International Meridian Conference | |
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Host country | United States |
Date | 1 October 1884 [1] |
Cities | Washington, D.C. |
Chair | C. R. P. Rodgers [1] |
Key points | |
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The International Meridian Conference was a conference held in October 1884 in Washington, D.C., in the United States, to determine a prime meridian for international use. [1] The conference was held at the request of U.S. President Chester A. Arthur. [1] The subject to discuss was the choice of "a meridian to be employed as a common zero of longitude and standard of time reckoning throughout the world". [1] It resulted in the recommendation of the Greenwich Meridian as the international standard for zero degrees longitude. [1]
By the 1870s there was pressure both to establish a prime meridian for worldwide navigation purposes and to unify local times for railway timetables. The first International Geographical Congress, held in Antwerp in 1871, passed a motion in favour of the use of the Greenwich Meridian for (smaller scale) passage charts, suggesting that it should become mandatory within 15 years. [2]
In Britain, the Great Western Railway had standardised time by 1840 and in 1847 the Railway Clearing Union decreed that "GMT be adopted at all stations as soon as the General Post Office permitted it". The Post Office was by this time transmitting time signals from Greenwich by telegraph to most parts of the country to set the clocks. By January 1848, Bradshaw's railway guide showed the unified times and met with general approval, although legal disputes meant that it was not until 1890 that GMT was formally established across the UK. [3]
In the United States, the problems were much more severe, with one table showing over 100 local times varying by more than 3 hours. In 1870, Charles F. Dowd published a pamphlet titled A System of national time and its application advocating three time zones across the country based on the Washington meridian, modifying this to four zones based on the Greenwich meridian in 1872.
The first proposal for a consistent treatment of time worldwide was a memoir entitled "Terrestrial Time" by Sandford Fleming, at the time the chief engineer of the Canadian Pacific Railway, presented to the Canadian Institute in 1876. This envisaged clocks showing 24-hour universal time with an extra dial having a local time rounded to the nearest hour. [4] He also pointed out that many of the corrections for local mean time were greater than those involved in abandoning solar time. In 1878/79, he produced modified proposals using the Greenwich meridian. Fleming's two papers were considered so important that in June 1879 the British Government forwarded copies to eighteen foreign countries and to various scientific bodies in England. [5] At the same time the American Metrological Society produced a "Report on Standard Time" by Cleveland Abbe, chief of the United States Weather Service proposing essentially the same scheme.
These proposals did not meet universal approval in the scientific community, being opposed by John Rodgers, Superintendent of the Naval Observatory, Washington and British Astronomer Royal, George Airy who had both established wire services supporting local time in various cities. The Naval Observatory had also foiled the onward transmission of the Greenwich time signal from Harvard, where it was received via transatlantic cable and used to time a time ball in Boston. [6]
The International Meridian Conference had its origins in the Third International Geographical Congress held in Venice in 1881, in which the establishment of a universal prime meridian and a uniform standard of time was high on the agenda. The Seventh International Geodesic Conference in Rome in October 1883 then thrashed out most of the technical details, leaving the diplomatic agreements to a later conference. The United States passed an Act of Congress on 3 August 1882 authorizing the President to call an international conference to fix on a common prime meridian for time and longitude throughout the world. [7]
On 11 October 1883, a convention of railroad executives met in Chicago and agreed to the implementation of five time zones in North America, using as a basis Greenwich Mean Time. [8] [9] Before the invitations to the Washington conference were sent out on 1 December, the joint efforts of Abbe, Fleming and William Frederick Allen, Secretary of the US railways' General Time Convention and Managing Editor of the Travellers' Official Guide to the Railways, had brought the US railway companies to an agreement which led to standard railway time being introduced at noon on 18 November 1883 across the nation. Thus, a strong sense of fait accompli preceded the Washington conference, although setting local times was not part of the remit of the conference [10] and it was not legally established until 1918.
Twenty-six countries, represented by 41 delegates, participated in the conference: [1]
On 22 October 1884, the following resolutions were adopted by the conference (voting took place on 13 October): [11] [12]
- That it is the opinion of this Congress that it is desirable to adopt a single prime meridian for all nations, in place of the multiplicity of initial meridians which now exist. (This resolution was unanimously adopted.)
- That the Conference proposes to the Governments here represented the adoption of the meridian passing through the centre of the transit instrument at the Observatory of Greenwich as the initial meridian for longitude. (Ayes, 22; noes, 1; abstaining, 2.)
- That from this meridian longitude shall be counted in two directions up to 180 degrees, east longitude being plus and west longitude minus. (Ayes, 14; noes, 5; abstaining, 6.)
- That the Conference proposes the adoption of a universal day for all purposes for which it may be found convenient, and which shall not interfere with the use of local or standard time where desirable. (Ayes, 23; abstaining, 2.)
- That this universal day is to be a mean solar day; is to begin for all the world at the moment of mean midnight of the initial meridian, coinciding with the beginning of the civil day and date of that meridian; and is to be counted from zero up to twenty-four hours. (Ayes, 14; noes, 3; abstaining, 7.)
- That the Conference expresses the hope that as soon as may be practicable the astronomical and nautical days will be arranged everywhere to begin at midnight.
- That the Conference expresses the hope that the technical studies designed to regulate and extend the application of the decimal system to the division of angular space and of time shall be resumed, so as to permit the extension of this application to all cases in which it presents real advantages. (Ayes, 21; abstaining, 3.)
Resolution 2, fixing the meridian at Greenwich, was passed 22–1 (San Domingo, now the Dominican Republic, voted against); France and Brazil abstained. The French did not adopt the Greenwich meridian as the beginning of the universal day until 1911. Even then it refused to use the name "Greenwich", instead using the term "Paris mean time, retarded by 9 minutes and 21 seconds". France finally replaced this phrase with "Coordinated Universal Time" (UTC) in 1978. [13]
Resolution 4 expressly exempts standard time from the universal day. Although two delegates, including Sandford Fleming, proposed the adoption of standard time by all nations, other delegates objected, stating that it was outside the purview of the conference, so neither proposal was subjected to a vote. Thus the conference did not adopt any time zones, contrary to popular belief.
Regarding resolution 6: Great Britain had already shifted the beginning of the nautical day from noon, twelve hours before midnight, to midnight in 1805, during the Battle of Trafalgar. The astronomical day was shifted from noon, twelve hours after midnight, to midnight effective 1 January 1925 by a resolution of the newly formed International Astronomical Union. [14]
On 13 October 1884, the following resolution was not adopted:
- That the initial meridian should have a character of absolute neutrality. It should be chosen exclusively so as to secure to science and to international commerce all possible advantages, and especially should cut no great continent—neither Europe nor America. (Ayes, 3; noes, 21.)
Twenty-one countries voted against the proposal, while three (France, Brazil, San Domingo) voted in favor.
From the Act of the Conference [1] the Delegates were:
Name | Designation | on behalf of ... |
---|---|---|
Present | ||
Baron Ignatz von Schäffer | Envoy Extraordinary and Minister Plenipotentiary | Austria-Hungary |
Luís Cruls | Director of the Imperial Observatory of Rio de Janeiro | Brazil |
Commodore S. R. Franklin | U.S. Navy, Superintendent U.S. Naval Observatory | Colombia |
Juan Francisco Echeverria | Civil Engineer | Costa Rica |
A. Lefaivre | Minister Plenipotentiary and Consul-General | France |
Pierre Janssen | Director of the Physical Observatory of Paris | France |
Baron H. von Alvensleben | Envoy Extraordinary and Minister Plenipotentiary | German Empire |
Captain Sir F. J. O. Evans | Royal Navy | Great Britain |
J. C. Adams | Director of the Cambridge Observatory | Great Britain |
Lieut.-General Richard Strachey | Member of the Council of India | Great Britain |
Sandford Fleming | representing the Dominion of Canada | Great Britain |
M. Miles Rock | President of the Boundary Commission | Guatemala |
Hon. W. D. Alexander | Surveyor-General | Hawaii |
Hon. Luther Aholo | Privy Counsellor | Hawaii |
Count Alberto De Foresta | First Secretary of Legation | Italy |
Professor Kikuchi Dairoku | Dean of the Scientific Department of the University of Tokyo | Japan |
Leandro Fernandez | Civil Engineer | Mexico |
Angel Anguiano | Director of the National Observatory of Mexico | Mexico |
Captain John Stewart | Counsul-General | Paraguay |
C. de Struve | Envoy Extraordinary and Minister Plenipotentiary | Russia |
Major-General Stebnitzki | Imperial Russian Staff | Russia |
J. de Kologrivoff | Conseiller d'État actuel | Russia |
M. de J. Galvan | Envoy extraordinary and Minister Plenipotentiary | San Domingo |
Antonio Batres | Envoy extraordinary and Minister Plenipotentiary | Salvador |
Juan Valera | Envoy Extraordinary and Minister Plenipotentiary | Spain |
Emilio Ruiz del Arbol | Naval Attaché to the Spanish Legation | Spain |
Juan Pastorin | Officer of the Navy | Spain |
Count Carl Lewenhaupt | Envoy Extraordinary and Minister Plenipotentiary | Sweden |
Colonel Emil Frey | Envoy Extraordinary and Minister Plenipotentiary | Switzerland |
Rear-Admiral C. R. P. Rodgers | U.S. Navy | United States |
Lewis Morris Rutherfurd | United States | |
W. F. Allen | Secretary Railway Time Conventions | United States |
Commander W. T. Sampson | U.S. Navy | United States |
Professor Cleveland Abbe | U.S. Signal Office | United States |
Señor A. M. Soteldo | Chargé d'Affaires | Venezuela |
Not present | ||
Francisco Vidal Gormaz | Director of the Hydrographic Office | Chile |
Alavaro Bianchi Tupper | Assistant Director | Chile |
Carl Steen Andersen de Bille | Minister Resident and Consul-General | Denmark |
Hinckeldeyn | Attaché of the German Legation | Germany |
William Coppinger | Consul-General | Liberia |
G. de Weckherlin | Envoy Extraordinary and Minister Plenipotentiary | Netherlands |
Ahmet Rüstem Bey | Secretary of Legation | Ottoman Empire |
This section needs additional citations for verification .(October 2018) |
The main issue at the conference, apart from procedural issues such as the provision of an authorized French translation of the proceedings, was France's insistence that the meridian should have a strictly neutral character in the same way that they maintained that the metre was a neutral measure. This requirement conflicted with the need to base measurements on an established observatory on land and Fleming's proposal of using the anti-meridian of Greenwich was not supported by the British delegation. In the end, the pragmatic argument for continuity with most nautical charts won the day and the French delegation abstained in the vote.
On the question of universal time, Fleming's opinion to one of the lead-up committees was borne out: "In my judgment, the nearest approach to it which may be attempted with any chance of success, is to have first, a primary standard time, based on the prime meridian that is to be used for non-local purposes; second, to have twenty-four secondary standard times to govern local reckoning." [15] There was discussion of setting zones as small as 10 minutes (2½°) (that's 10 minutes of time, not 10 minutes of arc/angular measure), but no motion was tabled, as there was little experience to guide the choice.
Most European countries aligned their clocks with Greenwich within ten years, Sweden and North America already having done so, and the trend continued. The French maintained Paris time till 1911 and the following year convened a second conference to address the differences between different observatories which had become apparent, leading to the establishment of the Bureau International de l'Heure after World War I. [16]
Greenwich Mean Time (GMT) is the local mean time at the Royal Observatory in Greenwich, London, counted from midnight. At different times in the past, it has been calculated in different ways, including being calculated from noon; as a consequence, it cannot be used to specify a particular time unless a context is given. The term "GMT" is also used as one of the names for the time zone UTC+00:00 and, in UK law, is the basis for civil time in the United Kingdom.
A time zone is an area which observes a uniform standard time for legal, commercial and social purposes. Time zones tend to follow the boundaries between countries and their subdivisions instead of strictly following longitude, because it is convenient for areas in frequent communication to keep the same time.
A time standard is a specification for measuring time: either the rate at which time passes or points in time or both. In modern times, several time specifications have been officially recognized as standards, where formerly they were matters of custom and practice. An example of a kind of time standard can be a time scale, specifying a method for measuring divisions of time. A standard for civil time can specify both time intervals and time-of-day.
Universal Time is a time standard based on Earth's rotation. While originally it was mean solar time at 0° longitude, precise measurements of the Sun are difficult. Therefore, UT1 is computed from a measure of the Earth's angle with respect to the International Celestial Reference Frame (ICRF), called the Earth Rotation Angle. UT1 is the same everywhere on Earth. UT1 is required to follow the relationship
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.
Sir Sandford Fleming was a Scottish Canadian engineer and inventor. Born and raised in Scotland, he emigrated to colonial Canada at the age of 18. He promoted worldwide standard time zones, a prime meridian, and use of the 24-hour clock as key elements to communicating the accurate time, all of which influenced the creation of Coordinated Universal Time. He designed Canada's first postage stamp, produced a great deal of work in the fields of land surveying and map making, engineered much of the Intercolonial Railway and the first several hundred kilometers of the Canadian Pacific Railway, and was a founding member of the Royal Society of Canada and founder of the Canadian Institute.
The modern 24-hour clock is the convention of timekeeping in which the day runs from midnight to midnight and is divided into 24 hours. This is indicated by the hours passed since midnight, from 00(:00) to 23(:59), with 24(:00) as an option to indicate the end of the day. This system, as opposed to the 12-hour clock, is the most commonly used time notation in the world today, and is used by the international standard ISO 8601.
The Greenwich meridian is a prime meridian, a geographical reference line that passes through the Royal Observatory, Greenwich, in London, England. From 1884 to 1974, the Greenwich meridian was the international standard prime meridian, used worldwide for timekeeping and navigation. The modern standard, the IERS Reference Meridian, is based on the Greenwich meridian, but differs slightly from it. This prime meridian was first established by Sir George Airy in 1851, and by 1884, over two-thirds of all ships and tonnage used it as the reference meridian on their charts and maps. In October of that year, at the invitation of the President of the United States, 41 delegates from 25 nations met in Washington, D.C., United States, for the International Meridian Conference. This conference selected the meridian passing through Greenwich as the world standard prime meridian due to its popularity. However, France abstained from the vote, and French maps continued to use the Paris meridian for several decades. In the 18th century, London lexicographer Malachy Postlethwayt published his African maps showing the "Meridian of London" intersecting the Equator a few degrees west of the later meridian and Accra, Ghana.
Indian Standard Time (IST), sometimes also called India Standard Time, is the time zone observed throughout the Republic of India, with a time offset of UTC+05:30. India does not observe daylight saving time or other seasonal adjustments. In military and aviation time, IST is designated E* ("Echo-Star"). It is indicated as Asia/Kolkata in the IANA time zone database.
In geography and geodesy, a meridian is the locus connecting points of equal longitude, which is the angle east or west of a given prime meridian. In other words, it is a line of longitude. The position of a point along the meridian is given by that longitude and its latitude, measured in angular degrees north or south of the Equator. On a Mercator projection or on a Gall-Peters projection, each meridian is perpendicular to all circles of latitude. A meridian is half of a great circle on Earth's surface. The length of a meridian on a modern ellipsoid model of Earth has been estimated as 20,003.93 km (12,429.87 mi).
Standard time is the synchronization of clocks within a geographical region to a single time standard, rather than a local mean time standard. Generally, standard time agrees with the local mean time at some meridian that passes through the region, often near the centre of the region. Historically, standard time was established during the 19th century to aid weather forecasting and train travel. Applied globally in the 20th century, the geographical regions became time zones. The standard time in each time zone has come to be defined as an offset from Universal Time. A further offset is applied for part of the year in regions with daylight saving time.
The Paris meridian is a meridian line running through the Paris Observatory in Paris, France – now longitude 2°20′14.02500″ East. It was a long-standing rival to the Greenwich meridian as the prime meridian of the world. The "Paris meridian arc" or "French meridian arc" is the name of the meridian arc measured along the Paris meridian.
Charles F. Dowd (1825–1904) was a co-principal of the Temple Grove Ladies Seminary in Saratoga Springs, New York. He was the first person to propose multiple time zones for any country, those for the railways of the United States. He did not propose their extension to the entire world, which was suggested by the Italian mathematician Quirico Filopanti, and championed by the Canadian engineer Sandford Fleming.
Bombay Time was one of the two official time zones established in British India in 1884. The time zone was established during the International Meridian Conference held at Washington, D.C. in the United States in 1884. It was then decided that India would have two time zones, Calcutta, and Bombay. Bombay Time was set at 4 hours and 51 minutes ahead of Greenwich Mean Time (GMT).
The 25th meridian of longitude west from Washington is a line of longitude approximately 102.05 degrees west of the Prime Meridian of Greenwich. In the United States of America, the meridian 25 degrees west of the Washington Meridian defines the eastern boundary of the State of Colorado, the western boundary of the State of Kansas, and the western boundary of the State of Nebraska south of the 41st parallel north.
Mecca Time was a proposed time standard that uses the line of longitude that goes through Mecca, Saudi Arabia as its Prime Meridian. A clock based on this meridian would be at approximately UTC+02:39:18.3.
Coordinated Universal Time (UTC) is the primary time standard globally used to regulate clocks and time. It establishes a reference for the current time, forming the basis for civil time and time zones. UTC facilitates international communication, navigation, scientific research, and commerce.
The IERS Reference Meridian (IRM), also called the International Reference Meridian, is the prime meridian maintained by the International Earth Rotation and Reference Systems Service (IERS). It passes about 5.3 arcseconds east of George Biddell Airy's 1851 transit circle which is 102 metres (335 ft) at the latitude of the Royal Observatory, Greenwich. Thus it differs slightly from the historical Greenwich Meridian.
Finland uses Eastern European Time (EET) during the winter as standard time and Eastern European Summer Time (EEST) during the summer as daylight saving time. EET is two hours ahead of coordinated universal time (UTC+02:00) and EEST is three hours ahead of coordinated universal time (UTC+03:00). Finland adopted EET on 30 April 1921, and has observed daylight saving time in its current alignment since 1981 by advancing the clock forward one hour at 03:00 EET on the last Sunday in March and back at 04:00 EET on the last Sunday in October, doing so an hour earlier for the first two years.
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