title: Pandya dynasty

text: Besides the poems, king Peruvaludi is also mentioned in later copper-plate grant (8th–9th century CE). In the work "Mathuraikkanci", the author Mankudi Maruthanar, refers to his patron, Talaihalanganum Nedunjeliyan, as the Lord of Korkai and the Warlord of the Southern Parathavar People. It contains a full-length description of Madurai and the Pandya country under the rule of Nedunjeliyan. In the famous battle of Talaiyalanganam (in east Tanjore), the Pandya is said to have defeated his enemies (which included the Chera and the Chola). He is also praised for his victory of Mizhalai and Mutturu, two "vel" centres along the ocean (in Pudukkottai). The "Netunalvatai" (in the collection of "Pattupattu") by Nakkirar contains a description of king Nedunjeliyan's palace.


title: Pandya dynasty

text: Greek and Latin sources (early centuries CE) refer to the ancient Tamil country, same as the Tamilakam, as "Lymyrike" or "Damirice" (or Dymirice/Dimirixe or Damirice) and its ruling families.


title: Pandya dynasty

text: Scholar John E. Hill identified Panyue as Pandya kingdom. However, others have identified it with an ancient state located in modern Burma or Assam.


title: Pandya dynasty

text: Maurya emperor Asoka (3rd century BCE) seems to have been on friendly terms with the people of south India and Sri Lanka (the Cholas, the Pandyas, the Satiya Putras, the Kerala Putras and the Tamraparnis). There are no indications that Asoka tried to conquer the extreme south India (the Tamilakam – the Abode of the Tamils).


title: Pandya dynasty

text: The three chiefly lines of the early historic south India – the Cheras, Pandyas and Cholas – were known as the mu-vendar ("the three vendars"). They traditionally based at their original headquarters in the interior Tamil Nadu (Karur, Madurai and Uraiyur respectively). The powerful chiefdoms of the three ventar dominated the political and economic life of early historic south India. The frequent conflicts between the Chera, the Chola and the Pandya are well documented in ancient (the Sangam) Tamil poetry. The Cheras, Cholas and Pandyas also controlled the ports of Muziris (Muchiri), Korkai and Kaveri respectively (for the trade with the Graeco-Roman world). The gradual shift from chiefdoms to kingdoms seems to have occurred in the following period.The famous inscription of king Kharavela at Hathigumpha (mid-first century BCE) mentions the defeat of a confederacy of the "Tramira" countries which had been a threat to Kalinga. It also remembers the precious pearls brought to the capital as booty from the "Pandya" realm. The Pandya chiefdom was famous for its pearl fisheries and silk industry. Korkai and Alagankulam are believed to have been the exchange centres of the Pandyas. Korkai, a port at the mouth of the river Tambraparni, was linked to the famous pearl fisheries and Alagankulam was also developed as a port.


title: Pandya dynasty

text: A number of coins attributed to early historic Pandyas are found from the region. Inscriptions, datable to c. 2nd century BCE, recording royal grants – both from royals and wealthy commoners – were also discovered from the Pandya country.


title: Pandya dynasty

text: The Pandya seems to be the most prominent of the three "ventar" rulers. There are even references to a Pandya queen from 3rd century BCE representing a confederacy of the Tamil countries. Madurai, in south Tamil Nadu, was the most important cultural centre in south India as the core of the Tamil speakers. Megalithic relics such as menhirs, dolmens, urn burials, stone circles and rock-cut chambers/passages can be found in south India. Burial goods include iron objects, ivory ornaments, Black-and-Red Ware and even some Roman Imperial coins. The so-called "velir" hill chieftains are assumed to be associated with these megalithic burials.


title: Pandya dynasty

text: Greek and Latin accounts (early centuries CE), coins with legends in Tamil-Brahmi script, and Tamil-Brahmi inscriptions suggest the continuity of the Pandya dynasty from the 3rd century BCE to early centuries CE. The early Pandyas, along with the Cheras and the Cholas, were eventually displaced by the Kalabhra dynasty.


title: Pandya dynasty

text: The Pandya kingdom was revived by king Kadungon (r. 590–620 CE) towards the end of the 6th century CE. In the Velvikudi inscription, a later copper-plate, Kadungon appears as the "destroyer" of the "anti-Brahmanical" Kalabhra kings. With the decline of the Kalabhra dynasty, the Pandyas grew steadily in power and territory. With the Cholas in obscurity in Uraiyur, the Tamil country was divided between the Pallavas of Kanchi and the Pandyas of Madurai.


title: Pandya dynasty

text: From 6th century to 9th century CE, the Chalukyas of Badami, the Pallavas of Kanchi, and Pandyas of Madurai dominated the politics of south India. The Badami Chalukyas were eventually replaced by the Rashtrakutas in the Deccan. The Pandyas took on the growing Pallava ambitions in south India, and from time to time they also joined in alliances with the kingdoms of the Deccan Plateau (such as with the Gangas of Talakad in late 8th century CE). In the middle of the 9th century, the Pandyas had managed to advance as far as Kumbakonam (north-east of Tanjore on the Kollidam river).


title: Pandya dynasty

text: Sendan (r. 654–70 CE), the third king of the Pandyas of Madurai, is known for expanding his kingdom to the Chera country (western Tamil Nadu and central Kerala). Arikesari Maravarman (r. 670–700 CE), the fourth Pandya ruler, is known for his battles against the Pallavas of Kanchi. Pallava king Narasimhavarman I (r. 630–68 CE), the famous conqueror of Badami, claimed to have defeated the Pandyas. Chalukya king Paramesvaravarman I "Vikramaditya" (r. 670–700 CE) is known to have fought battles with the Pallavas, the Gangas, and probably with the Pandyas too, on the Kaveri basin.


title: Pandya dynasty

text: Kirtivarman II (r. 744/5–55 CE), the last Chalukya king, managed to lose to his southern countries as a result of his battles with the Pandyas. Pandya kings Maravarman Rajasimha I (r. 730–65 CE) and Nedunjadaiyan/Varagunavarman I (r. 765–815 CE) threatened Pallava king Nandivarman II Pallavamalla (r. 731–96 CE) who had managed to defeat the Gangas in around 760 CE. Varagunavarman I invaded the Pallava country, conquered the Kongu country (western Tamil Nadu) and Venadu (south Kerala). King Srimara Srivallabha (r. 815–62 CE) sailed to Sri Lanka, subjugated king Sena I, and sacked his capital Anuradhapura (the Panya invasion of Sri Lanka followed a period of vassalage). However, Srimara Srivallabha was soon overpowerd by Pallava king Nripatunga (r. 859–99 CE). Sena II, the king of Sri Lanka, invaded the Pandya country, sacked Madurai and chose Varagunavarman II (r. c. 862–880 CE) as the new king soon after. It is proposed that the start of the Kollam Era, the Kerala calendar, in 825 CE marked the liberation of Venadu from Pandya control.


title: Pandya dynasty

text: During the rule of Dantivarman (r. 796–847 CE), the Pallava territory was reduced by the encroachment from the Pandyas from the south (and Rashtrakutas and the Telugu-Cholas from north). Pallava king Nandivarman III (r. 846–69 CE) was able to defeat the Pandyas and Telugu-Cholas (and even the Rashtrakutas) with the help of the Gangas and the emerging Cholas.


title: Pandya dynasty

text: While the Pandyas and the Rashtrakutas were busy engaging the Pallavas, with the Gangas and the Simhalas (Sri Lanka) also in the mix, the Cholas emerged from the Kaveri delta and took on the chieftains of Thanjavur (the Mutharaiyar chieftain had transferred their loyalty from the Pallava to the Pandya). The Chola king Vijayalaya conquered Thanjavur by defeating the Mutharaiyar chieftain around c. 850 CE. The Pandya control north of the Kaveri river was severely weakened by this move (and straightened the position of the Pallava ruler Nripatunga). Pandya ruler Varaguna-varman II (r. c. 862–880 CE) responded by marching into the Chola country and facing a formidable alliance of Pallava prince Aparajita, the Chola king Aditya I and the Ganga king Prithvipati I. The Pandya king suffered a crushing defeat (c. 880 CE) in a battle fought near Kumbakonam.


title: Pandya dynasty

text: By c. 897 CE, Chola king Aditya I was the master of the old Pallava, Ganga and Kongu countries. It is a possibility that Aditya I conquered the Kongu country from the Pandya king Parantaka Viranarayana (r. 880–900 CE). Parantaka I, successor to Aditya, invaded the Pandya territories in 910 CE and captured Madurai from king Maravarman Rajasimha II (hence the title "Madurai Konda"). Rajasimha II received help from the Sri Lankan king Kassapa V, still got defeated by Parantaka I in the battle of Vellur, and fled to Sri Lanka. Rajasimha then found refuge in the Chera country, leaving even his royal insignia in Sri Lanka, the home of his mother.


title: Pandya dynasty

text: The Cholas were defeated by a Rashtrakuta-lead confederacy in the battle of Takkolam in 949 CE. By mid-950s, the Chola kingdom had shrunk to the size of a small principality (its vassals in the extreme south had proclaimed their independence). It is a possibility that Pandya ruler Vira Pandya defeated Chola king Gandaraditya and claimed independence. Chola ruler Sundara Parantaka II (r. 957–73) responded by defeating Vira Pandya I in two battles (and Chola prince Aditya II killed Vira Pandya on the second occasion). The Pandyas were assisted by Sri Lanka forces of king Mahinda IV.


title: Pandya dynasty

text: Chola emperor Rajaraja I (r. 985–1014 CE) is known to have attacked the Pandyas. He fought against an alliance of the Pandya, Chera and Sri Lankan kings, and defeated the Cheras and "deprived" the Pandyas of their ancient capital Madurai. Emperor Rajendra I continued to occupy the Pandya kingdom, and even appointed a series of Chola viceroys with the title "Chola Pandya" to rule from Madurai (over Pandya and Western Chera/Kerala countries). The very of beginning of Chola emperor Kulottunga's rule (r. from 1070 CE) was marked by the loss of Sri Lanka and a rebellion in the Pandya country.


title: Pandya dynasty

text: The second half of the 12th century witnessed a major internal crisis in the Pandya country (between princes Parakrama Pandya and Kulasekhara Pandya). The neighbouring kingdoms of Sri Lanka, under Parakramabahu I, Venadu Chera/Kerala, under the Kulasekharas, and the Cholas, under Rajadhiraja II and Kulottunga III, joinined in and took sides with any of the two princes or their kins.


title: Pandya dynasty

text: The Pandya empire included extensive territories, at times including large portions of south India and Sri Lanka. The rule of the empire was shared among several royals, one of them enjoying primacy over the rest. The Pandya king at Madurai thus controlled these vast regions through the collateral family branches subject to Madurai.


title: Pandya dynasty

text: The foundation for the Pandya supremacy in south India was laid by Maravarman Sundara I early in the 13th century. He succeeded his older brother Jatavarman Kulasekhara in 1216. He invaded the Chola country, sacked Uraiyur and Thanjavur, and drove the Chola king Kulothunga III into exile. The Chola king subsequently made a formal submission to Maravarman Sundara I and acknowledged his overlordship. Attempts by the next Chola king Rajaraja III (1216 – 46 CE) for self-rule (to stop the Pandya invasion into the Chola country), with the help of the Hoysalas king Narasimha II (r. 1220 – 1238 CE), resulted in a battle between the Pandya and Hoysala forces at Mahendramangalam on the Kaveri Valley. Maravarman Sundara I was defeated and Rajaraja III was restored in the Chola country. Sometime later Chola prince Rajendra III attacked the Pandyas and defeated two Pandya royals including Maravarman Sundara II. Hoysala king Somesvara (r. 1233 – 1267 CE) then came to the aid of the Pandyas, defeated Rajendra III and then made peace with the Cholas.


title: Pandya dynasty

text: Jatavarman Sundara I ascended the Pandya throne in 1251 CE. He led his army to the Chola country (even as far as Nellore), to Sri Lanka and to south Kerala. He was also successful in confining the Hoysala control to the Mysore Plateau (the ancient Chola country was now overrun by the Pandyas). Kanchi functioned as the second major city in the kingdom. In his conquests, Jatavarman Sundara I was assisted by number of Pandya royals such as Jatavarman Vira Pandya.


title: Pandya dynasty

text: Jatavarman Sundara I subdued Rajendra II around 1258–1260 CE and made him pay tribute. The rule of the Cholas ended c. 1279 with Rajendra III. The Pandya attacked the Hoysalas in the Kaveri and captured the fort of Kannanur Koppam. Hoysala king Somesvara was forced to fall back into the Mysore Plateau. The Hoysala king, pressed by enemies from north and south, "assigned" the southern half of his kingdom to his younger son Ramanatha (r. 1254–1292). Somesvara was eventually killed by the Pandya in 1262 CE. Ramanatha managed to recover Kannanur and hold against the Pandya power. Jatavarman Sundara I also came into conflict with the Kadava ruler Kopperunjinga II. It seems that Bana (Magadai) and Kongu countries came under the Pandya rule during the wars against the Hoysalas and the Kadavas. Jatavarman Sundara I also fought the Kakatiya ruler Ganapati (1199–1262). Sri Lanka was invaded by Jatavarman Sundara I in 1258 and on his behalf by his younger brother Jatavarman Vira II between 1262 and 1264 CE. The island was again invaded and defeated by Jatavarman Vira II in 1270 CE.


title: Pandya dynasty

text: Sundara Pandya I (died in 1268) was succeeded by Maravarman Kulasekara I. Around 1279 the combined force of Hoysala king Ramanatha and Rajendra III was defeated by Maravarman Kulasekara I. Maravarman Kulasekara I, now virtually unchallenged, ruled over the Chola country and southern Tamil speaking portions of Hoysala kingdom. He also invaded Sri Lanka, ruled by Bhuvanaikabahu I, "carried away to the Pandya country the venerable Tooth Relic", and the wealth of the island. Sri Lanka remained under Pandya control until c. 1308–1309 CE.


title: Pandya dynasty

text: After the death of Maravarman Kulasekhara I (1310), his sons Vira Pandya IV and Sundara Pandya IV fought a war of succession for control of the empire. It seems that Maravarman Kulasekhara wanted Vira Pandya to succeed him (who in turn was defeated by Sundara Pandya after a short period of time). Unfortunately, the Pandya civil war coincided with the Khalji raids in south India. Taking advantage of the political situation, the neighbouring Hoysala king Ballala III invaded the Pandya territory. However, Ballala had to retreat to his capital, when Khalji general Malik Kafur invaded his kingdom at the same time. After subjugating Ballala III, the Khalji forces marched to the Pandya territory in March 1311. The Pandya brothers fled their headquarters, and the Khaljis pursued them unsuccessfully. By late April 1311, the Khaljis gave up their plans to pursue the Pandya princes, and returned to Delhi with the plunder. By 1312 the Pandya control over south Kerala was also lost.


title: Pandya dynasty

text: After the departure of the Khaljis, Vira and Sundara Pandya resumed their conflict. Sundara Pandya was defeated, and sought help from the Khaljis. With their help, he regained control of the South Arcot region by 1314. Subsequently, there were two more expeditions from the sultanate in 1314 led by Khusro Khan and in 1323 by Ulugh Khan (Muhammad bin Tughluq) under sultan Ghiyath al-Din Tughluq.


title: Pandya dynasty

text: The family quarrels and the sultanate invasions shattered the Pandya empire beyond revival and coinage discoveries made imply that the Pandyas were left with the old South Arcot region. In 1323, the Jaffna kingdom declared its independence from the crumbling Pandya influence.


title: Pandya dynasty

text: The Pandya kings from Sadaavarman Parakrama Pandya to his successors who ruled with Tenkasi as their capital. With the invasion of the Sultanates, Vijayanagaras, and Nayakars from the fourteenth century onwards, the Pandyas lost their traditional capital of Madurai and shifted to cities like Tenkasi and Tirunelveli. Tenkasi was the last capital of the Pandyas. All the Pandyas from Sadaavarman Parakrama Pandya and his next generations were crowned in the Adheenam Mutt in Kasi Viswanathar temple. During the same period, some Pandyas ruled with Tirunelveli as their capital. Kayatharu, Vadakkuvalliyur, and Ukkirankottai are some of their major cities. Inscriptions on them are found in Tenkasi's Kasi Viswanathar temple, Brahmadesam, Tirunelveli dt.Brahmadesam, Cheranmadevi, Ambasamudram, Kalakkad and Pudukkottai. The last Pandyan king to be known in the history of the Pandyas was Kolakonda, who was also among the Tenkasi Pandyas.


title: Pandya dynasty

text: Although the Vijayanagara Empire and the Nayaks ruled Madurai after the 14th century, they were occasionally opposed by the Pandyas. Sometimes they have ruled Madurai. Prominent among them were Saadavarman Vikrama Pandya (1401–1422 AD) and his son, Arikesari Parakrama Pandya. They had built 32 forts around Madurai. Later, when Vishwanatha Nayakkar became the Madurai Mandalasuvaran, he feared of Pandya resurgence in Madurai. He divided Madurai into 72 districts, including 16 districts of those closest to the Pandyas. He gave them positions and made them separate from the Pandyas. This made Pandyas to lose Madurai forever.


title: Pandya dynasty

text: While the previous sultanate raids were content with plunder, the Tughluqs under Ulugh Khan (later Muhammad bin Tughluq) annexed the former Pandya dominions to the sultanate as the province of Ma'bar. Most of south India came under the sultanate rule and was divided into five provinces – Devagiri, Tiling, Kampili, Dorasamudra and Ma'bar. Jalal ud-Din Hasan Khan was appointed governor of the newly created southernmost Ma'bar province. In c. 1334, Jalal ud-Din Hasan Khan declared his independence and created Madurai sultanate. The Pandyas shifted their capital to Tenkasi and continued to rule a small area until the end of the 16th century as Tenkasi Pandyas.


title: Pandya dynasty

text: Bukka Raya I of Vijayanagara empire conquered the city of Madurai in c. 1370, imprisoned the sultan, released and restored Arcot's prince Sambuva Raya to the throne. Bukka Raya I appointed his son Veera Kumara Kampana as the viceroy of the Tamil region. Meanwhile, Madurai sultanate was replaced by the Nayak governors of Vijayanagara in 1378. In 1529 the Nayak governors declared independence and established Madurai Nayak dynasty.


title: Pandya dynasty

text: The Pandya country, located at the extreme south-western tip of South Asia, served as an important meeting point throughout the history of the India. The location was economically and geopolitically significant as a key point connecting the shipping between Southeast Asia and the Middle East. Graeco-Roman merchants frequented the ancient Tamil country, present day south India and Sri Lanka, securing contacts with the Tamil chiefdoms of the Pandya, Chola and Chera families. The western sailors also established a number of trading settlements on the harbours of the ancient Tamil region.The trade with South Asia by the Greco-Roman world flourished since the time of the Ptolemaic dynasty a few decades before the start of the Common Era and remained long after the fall of the Western Roman Empire. The contacts between south India and the Middle East continued even after the Byzantium's loss of the ports of Egypt and the Red Sea in the 7th century CE.


title: Pandya dynasty

text: The early historic Pandya country was famous for its supply of pearls. The ancient port of Korkai, in present-day Thoothukudi, was the center of pearl trade. Written records from Graeco-Roman and Egyptian voyagers give details about the pearl fisheries off the Gulf of Mannar. Greek historian Megasthenes reported about the pearl fisheries, indicating that the Pandyas derived great wealth from the pearl trade. Convicts were according to the "Periplus of the Erythraean Sea" used as pearl divers in Korkai. The "Periplus" even mentions that "pearls inferior to the Indian sort are exported in great quantity from the marts of Apologas and Omana". The pearls from the Pandya country were also in demand in the kingdoms of north India. Literary references of the pearl fishing mention how the fishermen, who dive into the sea, avoid attacks from sharks, bring up the right-whorled chank and blow on the sounding shell.


title: Pandya dynasty

text: The early coins of Tamilakam bore the symbols of the Three Crowned Kings, the tiger, the fish and the bow, representing the symbols of the Cholas, Pandyas and Cheras. Coins of Pandyas bear the legend of different Pandya ruler in different times. The Pandyas had issued silver punch-marked and die struck copper coins in the early period. A few gold coins were attributed to the Pandya rulers of this period. These coins bore the image of fish, singly or in pairs, which were their emblem.


title: Pandya dynasty

text: Some of the coins had the names Sundara, Sundara Pandya or merely the letter 'Su' were etched. Some of the coins bore a boar with the legend of 'Vira-Pandya. It had been said that those coins were issued by the Pandyas and the feudatories of the Cholas but could not be attributed to any particular king. The coins of Pandyas were basically square. Those coins were etched with elephant on one side and the other side remained blank. The inscription on the silver and gold coins during the Pandyas, were in Tamil-Brahmi and the copper coins bore the Tamil legends. The coins of the Pandyas, which bore the fish symbols, were termed as 'Kodandaraman' and 'Kanchi' Valangum Perumal'. Apart from these, 'Ellamthalaiyanam' was seen on coins which had the standing king on one side and the fish on the other. 'Samarakolahalam' and 'Bhuvanekaviram' were found on the cois having a Garuda, 'Konerirayan' on coins having a bull and 'Kaliyugaraman' on coins that depict a pair of feet.


title: Pandya dynasty

text: The Pandya period (c. 13th century CE) was characterised by a temple-centered elite form of Hinduism, a popular bhakti religion and an even more widespread local forms of Hinduism. The distinctions between the three were not clearly differentiated. The worship of the gods Vishnu and Shiva was generally supported by the elite. The bhakti movement emphasized the mutual intense emotional attachment between the god and the devotee.


title: Pandya dynasty

text: The Pandya country was home to a number of renowned temples including Meenakshi Temple in Madurai. As some of the largest employers and landowners of the Pandya country, the temples played an important part in the Tamil economy and society. They generally also served as banks, schools, dispensaries, and poorhouses (thus performing valuable social functions). The large walled temple complexes of the Pandya country also contained several administrative offices and bazaars.


title: Pandya dynasty

text: It is known that the early Pandya rulers followed Jainism while at some point they converted to Hinduism. They supported the Bhakti movement from both Saivism and Vaishnavism of Hinduism.


title: Pandya dynasty

text: The Tamil country is home to the 'South Indian' or 'Dravidian' style of medieval temple architecture.


title: Pandya dynasty

text: The major Pandya contributions to the Dravidian architecture comes after the Pallava (7th–9th centuries) and the Chola periods (9th–12th centuries).


title: Oculus (film)

text: Oculus is a 2013 American supernatural psychological horror film co-written, edited, and directed by Mike Flanagan. It is based on his short film "Oculus: Chapter 3 – The Man with the Plan", and stars Karen Gillan and Brenton Thwaites as two young adult siblings who are convinced that an antique mirror is responsible for the death and misfortune that their family had suffered.


title: Oculus (film)

text: The film had its world premiere on September 5, 2013, at the 2013 Toronto International Film Festival (TIFF) and received a wide theatrical release on April 11, 2014. It received generally positive reviews from critics, and was a box office success.


title: Oculus (film)

text: The film takes place in two different times: the present and 11 years earlier. The two plot lines are told in parallel through flashbacks.


title: Oculus (film)

text: In 2002, software engineer Alan Russell moves into a new house with his wife Marie, 10-year-old son Tim, and 12-year-old daughter Kaylie. Alan purchases an antique mirror to decorate his office. Unbeknownst to them, the mirror supernaturally induces hallucinations. Marie is haunted by visions of her own body decaying, while Alan is seduced by a mysterious and ghostly woman named Marisol Chavez, who has mirrors in place of eyes.


title: Oculus (film)

text: In 2013, Tim is discharged from a psychiatric hospital, having come to believe that there were no supernatural events involved in his parents' deaths. Kaylie has spent most of her young adulthood researching the history of the mirror. Using her position as an employee of an auction house, she obtains access to the mirror and has it transported to the family home, where she places it in a room filled with surveillance cameras and a "kill switch" — an anchor weighted to the ceiling. Kaylie intends to destroy the mirror, but first wants to document its powers, proving Tim's innocence.


title: Oculus (film)

text: Over time back in 2002, the parents become psychotic; Alan isolates himself in his office, and Marie becomes withdrawn and paranoid. All of the plants in the house die, and their family dog Mason disappears after being shut in the office with the mirror. After Kaylie sees Alan with Marisol, she tells her mother, and the parents fight. One night, Marie goes insane and attempts to kill her children, but Alan locks her away. When the family runs out of food, the children realize that their father is under the influence of the mirror, so Kaylie goes to seek help from their mother, and finds her chained to the wall, acting like an animal. Kaylie and Tim try going to their neighbors for help, but the neighbors disbelieve their stories. When Kaylie attempts to use the phone, she discovers that all of her phone calls are answered by the same man.


title: Oculus (film)

text: One night, Alan unchains Marie, and both parents attack the children. Marie briefly comes to her senses, only to be shot dead by Alan. The children try to destroy the mirror but it tricks them, making them believe they are hitting the mirror when they are actually hitting the wall. Alan also experiences a moment of lucidity and kills himself by forcing Tim to pull the trigger of the gun and shoot him, causing a small crack in the corner of the mirror in the process. Before dying, he begs the children to run, but Marisol and other victims of the mirror appear as horrific ghosts. The police arrive and take Tim into custody. Before the siblings are separated, they promise to reunite as adults and destroy the mirror. As Tim is taken away and put behind bars, he sees the ghosts of his parents watching him from the house.


title: Oculus (film)

text: Back in 2013, Tim attempts to convince Kaylie that she's wrong and the siblings argue. When they notice the houseplants begin to wilt, they review the camera footage and see themselves performing actions they have no memory of. Tim finally accepts the mirror's supernatural power and attempts to escape the house with Kaylie, only for the pair to be drawn back by the mirror's influence. Seeing a hallucination of her mother, Kaylie stabs it in the neck, only to realize that she has stabbed Michael Dumont, her fiancé who has come to check on her. They try to call the police, but are only able to reach the same voice who spoke to them on the phone as children.


title: Oculus (film)

text: At this point, they see their doppelgangers inside the house standing in front of the mirror. Realizing that the 9-1-1 call is not going through, they go back inside the house. Kaylie and Tim begin hallucinating by seeing younger versions of each other. They get separated, and each of them relives the nightmare from their youth. Tim awakens alone in the room with the mirror, while simultaneously a younger Kaylie hallucinates her mother beckoning her from the mirror.


title: Oculus (film)

text: Tim activates the kill switch, realizing too late and unable to see that Kaylie stood in its path, and he has killed her. The police arrive and arrest Tim, who is hysterical, just as they did when he was younger. As both a boy and an adult, Tim claims the mirror is responsible. As he is taken away and put behind bars, Tim's adult incarnation sees Kaylie's ghost standing in the house with his parents.


title: Oculus (film)

text: "Oculus" was produced by Blumhouse Productions, WWE Studios, MICA Entertainment, Mist Entertainment, and Intrepid Pictures. During the scene in which the mirror is up for auction, the auctioneer mentions that the item was "recovered from the Levesque estate", a reference to WWE wrestler Triple H, whose real name is Paul Michael Levesque.


title: Oculus (film)

text: The film is based on Flanagan's earlier 2005 short horror film, "Oculus: Chapter 3 – The Man with the Plan". The short contained only one setting, a single actor, and a mirror. The short became highly acclaimed, and interest quickly arose regarding the adaptation of the short into a feature. Initially, studios were interested in making the film in accordance with the found footage genre; however, Flanagan was opposed to this and passed on such offers. Eventually, Intrepid Pictures expressed interest in producing the film "as long as you don't do it found footage".


title: Oculus (film)

text: Expanding the premise to a feature-length screenplay proved challenging, as Flanagan felt like he had "pushed the limit" of what could be done with the premise in the short. The solution Flanagan came across was to combine two storylines, past and present, intercut with one another. The idea was to "create a sense of distortion and disorientation that would be similar for the viewer as it was for Tim and Kaylie in the room." In early drafts, it was difficult to distinguish between the two timelines, until the team hit upon the idea of writing all of the scenes from the past in italics.


title: Oculus (film)

text: Inspired by the stories of H. P. Lovecraft, Flanagan chose to not explain the mirror's origins, explaining that he liked how Lovecraftian literature often seemed to be an "alien force that if you even were to try to comprehend it completely it would drive you mad." He expanded: "Evil in the world doesn't have an answer."


title: Oculus (film)

text: On July 12, 2012, it was announced that Karen Gillan, known for her work in "Doctor Who" and "Outcast", had been cast in the lead role of "Oculus". On September 20, 2012, Katee Sackhoff joined the cast as Marie, the mother of Gillan's character Kaylie. When writing the script for "Oculus", the character of Kaylie was based on Sackhoff's work on "Battlestar Galactica", and Flanagan was drawn to Gillan based on her work on "Doctor Who".


title: Oculus (film)

text: Brenton Thwaites was the last of the main cast to sign on to "Oculus", joining the project on October 5, 2012, after shooting for the production had already begun.


title: Oculus (film)

text: The film was first released on September 5, 2013, at the Toronto International Film Festival and received a worldwide theatrical release on April 11, 2014.


title: Oculus (film)

text: FilmDistrict acquired U.S. distribution rights to Oculus at the 2012 Cannes Film Festival, but later left the project due to an agreement which said the company would have to give the film a wide release, causing the film's U.S. distribution rights to be put up for sale again. On September 9, 2013, four days after Oculus' premiere at Toronto, Relativity Media acquired U.S. distribution rights to the film from Blumhouse and set it for a wide release.


title: Oculus (film)

text: The soundtrack to "Oculus" was composed by The Newton Brothers and released digitally on April 8, 2014, and on CD on April 15, 2014.


title: Oculus (film)

text: On review aggregator Rotten Tomatoes, 74% of critics have given the film a positive review based on 156 reviews, with an average rating of 6.50/10. The site's critics consensus reads, "With an emphasis on dread over gore and an ending that leaves the door wide open for sequels, "Oculus" could be just the first spine-tingling chapter in a new franchise for discerning horror fans." On Metacritic, the film has a weighted average score of 61 out of 100 based on 28 critics, indicating "generally favorable reviews". Audiences polled by CinemaScore gave the film an average grade of "C" on an A+ to F scale.


title: Oculus (film)

text: Richard Roeper of the "Chicago Sun-Times" wrote: ""Oculus" is one of the more elegant scary movies in recent memory." He also called it "a carefully paced, superbly photographed psychological thriller". Robert Abele of the "Los Angeles Times" wrote: "Less concerned with fake shocks and show-me violence than the grimly calibrated rotting of personalities, Oculus is one of the more intelligently nasty horror films in recent memory." Shock Till You Drop gave "Oculus" a positive review, stating that it was "smart and scary stuff". Mark Kermode of "The Observer" gave the film 3/5 stars, writing: "this unpretentiously efficient affair handles its dual-narrative past/present intercuts with aplomb and keeps a couple of nicely nasty tricks up its sleeve."


title: Oculus (film)

text: Film School Rejects gave a mixed review and stated that it was "well-acted, looks quite good, and manages some moments of entertainment, but as the minutes tick by it grows weaker and weaker until its final cheat is designed to allow for a shocker ending." Wendy Ide of "The Times" gave the film 2/5 stars, writing: "It's certainly worth taking a glance at this looking glass, but horror fans may find the reflection a little familiar. Substitute a videotape for the mirror and it's basically "Ring"."


title: Oculus (film)

text: Released in the United States on April 11, 2014, "Oculus" grossed $4,966,899 on its opening day, nearly equaling its production budget of $5 million. As of October 3, 2014, the film has taken in an estimated $27,695,246 at the North American box office and another $16,335,000 internationally for a worldwide total of $44,030,246.


title: Oculus (film)

text: In March 2015, Relativity Media, B4U Television Network, and Balaji Telefilms confirmed a Bollywood remake with the title "Zahhak". The title was later changed to "". This film is directed by Prawaal Raman and stars Huma Qureshi and Saqib Saleem. Director Mike Flanagan served as the executive producer. The film was released on June 2, 2017.


title: Kuiper belt

text: The Kuiper belt () is a circumstellar disc in the outer Solar System, extending from the orbit of Neptune at 30 astronomical units (AU) to approximately 50 AU from the Sun. It is similar to the asteroid belt, but is far larger—20 times as wide and 20–200 times as massive. Like the asteroid belt, it consists mainly of small bodies or remnants from when the Solar System formed. While many asteroids are composed primarily of rock and metal, most Kuiper belt objects are composed largely of frozen volatiles (termed "ices"), such as methane, ammonia, and water. The Kuiper belt is home to most of the objects that astronomers generally accept as dwarf planets: Orcus, Pluto, Haumea, Quaoar, and Makemake. Some of the Solar System's moons, such as Neptune's Triton and Saturn's Phoebe, may have originated in the region.


title: Kuiper belt

text: The Kuiper belt was named after Dutch astronomer Gerard Kuiper, although he did not predict its existence. In 1992, minor planet (15760) Albion was discovered, the first Kuiper belt object (KBO) since Pluto (in 1930) and Charon (in 1978). Since its discovery, the number of known KBOs has increased to thousands, and more than 100,000 KBOs over in diameter are thought to exist. The Kuiper belt was initially thought to be the main repository for periodic comets, those with orbits lasting less than 200 years. Studies since the mid-1990s have shown that the belt is dynamically stable and that comets' true place of origin is the scattered disc, a dynamically active zone created by the outward motion of Neptune 4.5 billion years ago; scattered disc objects such as Eris have extremely eccentric orbits that take them as far as 100 AU from the Sun.


title: Kuiper belt

text: The Kuiper belt is distinct from the hypothesized Oort cloud, which is believed to be a thousand times more distant and mostly spherical. The objects within the Kuiper belt, together with the members of the scattered disc and any potential Hills cloud or Oort cloud objects, are collectively referred to as trans-Neptunian objects (TNOs). Pluto is the largest and most massive member of the Kuiper belt and the largest and the second-most-massive known TNO, surpassed only by Eris in the scattered disc. Originally considered a planet, Pluto's status as part of the Kuiper belt caused it to be reclassified as a dwarf planet in 2006. It is compositionally similar to many other objects of the Kuiper belt, and its orbital period is characteristic of a class of KBOs, known as "plutinos," that share the same 2:3 resonance with Neptune.


title: Kuiper belt

text: The Kuiper belt and Neptune may be treated as a marker of the extent of the Solar System, alternatives being the heliopause and the distance at which the Sun's gravitational influence is matched by that of other stars (estimated to be between and ).


title: Kuiper belt

text: After the discovery of Pluto in 1930, many speculated that it might not be alone. The region now called the Kuiper belt was hypothesized in various forms for decades. It was only in 1992 that the first direct evidence for its existence was found. The number and variety of prior speculations on the nature of the Kuiper belt have led to continued uncertainty as to who deserves credit for first proposing it.


title: Kuiper belt

text: The first astronomer to suggest the existence of a trans-Neptunian population was Frederick C. Leonard. Soon after Pluto's discovery by Clyde Tombaugh in 1930, Leonard pondered whether it was "not likely that in Pluto there has come to light the "first" of a "series" of ultra-Neptunian bodies, the remaining members of which still await discovery but which are destined eventually to be detected". That same year, astronomer Armin O. Leuschner suggested that Pluto "may be one of many long-period planetary objects yet to be discovered."


title: Kuiper belt

text: In 1943, in the "Journal of the British Astronomical Association", Kenneth Edgeworth hypothesized that, in the region beyond Neptune, the material within the primordial solar nebula was too widely spaced to condense into planets, and so rather condensed into a myriad smaller bodies. From this he concluded that "the outer region of the solar system, beyond the orbits of the planets, is occupied by a very large number of comparatively small bodies" and that, from time to time, one of their number "wanders from its own sphere and appears as an occasional visitor to the inner solar system", becoming a comet.


title: Kuiper belt

text: In 1951, in a paper in "Astrophysics: A Topical Symposium", Gerard Kuiper speculated on a similar disc having formed early in the Solar System's evolution, but he did not think that such a belt still existed today. Kuiper was operating on the assumption, common in his time, that Pluto was the size of Earth and had therefore scattered these bodies out toward the Oort cloud or out of the Solar System. Were Kuiper's hypothesis correct, there would not be a Kuiper belt today.


title: Kuiper belt

text: The hypothesis took many other forms in the following decades. In 1962, physicist Al G.W. Cameron postulated the existence of "a tremendous mass of small material on the outskirts of the solar system". In 1964, Fred Whipple, who popularised the famous "dirty snowball" hypothesis for cometary structure, thought that a "comet belt" might be massive enough to cause the purported discrepancies in the orbit of Uranus that had sparked the search for Planet X, or, at the very least, massive enough to affect the orbits of known comets. Observation ruled out this hypothesis.


title: Kuiper belt

text: In 1977, Charles Kowal discovered 2060 Chiron, an icy planetoid with an orbit between Saturn and Uranus. He used a blink comparator, the same device that had allowed Clyde Tombaugh to discover Pluto nearly 50 years before. In 1992, another object, 5145 Pholus, was discovered in a similar orbit. Today, an entire population of comet-like bodies, called the centaurs, is known to exist in the region between Jupiter and Neptune. The centaurs' orbits are unstable and have dynamical lifetimes of a few million years. From the time of Chiron's discovery in 1977, astronomers have speculated that the centaurs therefore must be frequently replenished by some outer reservoir.


title: Kuiper belt

text: Further evidence for the existence of the Kuiper belt later emerged from the study of comets. That comets have finite lifespans has been known for some time. As they approach the Sun, its heat causes their volatile surfaces to sublimate into space, gradually dispersing them. In order for comets to continue to be visible over the age of the Solar System, they must be replenished frequently. A proposal for such an area of replenishment is the Oort cloud, possibly a spherical swarm of comets extending beyond 50,000 AU from the Sun first hypothesised by Dutch astronomer Jan Oort in 1950. The Oort cloud is thought to be the point of origin of long-period comets, which are those, like Hale–Bopp, with orbits lasting thousands of years.


title: Kuiper belt

text: There is another comet population, known as short-period or periodic comets, consisting of those comets that, like Halley's Comet, have orbital periods of less than 200 years. By the 1970s, the rate at which short-period comets were being discovered was becoming increasingly inconsistent with their having emerged solely from the Oort cloud. For an Oort cloud object to become a short-period comet, it would first have to be captured by the giant planets. In a paper published in "Monthly Notices of the Royal Astronomical Society" in 1980, Uruguayan astronomer Julio Fernández stated that for every short-period comet to be sent into the inner Solar System from the Oort cloud, 600 would have to be ejected into interstellar space. He speculated that a comet belt from between 35 and 50 AU would be required to account for the observed number of comets. Following up on Fernández's work, in 1988 the Canadian team of Martin Duncan, Tom Quinn and Scott Tremaine ran a number of computer simulations to determine if all observed comets could have arrived from the Oort cloud. They found that the Oort cloud could not account for all short-period comets, particularly as short-period comets are clustered near the plane of the Solar System, whereas Oort-cloud comets tend to arrive from any point in the sky. With a "belt", as Fernández described it, added to the formulations, the simulations matched observations. Reportedly because the words "Kuiper" and "comet belt" appeared in the opening sentence of Fernández's paper, Tremaine named this hypothetical region the "Kuiper belt".


title: Kuiper belt

text: In 1987, astronomer David Jewitt, then at MIT, became increasingly puzzled by "the apparent emptiness of the outer Solar System". He encouraged then-graduate student Jane Luu to aid him in his endeavour to locate another object beyond Pluto's orbit, because, as he told her, "If we don't, nobody will." Using telescopes at the Kitt Peak National Observatory in Arizona and the Cerro Tololo Inter-American Observatory in Chile, Jewitt and Luu conducted their search in much the same way as Clyde Tombaugh and Charles Kowal had, with a blink comparator. Initially, examination of each pair of plates took about eight hours, but the process was sped up with the arrival of electronic charge-coupled devices or CCDs, which, though their field of view was narrower, were not only more efficient at collecting light (they retained 90% of the light that hit them, rather than the 10% achieved by photographs) but allowed the blinking process to be done virtually, on a computer screen. Today, CCDs form the basis for most astronomical detectors. In 1988, Jewitt moved to the Institute of Astronomy at the University of Hawaii. Luu later joined him to work at the University of Hawaii's 2.24 m telescope at Mauna Kea. Eventually, the field of view for CCDs had increased to 1024 by 1024 pixels, which allowed searches to be conducted far more rapidly. Finally, after five years of searching, Jewitt and Luu announced on 30 August 1992 the "Discovery of the candidate Kuiper belt object 1992 QB". This object would later be named 15760 Albion. Six months later, they discovered a second object in the region, (181708) 1993 FW. By 2018, over 2000 Kuiper belts objects had been discovered.


title: Kuiper belt

text: Over one thousand bodies were found in a belt in the twenty years (1992–2012), after finding (named in 2018, 15760 Albion), showing a vast belt of bodies more than just Pluto and Albion. By the 2010s the full extent and nature of Kuiper belt bodies is largely unknown. Finally, in the late 2010s, two KBOs were closely flown past by an unmanned spacecraft, providing much closer observations of the Plutonian system and another KBO.


title: Kuiper belt

text: Studies conducted since the trans-Neptunian region was first charted have shown that the region now called the Kuiper belt is not the point of origin of short-period comets, but that they instead derive from a linked population called the scattered disc. The scattered disc was created when Neptune migrated outward into the proto-Kuiper belt, which at the time was much closer to the Sun, and left in its wake a population of dynamically stable objects that could never be affected by its orbit (the Kuiper belt proper), and a population whose perihelia are close enough that Neptune can still disturb them as it travels around the Sun (the scattered disc). Because the scattered disc is dynamically active and the Kuiper belt relatively dynamically stable, the scattered disc is now seen as the most likely point of origin for periodic comets.


title: Kuiper belt

text: Astronomers sometimes use the alternative name Edgeworth–Kuiper belt to credit Edgeworth, and KBOs are occasionally referred to as EKOs. Brian G. Marsden claims that neither deserves true credit: "Neither Edgeworth nor Kuiper wrote about anything remotely like what we are now seeing, but Fred Whipple did". David Jewitt comments: "If anything ... Fernández most nearly deserves the credit for predicting the Kuiper Belt."


title: Kuiper belt

text: KBOs are sometimes called "kuiperoids", a name suggested by Clyde Tombaugh. The term "trans-Neptunian object" (TNO) is recommended for objects in the belt by several scientific groups because the term is less controversial than all others—it is not an exact synonym though, as TNOs include all objects orbiting the Sun past the orbit of Neptune, not just those in the Kuiper belt.


title: Kuiper belt

text: At its fullest extent (but excluding the scattered disc), including its outlying regions, the Kuiper belt stretches from roughly 30–55 AU. The main body of the belt is generally accepted to extend from the 2:3 mean-motion resonance (see below) at 39.5 AU to the 1:2 resonance at roughly 48 AU. The Kuiper belt is quite thick, with the main concentration extending as much as ten degrees outside the ecliptic plane and a more diffuse distribution of objects extending several times farther. Overall it more resembles a torus or doughnut than a belt. Its mean position is inclined to the ecliptic by 1.86 degrees.


title: Kuiper belt

text: The presence of Neptune has a profound effect on the Kuiper belt's structure due to orbital resonances. Over a timescale comparable to the age of the Solar System, Neptune's gravity destabilises the orbits of any objects that happen to lie in certain regions, and either sends them into the inner Solar System or out into the scattered disc or interstellar space. This causes the Kuiper belt to have pronounced gaps in its current layout, similar to the Kirkwood gaps in the asteroid belt. In the region between 40 and 42 AU, for instance, no objects can retain a stable orbit over such times, and any observed in that region must have migrated there relatively recently.


title: Kuiper belt

text: Between the 2:3 and 1:2 resonances with Neptune, at approximately 42–48 AU, the gravitational interactions with Neptune occur over an extended timescale, and objects can exist with their orbits essentially unaltered. This region is known as the classical Kuiper belt, and its members comprise roughly two thirds of KBOs observed to date. Because the first modern KBO discovered (Albion, but long called (15760) 1992 QB), is considered the prototype of this group, classical KBOs are often referred to as cubewanos ("Q-B-1-os"). The guidelines established by the IAU demand that classical KBOs be given names of mythological beings associated with creation.


title: Kuiper belt

text: The classical Kuiper belt appears to be a composite of two separate populations. The first, known as the "dynamically cold" population, has orbits much like the planets; nearly circular, with an orbital eccentricity of less than 0.1, and with relatively low inclinations up to about 10° (they lie close to the plane of the Solar System rather than at an angle). The cold population also contains a concentration of objects, referred to as the kernel, with semi-major axes at 44–44.5 AU. The second, the "dynamically hot" population, has orbits much more inclined to the ecliptic, by up to 30°. The two populations have been named this way not because of any major difference in temperature, but from analogy to particles in a gas, which increase their relative velocity as they become heated up. Not only are the two populations in different orbits, the cold population also differs in color and albedo, being redder and brighter, has a larger fraction of binary objects, has a different size distribution, and lacks very large objects. The mass of the dynamically cold population is roughly 30 times less than the mass of the hot. The difference in colors may be a reflection of different compositions, which suggests they formed in different regions. The hot population is proposed to have formed near Neptune's original orbit and to have been scattered out during the migration of the giant planets. The cold population, on the other hand, has been proposed to have formed more or less in its current position because the loose binaries would be unlikely to survive encounters with Neptune. Although the Nice model appears to be able to at least partially explain a compositional difference, it has also been suggested the color difference may reflect differences in surface evolution.


title: Kuiper belt

text: When an object's orbital period is an exact ratio of Neptune's (a situation called a mean-motion resonance), then it can become locked in a synchronised motion with Neptune and avoid being perturbed away if their relative alignments are appropriate. If, for instance, an object orbits the Sun twice for every three Neptune orbits, and if it reaches perihelion with Neptune a quarter of an orbit away from it, then whenever it returns to perihelion, Neptune will always be in about the same relative position as it began, because it will have completed orbits in the same time. This is known as the 2:3 (or 3:2) resonance, and it corresponds to a characteristic semi-major axis of about 39.4 AU. This 2:3 resonance is populated by about 200 known objects, including Pluto together with its moons. In recognition of this, the members of this family are known as plutinos. Many plutinos, including Pluto, have orbits that cross that of Neptune, although their resonance means they can never collide. Plutinos have high orbital eccentricities, suggesting that they are not native to their current positions but were instead thrown haphazardly into their orbits by the migrating Neptune. IAU guidelines dictate that all plutinos must, like Pluto, be named for underworld deities. The 1:2 resonance (whose objects complete half an orbit for each of Neptune's) corresponds to semi-major axes of ~47.7 AU, and is sparsely populated. Its residents are sometimes referred to as twotinos. Other resonances also exist at 3:4, 3:5, 4:7, and 2:5. Neptune has a number of trojan objects, which occupy its Lagrangian points, gravitationally stable regions leading and trailing it in its orbit. Neptune trojans are in a 1:1 mean-motion resonance with Neptune and often have very stable orbits.


title: Kuiper belt

text: Additionally, there is a relative absence of objects with semi-major axes below 39 AU that cannot apparently be explained by the present resonances. The currently accepted hypothesis for the cause of this is that as Neptune migrated outward, unstable orbital resonances moved gradually through this region, and thus any objects within it were swept up, or gravitationally ejected from it.


title: Kuiper belt

text: The 1:2 resonance at 47.8 AU appears to be an edge beyond which few objects are known. It is not clear whether it is actually the outer edge of the classical belt or just the beginning of a broad gap. Objects have been detected at the 2:5 resonance at roughly 55 AU, well outside the classical belt; predictions of a large number of bodies in classical orbits between these resonances have not been verified through observation.


title: Kuiper belt

text: Based on estimations of the primordial mass required to form Uranus and Neptune, as well as bodies as large as Pluto "(see )", earlier models of the Kuiper belt had suggested that the number of large objects would increase by a factor of two beyond 50 AU, so this sudden drastic falloff, known as the "Kuiper cliff", was unexpected, and to date its cause is unknown. Bernstein, Trilling, et al. (2003) found evidence that the rapid decline in objects of 100 km or more in radius beyond 50 AU is real, and not due to observational bias. Possible explanations include that material at that distance was too scarce or too scattered to accrete into large objects, or that subsequent processes removed or destroyed those that did. Patryk Lykawka of Kobe University claimed that the gravitational attraction of an unseen large planetary object, perhaps the size of Earth or Mars, might be responsible.


title: Kuiper belt

text: The precise origins of the Kuiper belt and its complex structure are still unclear, and astronomers are awaiting the completion of several wide-field survey telescopes such as Pan-STARRS and the future LSST, which should reveal many currently unknown KBOs. These surveys will provide data that will help determine answers to these questions. Pan-STARRS 1 finished its primary science mission in 2014, and the full data from the Pan-STARRS 1 surveys were published in 2019, helping reveal many more KBOs.


title: Kuiper belt

text: The Kuiper belt is thought to consist of planetesimals, fragments from the original protoplanetary disc around the Sun that failed to fully coalesce into planets and instead formed into smaller bodies, the largest less than in diameter. Studies of the crater counts on Pluto and Charon revealed a scarcity of small craters suggesting that such objects formed directly as sizeable objects in the range of tens of kilometers in diameter rather than being accreted from much smaller, roughly kilometer scale bodies. Hypothetical mechanisms for the formation of these larger bodies include the gravitational collapse of clouds of pebbles concentrated between eddies in a turbulent protoplanetary disk or in streaming instabilities. These collapsing clouds may fragment, forming binaries.


title: Kuiper belt

text: Modern computer simulations show the Kuiper belt to have been strongly influenced by Jupiter and Neptune, and also suggest that neither Uranus nor Neptune could have formed in their present positions, because too little primordial matter existed at that range to produce objects of such high mass. Instead, these planets are estimated to have formed closer to Jupiter. Scattering of planetesimals early in the Solar System's history would have led to migration of the orbits of the giant planets: Saturn, Uranus, and Neptune drifted outwards, whereas Jupiter drifted inwards. Eventually, the orbits shifted to the point where Jupiter and Saturn reached an exact 1:2 resonance; Jupiter orbited the Sun twice for every one Saturn orbit. The gravitational repercussions of such a resonance ultimately destabilized the orbits of Uranus and Neptune, causing them to be scattered outward onto high-eccentricity orbits that crossed the primordial planetesimal disc.


title: Kuiper belt

text: While Neptune's orbit was highly eccentric, its mean-motion resonances overlapped and the orbits of the planetesimals evolved chaotically, allowing planetesimals to wander outward as far as Neptune's 1:2 resonance to form a dynamically cold belt of low-inclination objects. Later, after its eccentricity decreased, Neptune's orbit expanded outward toward its current position. Many planetesimals were captured into and remain in resonances during this migration, others evolved onto higher-inclination and lower-eccentricity orbits and escaped from the resonances onto stable orbits. Many more planetesimals were scattered inward, with small fractions being captured as Jupiter trojans, as irregular satellites orbiting the giant planets, and as outer belt asteroids. The remainder were scattered outward again by Jupiter and in most cases ejected from the Solar System reducing the primordial Kuiper belt population by 99% or more.


title: Kuiper belt

text: The original version of the currently most popular model, the "Nice model", reproduces many characteristics of the Kuiper belt such as the "cold" and "hot" populations, resonant objects, and a scattered disc, but it still fails to account for some of the characteristics of their distributions. The model predicts a higher average eccentricity in classical KBO orbits than is observed (0.10–0.13 versus 0.07) and its predicted inclination distribution contains too few high inclination objects. In addition, the frequency of binary objects in the cold belt, many of which are far apart and loosely bound, also poses a problem for the model. These are predicted to have been separated during encounters with Neptune, leading some to propose that the cold disc formed at its current location, representing the only truly local population of small bodies in the solar system.


title: Kuiper belt

text: A recent modification of the Nice model has the Solar System begin with five giant planets, including an additional ice giant, in a chain of mean-motion resonances. About 400 million years after the formation of the Solar System the resonance chain is broken. Instead of being scattered into the disc, the ice giants first migrate outward several AU. This divergent migration eventually leads to a resonance crossing, destabilizing the orbits of the planets. The extra ice giant encounters Saturn and is scattered inward onto a Jupiter-crossing orbit and after a series of encounters is ejected from the Solar System. The remaining planets then continue their migration until the planetesimal disc is nearly depleted with small fractions remaining in various locations.


title: Kuiper belt

text: As in the original Nice model, objects are captured into resonances with Neptune during its outward migration. Some remain in the resonances, others evolve onto higher-inclination, lower-eccentricity orbits, and are released onto stable orbits forming the dynamically hot classical belt. The hot belt's inclination distribution can be reproduced if Neptune migrated from 24 AU to 30 AU on a 30 Myr timescale. When Neptune migrates to 28 AU, it has a gravitational encounter with the extra ice giant. Objects captured from the cold belt into the 1:2 mean-motion resonance with Neptune are left behind as a local concentration at 44 AU when this encounter causes Neptune's semi-major axis to jump outward. The objects deposited in the cold belt include some loosely bound 'blue' binaries originating from closer than the cold belt's current location. If Neptune's eccentricity remains small during this encounter, the chaotic evolution of orbits of the original Nice model is avoided and a primordial cold belt is preserved. In the later phases of Neptune's migration, a slow sweeping of mean-motion resonances removes the higher-eccentricity objects from the cold belt, truncating its eccentricity distribution.


title: Kuiper belt

text: Being distant from the Sun and major planets, Kuiper belt objects are thought to be relatively unaffected by the processes that have shaped and altered other Solar System objects; thus, determining their composition would provide substantial information on the makeup of the earliest Solar System. Due to their small size and extreme distance from Earth, the chemical makeup of KBOs is very difficult to determine. The principal method by which astronomers determine the composition of a celestial object is spectroscopy. When an object's light is broken into its component colors, an image akin to a rainbow is formed. This image is called a spectrum. Different substances absorb light at different wavelengths, and when the spectrum for a specific object is unravelled, dark lines (called absorption lines) appear where the substances within it have absorbed that particular wavelength of light. Every element or compound has its own unique spectroscopic signature, and by reading an object's full spectral "fingerprint", astronomers can determine its composition.


title: Kuiper belt

text: Analysis indicates that Kuiper belt objects are composed of a mixture of rock and a variety of ices such as water, methane, and ammonia. The temperature of the belt is only about 50 K, so many compounds that would be gaseous closer to the Sun remain solid. The densities and rock–ice fractions are known for only a small number of objects for which the diameters and the masses have been determined. The diameter can be determined by imaging with a high-resolution telescope such as the Hubble Space Telescope, by the timing of an occultation when an object passes in front of a star or, most commonly, by using the albedo of an object calculated from its infrared emissions. The masses are determined using the semi-major axes and periods of satellites, which are therefore known only for a few binary objects. The densities range from less than 0.4 to 2.6 g/cm. The least dense objects are thought to be largely composed of ice and have significant porosity. The densest objects are likely composed of rock with a thin crust of ice. There is a trend of low densities for small objects and high densities for the largest objects. One possible explanation for this trend is that ice was lost from the surface layers when differentiated objects collided to form the largest objects.


title: Kuiper belt

text: Initially, detailed analysis of KBOs was impossible, and so astronomers were only able to determine the most basic facts about their makeup, primarily their color. These first data showed a broad range of colors among KBOs, ranging from neutral grey to deep red. This suggested that their surfaces were composed of a wide range of compounds, from dirty ices to hydrocarbons. This diversity was startling, as astronomers had expected KBOs to be uniformly dark, having lost most of the volatile ices from their surfaces to the effects of cosmic rays. Various solutions were suggested for this discrepancy, including resurfacing by impacts or outgassing. Jewitt and Luu's spectral analysis of the known Kuiper belt objects in 2001 found that the variation in color was too extreme to be easily explained by random impacts. The radiation from the Sun is thought to have chemically altered methane on the surface of KBOs, producing products such as tholins. Makemake has been shown to possess a number of hydrocarbons derived from the radiation-processing of methane, including ethane, ethylene and acetylene.


title: Kuiper belt

text: Although to date most KBOs still appear spectrally featureless due to their faintness, there have been a number of successes in determining their composition. In 1996, Robert H. Brown et al. acquired spectroscopic data on the KBO 1993 SC, which revealed that its surface composition is markedly similar to that of Pluto, as well as Neptune's moon Triton, with large amounts of methane ice. For the smaller objects, only colors and in some cases the albedos have been determined. These objects largely fall into two classes: gray with low albedos, or very red with higher albedos. The difference in colors and albedos is hypothesized to be due to the retention or the loss of hydrogen sulfide (HS) on the surface of these objects, with the surfaces of those that formed far enough from the Sun to retain HS being reddened due to irradiation.


title: Kuiper belt

text: The largest KBOs, such as Pluto and Quaoar, have surfaces rich in volatile compounds such as methane, nitrogen and carbon monoxide; the presence of these molecules is likely due to their moderate vapor pressure in the 30–50 K temperature range of the Kuiper belt. This allows them to occasionally boil off their surfaces and then fall again as snow, whereas compounds with higher boiling points would remain solid. The relative abundances of these three compounds in the largest KBOs is directly related to their surface gravity and ambient temperature, which determines which they can retain. Water ice has been detected in several KBOs, including members of the Haumea family such as , mid-sized objects such as 38628 Huya and 20000 Varuna, and also on some small objects. The presence of crystalline ice on large and mid-sized objects, including 50000 Quaoar where ammonia hydrate has also been detected, may indicate past tectonic activity aided by melting point lowering due to the presence of ammonia.


title: Kuiper belt

text: Despite its vast extent, the collective mass of the Kuiper belt is relatively low. The total mass of the dynamically hot population is estimated to be 1% the mass of the Earth. The dynamically cold population is estimated to be much smaller with only 0.03% the mass of the Earth. While the dynamically hot population is thought to be the remnant of a much larger population that formed closer to the Sun and was scattered outward during the migration of the giant planets, in contrast, the dynamically cold population is thought to have formed at its current location. The most recent estimate (2018) puts the total mass of the Kuiper belt at Earth masses based on the influence that it exerts on the motion of planets.


title: Kuiper belt

text: The small total mass of the dynamically cold population presents some problems for models of the Solar System's formation because a sizable mass is required for accretion of KBOs larger than in diameter. If the cold classical Kuiper belt had always had its current low density, these large objects simply could not have formed by the collision and mergers of smaller planetesimals. Moreover, the eccentricity and inclination of current orbits make the encounters quite "violent" resulting in destruction rather than accretion. The removal of a large fraction of the mass of the dynamically cold population is thought to be unlikely. Neptune's current influence is too weak to explain such a massive "vacuuming", and the extent of mass loss by collisional grinding is limited by the presence of loosely bound binaries in the cold disk, which are likely to be disrupted in collisions. Instead of forming from the collisions of smaller planetesimals, the larger object may have formed directly from the collapse of clouds of pebbles.


title: Kuiper belt

text: The size distributions of the Kuiper belt objects follow a number of power laws. A power law describes the relationship between "N"("D") (the number of objects of diameter greater than "D") and "D", and is referred to as brightness slope. The number of objects is inversely proportional to some power of the diameter "D":


title: Kuiper belt

text: Early estimates that were based on measurements of the apparent magnitude distribution found a value of q = 4 ± 0.5, which implied that there are 8 (=2) times more objects in the 100–200 km range than in the 200–400 km range.


title: Kuiper belt

text: Recent research has revealed that the size distributions of the hot classical and cold classical objects have differing slopes. The slope for the hot objects is q = 5.3 at large diameters and q = 2.0 at small diameters with the change in slope at 110 km. The slope for the cold objects is q = 8.2 at large diameters and q = 2.9 at small diameters with a change in slope at 140 km. The size distributions of the scattering objects, the plutinos, and the Neptune trojans have slopes similar to the other dynamically hot populations, but may instead have a divot, a sharp decrease in the number of objects below a specific size. This divot is hypothesized to be due to either the collisional evolution of the population, or to be due to the population having formed with no objects below this size, with the smaller objects being fragments of the original objects.


title: Kuiper belt

text: The smallest known Kuiper belt objects with radii below 1 km have only been detected by stellar occultations, as they are far too dim (magnitude 35) to be seen directly by telescopes such as the Hubble Space Telescope. The first reports of these occultations were from Schlichting et al. in December 2009, who announced the discovery of a small, sub-kilometre-radius Kuiper belt object in archival "Hubble" photometry from March 2007. With an estimated radius of or a diameter of , the object was detected by "Hubble" star tracking system when it briefly occulted a star for 0.3 seconds. In a subsequent study published in December 2012, Schlichting et al. performed a more thorough analysis of archival "Hubble" photometry and reported another occultation event by a sub-kilometre-sized Kuiper belt object, estimated to be in radius or in diameter. From the occultation events detected in 2009 and 2012, Schlichting et al. determined the Kuiper belt object size distribution slope to be q = 3.6 ± 0.2 or q = 3.8 ± 0.2, with the assumptions of a single power law and a uniform ecliptic latitude distribution. Their result implies a strong deficit of sub-kilometer-sized Kuiper belt objects compared to extrapolations from the population of larger Kuiper belt objects with diameters above 90 km.


title: Kuiper belt

text: The scattered disc is a sparsely populated region, overlapping with the Kuiper belt but extending to beyond 100 AU. Scattered disc objects (SDOs) have very elliptical orbits, often also very inclined to the ecliptic. Most models of Solar System formation show both KBOs and SDOs first forming in a primordial belt, with later gravitational interactions, particularly with Neptune, sending the objects outward, some into stable orbits (the KBOs) and some into unstable orbits, the scattered disc. Due to its unstable nature, the scattered disc is suspected to be the point of origin of many of the Solar System's short-period comets. Their dynamic orbits occasionally force them into the inner Solar System, first becoming centaurs, and then short-period comets.


title: Kuiper belt

text: According to the Minor Planet Center, which officially catalogues all trans-Neptunian objects, a KBO is any object that orbits exclusively within the defined Kuiper belt region regardless of origin or composition. Objects found outside the belt are classed as scattered objects. In some scientific circles the term "Kuiper belt object" has become synonymous with any icy minor planet native to the outer Solar System assumed to have been part of that initial class, even if its orbit during the bulk of Solar System history has been beyond the Kuiper belt (e.g. in the scattered-disc region). They often describe scattered disc objects as "scattered Kuiper belt objects". Eris, which is known to be more massive than Pluto, is often referred to as a KBO, but is technically an SDO. A consensus among astronomers as to the precise definition of the Kuiper belt has yet to be reached, and this issue remains unresolved.


title: Kuiper belt

text: The centaurs, which are not normally considered part of the Kuiper belt, are also thought to be scattered objects, the only difference being that they were scattered inward, rather than outward. The Minor Planet Center groups the centaurs and the SDOs together as scattered objects.


title: Kuiper belt

text: During its period of migration, Neptune is thought to have captured a large KBO, Triton, which is the only large moon in the Solar System with a retrograde orbit (it orbits opposite to Neptune's rotation). This suggests that, unlike the large moons of Jupiter, Saturn and Uranus, which are thought to have coalesced from rotating discs of material around their young parent planets, Triton was a fully formed body that was captured from surrounding space. Gravitational capture of an object is not easy: it requires some mechanism to slow down the object enough to be caught by the larger object's gravity. A possible explanation is that Triton was part of a binary when it encountered Neptune. (Many KBOs are members of binaries. See below.) Ejection of the other member of the binary by Neptune could then explain Triton's capture. Triton is only 14% larger than Pluto, and spectral analysis of both worlds shows that their surfaces are largely composed of similar materials, such as methane and carbon monoxide. All this points to the conclusion that Triton was once a KBO that was captured by Neptune during its outward migration.


title: Kuiper belt

text: Since 2000, a number of KBOs with diameters of between 500 and , more than half that of Pluto (diameter 2370 km), have been discovered. 50000 Quaoar, a classical KBO discovered in 2002, is over 1,200 km across. and , both announced on 29 July 2005, are larger still. Other objects, such as 28978 Ixion (discovered in 2001) and 20000 Varuna (discovered in 2000), measure roughly across.


title: Kuiper belt

text: The discovery of these large KBOs in orbits similar to Pluto's led many to conclude that, aside from its relative size, Pluto was not particularly different from other members of the Kuiper belt. Not only are these objects similar to Pluto in size, but many also have satellites, and are of similar composition (methane and carbon monoxide have been found both on Pluto and on the largest KBOs). Thus, just as Ceres was considered a planet before the discovery of its fellow asteroids, some began to suggest that Pluto might also be reclassified.


title: Kuiper belt

text: The issue was brought to a head by the discovery of Eris, an object in the scattered disc far beyond the Kuiper belt, that is now known to be 27% more massive than Pluto. (Eris was originally thought to be larger than Pluto by volume, but the "New Horizons" mission found this not to be the case.) In response, the International Astronomical Union (IAU) was forced to define what a planet is for the first time, and in so doing included in their definition that a planet must have "cleared the neighbourhood around its orbit". As Pluto shares its orbit with many other sizable objects, it was deemed not to have cleared its orbit and was thus reclassified from a planet to a dwarf planet, making it a member of the Kuiper belt.


title: Kuiper belt

text: Although Pluto is currently the largest known KBO, there is at least one known larger object currently outside the Kuiper belt that probably originated in it: Neptune's moon Triton (which, as explained above, is probably a captured KBO).


title: Kuiper belt

text: It is not clear how many KBOs are large enough to be dwarf planets. Consideration of the surprisingly low densities of many dwarf-planet candidates suggests that not many are. , Pluto, Haumea, , and Makemake are accepted by most astronomers; some have proposed other bodies, such as , , , and .


title: Kuiper belt

text: The six largest TNOs (Eris, Pluto, Gonggong, Makemake, Haumea and Quaoar) are all known to have satellites, and two of them have more than one. A higher percentage of the larger KBOs have satellites than the smaller objects in the Kuiper belt, suggesting that a different formation mechanism was responsible. There are also a high number of binaries (two objects close enough in mass to be orbiting "each other") in the Kuiper belt. The most notable example is the Pluto–Charon binary, but it is estimated that around 11% of KBOs exist in binaries.


title: Kuiper belt

text: On 19 January 2006, the first spacecraft to explore the Kuiper belt, "New Horizons", was launched, which flew by Pluto on 14 July 2015. Beyond the Pluto flyby, the mission's goal was to locate and investigate other, farther objects in the Kuiper belt.


title: Kuiper belt

text: On 15 October 2014, it was revealed that "Hubble" had uncovered three potential targets, provisionally designated PT1 ("potential target 1"), PT2 and PT3 by the "New Horizons" team. The objects' diameters were estimated to be in the 30–55 km range; too small to be seen by ground telescopes, at distances from the Sun of 43–44 AU, which would put the encounters in the 2018–2019 period. The initial estimated probabilities that these objects were reachable within "New Horizons" fuel budget were 100%, 7%, and 97%, respectively. All were members of the "cold" (low-inclination, low-eccentricity) classical Kuiper belt, and thus very different from Pluto. PT1 (given the temporary designation "1110113Y" on the HST web site), the most favorably situated object, was magnitude 26.8, 30–45 km in diameter, and was encountered in January 2019. Once sufficient orbital information was provided, the Minor Planet Center gave official designations to the three target KBOs: (PT1), (PT2), and (PT3). By the fall of 2014, a possible fourth target, , had been eliminated by follow-up observations. PT2 was out of the running before the Pluto flyby.


title: Kuiper belt

text: On 26 August 2015, the first target, (nicknamed "Ultima Thule" and later named 486958 Arrokoth), was chosen. Course adjustment took place in late October and early November 2015, leading to a flyby in January 2019. On 1 July 2016, NASA approved additional funding for "New Horizons" to visit the object.


title: Kuiper belt

text: On 2 December 2015, "New Horizons" detected what was then called (later named "15810 Arawn") from away.


title: Kuiper belt

text: On 1 January 2019, "New Horizons" successfully flew by Arrokoth, returning data showing Arrokoth to be a contact binary 32 km long by 16 km wide. The Ralph instrument aboard "New Horizons" confirmed Arrokoth's red color. Data from the fly-by will continue to be downloaded over the next 20 months.


title: Kuiper belt

text: No follow-up missions for "New Horizons" are planned, though at least two concepts for missions that would return to orbit or land on Pluto have been studied. Beyond Pluto, there exist many large KBOs that cannot be visited with "New Horizons", such as the dwarf planets Makemake and Haumea. New missions would be tasked to explore and study these objects in detail. Thales Alenia Space has studied the logistics of an orbiter mission to Haumea, a high priority scientific target due to its status as the parent body of a collisional family that includes several other TNOs, as well as Haumea's ring and two moons. The lead author, Joel Poncy, has advocated for new technology that would allow spacecraft to reach and orbit KBOs in 10–20 years or less. "New Horizons" Principal Investigator Alan Stern has informally suggested missions that would flyby the planets Uranus or Neptune before visiting new KBO targets, thus furthering the exploration of the Kuiper belt while also visiting these ice giant planets for the first time since the "Voyager 2" flybys in the 1980s.


title: Kuiper belt

text: Quaoar has been considered as a flyby target for a probe tasked with exploring the interstellar medium, as it currently lies near the heliospheric nose; Pontus Brandt at Johns Hopkins Applied Physics Laboratory and his colleagues have studied a probe that would flyby Quaoar in the 2030s before continuing to the interstellar medium through the heliospheric nose. Among their interests in Quaoar include its likely disappearing methane atmosphere and cryovolcanism. The mission studied by Brandt and his colleagues would launch using SLS and achieve 30 km/s using a Jupiter flyby. Alternatively, for an orbiter mission, a study published in 2012 concluded that Ixion and Huya are among the most feasible targets. For instance, the authors calculated that an orbiter mission could reach Ixion after 17 years cruise time if launched in 2039.


title: Kuiper belt

text: In the late 2010s, a design study by Glen Costigan and colleagues discussed orbital capture and multi-target scenarios for Kuiper belt objects. Some Kuiper belt objects studied in that particular paper included , , and 47171 Lempo. Another design study by Ryan McGranaghan and colleagues in 2011 explored a spacecraft survey of the large trans-Neptunian objects Quaoar, Sedna, Makemake, Haumea, and Eris.


title: Kuiper belt

text: Interstellar missions have evaluated including a flyby of Kuiper Belt objects as part of their mission.


title: Kuiper belt

text: By 2006, astronomers had resolved dust discs thought to be Kuiper belt-like structures around nine stars other than the Sun. They appear to fall into two categories: wide belts, with radii of over 50 AU, and narrow belts (tentatively like that of the Solar System) with radii of between 20 and 30 AU and relatively sharp boundaries. Beyond this, 15–20% of solar-type stars have an observed infrared excess that is suggestive of massive Kuiper-belt-like structures. Most known debris discs around other stars are fairly young, but the two images on the right, taken by the Hubble Space Telescope in January 2006, are old enough (roughly 300 million years) to have settled into stable configurations. The left image is a "top view" of a wide belt, and the right image is an "edge view" of a narrow belt. Computer simulations of dust in the Kuiper belt suggest that when it was younger, it may have resembled the narrow rings seen around younger stars.


title: 1971 Bangladesh genocide

text: The genocide in Bangladesh began on 25 March 1971 with the launch of Operation Searchlight, as the government of Pakistan, dominated by West Pakistan, began a military crackdown on East Pakistan (now Bangladesh) to suppress Bengali calls for self-determination. During the nine-month-long Bangladesh Liberation War, members of the Pakistan Armed Forces and supporting pro-Pakistani Islamist militias from Jamaat-e-Islami killed between 300,000 and 3,000,000 people and raped between 200,000 and 400,000 Bengali women, in a systematic campaign of genocidal rape. The Government of Bangladesh states 3,000,000 people were killed during the genocide, making it the largest genocide since the Holocaust during World War II.


title: 1971 Bangladesh genocide

text: The actions against women were supported by Pakistan's religious leaders, who declared that Bengali women were "gonimoter maal" (Bengali for "public property"). As a result of the conflict, a further eight to ten million people fled the country to seek refuge in neighbouring India. It is estimated that up to 30 million civilians were internally displaced out of 70 million. During the war, there was also ethnic violence between Bengalis and Urdu-speaking Biharis. Biharis faced reprisals from Bengali mobs and militias, and from 1,000 to 150,000 were killed.


title: 1971 Bangladesh genocide

text: There is an academic consensus that the events which took place during the Bangladesh Liberation War constituted a genocide; however, there are some scholars and authors who disagree that the killing was a genocide.


title: 1971 Bangladesh genocide

text: Following the partition of India, the new state of Pakistan represented a geographical anomaly, with two wings separated by of Indian territory. The wings were not only separated geographically, but also culturally. The authorities of the West viewed the Bengali Muslims in the East as "too 'Bengali'" and their application of Islam as "inferior and impure", believing this made the Bengalis unreliable "co-religionists". To this extent politicians in West Pakistan began a strategy to forcibly assimilate the Bengalis culturally.


title: 1971 Bangladesh genocide

text: The Bengali people were the demographic majority in Pakistan, making up an estimated 75 million in East Pakistan, compared with 55 million in the predominantly Punjabi-speaking West Pakistan. The majority in the East were Muslim, with large minorities of Hindus, Buddhists and Christians. The West considered the people of the East to be second-class citizens, and Amir Abdullah Khan Niazi, who served as head of the Pakistani Forces in East Pakistan in 1971, referred to Bengalis as inferior to Pathans and Punjabis.


title: 1971 Bangladesh genocide

text: In 1948, a few months after the creation of Pakistan, Governor-General Mohammad Ali Jinnah declared Urdu as the national language of the newly formed state, although only four per cent of Pakistan's population spoke Urdu at that time. He mentioned that the people of East Bengal could choose what would be its provincial language, and branded those who were against the use of Urdu as the national language of Pakistan as communists, traitors and enemies of the state. The refusal by successive governments to recognise Bengali as the second national language culminated in the Bengali language movement and strengthened support for the newly formed Awami League, which was founded in the East as an alternative to the ruling Muslim League. A 1952 protest in Dhaka, the capital of East Pakistan, was forcibly broken up, resulting in the deaths of several protesters. Bengali nationalists viewed those who had died as martyrs for their cause, and the violence led to calls for secession. The Indo-Pakistani War of 1965 caused further grievances, as the military had assigned no extra units to the defence of the East. This was a matter of concern to the Bengalis who saw their nation undefended in case of Indian attack during the conflict of 1965, and that Ayub Khan, the President of Pakistan, was willing to lose the East if it meant gaining Kashmir.


title: 1971 Bangladesh genocide

text: The slow response to the Bhola cyclone which struck on 12 November 1970 is widely seen as a contributing factor in the December 1970 general election. The East Pakistan-based Awami League, headed by Sheikh Mujibur Rahman, won a national majority in the first democratic election since the creation of Pakistan, sweeping East Pakistan. But, the West Pakistani establishment prevented them from forming a government. President Yahya Khan, encouraged by Zulfikar Ali Bhutto, banned the Awami League and declared martial law. The Pakistani Army demolished Ramna Kali Mandir (temple) and killed 85 Hindus. On 22 February 1971, General Yahya Khan is reported to have said "Kill three million of them, and the rest will eat out of our hands."


title: 1971 Bangladesh genocide

text: Some Bengalis supported a united Pakistan and opposed secession from it. According to Indian academic Sarmila Bose, these pro-Pakistan Bengalis constituted a significant minority, and included the Islamic parties. Moreover, many Awami League voters who hoped to achieve provincial autonomy may not have desired secession. Additionally, some Bengali officers and soldiers remained loyal to the Pakistani Army and were taken as prisoners of war by India along with other West Pakistani soldiers. Thus, according to Sarmila Bose, there were many pro-regime Bengalis who killed and persecuted the pro-liberation fighters. Sydney Schanberg reported the formation of armed civilian units by the Pakistani Army in June 1971. Only a minority of the recruits were Bengali, while most were Biharis and Urdu speakers. The units with local knowledge played an important role in the implementation of the Pakistani Army's genocide. American writer Gary J. Bass believes that the breakup of Pakistan was not inevitable, identifying 25 March 1971 as the point where the idea of a united Pakistan ended for Bengalis with the start of military operations. According to John H. Gill, since there was widespread polarisation between pro-Pakistan Bengalis and pro-liberation Bengalis during the war, those internal battles are still playing out in the domestic politics of modern-day Bangladesh.


title: 1971 Bangladesh genocide

text: Operation Searchlight was a planned military operation carried out by the Pakistani Army to curb elements of the separatist Bengali nationalist movement in East Pakistan in March 1971. The Pakistani state justified commencing Operation Searchlight on the basis of anti-Bihari violence by Bengalis in early March. Ordered by the government in West Pakistan, this was seen as the sequel to Operation Blitz which had been launched in November 1970. On 1 March 1971 East Pakistan governor Admiral Syed Mohammed Ahsan was replaced after disagreeing with military action in East Pakistan. His successor Sahibzada Yaqub Khan resigned after refusing to use soldiers to quell a mutiny and disagreement with military action in East Pakistan.


title: 1971 Bangladesh genocide

text: According to Indian academic Sarmila Bose, the postponement of the National Assembly on 1 March led to widespread lawlessness spread by Bengali protesters during the period of 1–25 March, in which the Pakistani government lost control over much of the province. Bose asserts that during this 25-day period of lawlessness, attacks by Bengalis on non-Bengalis were common as well as attacks by Bengalis on Pakistani military personnel who, according to Bose and Anthony Mascarenhas, showed great restraint until 25 March, when Operation Searchlight began. Bose also described the atrocities committed by the Pakistani Army in her book. According to Anthony Mascarenhas, the actions of the Pakistani Army compared to the violence by Bengalis was "altogether worse and on a grander scale".


title: 1971 Bangladesh genocide

text: On the night of 25 March 1971 the Pakistani Army launched Operation Searchlight. "Time" magazine dubbed General Tikka Khan the "Butcher of Bengal" for his role in Operation Searchlight. Targets of the operation included Jagannath Hall which was a dormitory for non-Muslim students of Dhaka University, Rajarbagh Police Lines, and Pilkhana, which is the headquarters of East Pakistan Rifles. About 34 students were killed in the dormitories of Dhaka University. Neighbourhoods of old Dhaka which had a majority Hindu population were also attacked. Robert Payne, an American journalist, estimated that 7,000 people had been killed and 3,000 arrested in that night. Teachers of Dhaka University were killed in the operation by the Pakistani Army. Sheikh Mujib was arrested by the Pakistani Army on 25 March. Ramna Kali Mandir was demolished by the Pakistani Army in March 1971.


title: 1971 Bangladesh genocide

text: The original plan envisioned taking control of the major cities on 26 March 1971, and then eliminating all opposition, political or military, within one month. The prolonged Bengali resistance was not anticipated by Pakistani planners. The main phase of Operation Searchlight ended with the fall of the last major town in Bengali hands in mid May. The countryside still remained almost evenly contested.


title: 1971 Bangladesh genocide

text: The first report of the Bangladesh genocide was published by West Pakistani journalist Anthony Mascarenhas in "The Sunday Times", London on 13 June 1971 titled "Genocide". He wrote: "I saw Hindus, hunted from village to village and door to door, shot off-hand after a cursory 'short-arm inspection' showed they were uncircumcised. I have heard the screams of men bludgeoned to death in the compound of the Circuit House (civil administrative headquarters) in Comilla. I have seen truckloads of other human targets and those who had the humanity to try to help them hauled off 'for disposal' under the cover of darkness and curfew." This article helped turn world opinion against Pakistan and decisively encouraged the Government of India to intervene. On 2 August 1971, "Time" magazine correspondent sent a dispatch that provided detailed description of the Pakistani army-led destruction in East Pakistan. It wrote that cities have whole sections damaged from shelling and aerial bombardments. The dispatch wrote: "In Dhaka, where soldiers set sections of the Old City ablaze with flamethrowers and then machine-gunned thousands as they tried to escape the cordon of fire, nearly 25 blocks have been bulldozed clear, leaving open areas set incongruously amid jam-packed slums." It quoted a senior US official as saying "It is the most incredible, calculated thing since the days of the Nazis in Poland."


title: 1971 Bangladesh genocide

text: Archer K. Blood, American diplomat wrote in the Blood Telegram addressing Richard Nixon administration's disregard for the situation: "with support of the Pak military, non-Bengali Muslims are systematically attacking poor people's quarters and murdering Bengalis and Hindus."


title: 1971 Bangladesh genocide

text: On the high end, Bangladeshi authorities claim that as many as 3 million people were killed; the lowest estimate comes from the controversial Hamoodur Rahman Commission, the official Pakistani government investigation, which claimed the figure was 26,000 civilian casualties. The figure of 3 million has become embedded in Bangladeshi culture and literature. Sayyid A. Karim, Bangladesh's first foreign secretary alleges that the source of the figure was "Pravda", the news-arm of the Communist Party of the Soviet Union. Independent researchers have estimated the death toll to be around 300,000 to 500,000 people while others estimate the casualty figure to be 3 million. Midway through the genocide, the CIA and the State Department conservatively estimated that 200,000 people had been killed.


title: 1971 Bangladesh genocide

text: According to Sarmila Bose's controversial book "", the number lies somewhere between 50,000 and 100,000. However, her book was the subject of strong criticism by journalists; writer and visual artist Naeem Mohaiemen; Nayanika Mookherjee, an anthropologist at Durham University; and others.


title: 1971 Bangladesh genocide

text: In 1976 the International Centre for Diarrhoeal Disease Research, Bangladesh undertook a comprehensive population survey in Matlab, Noakhali where a total of 868 excess wartime deaths were recorded; this led to an estimated overall excess number of deaths in the whole of Bangladesh of nearly 500,000. Based on this study, the "British Medical Journal" in 2008, conducted a study by Ziad Obermeyer, Christopher J. L. Murray, and Emmanuela Gakidou which estimated that 125,000–505,000 civilians died as a result of the conflict; the authors note that this is far higher than a previous estimate of 58,000 by Uppsala University and the Peace Research Institute, Oslo. This figure is supported by the statements of Bangladeshi author Ahmed Sharif in 1996, who added that "they kept the truth hidden for getting political advantages". American political scientists Richard Sisson and Leo E. Rose give a low-end estimate of 300,000 dead, killed by all parties, and they deny that a genocide occurred, while American political scientist R. J. Rummel estimated that about 1.5 million people were killed in Bangladesh. Indian journalist Nirmal Sen claims that the total number killed was about 250,000 and among them, about 100,000 were Bengalis and the rest were Biharis.


title: 1971 Bangladesh genocide

text: A 2018 paper by Christian Gerlach concluded that overall deaths due to the war in East Pakistan slightly exceeded half a million and could not have exceeded 1 million, adding that the majority of death were rural dwellers who died of "hunger, want, and exhaustion" with many deaths occurring in the year following the conflict. Out of 200,000 member of the Awami League the paper states 17,000 were killed with the leaders of the league experiencing a death ratio of 15 to 20 out of 167. The paper also denies based on statistical evidence that there was a coordinated attempt to exterminate the Bengali intelligentsia stating: "if one accepts the data published by the Bangladesh propaganda ministry, 4.2 per cent of all university professors were killed, along with 1.4 per cent of all college teachers, 0.6 per cent of all secondary and primary school teachers, and 0.6 per cent of all teaching personnel. On the basis of the aforementioned Ministry of Education data, 1.2 per cent of all teaching personnel were killed. This is hardly proof of an extermination campaign."


title: 1971 Bangladesh genocide

text: Many of those killed were the victims of radical religious paramilitary militias formed by the West Pakistani Army, including the Razakars, Al-Shams and Al-Badr forces. There are many mass graves in Bangladesh, and more are continually being discovered (such as one in an old well near a mosque in Dhaka, located in the Mirpur region of the city, which was discovered in August 1999). The first night of war on Bengalis, which is documented in telegrams from the American Consulate in Dhaka to the United States State Department, saw indiscriminate killings of students of Dhaka University and other civilians.


title: 1971 Bangladesh genocide

text: On 16 December 2002, the George Washington University's National Security Archive published a collection of declassified documents, consisting mostly of communications between US embassy officials and USIS centres in Dhaka and India, and officials in Washington, D.C. These documents show that US officials working in diplomatic institutions within Bangladesh used the terms "selective genocide" and "genocide" (see Blood telegram) to describe events they had knowledge of at the time. The complete chronology of events as reported to the Nixon administration can be found on the Department of State website.