Chinese records of comets are the most extensive and accurate in existence from the ancient and medieval periods, and stretch back across three millennia. Records exist at least as far back as 613 BC, and records may have been kept for many centuries before this. There are continuous records all the way through to the nineteenth century, using substantially consistent methods throughout. Chinese data accuracy is unsurpassed in the ancient world and was not overtaken by Western accuracy until the fifteenth century or, in some respects, not until the twentieth century.
Comets were observed in great detail because of their astrological significance. However, these observations are now of great use to modern astronomers. Their accuracy is sufficient to allow the calculation of orbital elements, and modern astronomers have done this for many comets. Most notably, ancient orbits of Halley's Comet have been determined using Chinese records, a feat not possible solely from modern data due to a close approach of the comet to Earth in the ninth century. Such close approaches cause comet orbits to change abruptly, and ancient changes of this sort cannot be accurately modelled from the comet's present-day orbital data.
Ancient Chinese records of comet observations are the most extensive historical records in existence. They are far more complete than European observations. [2] The earliest confirmed Chinese comet observation is from 613 BC, [3] but there is also a possible sighting of Halley's Comet in 1059 BC. [4] However, this may not be an actual sighting, but the result of later back calculation. [5]
Early records call comets beixing (or boxing: 孛星, "bushy star" or "sparkling star" [6] according to Yeomans et al.). Later on, a distinction is made between beixing and huixing (彗星, "broom star"), that is, comets without, and with a tail respectively. The broomstick here is a metaphor for the tail and the broomhead the head of the comet. Chinese astronomers were the first to observe that comet tails point away from the sun. They knew this by at least 635 AD, many centuries before the phenomenon was observed in the West. [7] Other descriptive Chinese names for comet include saoxing (掃星, "sweeping star"), tianchan (天攙, "heavenly intermingler"), fengxing (篷星, "sailing star"), changxing (長星, "long star"), and zhuxing (燭星, "candle-flame star"). [8]
The Chinese records are not only the most extensive from ancient times, they are also the most accurate, often to within half a degree of right ascension. Western measurements did not overtake them for accuracy until the fifteenth century: in 1456 AD Paolo Toscanelli tracked the progress of Halley's Comet to within a fraction of a degree. [3]
Finding the time of a Chinese observation is a little more problematic. This can be very important for fast moving objects like comets. However, the dates are recorded, and the time can be estimated to within one or two hours by considering when the Chinese observers would have had good viewing conditions. [9] Comets that actually have a tail can be described as beixing when they are in opposition and the tail is not visible, giving a further clue. [8]
Chinese records of comet brightness are superior to Western observations to an even later date. The West did not overtake Chinese astronomers in this respect until the twentieth century, at least in the matter of diligent recording of brightnesses. [9]
The following documents contain substantial comet observations. Many other local documents have useful information and have been incorporated into various compilations.
An astronomical text recovered from Tomb no.3 in Mawangdui contains images and descriptions of 29 different comets. The descriptions often include the comet's name, notes about its apparition, and its associated portent, usually military, [11] but lack detailed dates of the comets' sightings. This text can be solidly dated as being prior to 168 BC, the date assigned to the tomb. It may be associated with a similar astronomical text from the same tomb, which details planetary motions for the seventy years ending 177 BC. [12]
Wenxian Tongkao , a thirteenth century compilation by Ma Duanlin, includes a list of comets up to 1222 AD. Various European authors used this list as a basis for their own lists starting with Antoine Gaubil who translated it from the Chinese and later extended the list to 1644 AD. The most complete European list was published by John Williams (1797–1874) in 1871. Williams' list contains 372 comets from 613 BC to 1621 AD. [2] A Chinese compilation published in 1988, A Comprehensive Collection of Ancient Chinese Astronomical Records (Zhongguo gudai tianxiang jilu zongji), has over a thousand comet observations. [13]
The Chinese records have some importance to modern science because they allow astronomers to deduce the past orbits and brightnesses of comets. [3] This is important because comet orbits are not always entirely regular. They can be changed by gravitational encounters with the planets. Without ancient records, such past changes would be very difficult to determine. [10] A feature of the Chinese records that makes them particularly useful for modern scientists and scholars is that there is a high degree of consistency in the methods of observation and recording over a very long period. Chinese astronomers were still using naked eye observation in 1835, long after the invention of the telescope. [9]
Around forty comets have had their orbits calculated based entirely on ancient Chinese records. [2] Of the well known comets, besides Halley, Brian G. Marsden suggested, based on Chinese and other ancient observations, that the Great Comet of 1106 was a previous apparition of Comet Ikeya–Seki. [14] Ikeya–Seki is a member of the Kreutz sungrazer family of comets. These are thought to all have originated from the break up of a large parent comet. Several previously unknown members of this group have been found in the Chinese records. [15]
Chinese observations of Halley's Comet are of especial importance to astronomers because of the important place this comet had in their growing understanding of them. [8] The earliest confirmed sighting was in 240 BC (in the Records of the Grand Historian ) [10] —with a continuous record after 164 BC. [16] A comet observed in 467 BC may have been Halley, but there is insufficient information to be sure. [17] The most accurate records of Halley begin in 12 BC. [10]
In 1843 engineer and sinologist Édouard Biot translated Chinese records of comets. Astronomer John Russell Hind observed that past apparitions of Halley back to 12 BC in most cases could be matched to these Chinese records.
A computer calculation of the past orbits of Halley using numerical integration [18] could not continue past 837 AD because a very close approach to Earth made calculation of orbits prior to that too inaccurate. The researchers had started with accurate European measurements from 1759, 1682 and 1607 AD and calculated backwards. However, no accurate European records exist for 837 AD so the researchers looked to Chinese records. From these they obtained a good estimate of the perihelion of Halley for that year. They used that, together with perihelions found from Chinese data for 374 and 141 AD, to provide constraints for their calculation. [10] They were finally able to calculate the orbits of Halley back to 1404 BC. [19]
Studies of historical changes in brightness of Halley's Comet have also been carried out using ancient Chinese data. [9] There has been no regular recording of the brightness of Halley in the West prior to the 1910 apparition. The Chinese records, on the other hand, are almost complete from 12 BC to 1835 AD. [9]
Ancient Chinese astrology set great store by celestial omens and comets were an important omen, always disastrous. [20] Under the theory of Wu Xing, comets were thought to signify an imbalance of yin and yang. [21] Chinese emperors employed observers specifically to watch for them. Some important decisions were made as a result. For instance, Emperor Ruizong of Tang abdicated after a comet appearance in 712 AD. [3]
Comets were thought to have military significance. For instance, the breakup of a comet on 25 January 35 AD was interpreted as portending the destruction of Gongsun Shu by Wu Han, general to emperor Guangwu. [22]
A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or coma surrounding the nucleus, and sometimes a tail of gas and dust gas blown out from the coma. These phenomena are due to the effects of solar radiation and the outstreaming solar wind plasma acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently close and bright, a comet may be seen from Earth without the aid of a telescope and can subtend an arc of up to 30° across the sky. Comets have been observed and recorded since ancient times by many cultures and religions.
Comet Hale–Bopp is a comet that was one of the most widely observed of the 20th century and one of the brightest seen for many decades.
Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, cosmological, calendrical, and astrological beliefs and practices of prehistory: vestiges of these are still found in astrology, a discipline long interwoven with public and governmental astronomy. It was not completely separated in Europe during the Copernican Revolution starting in 1543. In some cultures, astronomical data was used for astrological prognostication.
Zhang Heng, formerly romanized as Chang Heng, was a Chinese polymathic scientist and statesman who lived during the Han dynasty. Educated in the capital cities of Luoyang and Chang'an, he achieved success as an astronomer, mathematician, seismologist, hydraulic engineer, inventor, geographer, cartographer, ethnographer, artist, poet, philosopher, politician, and literary scholar.
Halley's Comet, Comet Halley, or sometimes simply Halley, officially designated 1P/Halley, is a short-period comet visible from Earth every 75–79 years. Halley is the only known short-period comet that is regularly visible to the naked eye from Earth, and thus the only naked-eye comet that can appear twice in a human lifetime. It last appeared in the inner parts of the Solar System in 1986 and will next appear in mid-2061.
12P/Pons–Brooks is a periodic comet with an orbital period of 71 years. It fits the classical definition of a Halley-type comet with, and is also one of the brightest known periodic comets, reaching an absolute visual magnitude ~5 in its approach to perihelion. Comet Pons-Brooks was discovered at Marseilles Observatory in July 1812 by Jean-Louis Pons, and then later recovered in 1883 by William Robert Brooks.
Biela's Comet or Comet Biela was a periodic Jupiter-family comet first recorded in 1772 by Montaigne and Messier and finally identified as periodic in 1826 by Wilhelm von Biela. It was subsequently observed to split in two and has not been seen since 1852. As a result, it is currently considered to have been destroyed, although remnants appeared to have survived for some time as a meteor shower, the Andromedids.
Astronomy in China has a long history stretching from the Shang dynasty, being refined over a period of more than 3,000 years. The ancient Chinese people have identified stars from 1300 BCE, as Chinese star names later categorized in the twenty-eight mansions have been found on oracle bones unearthed at Anyang, dating back to the mid-Shang dynasty. The core of the "mansion" system also took shape around this period, by the time of King Wu Ding.
The Kreutz sungrazers are a family of sungrazing comets, characterized by orbits taking them extremely close to the Sun at perihelion. They are believed to be fragments of one large comet that broke up several centuries ago and are named for German astronomer Heinrich Kreutz, who first demonstrated that they were related. A Kreutz sungrazer's aphelion is about 170 AU from the Sun; these sungrazers make their way from the distant outer Solar System from a patch in the sky in Canis Major, to the inner Solar System, to their perihelion point near the Sun, and then leave the inner Solar System in their return trip to their aphelion.
F. Richard Stephenson is an Emeritus Professor at the University of Durham, in the Physics department and the East Asian Studies department. His research concentrates on historical aspects of astronomy, in particular analyzing ancient astronomical records to reconstruct the history of Earth's rotation. He has an asteroid named after him: 10979 Fristephenson.
Historical astronomy is the science of analysing historic astronomical data. The American Astronomical Society (AAS), established 1899, states that its Historical Astronomy Division "...shall exist for the purpose of advancing interest in topics relating to the historical nature of astronomy. By historical astronomy we include the history of astronomy; what has come to be known as archaeoastronomy; and the application of historical records to modern astrophysical problems." Historical and ancient observations are used to track theoretically long term trends, such as eclipse patterns and the velocity of nebular clouds. Conversely, utilizing known and well documented phenomenological activity, historical astronomers apply computer models to verify the validity of ancient observations, as well as dating such observations and documents which would otherwise be unknown.
In Chinese astronomy, a guest star is a star which has suddenly appeared in a place where no star had previously been observed and becomes invisible again after some time. The term is a literal translation from ancient Chinese astronomical records.
D/1770 L1, popularly known as Lexell's Comet after its orbit computer Anders Johan Lexell, was a comet discovered by astronomer Charles Messier in June 1770. It is notable for having passed closer to Earth than any other comet in recorded history, approaching to a distance of only 0.015 astronomical units, or six times the distance from the Earth to the Moon. The comet has not been seen since 1770 and is considered a lost comet.
122P/de Vico is a periodic comet with an orbital period of 74 years. It fits the classical definition of a Halley-type comet with. It was discovered by Francesco de Vico in Rome on February 20, 1846.
Caesar's Comet was a seven-day cometary outburst seen in July 44 BC. It was interpreted by Romans as a sign of the deification of recently assassinated dictator, Julius Caesar. It was perhaps the most famous comet of antiquity.
Comet Swift–Tuttle is a large periodic comet with a 1995 (osculating) orbital period of 133 years that is in a 1:11 orbital resonance with Jupiter. It fits the classical definition of a Halley-type comet, which has an orbital period between 20 and 200 years. The comet was independently discovered by Lewis Swift on July 16, 1862 and by Horace Parnell Tuttle on July 19, 1862.
EdmondHalley was an English astronomer, mathematician and physicist. He was the second Astronomer Royal in Britain, succeeding John Flamsteed in 1720.
Comets have been observed by humanity for thousands of years, but only in the past few centuries have they been studied as astronomical phenomena. Before modern times, great comets caused worldwide fear, considered bad omens foreboding disaster and turmoil, for example the 1066 passage of Halley's Comet depicted as heralding the Norman conquest of England. As the science of astronomy developed planetary theories, understanding the nature and composition of comets became a challenging mystery and a large area of study.
A great comet is a comet that becomes exceptionally bright. There is no official definition; often the term is attached to comets such as Halley's Comet, which during certain appearances are bright enough to be noticed by casual observers who are not looking for them, and become well known outside the astronomical community. Great comets appear at irregular, unpredictable intervals, on average about once per decade. Although comets are officially named after their discoverers, great comets are sometimes also referred to by the year in which they appeared great, using the formulation "The Great Comet of ...", followed by the year.