground-based observations
thumb|The 70m antenna at Goldstone Observatory
thumb|Radar observations of near-Earth asteroid as seen by Arecibo
As asteroids are rather small and faint objects, the data that can be obtained from ground-based observations (GBO) are limited. By means of ground-based optical telescopes the visual magnitude can be obtained; when converted into the absolute magnitude it gives a rough estimate of the asteroid's size. Light-curve measurements can also be made by GBO; when collected over a long period of time it allows an estimate of the rotational period, the pole orientation (sometimes), and a rough estimate of the asteroid's shape. Spectral data (both visible-light and near-infrared spectroscopy) gives information about the object's composition, used to classify the observed asteroids. Such observations are limited as they provide information about only the thin layer on the surface (up to several micrometers). As planetologist Patrick Michel writes:
Mid- to thermal-infrared observations, along with polarimetry measurements, are probably the only data that give some indication of actual physical properties. Measuring the heat flux of an asteroid at a single wavelength gives an estimate of the dimensions of the object; these measurements have lower uncertainty than measurements of the reflected sunlight in the visible-light spectral region. If the two measurements can be combined, both the effective diameter and the geometric albedo—the latter being a measure of the brightness at zero phase angle, that is, when illumination comes from directly behind the observer—can be derived. In addition, thermal measurements at two or more wavelengths, plus the brightness in the visible-light region, give information on the thermal properties. The thermal inertia, which is a measure of how fast a material heats up or cools off, of most observed asteroids is lower than the bare-rock reference value but greater than that of the lunar regolith; this observation indicates the presence of an insulating layer of granular material on their surface. Moreover, there seems to be a trend, perhaps related to the gravitational environment, that smaller objects (with lower gravity) have a small regolith layer consisting of coarse grains, while larger objects have a thicker regolith layer consisting of fine grains. However, the detailed properties of this regolith layer are poorly known from remote observations. Moreover, the relation between thermal inertia and surface roughness is not straightforward, so one needs to interpret the thermal inertia with caution.
Near-Earth asteroids that come into close vicinity of the planet can be studied in more details with radar; it provides information about the surface of the asteroid (for example can show the presence of craters and boulders). Such observations were conducted by the Arecibo Observatory in Puerto Rico (305 meter dish) and Goldstone Observatory in California (70 meter dish). Radar observations can also be used for accurate determination of the orbital and rotational dynamics of observed objects. |
Asteroid | Space-based observations | Space-based observations
thumb|WISE infrared space telescope
thumb|Asteroid 6481 Tenzing, center, is seen moving against a background of stars in this series of images taken by the James Webb Space Telescope's instrument NIRCam.
Both space and ground-based observatories conducted asteroid search programs; the space-based searches are expected to detect more objects because there is no atmosphere to interfere and because they can observe larger portions of the sky. NEOWISE observed more than 100,000 asteroids of the main belt, Spitzer Space Telescope observed more than 700 near-Earth asteroids. These observations determined rough sizes of the majority of observed objects, but provided limited detail about surface properties (such as regolith depth and composition, angle of repose, cohesion, and porosity).
Asteroids were also studied by the Hubble Space Telescope, such as tracking the colliding asteroids in the main belt, break-up of an asteroid, observing an active asteroid with six comet-like tails, and observing asteroids that were chosen as targets of dedicated missions. |
Asteroid | Space probe missions | Space probe missions
According to Patrick Michel
The internal structure of asteroids is inferred only from indirect evidence: bulk densities measured by spacecraft, the orbits of natural satellites in the case of asteroid binaries, and the drift of an asteroid's orbit due to the Yarkovsky thermal effect. A spacecraft near an asteroid is perturbed enough by the asteroid's gravity to allow an estimate of the asteroid's mass. The volume is then estimated using a model of the asteroid's shape. Mass and volume allow the derivation of the bulk density, whose uncertainty is usually dominated by the errors made on the volume estimate. The internal porosity of asteroids can be inferred by comparing their bulk density with that of their assumed meteorite analogues, dark asteroids seem to be more porous (>40%) than bright ones. The nature of this porosity is unclear. |
Asteroid | Dedicated missions | Dedicated missions
The first asteroid to be photographed in close-up was 951 Gaspra in 1991, followed in 1993 by 243 Ida and its moon Dactyl, all of which were imaged by the Galileo probe en route to Jupiter. Other asteroids briefly visited by spacecraft en route to other destinations include 9969 Braille (by Deep Space 1 in 1999), 5535 Annefrank (by Stardust in 2002), 2867 Šteins and 21 Lutetia (by the Rosetta probe in 2008), and 4179 Toutatis (China's lunar orbiter Chang'e 2, which flew within in 2012).
The first dedicated asteroid probe was NASA's NEAR Shoemaker, which photographed 253 Mathilde in 1997, before entering into orbit around 433 Eros, finally landing on its surface in 2001. It was the first spacecraft to successfully orbit and land on an asteroid. From September to November 2005, the Japanese Hayabusa probe studied 25143 Itokawa in detail and returned samples of its surface to Earth on 13 June 2010, the first asteroid sample-return mission. In 2007, NASA launched the Dawn spacecraft, which orbited 4 Vesta for a year, and observed the dwarf planet Ceres for three years.
Hayabusa2, a probe launched by JAXA 2014, orbited its target asteroid 162173 Ryugu for more than a year and took samples that were delivered to Earth in 2020. The spacecraft is now on an extended mission and expected to arrive at a new target in 2031.
NASA launched the OSIRIS-REx in 2016, a sample return mission to asteroid 101955 Bennu. In 2021, the probe departed the asteroid with a sample from its surface. Sample was delivered to Earth in September 2023. The spacecraft continues its extended mission, designated OSIRIS-APEX, to explore near-Earth asteroid Apophis in 2029.
In 2021, NASA launched Double Asteroid Redirection Test (DART), a mission to test technology for defending Earth against potential hazardous objects. DART deliberately crashed into the minor-planet moon Dimorphos of the double asteroid Didymos in September 2022 to assess the potential of a spacecraft impact to deflect an asteroid from a collision course with Earth. In October, NASA declared DART a success, confirming it had shortened Dimorphos's orbital period around Didymos by about 32 minutes.
NASA's Lucy, launched in 2021, is a multiple-asteroid flyby probe focused on flying by 7 Jupiter trojans of varying types. While not yet set to reach its first main target, 3548 Eurybates, until 2027, it has made flybys of the main-belt asteroids 152830 Dinkinesh and 52246 Donaldjohanson. |
Asteroid | Planned missions | Planned missions
thumb|upright=1.3|Asteroids and comets visited by spacecraft as of 2019 (except Ceres and Vesta), to scale
NASA's Psyche, launched in October 2023, is intended to study the large metallic asteroid of the same name, and is on track to arrive there in 2029.
ESA's Hera, launched in October 2024, is intended study the results of the DART impact. It is expected to measure the size and morphology of the crater, and momentum transmitted by the impact, to determine the efficiency of the deflection produced by DART.
JAXA's DESTINY+ is a mission for a flyby of the Geminids meteor shower parent body 3200 Phaethon, as well as various minor bodies. Its launch is planned for 2024.
CNSA's Tianwen-2 is planned to launch in 2025. If all goes as planned, it will use solar electric propulsion to explore the co-orbital near-Earth asteroid 469219 Kamoʻoalewa and the active asteroid 311P/PanSTARRS. The spacecraft is tasked with collecting samples of the regolith of Kamo'oalewa. |
Asteroid | Asteroid mining | Asteroid mining
thumb|Artist's concept of a crewed mission to an asteroid
The concept of asteroid mining was proposed in 1970s. Matt Anderson defines successful asteroid mining as "the development of a mining program that is both financially self-sustaining and profitable to its investors". It has been suggested that asteroids might be used as a source of materials that may be rare or exhausted on Earth, or materials for constructing space habitats. Materials that are heavy and expensive to launch from Earth may someday be mined from asteroids and used for space manufacturing and construction.
As resource depletion on Earth becomes more real, the idea of extracting valuable elements from asteroids and returning these to Earth for profit, or using space-based resources to build solar-power satellites and space habitats, becomes more attractive. Hypothetically, water processed from ice could refuel orbiting propellant depots.
From the astrobiological perspective, asteroid prospecting could provide scientific data for the search for extraterrestrial intelligence (SETI). Some astrophysicists have suggested that if advanced extraterrestrial civilizations employed asteroid mining long ago, the hallmarks of these activities might be detectable. |
Asteroid | Threats to Earth | Threats to Earth
thumb|Frequency of bolides, small asteroids roughly 1 to 20 meters in diameter impacting Earth's atmosphere
There is increasing interest in identifying asteroids whose orbits cross Earth's, and that could, given enough time, collide with Earth. The three most important groups of near-Earth asteroids are the Apollos, Amors, and Atens.
The near-Earth asteroid 433 Eros had been discovered as long ago as 1898, and the 1930s brought a flurry of similar objects. In order of discovery, these were: 1221 Amor, 1862 Apollo, 2101 Adonis, and finally 69230 Hermes, which approached within 0.005 AU of Earth in 1937. Astronomers began to realize the possibilities of Earth impact.
Two events in later decades increased the alarm: the increasing acceptance of the Alvarez hypothesis that an impact event resulted in the Cretaceous–Paleogene extinction, and the 1994 observation of Comet Shoemaker-Levy 9 crashing into Jupiter. The U.S. military also declassified the information that its military satellites, built to detect nuclear explosions, had detected hundreds of upper-atmosphere impacts by objects ranging from one to ten meters across.
All of these considerations helped spur the launch of highly efficient surveys, consisting of charge-coupled device (CCD) cameras and computers directly connected to telescopes. , it was estimated that 89% to 96% of near-Earth asteroids one kilometer or larger in diameter had been discovered. , the LINEAR system alone had discovered 147,132 asteroids. Among the surveys, 19,266 near-Earth asteroids have been discovered including almost 900 more than in diameter.
In June 2018, the National Science and Technology Council warned that the United States is unprepared for an asteroid impact event, and has developed and released the "National Near-Earth Object Preparedness Strategy Action Plan" to better prepare. According to expert testimony in the United States Congress in 2013, NASA would require at least five years of preparation before a mission to intercept an asteroid could be launched. |
Asteroid | Asteroid deflection strategies | Asteroid deflection strategies
thumb|Double Asteroid Redirection Test in 2022 demonstrated that spacecraft impact is a viable option for planetary defense.
Various collision avoidance techniques have different trade-offs with respect to metrics such as overall performance, cost, failure risks, operations, and technology readiness. There are various methods for changing the course of an asteroid/comet.C. D. Hall and I. M. Ross, "Dynamics and Control Problems in the Deflection of Near-Earth Objects", Advances in the Astronautical Sciences, Astrodynamics 1997, Vol. 97, Part I, 1997, pp. 613–631. These can be differentiated by various types of attributes such as the type of mitigation (deflection or fragmentation), energy source (kinetic, electromagnetic, gravitational, solar/thermal, or nuclear), and approach strategy (interception,Solem, J. C.; Snell, C. (1994). "Terminal intercept for less than one orbital period warning ", a chapter in Hazards Due to Comets and Asteroids, Geherels, T., ed. (University of Arizona Press, Tucson), pp. 1013–1034. rendezvous, or remote station).
Strategies fall into two basic sets: fragmentation and delay. Fragmentation concentrates on rendering the impactor harmless by fragmenting it and scattering the fragments so that they miss the Earth or are small enough to burn up in the atmosphere. Delay exploits the fact that both the Earth and the impactor are in orbit. An impact occurs when both reach the same point in space at the same time, or more correctly when some point on Earth's surface intersects the impactor's orbit when the impactor arrives. Since the Earth is approximately 12,750 km in diameter and moves at approx. 30 km per second in its orbit, it travels a distance of one planetary diameter in about 425 seconds, or slightly over seven minutes. Delaying, or advancing the impactor's arrival by times of this magnitude can, depending on the exact geometry of the impact, cause it to miss the Earth.
"Project Icarus" was one of the first projects designed in 1967 as a contingency plan in case of collision with 1566 Icarus. The plan relied on the new Saturn V rocket, which did not make its first flight until after the report had been completed. Six Saturn V rockets would be used, each launched at variable intervals from months to hours away from impact. Each rocket was to be fitted with a single 100-megaton nuclear warhead as well as a modified Apollo Service Module and uncrewed Apollo Command Module for guidance to the target. The warheads would be detonated 30 meters from the surface, deflecting or partially destroying the asteroid. Depending on the subsequent impacts on the course or the destruction of the asteroid, later missions would be modified or cancelled as needed. The "last-ditch" launch of the sixth rocket would be 18 hours prior to impact. |
Asteroid | Fiction | Fiction
Asteroids and the asteroid belt are a staple of science fiction stories. Asteroids play several potential roles in science fiction: as places human beings might colonize, resources for extracting minerals, hazards encountered by spacecraft traveling between two other points, and as a threat to life on Earth or other inhabited planets, dwarf planets, and natural satellites by potential impact. |
Asteroid | See also | See also
Exoasteroid
List of minor planets
List of exceptional asteroids
List of asteroid close approaches to Earth
Lost minor planet
Meanings of minor-planet names |
Asteroid | Notes | Notes |
Asteroid | References | References |
Asteroid | Further reading | Further reading
|
Asteroid | External links | External links
NASA Asteroid and Comet Watch site
Category:Minor planets
Category:Solar System |
Asteroid | Table of Content | Short description, Terminology{{anchor, History of observations, Discovery of Ceres, Further search, 19th and 20th centuries, Naming, Symbols, Formation, Distribution within the Solar System, Asteroid belt, Trojans, Near-Earth asteroids, Martian moons, Characteristics, Size distribution, Largest asteroids, Rotation, Color, Surface features, Composition, Water, Organic compounds, Classification, Orbital classification, Spectral classification, Problems, Active asteroids, Observation and exploration, Ground-based observations, Space-based observations, Space probe missions, Dedicated missions, Planned missions, Asteroid mining, Threats to Earth, Asteroid deflection strategies, Fiction, See also, Notes, References, Further reading, External links |
Allocution | Short description | An allocution, or allocutus, is a formal statement made to a court by the defendant who has been found guilty before being sentenced. It is part of the criminal procedure in some jurisdictions using common law. |
Allocution | Concept | Concept
An allocution allows the defendant to explain why the sentence should be lenient. In plea bargains, an allocution may be required of the defendant. The defendant explicitly admits specifically and in detail the actions and their reasons in exchange for a reduced sentence.
In principle, that removes any doubt as to the exact nature of the defendant's guilt in the matter.
The term allocution is used generally only in jurisdictions in the United States, but there are vaguely similar processes in other common law countries. In many other jurisdictions, it is for the defense lawyer to mitigate on their client's behalf, and the defendant rarely has the opportunity to speak. |
Allocution | Australia | Australia
In Australia, the term allocutus is used by the Clerk of Arraigns or another formal associate of the court.
It is generally phrased as: "Prisoner at the Bar, you have been found Guilty by a jury of your peers of the offence of XYZ. Do you have anything to say as to why the sentence of this Court should not now be passed upon you?"e.g. in Queensland, Criminal Practice Rules 1999 s51
The defense counsel will then make a plea in mitigation (also called submissions on penalty) in an attempt to mitigate the relative seriousness of the offense, and heavily refer to and rely upon the defendant's previous good character and good works, if any.
The right to make a plea in mitigation is absolute: if a judge or magistrate refuses to hear such a plea or does not properly consider it, the sentence can be overturned on appeal. |
Allocution | United States | United States
In most of the United States, defendants are allowed the opportunity to allocute before a sentence is passed. Some jurisdictions hold that as an absolute right. In its absence, a sentence but not the conviction may be overturned, resulting in the need for a new sentencing hearing. In the federal system, Federal Rules of Criminal Procedure 32(i)(4) provides that the court must "address the defendant personally in order to permit the defendant to speak or present any information to mitigate the sentence".
The Federal Public Defender recommends that defendants speak in terms of how a lenient sentence will be sufficient but not greater than necessary to comply with the statutory directives set forth in . |
Allocution | See also | See also
Confession (law)
Newton hearing, the equivalent in England and Wales |
Allocution | References | References
Category:Criminal procedure
Category:Evidence law |
Allocution | Table of Content | Short description, Concept, Australia, United States, See also, References |
Affidavit | Short description | thumb|Vasil Levski's affidavit, 16 June 1872, Bucharest, Romania
An ( ; Medieval Latin for "he has declared under oath") is a written statement voluntarily made by an affiant or deponent under an oath or affirmation which is administered by a person who is authorized to do so by law. Such a statement is witnessed as to the authenticity of the affiant's signature by a taker of oaths, such as a notary public or commissioner of oaths. An affidavit is a type of verified statement or showing, or containing a verification, meaning it is made under oath on penalty of perjury. It serves as evidence for its veracity and is required in court proceedings. |
Affidavit | Definition | Definition
An affidavit is typically defined as a written declaration or statement that is sworn or affirmed before a person who has authority to administer an oath. There is no general defined form for an affidavit, although for some proceedings an affidavit must satisfy legal or statutory requirements in order to be considered. An affidavit may include,
a commencement which identifies the affiant;
an attestation clause, usually a jurat, at the end certifying that the affiant made the statement under oath on the specified date;
signatures of the affiant and person who administered the oath.
In some cases, an introductory clause, called a preamble, is added attesting that the affiant personally appeared before the authenticating authority. An affidavit may also recite that the statement it records was made under penalty of perjury.
An affidavit that is prepared for use within the context of litigation may also include a caption that identifies the venue and parties to the relevant judicial proceedings. |
Affidavit | Worldwide | Worldwide |
Affidavit | Australia | Australia
On 2 March 2016, the High Court of Australia held that the ACT Uniform Evidence Legislation is neutral in the way sworn evidence and unsworn evidence is treated as being of equal weight. |
Affidavit | United Kingdom | United Kingdom
The term "affidavit" is used in the UK. According to the UK government website, "The affidavit can be sworn or affirmed by a solicitor, notary or commissioner for oaths (for a charge) or by an authorised member of court staff." |
Affidavit | India | India
In Indian law, although an affidavit may be taken as proof of the facts stated therein, the courts have no jurisdiction to admit evidence by way of affidavit. Affidavit is not treated as "evidence" within the meaning of Section 3 of the Evidence Act. However, it was held by the Supreme Court that an affidavit can be used as evidence only if the court so orders for sufficient reasons, namely, the right of the opposite party to have the deponent produced for cross-examination.Khandesh Spg & Wvg Mills Co. Ltd. vs Rashtriya Girni Kamgar Sangh, citation 1960 AIR571, 1960 SCR(2) 841) Therefore, an affidavit cannot ordinarily be used as evidence in absence of a specific order of the court. |
Affidavit | Sri Lanka | Sri Lanka
In Sri Lanka, under the Oaths Ordinance, with the exception of a court-martial, a person may submit an affidavit signed in the presence of a commissioner for oaths or a justice of the peace. |
Affidavit | Ireland | Ireland
Affidavits are made in a similar way as to England and Wales, although "make oath" is sometimes omitted. An affirmed affidavit may be substituted for an sworn affidavit in most cases for those opposed to swearing oaths. The person making the affidavit is known as the deponent and signs the affidavit. The affidavit concludes in the standard format "sworn/affirmed (declared) before me, [name of commissioner for oaths/solicitor], a commissioner for oaths (solicitor), on the [date] at [location] in the county/city of [county/city], and I know the deponent", and it is signed and stamped by the commissioner for oaths. It is important that the Commissioner states his/her name clearly, sometimes documents are rejected when the name cannot be ascertained.
In August 2020, a new method of filing affidavits came into force. Under Section 21 of the Civil Law and Criminal Law (Miscellaneous Provisions) Act 2020 witnesses are no longer required to swear before God or make an affirmation when filing an affidavit. Instead, witnesses will make a non-religious "statement of truth" and, if it is breached, will be liable for up to one year in prison if convicted summarily or, upon conviction on indictment, to a maximum fine of €250,000 or imprisonment for a term not exceeding 5 years, or both.
This is designed to replace affidavits and statutory declarations in situations where the electronic means of lodgement or filing of documents with the Court provided for in Section 20 is utilised. As of January 2022, it has yet to be adopted widely, and it is expected it will not be used for some time by lay litigants who will still lodge papers in person. |
Affidavit | United States | United States
thumb|upright=0.9|Affidavit signed by Harriet Tubman
In American jurisprudence, under the rules for hearsay, admission of an unsupported affidavit as evidence is unusual (especially if the affiant is not available for cross-examination) with regard to material facts which may be dispositive of the matter at bar. Affidavits from persons who are dead or otherwise incapacitated, or who cannot be located or made to appear, may be accepted by the court, but usually only in the presence of corroborating evidence. An affidavit which reflected a better grasp of the facts close in time to the actual events may be used to refresh a witness's recollection. Materials used to refresh recollection are admissible as evidence. If the affiant is a party in the case, the affiant's opponent may be successful in having the affidavit admitted as evidence, as statements by a party-opponent are admissible through an exception to the hearsay rule.
Affidavits are typically included in the response to interrogatories.Rule 33. Interrogatories to Parties. Cornell Legal Information Institute.Interrogatories. Requests for admissions under Federal Rule of Civil Procedure 36, however, are not required to be sworn.Federal Rule of Civil Procedure 36.Cornell Legal Information Institute.
When a person signs an affidavit, that person is eligible to take the stand at a trial or evidentiary hearing. One party may wish to summon the affiant to verify the contents of the affidavit, while the other party may want to cross-examine the affiant about the affidavit.
Some types of motions will not be accepted by the court unless accompanied by an independent sworn statement or other evidence in support of the need for the motion. In such a case, a court will accept an affidavit from the filing attorney in support of the motion, as certain assumptions are made, to wit: The affidavit in place of sworn testimony promotes judicial economy. The lawyer is an officer of the court and knows that a false swearing by them, if found out, could be grounds for severe penalty up to and including disbarment. The lawyer if called upon would be able to present independent and more detailed evidence to prove the facts set forth in his affidavit.
Affidavits should not be confused with unsworn declarations under penalty of perjury. In federal courts and about 20 states as of 2006, unsworn declarations under penalty of perjury are authorized by statute as acceptable in lieu of affidavits. The key differences are that an unsworn declaration does not bear the jurat of a notary public and the declarant is not required to swear an oath or affirmation. Rather, the signature of the declarant under a carefully worded phrase binding them to the truth of their statements "under penalty of perjury" is deemed as a matter of law to be sufficiently solemn to remind the declarant of their duty to tell the truth, the whole truth, and nothing but the truth (that is, the oath they would normally swear if they were testifying in person in a court of law). The point of such affidavit substitution statutes is that unsworn declarations can be prepared and executed far more quickly and economically than affidavits, in that the witness need not meet personally with a notary public for the notarization process.
The acceptance of an affidavit by one society does not confirm its acceptance as a legal document in other jurisdictions. Equally, the acceptance that a lawyer is an officer of the court (for swearing the affidavit) is not a given. This matter is addressed by the use of the apostille, a means of certifying the legalization of a document for international use under the terms of the 1961 Hague Convention Abolishing the Requirement of Legalization for Foreign Public Documents. Documents which have been notarized by a notary public, and certain other documents, and then certified with a conformant apostille, are accepted for legal use in all the nations that have signed the Hague Convention. Thus most affidavits now require to be apostilled if used for cross border issues. |
Affidavit | See also | See also
Declaration (law)
Deposition (law)
Fishman Affidavit, a well-known example of an affidavit
Performativity
Statutory declaration
Sworn declaration |
Affidavit | References | References
Category:Evidence law
Category:Legal documents
Category:Notary
Category:Oaths |
Affidavit | Table of Content | Short description, Definition, Worldwide, Australia, United Kingdom, India, Sri Lanka, Ireland, United States, See also, References |
Aries (constellation) | Short description | Aries is one of the constellations of the zodiac. It is located in the Northern celestial hemisphere between Pisces to the west and Taurus to the east. The name Aries is Latin for ram. Its old astronomical symbol is 20px (♈︎). It is one of the 48 constellations described by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is a mid-sized constellation ranking 39th in overall size, with an area of 441 square degrees (1.1% of the celestial sphere).
Aries has represented a ram since late Babylonian times. Before that, the stars of Aries formed a farmhand. Different cultures have incorporated the stars of Aries into different constellations including twin inspectors in China and a porpoise in the Marshall Islands. Aries is a relatively dim constellation, possessing only four bright stars: Hamal (Alpha Arietis, second magnitude), Sheratan (Beta Arietis, third magnitude), Mesarthim (Gamma Arietis, fourth magnitude), and 41 Arietis (also fourth magnitude). The few deep-sky objects within the constellation are quite faint and include several pairs of interacting galaxies. Several meteor showers appear to radiate from Aries, including the Daytime Arietids and the Epsilon Arietids. |
Aries (constellation) | History and mythology | History and mythology
Aries is now recognized as an official constellation, albeit as a specific region of the sky, by the International Astronomical Union. It was originally defined in ancient texts as a specific pattern of stars, and has remained a constellation since ancient times; it now includes the ancient pattern and the surrounding stars. In the description of the Babylonian zodiac given in the clay tablets known as the MUL.APIN, the constellation, now known as Aries, was the final station along the ecliptic. The MUL.APIN was a comprehensive table of the rising and settings of stars, which likely served as an agricultural calendar. Modern-day Aries was known as , "The Agrarian Worker" or "The Hired Man". Although likely compiled in the 12th or 11th century BC, the MUL.APIN reflects a tradition that marks the Pleiades as the vernal equinox, which was the case with some precision at the beginning of the Middle Bronze Age. The earliest identifiable reference to Aries as a distinct constellation comes from the boundary stones that date from 1350 to 1000 BC. On several boundary stones, a zodiacal ram figure is distinct from the other characters. The shift in identification from the constellation as the Agrarian Worker to the Ram likely occurred in later Babylonian tradition because of its growing association with Dumuzi the Shepherd. By the time the MUL.APIN was created—in 1000 BC—modern Aries was identified with both Dumuzi's ram and a hired labourer. The exact timing of this shift is difficult to determine due to the lack of images of Aries or other ram figures.
In ancient Egyptian astronomy, Aries was associated with the god Amun-Ra, who was depicted as a man with a ram's head and represented fertility and creativity. Because it was the location of the vernal equinox, it was called the "Indicator of the Reborn Sun". During the times of the year when Aries was prominent, priests would process statues of Amon-Ra to temples, a practice that was modified by Persian astronomers centuries later. Aries acquired the title of "Lord of the Head" in Egypt, referring to its symbolic and mythological importance.
thumb|left|300px|Aries and Musca Borealis as depicted in Urania's Mirror, a set of constellation cards published in London
thumb|Aries depicted in an early medieval manuscript,
Aries was not fully accepted as a constellation until classical times. In Hellenistic astrology, the constellation of Aries is associated with the golden ram of Greek mythology that rescued Phrixus and Helle on orders from Hermes, taking Phrixus to the land of Colchis. Phrixus and Helle were the son and daughter of King Athamas and his first wife Nephele. The king's second wife, Ino, was jealous and wished to kill his children. To accomplish this, she induced famine in Boeotia, then falsified a message from the Oracle of Delphi that said Phrixus must be sacrificed to end the famine. Athamas was about to sacrifice his son atop Mount Laphystium when Aries, sent by Nephele, arrived. Helle fell off of Aries's back in flight and drowned in the Dardanelles, also called the Hellespont in her honour.
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.
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.
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. |
Aries (constellation) | In non-Western astronomy | 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.
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. |
Aries (constellation) | Features | Features
thumb|left|256px|The constellation Aries as it can be seen with the naked eye |
Aries (constellation) | Stars | Stars |
Aries (constellation) | Bright 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.
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.
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.
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. |
Aries (constellation) | Variable stars | 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. |
Aries (constellation) | Deep sky objects | Deep sky objects
thumb|right|NGC 772, with a notated supernova
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.
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.
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. |
Aries (constellation) | Meteor showers | 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.
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. |
Aries (constellation) | Planetary systems | Planetary systems
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. |
Aries (constellation) | See also | See also
Aries (Chinese astronomy) |
Aries (constellation) | References | References |
Aries (constellation) | Explanatory notes | Explanatory notes |
Aries (constellation) | Citations | Citations |
Aries (constellation) | Bibliography | Bibliography
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Aries (constellation) | Online sources | Online sources
SIMBAD
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Aries (constellation) | External links | External links
The Deep Photographic Guide to the Constellations: Aries
The clickable Aries
Star Tales – Aries
Warburg Institute Iconographic Database (medieval and early modern images of Aries)
Category:Constellations
Category:Constellations listed by Ptolemy
Category:Northern constellations |
Aries (constellation) | Table of Content | Short description, History and mythology, In non-Western astronomy, Features, Stars, Bright stars, Variable stars, Deep sky objects, Meteor showers, Planetary systems, See also, References, Explanatory notes, Citations, Bibliography, Online sources, External links |
Aquarius (constellation) | Short description | 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 20px (♒︎), 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. |
Aquarius (constellation) | History and mythology | 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.
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. |
Aquarius (constellation) | Depictions | Depictions
left|thumb|upright=1.25|A representation of Aquarius printed in 1825 as part of Urania's Mirror (including a now-obsolete constellation, Ballon Aerostatique south of it)
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. |
Aquarius (constellation) | In Eastern astronomy | 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.
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. |
Aquarius (constellation) | Features | Features |
Aquarius (constellation) | Stars | Stars
thumb|The constellation Aquarius as it can be seen by the naked eye
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.
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
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 |
Aquarius (constellation) | Planetary systems | 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.
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.
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.
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. |
Aquarius (constellation) | Deep sky objects | Deep sky objects
thumb|The green bean galaxy J2240 lies in the constellation of Aquarius
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.
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. |
Aquarius (constellation) | Meteor showers | 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.
The Iota Aquariids is a fairly weak meteor shower that peaks on 6 August, with a rate of approximately 8 meteors per hour. |
Aquarius (constellation) | Astrology | 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. |
Aquarius (constellation) | Notes | Notes |
Aquarius (constellation) | See also | See also
Aquarius (Chinese astronomy) |
Aquarius (constellation) | References | References
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Aquarius (constellation) | External links | External links
The Deep Photographic Guide to the Constellations: Aquarius
The clickable Aquarius
Warburg Institute Iconographic Database (medieval and early modern images of Aquarius)
Category:Constellations
Category:Equatorial constellations
Category:Constellations listed by Ptolemy |
Aquarius (constellation) | Table of Content | Short description, History and mythology, Depictions, In Eastern astronomy, Features, Stars, Planetary systems, Deep sky objects, Meteor showers, Astrology, Notes, See also, References, External links |
Anime | Short description | is a 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.
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. |
Anime | Etymology | 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".
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. |
Anime | History | History |
Anime | Precursors | 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. |
Anime | Pioneers | Pioneers
thumb|right|Namakura Gatana (1917), the oldest surviving Japanese animated short film made for cinemas
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.
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 Momotaro: Sacred Sailors (1945), produced by Seo with a sponsorship from the Imperial Japanese Navy. The 1950s saw a proliferation of short, animated advertisements created for television. |
Anime | Modern era | Modern era
thumb|left|Frame from the opening sequence of Tezuka's 1963 TV series Astro Boy
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).
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), Royal Space Force: The Wings of Honnêamise (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). Demon Slayer: Kimetsu no Yaiba the Movie: Mugen Train 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.
In 2021, the anime adaptations of Jujutsu Kaisen, Demon Slayer: Kimetsu no Yaiba 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. |
Anime | Attributes | Attributes
thumb|upright=1.5|Anime artists employ many distinct visual styles.Clockwise from the top left: Dead Leaves, Flag, Serial Experiments Lain, Monster, Mind Game, Lucky Star, Cat Soup, and Gurren Lagann.
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.
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. |
Anime | Technique | 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.
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".
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. |
Anime | Characters | Characters
thumb|left|Anime character design is diverse, but often incorporates common elements depending on the target demographic and era. These are representative samples. Clockwise from the top left: Ashita no Joe (1970), Macross: Do You Remember Love? (1984), Ghost in the Shell (1995), K-On! (2009), Your Name (2016), The Hidden Dungeon Only I Can Enter (2021), Fruits Basket (2001), and Rurouni Kenshin (1996).
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.
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.
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. |
Anime | Music | Music
thumb|250px|An example of a 2022 anime video with 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.
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. |
Anime | Genres | 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.Ask John: Why Do Americans Hate Harem Anime? . animenation.net. May 20. 2005. Note: fan service and ecchi are often considered the same in wording. 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.
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. |
Anime | Formats | 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.
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. |
Anime | Industry | Industry
upright=1.15|thumb|Akihabara district of Tokyo is popular with anime and manga fans as well as otaku subculture in Japan.
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. 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. This type of anime is less popular outside Japan, being considered "more of a niche product". Spirited Away (2001) was the all-time highest-grossing film in Japan until overtaken by Demon Slayer: Kimetsu no Yaiba – The Movie: Mugen Train in 2020.Gross
North American gross: $10,055,859
Japanese gross: $229,607,878 (March 31, 2002)
Other territories: $
Japanese gross
End of 2001: $227 million
Across 2001 and 2002: $270 million
As of 2008: $290 million It was also the highest-grossing anime film worldwide until it was overtaken by Makoto Shinkai's 2016 film Your Name. Anime films represent a large part of the highest-grossing Japanese films yearly in Japan, with 6 out of the top 10 in 2014, 2015 and also in 2016.
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.
Licenses are expensive, often hundreds of thousands of dollars for one series and tens of thousands for one movie.ADV Court Documents Reveal Amounts Paid for 29 Anime Titles The prices vary widely; for example, Jinki: Extend 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,"The Anime Economy Part 3: Digital Pennies" 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.
The industry has been subject to both praise and condemnation for fansubs, the addition of unlicensed and unauthorized subtitled translations of anime series or films. Fansubs, which were originally distributed on VHS bootlegged cassettes in the 1980s, have been freely available and disseminated online since the 1990s. Since this practice raises concerns for copyright and piracy issues, fansubbers tend to adhere to an unwritten moral code to destroy or no longer distribute an anime once an official translated or subtitled version becomes licensed. They also try to encourage viewers to buy an official copy of the release once it comes out in English, although fansubs typically continue to circulate through file-sharing networks. Even so, the laid back regulations of the Japanese animation industry tend to overlook these issues, allowing it to grow underground and thus increasing its popularity until there is a demand for official high-quality releases for animation companies. This has led to an increase in global popularity of Japanese animation, reaching $40 million in sales in 2004. Fansub practices have rapidly declined since the early-2010s due to the advent of legal streaming services which simulcast new anime series often within a few hours of their domestic release.
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. |
Anime | Markets | 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%.
In 2019, the annual overseas exports of Japanese animation exceeded $10 billion for the first time in history. |
Anime | Awards | 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. |
Anime | Working conditions | 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. |
Anime | Global popularity and cultural impact | Global popularity and cultural impact
thumb|300x300px|Anime Expo in Los Angeles, California, United States – one of the largest fan conventions in the Western world.
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,The Latin American Appetite for Asian Content. Ark One Studios.Exploring Asian Heritage in Latin America. Luz Media. Arabic and German markets.
The beginning of 1980 saw the introduction of Japanese anime series into the American culture. In the 1990s, Japanese animation slowly gained popularity in America. Media companies such as Viz and Mixx began publishing and releasing animation into the American market. The 1988 film Akira is largely credited with popularizing anime in the Western world during the early 1990s, before anime was further popularized by television shows such as Pokémon and Dragon Ball Z in the late 1990s. By 1997, Japanese anime was the fastest-growing genre in the American video industry. The growth of the Internet later provided international audiences with an easy way to access Japanese content. Early on, online piracy played a major role in this, through over time legal alternatives appeared which significantly reduced illegal practices. Since the 2010s streaming services have become increasingly involved in the production, licensing and distribution of anime for the international markets. This is especially the case with net services such as Netflix, Crunchyroll and others which have large catalogs in many countries, although until 2020 anime fans in multiple developing countries, such as India and the Philippines, had fewer options for obtaining access to legal content, and therefore would still turn to online piracy. However beginning with the 2020s anime has been experiencing yet another boom in global popularity and demand due to the COVID-19 pandemic and streaming services like Netflix, Amazon Prime Video, HBO Max, Disney+, Hulu and anime-only services like Crunchyroll and Hidive, increasing the international availability of the amount of new licensed anime shows as well as the size of their catalogs.
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.
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 Alita: Battle Angel, 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.
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.
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. |
Anime | Fan response | Fan response
thumb|Cosplay of Madoka Kaname and Kyubey from Puella Magi Madoka Magica during Tracon 2013 event at the Tampere Hall in Tampere, Finland
Anime clubs gave rise to anime conventions in the 1990s with the "anime boom", a period marked by anime's increased global popularity. These conventions are dedicated to anime and manga and include elements like cosplay contests and industry talk panels. Cosplay, a portmanteau of "costume play", is not unique to anime and has become popular in contests and masquerades at anime conventions. Japanese culture and words have entered English usage through the popularity of the medium, including otaku, an unflattering Japanese term commonly used in English to denote an obsessive fan of anime or manga. Another word that has arisen describing obsessive fans in the United States is wapanese meaning 'white individuals who want to be Japanese, or later known as weeaboo or weeb, individuals who demonstrate an obsession with Japanese anime subculture, a term that originated from abusive content posted on the website 4chan.org. While originally derogatory, the terms "Otaku" and "Weeb" have been reappropriated by the anime fandom overtime and today are used by some fans to refer to themselves in a comedic and more positive way.
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.
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 | Anime style | 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 Parks "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 Avatar: The Last Airbender and Avatar: The Legend of Korra. 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."
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.Bîrlea, Oana-Maria. “Soft Power: ’Cute Culture’, a Persuasive Strategy in Japanese Advertising.” TRAMES: A Journal of the Humanities & Social Sciences, vol. 27, no. 3, July 2023, pp. 311–24. EBSCOhost via Wikipedia Library, https://doi.org/10.3176/tr.2023.3.07.Altiok, Revna. "What Is Mukokuseki in Anime – And Why Is It Important? " from Comic Book Resources, 24 June 2022.
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." |
Anime | Media franchises | Media franchises
thumb|Pokémon Center at Jewel Changi Airport in Singapore
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.Henry Jenkins, Convergence Culture: Where Old and New Media Collide, p. 110 It is the Japanese term for a transmedia franchise.Marc Steinberg, Anime's Media Mix: Franchising Toys and Characters in Japan 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.Steinberg, p. vi
A number of anime and manga media franchises such as Demon Slayer: Kimetsu no Yaiba, 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. |
Anime | See also | See also
Cool Japan
Hentai
History of anime
Japanese popular culture
Japanophilia
Lists of anime
La nouvelle manga
Manfra
Mechademia
OEL manga
Otaku
Soft power § Japan
Television in Japan
Video games in Japan
Voice acting in Japan
Vtuber |
Anime | Notes | Notes |
Anime | References | References |
Anime | Sources | Sources
Category:1917 introductions
Category:Anime and manga terminology
Category:Japanese inventions |
Anime | Table of Content | Short description, Etymology, History, Precursors, Pioneers, Modern era, Attributes, Technique, Characters, Music, Genres, Formats, Industry, Markets, Awards, Working conditions, Global popularity and cultural impact, Fan response, Anime style, Media franchises, See also, Notes, References, Sources |
Asterism | Wiktionary | Asterism may refer to:
Asterism (astronomy), a pattern of stars
Asterism (band), a Japanese rock band
Asterism (gemology), an optical phenomenon in gemstones
Asterism (typography), (⁂) a moderately rare typographical symbol denoting a break in passages |
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