Halley's Comet

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Template:Use dmy dates Template:For Template:Bots Template:Infobox Planet Halley's Comet or Comet Halley (Template:IPAc-en or Template:IPAc-en), officially designated 1P/Halley,<ref name=jpldata/> is the best-known of the short-period comets and is visible from Earth every 75–76 years.<ref name=jpldata/><ref name=kronk>Template:Cite web</ref> Halley is the only short-period comet that is clearly visible to the naked eye from Earth, and thus the only naked-eye comet that might appear twice in a human lifetime.<ref name=Delehanty/> Other naked-eye comets may be brighter and more spectacular, but will appear only once in thousands of years.

Halley's returns to the inner Solar System have been observed and recorded by astronomers since at least 240 BCE. Clear records of the comet's appearances were made by Chinese, Babylonian, and medieval European chroniclers, but were not recognized as reappearances of the same object at the time. The comet's periodicity was first determined in 1705 by English astronomer Edmond Halley, after whom it is now named. Halley's Comet last appeared in the inner Solar System in 1986 and will next appear in mid-2061.<ref name=diagram>Template:Cite web</ref>

During its 1986 apparition, Halley became the first comet to be observed in detail by spacecraft, providing the first observational data on the structure of a comet nucleus and the mechanism of coma and tail formation.<ref name=post/><ref name=situ/> These observations supported a number of longstanding hypotheses about comet construction, particularly Fred Whipple's "dirty snowball" model, which correctly predicted that Halley would be composed of a mixture of volatile ices – such as water, carbon dioxide and ammonia – and dust. The missions also provided data which substantially reformed and reconfigured these ideas; for instance it is now understood that Halley's surface is largely composed of dusty, non-volatile materials, and that only a small portion of it is icy.

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Contents

Pronunciation

Comet Halley is commonly pronounced Template:IPAc-en, rhyming with valley, or more recently Template:IPAc-en, rhyming with daily.<ref>Template:Cite web</ref> Spellings of Edmond Halley's name during his lifetime included Hailey, Haley, Halley, Hawley, and Hawly, so its correct pronunciation is uncertain. <ref>Template:Cite news</ref>

Computation of orbit

Halley was the first comet to be recognized as periodic. Until the Renaissance, the philosophical consensus on the nature of comets, promoted by Aristotle, was that they were disturbances in the Earth's atmosphere. This idea was disproved in 1577 by Tycho Brahe, who used parallax measurements to show that comets must lie beyond the Moon. Many were still unconvinced that comets actually orbited the Sun, and assumed they must instead follow straight paths through the Solar System.<ref name=lancs>Lancaster-Brown pp. 14, 25</ref>

In 1687, Sir Isaac Newton published his Principia, in which he outlined his laws of gravity and motion. His work on comets was decidedly incomplete. Although he had suspected that two comets that had appeared in succession in 1680 and 1681 were the same comet before and after passing behind the Sun (he was later found to be correct; see Newton's Comet),<ref>Lancaster-Brown p. 35</ref> he was unable to completely reconcile comets into his model. Ultimately, it was Newton's friend, editor and publisher, Edmond Halley, who, in his 1705 Synopsis of the Astronomy of Comets, used Newton's new laws to calculate the gravitational effects of Jupiter and Saturn on cometary orbits.<ref name=lancs2>Lancaster-Brown p. 76</ref> This calculation enabled him, after examining historical records, to determine that the orbital elements of a second comet which had appeared in 1682 were nearly the same as those of two comets which had appeared in 1531 (observed by Petrus Apianus) and 1607 (observed by Johannes Kepler).<ref name=lancs2/> Halley thus concluded that all three comets were in fact the same object returning every 76 years, a period that has since been amended to every 75–76 years. After a rough estimate of the perturbations the comet would sustain from the gravitational attraction of the planets, he predicted its return for 1758.<ref>Lancaster-Brown p. 78</ref>

Halley's prediction of the comet's return proved to be correct, although it was not seen until 25 December 1758, by Johann Georg Palitzsch, a German farmer and amateur astronomer. It did not pass through its perihelion until 13 March 1759, the attraction of Jupiter and Saturn having caused a retardation of 618 days.<ref>Lancaster-Brown p. 86</ref> This effect was computed prior to its return (with a one-month error to 13 April)<ref>Sagan and Druyan p. 74</ref> by a team of three French mathematicians, Alexis Clairaut, Joseph Lalande, and Nicole-Reine Lepaute.<ref>Lancaster-Brown pp. 84–85</ref> Halley himself did not live to see the comet return, as he died in 1742.<ref>Lancaster-Brown p. 80</ref> The confirmation of the comet's return was the first time anything other than planets had been shown to orbit the Sun. It was also one of the earliest successful tests of Newtonian physics, and a clear demonstration of its explanatory power.<ref name=hughes/> The comet was first named in his honour by French astronomer Nicolas Louis de Lacaille in 1759.<ref name=hughes/>

The possibility has been raised that 1st-century Jewish astronomers had already recognized Halley's Comet as periodic.<ref>S. Brodetsky, "Astronomy in the Babylonian Talmud", Jewish Review, 1911, p. 60.</ref> This theory notes a passage in the Talmud<ref>Tractate Horioth page 10a</ref> which refers to "a star which appears once in seventy years that makes the captains of the ships err."<ref>Template:Cite book</ref>

Orbit and origin

The orbital paths of Halley, outlined in blue, against the orbits of Jupiter, Saturn, Uranus and Neptune, outlined in red
The orbit of Halley's Comet (blue) set against the orbits of the outer planets (red)

Halley's orbital period over the last 3 centuries has been between 75–76 years, though it has varied between 74–79 years since 240 BCE.<ref name=hughes/><ref name=yeo/> Its orbit around the Sun is highly elliptical, with an orbital eccentricity of 0.967 (with 0 being a perfect circle and 1 being a parabolic trajectory). The perihelion, the point in the comet's orbit when it is nearest the Sun, is just 0.6 AUTemplate:Ref label (between the orbits of Mercury and Venus), while its aphelion, or farthest distance from the Sun, is 35 AU (roughly the distance of Pluto). Unusually for an object in the Solar System, Halley's orbit is retrograde; it orbits the Sun in the opposite direction to the planets, or clockwise from above the Sun's north pole. The orbit is inclined by 18° to the ecliptic, with much of it lying south of the ecliptic, but is retrograde (true inclination is 162°).<ref>Template:Cite web</ref> Due to the retrograde orbit, it has one of the highest velocities relative to the Earth of any object in the Solar System. The 1910 passage was at a relative velocity of 70.56 km/s (157,838 mph or 254,016 km/h).<ref name=velocity>Template:Cite web</ref> Because its orbit comes close to Earth's in two places, Halley's Comet is the parent body of two meteor showers: the Eta Aquariids in early May, and the Orionids in late October.<ref>Template:Cite web</ref> However, observations conducted around the time of Halley's Comet's appearance in 1986 suggest that the Eta Aquarid meteor shower might not originate from Halley's Comet, though it might be perturbed by the comet.<ref name=mitra1986>Template:Cite journal</ref>

Halley is classified as a periodic or short-period comet; one with an orbit lasting 200 years or less.<ref name="Morbidelli2006"/> This contrasts it with long-period comets, whose orbits last for thousands of years. Periodic comets have an average inclination to the ecliptic of only ten degrees, and an orbital period of just 6.5 years, so Halley's orbit is atypical.<ref name=hughes>Template:Cite journal</ref> Most short-period comets (those with orbital periods shorter than 20 years and inclinations of 20–30 degrees or less) are called Jupiter-family comets. Those like Halley, with orbital periods of between 20 and 200 years and inclinations extending from zero to more than 90 degrees, are called Halley-type comets.<ref name="Morbidelli2006"> Template:Cite arxiv</ref><ref name=jewitt2002>Template:Cite journal</ref> To date, only 54 Halley-type comets have been observed, compared with nearly 400 identified Jupiter-family comets.<ref>Template:Cite web</ref>

The orbits of the Halley-type comets suggest that they were originally long-period comets whose orbits were perturbed by the gravity of the giant planets and directed into the inner Solar System.<ref name="Morbidelli2006"/> If Halley was once a long-period comet, it is likely to have originated in the Oort Cloud,<ref name=jewitt2002/> a sphere of cometary bodies that has an inner edge of 20,000–50,000 AU. Conversely the Jupiter-family comets are believed to originate in the Kuiper belt,<ref name=jewitt2002/> a flat disc of icy debris between 30 AU (Neptune's orbit) and 50 AU from the Sun (in the scattered disc). Another point of origin for the Halley-type comets has been proposed. In 2008, a trans-Neptunian object with a retrograde orbit similar to Halley's was discovered, Template:Mpl, whose orbit takes it from just outside that of Uranus to twice the distance of Pluto. It may be a member of a new population of small Solar System bodies that serves as the source of Halley-type comets.<ref name=Gladman2009>Template:Cite journal</ref>

A meteor strikes the bottom left, while the Milky Way arcs overhead and a dawn-like light lines the lower horizon. The image was taken through a curved lens.
Orionid meteor striking the sky below the Milky Way and to the right of Venus. Zodiacal light is also seen at the image.

Halley's Comet has probably been in its current orbit for 16,000–200,000 years, although it is not possible to numerically integrate its orbit for more than a few tens of apparitions, and close approaches before 837 CE can only be verified from recorded observations.<ref name=Olsson1987>Template:Cite journal</ref> The non-gravitational effects can be crucial;<ref name=Olsson1987/> as Halley approaches the Sun, it expels jets of sublimating gas from its surface, which knock it very slightly off its orbital path. These orbital changes can cause deviations in its perihelion of four days.<ref>Template:Cite book</ref>

In 1989, Boris Chirikov and Vitaly Vecheslavov performed an analysis of 46 apparitions of Halley's Comet taken from historical records and computer simulations. These studies showed that its dynamics were chaotic and unpredictable on long timescales.<ref>Template:Cite journal</ref> Halley's projected lifetime could be as long as 10 million years. More recent work suggests that Halley will evaporate, or split in two, within the next few tens of thousands of years, or will be ejected from the Solar System within a few hundred thousand years.<ref name=jewitt2002/> Observations by D.W. Hughes suggest that Halley's nucleus has been reduced in mass by 80–90% over the last 2000–3000 revolutions.<ref name=situ/>

Structure and composition

File:Halley Giotto.jpg
The nucleus of Halley's Comet, imaged by the Giotto probe in 1986. The dark coloration of the nucleus can be observed, as well as the jets of dust and gas erupting from its surface.

The Giotto and Vega missions gave planetary scientists their first view of Halley's surface and structure. Like all comets, as Halley nears the Sun, its volatile compounds (those with low boiling points, such as water, carbon monoxide, carbon dioxide and other ices) begin to sublime from the surface of its nucleus.<ref name=graw/> This causes the comet to develop a coma, or atmosphere, up to 100,000 km across.<ref name=Learn>Template:Cite web</ref> Evaporation of this dirty ice releases dust particles, which travel with the gas away from the nucleus. Gas molecules in the coma absorb solar light and then re-radiate it at different wavelengths, a phenomenon known as fluorescence, whereas dust particles scatter the solar light. Both processes are responsible for making the coma visible.<ref name=Delehanty>Template:Cite web</ref> As a fraction of the gas molecules in the coma are ionized by the solar ultraviolet radiation,<ref name=Delehanty/> pressure from the solar wind, a stream of charged particles emitted by the Sun, pulls the coma's ions out into a long tail, which may extend more than 100 million kilometers into space.<ref name=graw/><ref>Template:Cite book</ref> Changes in the flow of the solar wind can cause disconnection events, in which the tail completely breaks off from the nucleus.<ref name=post/>

Despite the vast size of its coma, Halley's nucleus is relatively small: barely 15 kilometers long, 8 kilometers wide and perhaps 8 kilometers thick.Template:Ref label Its shape vaguely resembles that of a peanut.<ref name=Learn/> Its mass is relatively low (roughly 2.2Template:Esp kg)<ref name=mass>Template:Cite journal</ref> and its average density is about 0.6 g/cm3, indicating that it is made of large number of small pieces, held together very loosely, forming a structure known as a rubble pile.<ref name=density>Template:Cite journal</ref> Ground-based observations of coma brightness suggested that Halley's rotation period was about 7.4 days. Images taken by the various spacecraft, along with observations of the jets and shell, suggested a period of 52 hours.<ref name=situ>Template:Cite book</ref> Given the irregular shape of the nucleus, Halley's rotation is likely to be complex.<ref name=graw>Template:Cite web</ref> Although only 25% of Halley's surface was imaged in detail during the flyby missions, the images revealed an extremely varied topography, with hills, mountains, ridges, depressions, and at least one crater.<ref name=situ/>

Halley is the most active of all the periodic comets, with others, such as Comet Encke and Comet Holmes, displaying activity one or two orders of magnitude weaker.<ref name=situ/> Its day side (the side facing the Sun) is far more active than the night side. Spacecraft observations showed that the gases ejected from the nucleus were 80% water vapor, 17% carbon monoxide and 3–4% carbon dioxide,<ref>Template:Cite journal</ref> with traces of hydrocarbons<ref>Template:Cite journal</ref> although more recent sources give a value of 10% for carbon monoxide and also include traces of methane and ammonia.<ref>Template:Cite web</ref> The dust particles were found to be primarily a mixture of carbon-hydrogen-oxygen-nitrogen (CHON) compounds common in the outer Solar System, and silicates, such as are found in terrestrial rocks.<ref name=graw/> The dust particles decreased in size down to the limits of detection (~0.001 µm).<ref name=post/> The ratio of deuterium to hydrogen in the water released by Halley was initially thought to be similar to that found in Earth's ocean water, suggesting that Halley-type comets may have delivered water to Earth in the distant past. Subsequent observations showed Halley's deuterium ratio to be far higher than that in found in the Earth's oceans, making such comets unlikely sources for Earth's water.<ref name=graw/>

Giotto provided the first evidence in support of Fred Whipple's "dirty snowball" hypothesis for comet construction; Whipple postulated that comets are icy objects warmed by the Sun as they approach the inner Solar System, causing ices on their surfaces to sublimate (change directly from a solid to a gas), and jets of volatile material to burst outward, creating the coma. Giotto showed that this model was broadly correct,<ref name=graw/> though with modifications. Halley's albedo, for instance, is about 4%, meaning that it reflects only 4% of the sunlight hitting it; about what one would expect for coal.<ref>Template:Cite journal</ref> Thus, despite appearing brilliant white to observers on Earth, Halley's Comet is in fact pitch black. The surface temperature of evaporating "dirty ice" ranges from 170 K (−103 °C) at higher albedo to 220 K (−53 °C) at low albedo; Vega 1 found Halley's surface temperature to be in the range 300–400 K (30–130 °C). This suggested only 10% of Halley's surface was active, and that large portions of it were coated in a layer of dark dust, which retained heat.<ref name=post/> Together, these observations suggested that Halley was in fact predominantly composed of non-volatile materials, and thus more closely resembled a "snowy dirtball" than a "dirty snowball".<ref name=situ/><ref>Template:Cite web</ref>

Apparitions

Halley's calculations enabled the comet's earlier appearances to be found in the historical record. The following table sets out the astronomical designations for every apparition of Halley's Comet from 240 BCE, the earliest documented widespread sighting.<ref name=jpldata>Template:Cite web</ref><ref name="icqdes">Template:Cite web</ref> For example, "1P/1982 U1, 1986 III, 1982i" indicates that for the perihelion in 1986, Halley's Comet was the first period comet known (designated 1P) and this apparition was the first seen in "half-month" U (the first half of November) in 1982 (giving 1P/1982 U1); it was the third comet past perihelion in 1986 (1986 III); and it was the ninth comet spotted in 1982 (provisional designation 1982i). The perihelion dates of each apparition are shown.<ref>Template:Cite journal</ref> The perihelion dates farther from the present are approximate, mainly because of uncertainties in the modeling of non-gravitational effects. Perihelion dates 1607 and later are in the Gregorian calendar, while perihelion dates of 1531 and earlier are in the Julian calendar.<ref>Template:Cite journal</ref>

Template:Col-begin Template:Col-break

  • 1P/−239 K1, −239 (25 May 240 BCE)
  • 1P/−163 U1, −163 (12 November 164 BCE)
  • 1P/−86 Q1, −86 (6 August 87 BCE)
  • 1P/−11 Q1, −11 (10 October 12 BCE)
  • 1P/66 B1, 66 (25 January 66 CE)
  • 1P/141 F1, 141 (22 March 141)
  • 1P/218 H1, 218 (17 May 218)
  • 1P/295 J1, 295 (20 April 295)
  • 1P/374 E1, 374 (16 February 374)
  • 1P/451 L1, 451 (28 June 451)
  • 1P/530 Q1, 530 (27 September 530)
  • 1P/607 H1, 607 (15 March 607)
  • 1P/684 R1, 684 (2 October 684)
  • 1P/760 K1, 760 (20 May 760)
  • 1P/837 F1, 837 (28 February 837)
  • 1P/912 J1, 912 (18 July 912)

Template:Col-break

  • 1P/989 N1, 989 (5 September 989)
  • 1P/1066 G1, 1066 (20 March 1066)
  • 1P/1145 G1, 1145 (18 April 1145)
  • 1P/1222 R1, 1222 (28 September 1222)
  • 1P/1301 R1, 1301 (25 October 1301)
  • 1P/1378 S1, 1378 (10 November 1378)
  • 1P/1456 K1, 1456 (9 June 1456)
  • 1P/1531 P1, 1531 (26 August 1531)
  • 1P/1607 S1, 1607 (27 October 1607)
  • 1P/1682 Q1, 1682 (15 September 1682)
  • 1P/1758 Y1, 1759 I (13 March 1759)
  • 1P/1835 P1, 1835 III (16 November 1835)
  • 1P/1909 R1, 1910 II, 1909c (20 April 1910)
  • 1P/1982 U1, 1986 III, 1982i (9 February 1986)
  • Next perihelion predicted 28 July 2061

Template:Col-end

Prior to 1066

Observation of Halley's Comet, recorded in cuneiform on a clay tablet between 22 and 28 September 164 BCE, Babylon, Iraq. British Museum.

Halley may have been recorded as early as 467 BCE, but this is uncertain. A comet was recorded in ancient Greece between 468 and 466 BCE; its timing, location, duration, and associated meteor shower all suggest it was Halley.<ref>Template:Cite news</ref> According to Pliny the Elder, that same year a meteorite fell in the town of Aegospotami, in Thrace. He described it as brown in colour and the size of a wagon load.<ref>Template:Cite book</ref> Chinese chroniclers also mention a comet in that year.<ref>M. A. Vilyev, 1917, "Investigations on the Theory of Motion of Halley's Comet"; cited by A. D. Dubyago, 1961, "The Determination of Orbits", Ch. 1, The Macmillan Company, New York</ref>

The first certain appearance of Halley's Comet in the historical record is a description from 240 BCE, in the Chinese chronicle Records of the Grand Historian or Shiji, which describes a comet that appeared in the east and moved north.<ref name="Gary Kronk 1999 p.14">Template:Cite book</ref> The only surviving record of the 164 BCE apparition is found on two fragmentary Babylonian tablets, now owned by the British Museum.<ref name="Gary Kronk 1999 p.14"/>

The apparition of 87 BCE was recorded in Babylonian tablets which state that the comet was seen "day beyond day" for a month.<ref>Template:Cite journal</ref> This appearance may be recalled in the representation of Tigranes the Great, an Armenian king who is depicted on coins with a crown that features, according to V. G. Gurzadyan and R. Vardanyan, "a star with a curved tail [that] may represent the passage of Halley's Comet in 87 BCE." Gurzadyan and Vardanyan argue that "Tigranes could have seen Halley's Comet when it passed closest to the Sun on August 6 in 87 BCE" as the comet would have been a "most recordable event"; for ancient Armenians it could have heralded the New Era of the brilliant King of Kings.<ref>Template:Cite journal</ref>

The apparition of 12 BCE was recorded in the Book of Han by Chinese astronomers of the Han Dynasty who tracked it from August through October.<ref name=kronk/> It passed within 0.16 AU of the Earth.<ref name=greatcomets/> Halley's appearance in 12 BCE, only a few years distant from the conventionally assigned date of the birth of Jesus Christ, has led some theologians and astronomers to suggest that it might explain the biblical story of the Star of Bethlehem. There are other explanations for the phenomenon, such as planetary conjunctions, and there are also records of other comets that appeared closer to the date of Jesus' birth.<ref>Template:Cite journal</ref>

If, as has been suggested, the reference in the Talmud to "a star which appears once in seventy years that makes the captains of the ships err"<ref name="sacred-texts.com">Template:Cite web</ref> (see above) refers to Halley's Comet, it may be a reference to the 66 CE appearance, because this passage is attributed to the Rabbi Yehoshua ben Hananiah. This apparition was the only one to occur during ben Hananiah's lifetime.<ref>Template:Cite web</ref>

The 141 CE apparition was recorded in Chinese chronicles.<ref>Template:Cite journal</ref> The 374 CE and 607 approaches each came within 0.09 AU of the Earth.<ref name=greatcomets/> The 684 CE apparition was recorded in Europe in one of the sources used by the compiler of the 1493 Nuremberg Chronicles. Chinese records also report it as the "broom star".<ref name=art/>

In 837, Halley's Comet may have passed as close as 0.03 AU (3.2 million miles; 5.1 million kilometers) from Earth, by far its closest approach.<ref name=greatcomets>Template:Cite web</ref> Its tail may have stretched 60 degrees across the sky. It was recorded by astronomers in China, Japan, Germany and the greater Middle East.<ref name=kronk/> In 912, Halley's Comet is recorded in the Annals of Ulster, which state "A dark and rainy year. A comet appeared."<ref name="ucc.ie">Template:Cite web</ref>

1066

White embroidery showing several people on the left pointing to Halley, top right, over a tower
The comet's appearance in 1066 was recorded on the Bayeux Tapestry.

In 1066, the comet was seen in England and thought to be an omen: later that year Harold II of England died at the Battle of Hastings; it was a bad omen for Harold, but a good omen for the man who defeated him, William the Conqueror. The comet is represented on the Bayeux Tapestry as a fiery star, and the surviving accounts describe it as appearing to be four times the size of Venus and shining with a light equal to a quarter of that of the Moon. Halley came within 0.10 AU of the Earth at that time.<ref name=greatcomets/>

This appearance of the comet is also noted in the Anglo-Saxon Chronicle. Eilmer of Malmesbury may have seen Halley previously in 989, as he wrote of it in 1066: "You've come, have you? ... You've come, you source of tears to many mothers, you evil. I hate you! It is long since I saw you; but as I see you now you are much more terrible, for I see you brandishing the downfall of my country. I hate you!"<ref name="William">William of Malmesbury, Gesta regum Anglorum / The history of the English Kings, ed. and trans. R. A. B. Mynors, R. M. Thomson, and M. Winterbottom, 2 vols., Oxford Medieval Texts (1998–9) p. 121</ref>

The Irish Annals of the Four Masters recorded the comet as "A star [that] appeared on the seventh of the Calends of May, on Tuesday after Little Easter, than whose light the brilliance or light of the moon was not greater; and it was visible to all in this manner till the end of four nights afterwards."<ref name="ucc.ie"/> Chaco Native Americans in New Mexico may have recorded the 1066 apparition in their petroglyphs.<ref>Template:Cite news</ref>

1145–1378

The wise men and several animals cluster around the baby Jesus, while a comet-like object streaks overhead
The Adoration of the Magi (circa 1305) by Giotto, who purportedly modeled the star of Bethlehem on Halley, which had been sighted 4 years prior to this painting.

The 1145 apparition was recorded by the monk Eadwine. The 1986 apparition exhibited a fan tail similar to Eadwine's drawing.<ref name=art/> Some claim that Genghis Khan was inspired to turn his conquests toward Europe by the 1222 apparition.<ref>Template:Cite news</ref> The 1301 apparition may have been seen by the artist Giotto di Bondone, who represented the Star of Bethlehem as a fire-colored comet in the Nativity section of his Arena Chapel cycle, completed in 1305.<ref name=art>Template:Cite journal</ref> No record survives of the 1378 apparition.

1456

In 1456, the year of Halley's next apparition, the Ottoman Empire invaded the Balkans, culminating in the Siege of Belgrade in July of that year. In a Papal Bull, Pope Calixtus III ordered special prayers be said for the city's protection. In 1470, the humanist scholar Bartolomeo Platina wrote in his Lives of the Popes that,<ref>Template:Cite book</ref>

A hairy and fiery star having then made its appearance for several days, the mathematicians declared that there would follow grievous pestilence, dearth and some great calamity. Calixtus, to avert the wrath of God, ordered supplications that if evils were impending for the human race He would turn all upon the Turks, the enemies of the Christian name. He likewise ordered, to move God by continual entreaty, that notice should be given by the bells to call the faithful at midday to aid by their prayers those engaged in battle with the Turk.

Platina's account is not mentioned in official records. In the 18th century, a Frenchman further embellished the story, in anger at the Church, by claiming that the Pope had "excommunicated" Halley's Comet, though this story was most likely his own invention.<ref>Template:Cite journal</ref>

Halley's apparition of 1456 was also witnessed in Kashmir and depicted in great detail by Śrīvara, a Sanskrit poet and biographer to the Sultans of Kashmir. He read the apparition as a cometary portent of doom foreshadowing the imminent fall of Sultan Zayn al-Abidin ( AD 1418/1420-1470). <ref>Walter Slaje, Inter alia, realia: An Apparition of Halley’s Comet in Kashmir. Observed by Śrīvara in AD 1456. In: Roland Steiner (ed.), Highland Philology. Results of a Text-Related Kashmir Panel at the 31st DOT, Marburg 2010. (Studia Indologica Universitatis Halensis. 4). Halle 2012: 33-48.</ref>

After witnessing a bright light in the sky (which most historians have identified as Halley's Comet, visible in Ethiopia in 1456), Emperor Zara Yaqob, ruler from 1434–1468, founded the city of Debre Berhan (tr. City of Light) and made it his capital for the remainder of his reign.<ref>The founding of Debre Berhan is described in the Royal Chronicles (Pankhurst, pp.36–38).</ref>

1531–1835

Black and white photograph of the comet, its nucleus brilliant white, and its tail very prominent, moving up and to the right
A photograph of Halley's Comet taken during its 1910 approach

Halley's periodic returns have been subject to scientific investigation since the 16th century. The three apparitions from 1531 to 1682 were noted by Edmond Halley, enabling him to predict its 1759 return. Streams of vapour observed during the comet's 1835 apparition prompted astronomer Friedrich Wilhelm Bessel to propose that the jet forces of evaporating material could be great enough to significantly alter a comet's orbit.<ref>Sagan and Druyan p. 117</ref>

1910

The 1910 approach, which came into naked-eye view around 10 April<ref name=greatcomets/> and came to perihelion on 20 April,<ref name=greatcomets/> was notable for several reasons: it was the first approach of which photographs exist, and the first for which spectroscopic data were obtained.<ref name=post>Template:Cite journal</ref> Furthermore, the comet made a relatively close approach of 0.15AU,<ref name=greatcomets/> making it a spectacular sight. Indeed, on 19 May, the Earth actually passed through the tail of the comet.<ref name="Ridpath">Template:Cite web</ref><ref name="pfizer">Template:Cite web</ref> One of the substances discovered in the tail by spectroscopic analysis was the toxic gas cyanogen,<ref>Template:Cite news</ref> which led astronomer Camille Flammarion to claim that, when Earth passed through the tail, the gas "would impregnate the atmosphere and possibly snuff out all life on the planet."<ref name=smith/> His pronouncement led to panicked buying of gas masks and quack "anti-comet pills" and "anti-comet umbrellas" by the public.<ref>Template:Cite web</ref> The Sacred Followers, an Oklahoma religious group, attempted to sacrifice a virgin to ward off the impending disaster, but were stopped by the police.<ref>Template:Cite news</ref> In reality, as other astronomers were quick to point out, the gas is so diffuse that the world suffered no ill effects from the passage through the tail.<ref name=smith>Template:Cite news</ref>

American satirist and writer Mark Twain was born on 30 November 1835, exactly two weeks after the comet's perihelion. In his autobiography, published in 1909, he said,

I came in with Halley's comet in 1835. It is coming again next year, and I expect to go out with it. It will be the greatest disappointment of my life if I don't go out with Halley's comet. The Almighty has said, no doubt: 'Now here are these two unaccountable freaks; they came in together, they must go out together.'<ref> Template:Cite book</ref><ref>Template:Cite web</ref>

Twain died on 21 April 1910, the day following the comet's subsequent perihelion.<ref>Template:Cite web</ref> The 1985 fantasy film The Adventures of Mark Twain was inspired by the quotation.

Halley's 1910 apparition is distinct from the Great Daylight Comet of 1910, which surpassed Halley in brilliance and was actually visible in broad daylight for a short period, approximately four months before Halley made its appearance.<ref name="Comet1910">Template:Cite web</ref><ref name="Bortle1998">Template:Cite web</ref>

1986

Halley's Comet, tail barely visible, against a background of stars. The Milky Way is seen in the background.
Halley's Comet in 1986

Halley's 1986 apparition was the least favorable on record. The comet and the Earth were on opposite sides of the Sun in February 1986, creating the worst viewing circumstances for Earth observers for the last 2,000 years.<ref>Template:Cite journal</ref> Halley's closest approach was 0.42 AU.<ref>Template:Cite web</ref> Additionally, with increased light pollution from urbanization, many people never saw the comet at all. It was possible to observe it in areas outside of cities with the help of binoculars.<ref>Template:Cite web</ref> Further, the comet appeared brightest when it was almost invisible from the northern hemisphere in March and April.<ref>Template:Cite news</ref> Halley's approach was first detected by astronomers David Jewitt and G. Edward Danielson on 16 October 1982 using the 5.1 m Hale telescope at Mount Palomar and a CCD camera.<ref>Template:Cite web</ref> The first person to visually observe the comet on its 1986 return was amateur astronomer Stephen James O'Meara on 24 January 1985. O'Meara used a home-built 24-inch telescope on top of Mauna Kea to detect the magnitude 19.6 comet.<ref name=Jan24>Template:Cite news (Horizons shows the nucleus @ APmag +20.5; the coma up to APmag +14.3)</ref> On 8 November 1985, Stephen Edberg (then serving as the Coordinator for Amateur Observations at NASA's Jet Propulsion Laboratory) and Charles Morris were the first to observe Halley's Comet with the naked eye in its 1986 apparition.<ref>Template:Cite news {subscription required}</ref><ref>Template:Cite news</ref>

The development of space travel gave scientists the opportunity to study the comet at close quarters, and several probes were launched to do so. The Soviet Vega 1 started returning images of Halley on 4 March 1986, and the first ever of its nucleus,<ref name=situ/> and made its flyby on 6 March, followed by Vega 2 making its flyby on 9 March. On 14 March, the Giotto space probe, launched by the European Space Agency, made the closest pass of the comet's nucleus.<ref name=situ/> There were also two Japanese probes, Suisei and Sakigake. The probes were unofficially known as the Halley Armada.<ref>Template:Cite web</ref>

Based on data retrieved by Astron, the largest ultraviolet space telescope of the time, during its Halley's Comet observations in December 1985, a group of Soviet scientists developed a model of the comet's coma.<ref>Template:Cite journal</ref> The comet was also observed from space by the International Cometary Explorer. Originally International Sun-Earth Explorer 3, the probe was renamed and freed from its Template:L1 Lagrangian point location in Earth's orbit to intercept comets 21P/Giacobini-Zinner and Halley.<ref>Template:Cite journal</ref>

Two Space Shuttle missions – the ill-fated STS-51-L (ended by the Challenger disaster)<ref>Template:Cite web</ref> and STS-61-E – were scheduled to observe Halley's Comet from low Earth orbit. STS-51-L carried the Shuttle-Pointed Tool for Astronomy (SPARTAN-203) satellite, also called the Halley's Comet Experiment Deployable (HCED).<ref>Template:Cite web</ref> STS-61-E was a Columbia mission scheduled for March 1986, carrying the ASTRO-1 platform to study the comet.<ref>Template:Cite book</ref> Due to the suspension of America's manned space program after the Challenger explosion, the mission was canceled, and ASTRO-1 would not fly until late 1990 on STS-35.<ref>Template:Cite web</ref>

After 1986

Grainy, white-on-black image showing Halley as a barely distinguishable black dot
Halley's Comet observed in 2003 at 28 AU from the Sun

On 12 February 1991, at a distance of Template:Convert from the Sun, Halley displayed an outburst that lasted for several months, releasing a cloud of dust 300,000 km across.<ref name=graw/> The outburst likely started in December 1990, and then the comet brightened from magnitude 24.3 to magnitude 18.9.<ref name=Prialnik1992>Template:Cite journal</ref> Halley was most recently observed in 2003 by three of the Very Large Telescopes at Paranal, Chile, when Halley's magnitude was 28.2. The telescopes observed Halley, at the faintest and furthest any comet has ever been imaged, in order to verify a method for finding very faint trans-Neptunian objects.<ref name="ESO2003">Template:Cite web</ref> Astronomers are now able to observe the comet at any point in its orbit.<ref name="ESO2003"/>

The next predicted perihelion of Halley's Comet is 28 July 2061,<ref name=horizons>Template:Cite web</ref> when it is expected to be better positioned for observation than during the 1985–1986 apparition, as it will be on the same side of the Sun as Earth.<ref name=yeo>Template:Cite journal</ref> It is expected to have an apparent magnitude of −0.3, compared with only +2.1 for the 1986 apparition.<ref name=sten>Template:Cite web</ref> On 9 September 2060, Halley has been calculated to pass within Template:Convert of Jupiter, and then on 20 August 2061, pass within Template:Convert of Venus.<ref name=jpl2061>Template:Cite web</ref> In 2134, Halley is expected to pass within Template:Convert of the Earth.<ref name=jpl2061/> Its apparent magnitude is expected to be −2.0.<ref name=sten/>

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