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Astronomer Royal is a senior post in the Royal Households of the United Kingdom. There are two officers, the senior being the astronomer royal dating from 22 June 1675; the junior is the astronomer royal for Scotland dating from 1834. The Astronomer Royal works to make observations to improve navigation, cartography, instrument design, and applications of geomagnetism. [1] The position was created with the overall goal of discovering a way to determine longitude at sea when out of sight of land [2] .
The post was created by King Charles II in 1675, at the same time as he founded the Royal Observatory, Greenwich. He appointed John Flamsteed, instructing him "forthwith to apply himself with the most exact care and diligence to the rectifying the tables of the motions of the heavens, and the places of the fixed stars, so as to find out the so-much desired longitude of places, for the perfecting the art of navigation." [3] [4] [5] The first six Astronomer Royals dedicated themselves primarily to this task and focused on astronomical observations that would benefit navigation. [2]
The astronomer royal was director of the Royal Observatory, Greenwich from the establishment of the post in 1675 until 1972. The astronomer royal became an honorary title in 1972 without executive responsibilities, and a separate post of director of the Royal Greenwich Observatory was created to manage the institution. [5] [6]
The origin of the title Astronomer Royal is unknown. [7] Although John Flamsteed is widely considered the first Astronomer Royal, he was never appointed with the title and only referred to in the Warrant to Ordinance as "Our Astronomical Observer". [7] Similar language was used to appoint all the Astronomers Royal until 1881 with William Christie's appointment. The term Astronomer Royal did not become commonly used until the late 18th Century while the Royal Warrants still used "Our Astronomical Observer". [7] Other titles such as Royal Professor at Greenwich were also used in less formal documents during this time. [7]
In 1703, Isaac Newton was elected President of the Royal Society and was upset with the lack of publications coming from the Greenwich Observatory under Flamsteed. [8] This eventually led to Queen Anne's Warrant of 1710 where members of the Royal Society were appointed as the Board of Visitors to the Royal Observatory to oversee Flamsteed. [7] The original Board of Visitors consisted entirely of associates and allies of Newton which enraged Flamsteed. [8]
In 1765, the Board of Longitude decided that the Astronomer Royal's observations were the property of the Crown and must be printed and published each year. [9] John Pond and subsequent Astronomers Royal elected to publish their findings quarterly instead. [10]
Sir George Airy transformed the position from its original purpose of improving navigation to conducting more general astronomical and scientific research. [11] With approval from the Board of Visitors in 1836, Airy created a Magnetic and Meteorological Department in the Royal Observatory Greenwich. Following this, in 1873 he created the Solar Photography Department. [11]
Astronomers Royal are responsible for many different discoveries and theories. They had several assistants who aided in their research at the Royal Observatory, Greenwich. The most important position was that of the computers or people that would perform all the mathematical computations behind the astronomers' observations. Many of these computers were women, but they were often left out of articles and books, thus leaving them out of most common historical sources. [12]
Originally, the Astronomer Royal had one assistant but increased to six during John Pond's appointment as Astronomer Royal. [13] The astronomer royal today receives a stipend of 100 GBP per year and is a member of the royal household, under the general authority of the Lord Chamberlain. After the separation of the two offices of Astronomer Royal and Director of the Royal Greenwich Observatory, the position of astronomer royal has been largely honorary, although the holder remains available to advise the Sovereign on astronomical and related scientific matters, [14] and the office is of great prestige.
There was formerly a Royal Astronomer of Ireland who was also the Andrew's Professor of Astronomy at the University of Dublin. [15] Both became vacant in 1921 with Irish Independence but a new Andrew's Professor of Astronomy was appointed in 1985. [15]
# | Image | Name | Start year | End year | Reference |
---|---|---|---|---|---|
1. | John Flamsteed | 1675 | 1719 | [4] [14] | |
2. | Edmond Halley | 1720 | 1742 | [4] [14] | |
3. | James Bradley | 1742 | 1762 | [4] [14] | |
4. | Nathaniel Bliss | 1762 | 1764 | [4] [14] | |
5. | Nevil Maskelyne | 1765 | 1811 | [4] [14] | |
6. | John Pond | 1811 | 1835 | [4] [14] | |
7. | Sir George Biddell Airy | 1835 | 1881 | [6] [14] | |
8. | Sir William Christie | 1881 | 1910 | [6] [14] | |
9. | Sir Frank Dyson | 1910 | 1933 | [6] [14] | |
10. | Sir Harold Spencer Jones | 1933 | 1955 | [6] [14] | |
11. | Sir Richard van der Riet Woolley | 1956 | 1971 | [6] [14] | |
12. | Sir Martin Ryle | 1972 | 1982 | [6] [14] | |
13. | Sir Francis Graham-Smith | 1982 | 1990 | [14] | |
14. | Sir Arnold Wolfendale | 1991 | 1995 | [14] | |
15. | Martin Rees, Baron Rees of Ludlow | 1995 | Incumbent | [14] |
John Flamsteed is responsible for a few important discoveries including proving his theory of annual stellar parallax and the discovery of the planet Uranus, even though he thought it was a star. [16] In 1694, he gathered evidence of the stellar parallax and became the first person to prove that the Earth revolves around the sun. [16] However, his most significant contribution to the Royal Observatory and later to the Astronomers Royal was his high standard of work.
Six years after the death of Flamsteed, Historia Coelestis Britannica was published containing much of the data and theories he had spent his life working on both before and after his appointment as Astronomer Royal. [17] It contains accurate tables of lunar motion, planetary motion, and detailed stellar catalog of 2935 stars. [17] This publication made the Astronomer Royal and the Royal Observatory, Greenwich internationally renown for precise observation. [8]
Edmond Halley was determined to find a way to find longitude at sea without sight of land. [9] Starting in 1725, Halley while serving as Astronomer Royal and a Commissioner on the Board of Longitude made very detailed and precise observations of the moon. [9] From these observations he was able to show that longitude could be calculated using the moon in 1731. [9] Although the error is his calculations was about 69 miles at the equator, it was more accurate than any other methods until the use of the marine chronometer for finding longitude. [9]
In 1833, John Pond published his catalog of 1113 different stars. [18] The catalog contained more stars recorded to a much higher degree of accuracy than any other publication at the time, and impressed many other astronomers across Europe. [19]
Another notable Astronomer Royal was Sir George Biddell Airy. While still in college at Trinity College, Cambridge, he noticed he was having trouble reading with his left eye. [20] Eventually, his condition would be classified as an astigmatism, but at the time, there was no cure that worked for everyone. After consulting with others who had the same condition, he specially crafted a lens to refract the light rays and correct the astigmatism. [20] With experience working with lenses, he spent a significant amount of his time as the Astronomer Royal improving the measuring instruments in the Royal Observatory, Greenwich. [21] Using these improved instruments, he meticulously double-checked measurements and discoveries made by past astronomers. [21]
Frank Dyson, the ninth Astronomer Royal, determined latitude variation caused by irregular movement of Earth's magnetic poles. [22] He used a telescope floating in mercury and was able to detect when the poles of the earth wobbled any distance greater than one foot. [22] During the 1919 eclipse, Dyson was crucial in designing the Eddington experiment with Arthur Stanley Edington to test Albert Einstein's Theory of Relativity. [23] Starting months before the eclipse, stars were photographed and carefully charted, and during the total eclipse the same stars would be photographed and charted again. [23] If Einstein's theory was correct then the light from the selected stars would be bent passing around the sun and show more deflection than Newtonian theory could account for. [23] When the photographs from the eclipse were developed it became clear that Einstein's theory had accurately predicted the position of stars. This was one of the first experiments done to test general relativity. [23]
The astronomer royal is mentioned in H. G. Wells' novel The War of the Worlds , in George Orwell's Down and Out in Paris and London , [24] and in Thomas Pynchon,s novel Mason & Dixon', [25] . 'He also makes an appearance in the lyrics of Gilbert and Sullivan's The Pirates of Penzance [26] and plays an important role in Fred Hoyle's novel The Black Cloud . [27]
John Flamsteed was an English astronomer and the first Astronomer Royal. His main achievements were the preparation of a 3,000-star catalogue, Catalogus Britannicus, and a star atlas called Atlas Coelestis, both published posthumously. He also made the first recorded observations of Uranus, although he mistakenly catalogued it as a star, and he laid the foundation stone for the Royal Greenwich Observatory.
The Royal Observatory, Greenwich is an observatory situated on a hill in Greenwich Park in south east London, overlooking the River Thames to the north. It played a major role in the history of astronomy and navigation, and because the Prime Meridian passed through it, it gave its name to Greenwich Mean Time, the precursor to today's Coordinated Universal Time (UTC). The ROG has the IAU observatory code of 000, the first in the list. ROG, the National Maritime Museum, the Queen's House and the clipper ship Cutty Sark are collectively designated Royal Museums Greenwich.
A prime meridian is an arbitrarily chosen meridian in a geographic coordinate system at which longitude is defined to be 0°. Together, a prime meridian and its anti-meridian form a great circle. This great circle divides a spheroid, like Earth, into two hemispheres: the Eastern Hemisphere and the Western Hemisphere. For Earth's prime meridian, various conventions have been used or advocated in different regions throughout history. Earth's current international standard prime meridian is the IERS Reference Meridian. It is derived, but differs slightly, from the Greenwich Meridian, the previous standard.
John Couch Adams was a British mathematician and astronomer. He was born in Laneast, near Launceston, Cornwall, and died in Cambridge.
Sir George Biddell Airy was an English mathematician and astronomer, as well as the Lucasian Professor of Mathematics from 1826 to 1828 and the seventh Astronomer Royal from 1835 to 1881. His many achievements include work on planetary orbits, measuring the mean density of the Earth, a method of solution of two-dimensional problems in solid mechanics and, in his role as Astronomer Royal, establishing Greenwich as the location of the prime meridian.
Sir Frank Watson Dyson, KBE, FRS, FRSE was an English astronomer and the ninth Astronomer Royal who is remembered today largely for introducing time signals ("pips") from Greenwich, England, and for the role he played in proving Einstein's theory of general relativity.
George Graham, FRS was an English clockmaker, inventor, and geophysicist, and a Fellow of the Royal Society.
Herbert Hall Turner was a British astronomer and seismologist.
The Madras Observatory was an astronomical observatory which had its origins in a private observatory set up by William Petrie in 1786 and later moved and managed by the British East India Company from 1792 in Madras. The main purpose for establishing it was to assist in navigation and mapping by recording the latitude and maintaining time standards. In later years the observatory also made observations on stars and geomagnetism. The observatory ran from around 1792 to 1931 and a major work was the production of a comprehensive catalogue of stars.
The planet Neptune was mathematically predicted before it was directly observed. With a prediction by Urbain Le Verrier, telescopic observations confirming the existence of a major planet were made on the night of September 23–24, Autumnal Equinox of 1846, at the Berlin Observatory, by astronomer Johann Gottfried Galle, working from Le Verrier's calculations. It was a sensational moment of 19th-century science, and dramatic confirmation of Newtonian gravitational theory. In François Arago's apt phrase, Le Verrier had discovered a planet "with the point of his pen".
The history of longitude describes the centuries-long effort by astronomers, cartographers and navigators to discover a means of determining the longitude of any given place on Earth. The measurement of longitude is important to both cartography and navigation. In particular, for safe ocean navigation, knowledge of both latitude and longitude is required, however latitude can be determined with good accuracy with local astronomical observations.
Edwin Dunkin FRS, FRAS was a British astronomer and the president of the Royal Astronomical Society and the Royal Institution of Cornwall.
The Shuckburgh telescope or Shuckburgh equatorial refracting telescope was a 4.1 inches (10.4 cm) diameter aperture telescope on an equatorial mount completed in 1791 for Sir George Shuckburgh (1751–1804) in Warwickshire, England, and built by British instrument maker Jesse Ramsden (1735–1800). It was transferred to the Royal Observatory, Greenwich in 1811 and the London Science Museum in 1929. Even though it has sometimes not been regarded as particularly successful, its design was influential. It was one of the larger achromatic doublet telescopes at the time, and one of the largest to have an equatorial mount. It was also known as the eastern equatorial for its location.
Robert Grant, FRS was a Scottish astronomer.
The 1874 Transit of Venus Expedition to Hawaii was an astronomical expedition by British scientists to observe the December 8 transit of Venus at three separate observing sites in the Hawaiian Islands, then known as the Sandwich Islands. It was one of five 1874 transit expeditions organized by George Biddell Airy, Astronomer Royal at the Royal Observatory, Greenwich. The purpose of the expedition was to obtain an accurate estimate of the astronomical unit (AU), the distance from the Earth to the Sun, by measuring solar parallax. Previous efforts to obtain a precise value of an AU in 1769 had been hampered by the black drop effect. There is a collection of papers relating to this expedition at the Cambridge Digital Library.
Norman Robert Pogson, CIE was an English astronomer who worked in India at the Madras observatory. He discovered several minor planets and made observations on comets. He introduced a mathematical scale of stellar magnitudes with the ratio of two successive magnitudes being the fifth root of one hundred (~2.512) and referred to as Pogson's ratio.
Alice Everett was a British astronomer and engineer who grew up in Belfast. Everett is best known for being the first woman to be paid for astronomical work at the Royal Observatory, Greenwich, when she began her employment at the observatory January 1890. In 1903 she was the first woman to have a paper published by the Physical Society of London. She also contributed to the fields of optics and early television.
George Lyon Tupman FRAS was the Chief Astronomer for the British astronomical expedition to Hawaii to observe the 1874 transit of Venus.
Thomas Glanville Taylor was an English astronomer who worked extensively at the Madras Observatory and produced the Madras Catalogue of Stars from around 1831 to 1839.
The Greenwich 28-inch refractor is a telescope at the Royal Observatory, Greenwich, where it was first installed in 1893. It is a 28-inch ( 71 cm) aperture objective lens telescope, otherwise known as a refractor, and was made by the telescope maker Sir Howard Grubb. The achromatic lens was made Grubb from Chance Brothers glass. The mounting is older however and dates to the 1850s, having been designed by Royal Observatory director George Airy and the firm Ransomes and Simms. The telescope is noted for its spherical dome which extends beyond the tower, nicknamed the "onion" dome. Another name for this telescope is "The Great Equatorial" which it shares with the building, which housed an older but smaller telescope previously.