A marine chronometer is a precision timepiece that is carried on a ship and employed in the determination of the ship's position by celestial navigation . It is used to determine longitude by comparing Greenwich Mean Time (GMT), and the time at the current location found from observations of celestial bodies. When first developed in the 18th century, it was a major technical achievement, as accurate knowledge of the time over a long sea voyage was vital for effective navigation , lacking electronic or communications aids. The first true chronometer was the life work of one man, John Harrison , spanning 31 years of persistent experimentation and testing that revolutionized naval (and later aerial) navigation.
69-507: A time ball or timeball is a time-signalling device. It consists of a large, painted wooden or metal ball that is dropped at a predetermined time, principally to enable navigators aboard ships offshore to verify the setting of their marine chronometers . Accurate timekeeping is essential to the determination of longitude at sea. Although time balls have since been replaced by electronic time signals , some time balls have remained operational as historical tourist attractions . The fall of
138-538: A chain drive fusee and its second hand advanced in 1 ⁄ 2 -second increments over a 60 seconds marked sub dial. In Germany, where marine chronometers were imported or used foreign key components, a Drei-Pfeiler Werk Einheitschronometer (three-pillar movement unified chronometer) was developed by a collaboration between the Wempe Chronometerwerke and A. Lange & Söhne companies to make more efficient production possible. The development of
207-437: A brief moment at the centre of oscillation, when it is least susceptible to outside influences. At the centre of oscillation, a roller on the balance staff momentarily displaces the detent, allowing one tooth of the escape wheel to pass. The escape wheel tooth then imparts its energy on a second roller on the balance staff. Since the escape wheel turns in only one direction, the balance receives impulse in only one direction. On
276-422: A day or two of instruction and practice, even using manual calculation methods. The use of a marine chronometer to determine longitude by chronometer permits navigators to obtain a reasonably accurate position fix. For every four seconds that the time source is in error, the east–west position may be off by up to just over one nautical mile as the angular speed of Earth is latitude dependent. The creation of
345-429: A little ball was in antiquity a way to show to people the time. Ancient Greek clocks had this system in the main square of a city, as in the city of Gaza in the post-Alexander era, and as described by Procopius in his book on Edifices. Time ball stations set their clocks according to transit observations of the positions of the sun and stars. Originally they either had to be stationed at the observatory , or had to keep
414-636: A marine chronometer in 1673 in France , under the sponsorship of Jean-Baptiste Colbert . In 1675, Huygens, who was receiving a pension from Louis XIV , invented a chronometer that employed a balance wheel and a spiral spring for regulation, instead of a pendulum, opening the way to marine chronometers and modern pocket watches and wristwatches. He obtained a patent for his invention from Colbert, but his clock remained imprecise at sea. Huygens' attempt in 1675 to obtain an English patent from Charles II stimulated Robert Hooke , who claimed to have conceived of
483-419: A marine chronometer to measure time, a sextant to measure the angles, an almanac giving schedules of the coordinates of celestial objects, a set of sight reduction tables to help perform the height and azimuth computations, and a chart of the region. With sight reduction tables, the only calculations required are addition and subtraction. Most people can master simpler celestial navigation procedures after
552-446: A pair of counter-oscillating weighted beams connected by springs whose motion was not influenced by gravity or the motion of a ship. His first two sea timepieces H1 and H2 (completed in 1741) used this system, but he realised that they had a fundamental sensitivity to centrifugal force , which meant that they could never be accurate enough at sea. Construction of his third machine, designated H3, in 1759 included novel circular balances and
621-686: A phalanx of astronomical observatories located in Western Europe to conduct accuracy assessments of their timepieces. Once mechanical timepiece movements developed sufficient precision to allow for adequately accurate marine navigation, these third party independent assessments also developed into what became known as "chronometer competitions" at the astronomical observatories located in Western Europe. The Neuchâtel Observatory , Geneva Observatory , Besançon Observatory , Kew Observatory , German Naval Observatory Hamburg and Glashütte Observatory are prominent examples of observatories that certified
690-459: A position on the Earth's surface, it is necessary and sufficient to know the latitude , longitude , and altitude . Altitude considerations can naturally be ignored for vessels operating at sea level . Until the mid-1750s, accurate navigation at sea out of sight of land was an unsolved problem due to the difficulty in calculating longitude. Navigators could determine their latitude by measuring
759-641: A precise and inexpensive Einheitschronometer was a 1939 German naval command and Aviation ministry driven initiative. Serial production began in 1942. All parts were made in Germany and interchangeable. During the course of World War II modifications that became necessary when raw materials became scarce were applied and work was compulsory and sometimes voluntarily shared between various German manufacturers to speed up production. The production of German unified design chronometers with their harmonized components continued until long after World War II in Germany and
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#1732783988803828-531: A reliable chronometer at sea, but these developments by Le Roy are considered by Rupert Gould to be the foundation of the modern chronometer. Le Roy's innovations made the chronometer a much more accurate piece than had been anticipated. Ferdinand Berthoud in France, as well as Thomas Mudge in Britain also successfully produced marine timekeepers. Although none were simple, they proved that Harrison's design
897-499: A requirement for certain international mariner certifications such as Officer in Charge of Navigational Watch, and Master and Chief Mate deck officers, and supplements offshore yachtmasters on long-distance private cruising yachts. Modern marine chronometers can be based on quartz clocks that are corrected periodically by satellite time signals or radio time signals (see radio clock ). These quartz chronometers are not always
966-513: A spring-driven clock years earlier, to attempt to produce one and patent it. During 1675 Huygens and Hooke each delivered two such devices to Charles, but none worked well and neither Huygens nor Hooke received an English patent. It was during this work that Hooke formulated Hooke's law . The first published use of the term chronometer was in 1684 in Arcanum Navarchicum , a theoretical work by Kiel professor Matthias Wasmuth. This
1035-406: A timepiece which would work reliably at sea was difficult. Until the 20th century, the best timekeepers were pendulum clocks , but both the rolling of a ship at sea and the up to 0.2% variations in the gravity of Earth made a simple gravity-based pendulum useless both in theory and in practice. Christiaan Huygens , following his invention of the pendulum clock in 1656, made the first attempt at
1104-645: A variety of papers to the Transactions of the Royal Society . He revised the Miscellanea Curiosa . He edited the correspondence and wrote a biography of John Ray , whose 'physico-theology' ( natural theology ) tradition he continued, making him an early parson-naturalist . He edited Eleazar Albin 's Natural History , and published some of the manuscripts of the scientist Robert Hooke . His meteorological observations at Upminster (in
1173-464: A very accurate clock at the station which was set manually to observatory time. Following the introduction of the electric telegraph around 1850, time balls could be located at a distance from their source of mean time and operated remotely. The first modern time ball was erected at Portsmouth , England, in 1829 by its inventor Robert Wauchope , a captain in the Royal Navy . Others followed in
1242-552: Is at the Royal Observatory, Greenwich , in London , UK. The crucial problem was to find a resonator that remained unaffected by the changing conditions met by a ship at sea. The balance wheel , harnessed to a spring, solved most of the problems associated with the ship's motion. Unfortunately, the elasticity of most balance spring materials changes relative to temperature. To compensate for ever-changing spring strength,
1311-407: Is being wound, and a power reserve indicator to show how long the chronometer will continue to run without being wound. These technical provisions usually yield timekeeping in mechanical marine chronometers accurate to within 0.5 second per day. In strictly horological terms, "rating" a chronometer means that prior to the instrument entering service, the average rate of gaining or losing per day
1380-399: Is observed and recorded on a rating certificate which accompanies the instrument. This daily rate is used in the field to correct the time indicated by the instrument to get an accurate time reading. Even the best-made chronometer with the finest temperature compensation etc. exhibits two types of error, (1) random and (2) consistent. The quality of design and manufacture of the instrument keeps
1449-464: Is particularly important for navigation. As the Earth rotates at a regular predictable rate, the time difference between the chronometer and the ship's local time can be used to calculate the longitude of the ship relative to the Prime Meridian (defined as 0°) (or another starting point) if accurately enough known, using spherical trigonometry . Practical celestial navigation usually requires
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#17327839888031518-636: Is the former observatory and time ball tower. In March 1864 New Zealand's first time ball was established at Wellington. This was followed by Port Chalmers in June 1867, Wanganui in October 1874, Lyttelton in December 1876 and Timaru in 1888. Attempts were made by some people in Auckland to establish time balls there from 1864 onwards, but these were not recognized by the authorities until a permanent time ball
1587-542: The Einheitschronometer and Hamilton's success, chronometers made in the old way never disappeared from the marketplace during the era of mechanical timekeepers. Thomas Mercer Chronometers was among the companies that continued to make them. Ship’s marine chronometers are the most exact portable mechanical timepieces ever produced and in a static environment were only trumped by non-portable precision pendulum clocks for observatories. They served, alongside
1656-598: The Transactions of the Royal Society ) are amongst the earliest series in England. In 1709 Derham published a more accurate measure of the speed of sound, at 1,072 Parisian feet per second. Derham used a telescope from the tower of the church of St Laurence, Upminster , to observe the flash of a distant shotgun being fired, and then measured the time until he heard the gunshot with a half second pendulum. Measurements were made of gunshots from local landmarks including
1725-737: The Loran-C hyperbolic radio navigation system until 1988, when the GPS global navigation satellite system was approved as reliable. At the end of the 20th century the production of mechanical marine chronometers had declined to the point where only a few were being made to special order by the First Moscow Watch Factory 'Kirov' ( Poljot ) in Russia, Wempe in Germany and Mercer in England. The most complete international collection of marine chronometers, including Harrison's H1 to H4,
1794-565: The NMEA 0183 interface, and can also improve the security of shipping traffic by enabling Automatic Identification Systems (AIS). Even with these convenient 21st-century technological tools, modern practical navigators usually use celestial navigation using electric-powered time sources in combination with satellite navigation. Small handheld computers, laptops, navigational calculators and even scientific calculators enable modern navigators to "reduce" sextant sights in minutes, by automating all
1863-407: The 1920 Nobel Prize for physics in recognition for his metallurgical work. The escapement serves two purposes. First, it allows the train to advance fractionally and record the balance's oscillations. At the same time, it supplies minute amounts of energy to counter tiny losses from friction, thus maintaining the momentum of the oscillating balance. The escapement is the part that ticks. Since
1932-471: The 1960s onwards mechanical spring detent marine chronometers were gradually replaced and supplanted by chronometers based on electric engineering techniques and technologies. In 1985 the British Ministry of Defence invited bids by tender for the disposal of their mechanical Hamilton Model 21 Marine Chronometers. The US Navy kept their Hamilton Model 21 Marine Chronometers in service as backups to
2001-434: The 1990s boats and ships can use several Global Navigation Satellite Systems (GNSS) to navigate all the world's lakes, seas and oceans. Maritime GNSS units include functions useful on water, such as "man overboard" (MOB) functions that allow instantly marking the location where a person has fallen overboard, which simplifies rescue efforts. GNSS may be connected to the ship's self-steering gear and Chartplotters using
2070-579: The Soviet Union, who confiscated the original Einheitschronometer technical drawings, and set up a production line in Moscow in 1949 that produced the first Soviet MX6 chronometers containing German made movements. From 1952 onwards until 1997 MX6 chronometers with minor НИИ ЧАСПРОМ (NII Chasprom — Horological institute of the Soviet era) devised alterations were produced from components all made in
2139-575: The Soviet Union. The German Einheitschronometer ultimately became the mechanical marine timekeeper design produced in the highest volume, with about 58,000 units produced. Of these, less than 3,000 were produced during World War II, about 5,000 after the war in West and East Germany and about 50,000 in the Soviet Union and later post-Soviet Russia. Of the Hamilton 21 Marine Chronometer during and after World War II about 13,000 units were produced. Despite
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2208-491: The accuracy of mechanical timepieces. The observatory testing regime typically lasted for 30 to 50 days and contained accuracy standards that were far more stringent and difficult than modern standards such as those set by the Contrôle Officiel Suisse des Chronomètres (COSC) . When a movement passed the observatory test, it became certified as an observatory chronometer and received a Bulletin de Marche from
2277-523: The being and attributes of God , and were used by William Paley nearly a century later. However, these books also include quantities of original scientific observations. For example, Physico-Theology contains his recognition of natural variation within species and that he knew that Didelphis virginialis (the Virginia opossum ) was the only marsupial in North America . It also includes one of
2346-411: The bottom. With the commencement of radio time signals (in Britain from 1924), time balls gradually became obsolete and many were demolished in the 1920s. A contemporary version of the concept has been used since 31 December 1907 at New York City 's Times Square as part of its New Year's Eve celebrations; at 11:59 p.m., a lit ball is lowered down a pole on the roof of One Times Square over
2415-452: The calculation and/or data lookup steps. Using multiple independent position fix methods without solely relying on subject-to-failure electronic systems helps the navigator detect errors. Professional mariners are still required to be proficient in traditional piloting and celestial navigation, which requires the use of a precisely adjusted and rated autonomous or periodically external time-signal corrected chronometer. These abilities are still
2484-429: The chronometer would be mounted in a sheltered location below decks to avoid damage and exposure to the elements. Mariners would use the chronometer to set a so-called hack watch , which would be carried on deck to make the astronomical observations. Though much less accurate (and less expensive) than the chronometer, the hack watch would be satisfactory for a short period of time after setting it (i.e., long enough to make
2553-536: The course of the sixty seconds ending at midnight. The spectacle was inspired by an organizer having seen the time ball on the Western Union Building in operation. Over sixty time balls remain standing, though many are no longer operational. Existing time balls include: Clearly seen from the river and aligned on the meridian for observation purposes, Building 20, also known as the Ball House,
2622-522: The earliest theoretical descriptions of a marine chronometer , accompanied by a discussion of the use of vacuum seals to reduce inaccuracies in the operation of timepieces. He is the first person known to have used the word chronometer . Similarly, Astro-Theology includes several newly identified nebulae (this was the name used at the time for all extended astronomical objects: some of his nebulae are what we would now call star clusters ). His 16-foot-long (4.9 m) telescope (also used when measuring
2691-718: The electronic era. The new technology was initially so expensive that not all ships carried chronometers, as illustrated by the fateful last journey of the East Indiaman Arniston , shipwrecked with the loss of 372 lives. However, by 1825, the Royal Navy had begun routinely supplying its vessels with chronometers. Beginning in 1820, the British Royal Observatory in Greenwich tested marine chronometers in an Admiralty instigated trial or "chronometer competition" program intended to encourage
2760-404: The elements and kept below decks in a fixed position in a traditional box suspended in gimbals (a set of rings connected by bearings). This keeps the chronometer isolated in a horizontal "dial up" position to counter ship inclination (rocking) movements induced timing errors on the balance wheel . Marine chronometers always contain a maintaining power which keeps the chronometer going while it
2829-565: The escapement. A detent escapement has a strong advantage over other escapements as it needs no lubrication. An impulse from the escape wheel to the impulse roller is nearly dead-beat, meaning little sliding action needing lubrication. Chronometer escape wheels and passing springs are typically gold due to the metal's lower slide friction over brass and steel. Chronometers often included other innovations to increase their efficiency and precision. Hard stones such as ruby and sapphire were often used as jewel bearings to decrease friction and wear of
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2898-404: The first measurement of longitude using marine chronometers aboard Aurore in 1767. In France, 1748, Pierre Le Roy invented the detent escapement characteristic of modern chronometers. In 1766, he created a revolutionary chronometer that incorporated a detent escapement , the temperature-compensated balance and the isochronous balance spring : Harrison showed the possibility of having
2967-585: The formation of the empire by wars and conquests of colonies abroad took place in a period in which British vessels had reliable navigation due to the chronometer, while their Portuguese, Dutch, and French opponents did not. For example: the French were well established in India and other places before Britain, but were defeated by naval forces in the Seven Years' War . Rating and maintaining marine chronometers
3036-466: The improvement of chronometers. In 1840 a new series of trials in a different format was begun by the seventh Astronomer Royal George Biddell Airy . These trials continued in much the same format until the outbreak of World War I in 1914, at which point they were suspended. Although the formal trials ceased, the testing of chronometers for the Royal Navy did not. Marine chronometer makers looked to
3105-423: The invention of the bi-metallic strip and caged roller bearings , inventions which are still widely used. However, H3's circular balances still proved too inaccurate and he eventually abandoned the large machines. Harrison solved the precision problems with his much smaller H4 chronometer design in 1761. H4 looked much like a large five-inch (12 cm) diameter pocket watch. In 1761, Harrison submitted H4 for
3174-778: The major ports of the United Kingdom (including Liverpool ) and around the maritime world. One was installed in 1833 at the Greenwich Observatory in London by the Astronomer Royal , John Pond , originally to enable tall ships in the Thames to set their marine chronometers, and the time ball has dropped at 1 p.m. every day since then. Wauchope submitted his scheme to American and French ambassadors when they visited England. The United States Naval Observatory
3243-402: The majority of chronometer balances used bi-metallic strips to move small weights toward and away from the centre of oscillation, thus altering the period of the balance to match the changing force of the spring. The balance spring problem was solved with a nickel-steel alloy named Elinvar for its invariable elasticity at normal temperatures. The inventor was Charles Édouard Guillaume , who won
3312-529: The most accurate quartz clocks when no signal is received, and their signals can be lost or blocked. However, there are autonomous quartz movements, even in wrist watches, that are accurate to within 5 or 20 seconds per year. At least one quartz chronometer made for advanced navigation utilizes multiple quartz crystals which are corrected by a computer using an average value, in addition to GPS time signal corrections. William Derham William Derham FRS (26 November 1657 – 5 April 1735)
3381-433: The natural resonance of an oscillating balance serves as the heart of a chronometer, chronometer escapements are designed to interfere with the balance as little as possible. There are many constant-force and detached escapement designs, but the most common are the spring detent and pivoted detent. In both of these, a small detent locks the escape wheel and allows the balance to swing completely free of interference except for
3450-425: The observations). Although industrial production methods began revolutionizing watchmaking in the middle of the 19th century, chronometer manufacture remained craft-based much longer and was dominated by British and Swiss manufacturers. Around the turn of the 20th century, Swiss makers such as Ulysse Nardin made great strides toward incorporating modern production methods and using fully interchangeable parts, but it
3519-492: The observatory, stipulating the performance of the movement. It was common for ships at the time to observe a time ball , such as the one at the Royal Observatory, Greenwich , to check their chronometers before departing on a long voyage. Every day, ships would anchor briefly in the River Thames at Greenwich, waiting for the ball at the observatory to drop at precisely 1pm. This practice was in small part responsible for
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#17327839888033588-407: The pivots and escapement. Diamond was often used as the cap stone for the lower balance staff pivot to prevent wear from years of the heavy balance turning on the small pivot end. Until the end of mechanical chronometer production in the third quarter of the 20th century, makers continued to experiment with things like ball bearings and chrome-plated pivots. The timepieces were normally protected from
3657-500: The random errors small. In principle, the consistent errors should be amenable to elimination by adjustment, but in practice it is not possible to make the adjustment so precisely that this error is completely eliminated, so the technique of rating is used. The rate will also change while the instrument is in service due to e.g. thickening of the oil, so on long expeditions the instrument's rate would be periodically checked against accurate time determined by astronomical observations. Since
3726-429: The return oscillation, a passing spring on the tip of the detent allows the unlocking roller on the staff to move by without displacing the detent. The weakest link of any mechanical timekeeper is the escapement's lubrication. When the oil thickens through age or temperature or dissipates through humidity or evaporation, the rate will change, sometimes dramatically as the balance motion decreases through higher friction in
3795-460: The rolling of the seas and keep precise time while in shipboard conditions. In 1714, the British government offered a longitude prize for a method of determining longitude at sea, with the awards ranging from £10,000 to £20,000 (£2 million to £4 million in 2024 terms) depending on accuracy. John Harrison , a Yorkshire carpenter, submitted a project in 1730, and in 1735 completed a clock based on
3864-518: The sextant, to determine the location of ships at sea. The seafaring nations invested richly in the development of these precision instruments, as pinpointing location at sea gave a decisive naval advantage. Without their accuracy and the accuracy of the feats of navigation that marine chronometers enabled, it is arguable that the ascendancy of the Royal Navy , and by extension that of the British Empire , might not have occurred so overwhelmingly;
3933-430: The subsequent adoption of Greenwich Mean Time as an international standard. (Time balls became redundant around 1920 with the introduction of radio time signals , which have themselves largely been superseded by GPS time .) In addition to setting their time before departing on a voyage, ship chronometers were also routinely checked for accuracy while at sea by carrying out lunar or solar observations. In typical use,
4002-568: The sun's angle at noon (i.e., when it reached its highest point in the sky, or culmination ) or, in the Northern Hemisphere, by measuring the angle of Polaris (the North Star) from the horizon (usually during twilight ). To find their longitude , however, they needed a time standard that would work aboard a ship. Observation of regular celestial motions, such as Galileo's method based on observing Jupiter's natural satellites ,
4071-537: The velocity of sound) was at the top of the tower of St Laurence's Church, where the necessary doors are still in place. On 3 February 1703, Derham was elected Fellow of the Royal Society . He was Boyle lecturer in 1711–1712. His last known work, entitled A Defence of the Church's Right in Leasehold Estates , appeared as early as 1731. But besides the works published in his own name, Derham contributed
4140-592: The £20,000 longitude prize. His design used a fast-beating balance wheel controlled by a temperature-compensated spiral spring. These features remained in use until stable electronic oscillators allowed very accurate portable timepieces to be made at affordable cost. In 1767, the Board of Longitude published a description of his work in The Principles of Mr. Harrison's time-keeper . A French expedition under Charles-François-César Le Tellier de Montmirail performed
4209-681: Was Rector at Upminster , Essex . While at Upminster, in 1716 he became a Canon of Windsor and the vestry minutes show that thereafter he divided his time between those two places. The parish registers of Upminster record his burial at St. Laurence's in 1735. However, the precise site of his grave is unknown and, in accordance with his wishes, there is no memorial to him in the church. In 1696, he published his Artificial Clockmaker , which went through several editions. The best known of his subsequent works are Physico-Theology , published in 1713; Astro-Theology , 1714; and Christo-Theology , 1730. All three of these books are teleological arguments for
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#17327839888034278-551: Was an English clergyman, natural theologian , natural philosopher and scientist . He produced the earliest reasonably accurate measurement of the speed of sound . William Derham was the son of Thomas Derham. He was born at Stoulton , in Worcestershire , England. He was educated at Blockley , Gloucestershire , and at Trinity College, Oxford , from 1675 to 1679. He was ordained on 29 May 1681. In 1682, he became vicar of Wargrave , Berkshire , and from 1689 to 1735 he
4347-740: Was deemed important well into the 20th century, as after World War I the work of the British Royal Observatory’s Chronometer Department became largely confined to rating of chronometers and watches that the Admiralty already owned and providing acceptance testing. In 1937 a workshop was set up for the first time by the Time Department for the repair and adjustment of British armed forces issued chronometers and watches. These maintenance activities had previously been outsourced to commercial workshops. From about
4416-525: Was established in Washington, D.C., and the first American time ball went into service in 1845. Time balls were usually dropped at 1 p.m. (although in the United States they were dropped at noon). They were raised half way about 5 minutes earlier to alert the ships, then with 2–3 minutes to go they were raised the whole way. The time was recorded when the ball began descending, not when it reached
4485-652: Was followed by a further theoretical description of a chronometer in works published by English scientist William Derham in 1713. Derham's principal work, Physico-theology, or a demonstration of the being and attributes of God from his works of creation , also proposed the use of vacuum sealing to ensure greater accuracy in the operation of clocks. Attempts to construct a working marine chronometer were begun by Jeremy Thacker in England in 1714, and by Henry Sully in France two years later. Sully published his work in 1726 with Une Horloge inventée et executée par M. Sulli , but neither his nor Thacker's models were able to resist
4554-743: Was mounted on the Ferry Building in August 1901. Marine chronometer The term chronometer was coined from the Greek words χρόνος ( chronos ) (meaning time) and meter (meaning measure). The 1713 book Physico-Theology by the English cleric and scientist William Derham includes one of the earliest theoretical descriptions of a marine chronometer. It has recently become more commonly used to describe watches tested and certified to meet certain precision standards. To determine
4623-424: Was not the only answer to the problem. The greatest strides toward practicality came at the hands of Thomas Earnshaw and John Arnold , who in 1780 developed and patented simplified, detached, "spring detent" escapements , moved the temperature compensation to the balance, and improved the design and manufacturing of balance springs . This combination of innovations served as the basis of marine chronometers until
4692-549: Was only with the onset of World War II that the Hamilton Watch Company in the United States perfected the process of mass production , which enabled it to produce thousands of its Hamilton Model 21 and Model 22 chronometers from 1942 onwards for the branches of the United States military and merchant marine as well as other Allied forces during World War II. The Hamilton 21 Marine Chronometer had
4761-406: Was usually not possible at sea due to the ship's motion. The lunar distances method , initially proposed by Johannes Werner in 1514, was developed in parallel with the marine chronometer. The Dutch scientist Gemma Frisius was the first to propose the use of a chronometer to determine longitude in 1530. The purpose of a chronometer is to measure accurately the time of a known fixed location. This
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