The Prime Meridian is the line of longitude at which the longitude is defined to be 0°.
The Prime Meridian and its opposite the 180th meridian (at 180° longitude), which the International Date Line generally follows, form a great circle that divides the Earth into the Eastern and Western Hemispheres.
An international conference in 1884 decided the modern Prime Meridian passes through the Royal Observatory, Greenwich in southeast London, United Kingdom, known as the International Meridian or Greenwich Meridian, although the Prime Meridian is ultimately arbitrary unlike the parallels of latitude, which are defined by the rotational axis of the Earth with the Poles at 90° and the Equator at 0°.
Historically, various meridians have been used, including four different ones through Greenwich.
The Prime Meridian is ultimately arbitrary—a matter of convention—and various conventions have been used or advocated in different regions and throughout history:
The modern Greenwich Meridian, based at the Royal Observatory, Greenwich, was established by Sir George Airy in 1851. By 1884, over two-thirds of all ships and tonnage used it as the reference meridian on their maps. In October of that year, at the behest of U.S. President Chester A. Arthur, 41 delegates from 25 nations met in Washington, D.C., USA, for the International Meridian Conference. This conference selected the Greenwich Meridian as the official Prime Meridian due to its popularity. However, France abstained from the vote and French maps continued to use the Paris Meridian for several decades.
The Greenwich Meridian is now marked at night by a laser beam emitted northwards from the observatory.
The International Earth Rotation and Reference Systems Service (IERS) maintains the IERS Reference Meridian (IRM), also called the International Reference Meridian, which is the reference meridian (Prime Meridian, 0° longitude) of the Global Positioning System operated by the United States Department of Defense. It is the reference meridian in WGS84 and its two formal versions, the ideal International Terrestrial Reference System (ITRS) and its realization, the International Terrestrial Reference Frame (ITRF).
The IRM is 5.31 arcseconds east of Airy's transit circle or 102.5 metres (336.3 feet) at the latitude of the Royal Observatory, Greenwich. This shift is a legacy of the first satellite navigation system, the Doppler based TRANSIT system. TRANSIT was developed by the Applied Physics Laboratory of Johns Hopkins University. Its lab is located in Howard County, Maryland, which was the location of TRANSIT's first ground station. The station's surveyed coordinates in the North American Datum 1927 (NAD27) — a non-Earth centered ellipsoid — became its coordinates in an Earth-centered ellipsoid, such as the World Geodetic System. This shifted the coordinates of any other location on an Earth-centered ellipsoid, especially those far away.
When the antenna of a TRANSIT ground station was mounted directly above Airy's transit circle in June 1969, its longitude on an Earth-centered ellipsoid was 5.64 arcseconds west of TRANSIT's reference meridian. Several small additional longitude shifts were created by further improvement in gravitational models such as the Earth Geopotential Model 1996 (EGM96), a dramatic increase in the number of ground stations from only four to over 500, and the use of time-based GPS.
The International Hydrographic Organization adopted an early version of the IRM in 1983 for all nautical charts. The IRM was adopted for air navigation by the International Civil Aviation Organization on 3 March 1989. Tectonic plates slowly move over the surface of the Earth, so most countries have adopted for their maps an IRM version fixed relative to their own tectonic plate as it existed at the beginning of a specific year. Examples include the North American Datum 1983 (NAD83), the European Terrestrial Reference Frame 1989 (ETRF89), and the Geocentric Datum of Australia 1994 (GDA94). Versions fixed to a tectonic plate differ from the global version by at most a few centimetres.
However, the IRM is not fixed to any point on Earth. Instead, all points on the European portion of the Eurasian plate, including the Royal Observatory, are slowly moving northeast about 2.5 cm per year relative to it. Thus this IRM is the weighted average (in the least squares sense) of the reference meridians of the hundreds of ground stations contributing to the IERS network. The network includes GPS stations, Satellite Laser Ranging (SLR) stations, Lunar Laser Ranging (LLR) stations, and the highly accurate Very Long Baseline Interferometry (VLBI) stations. All stations' coordinates are adjusted annually to remove net rotation relative to the major tectonic plates. If Earth had only two hemispherical plates moving relative to each other around any axis which intersects their centres or their junction, then the longitudes (around any other rotation axis) of any two, diametrically opposite, stations must move in opposite directions by the same amount.
Universal Time is notionally based on the WGS84 meridian. Because of changes in the Earth's rotation, the standard international time UTC can differ from the mean observed time on the meridian by up to 0.9 second (equivalent to about 260 metres at Greenwich). Leap seconds are inserted periodically to keep UTC close to Earth's angular position relative to the Sun — mean solar time.
Category:Time zones Category:Geodesy Category:Lines of longitude Category:1884 establishments Category:English inventions Category:Geography of Greenwich
af:Greenwich ar:خط غرينتش ast:Meridianu de Greenwich be:Грынвіцкі мерыдыян be-x-old:Грынвіцкі мэрыдыян bg:Начален меридиан ca:Meridià de Greenwich cs:Základní poledník da:Nulmeridianen de:Nullmeridian et:Algmeridiaan es:Meridiano de Greenwich eo:Grenviĉa Meridiano eu:Greenwich meridianoa fa:نصفالنهار مبدأ fo:Greenwichmeridianin fr:Méridien de Greenwich fy:Nulmeridiaan gl:Meridiano de Greenwich ko:본초 자오선 hi:मध्याह्न रेखा hr:Grinički meridijan id:Meridian utama is:Núllbaugur it:Meridiano di Greenwich he:קו גריניץ' ka:გრინვიჩის მერიდიანი ht:Premye meridyen lv:Griničas meridiāns hu:Nullmeridián mk:Нулти меридијан ms:Meridian Perdana nl:Meridiaan van Greenwich ja:グリニッジ子午線 no:Nullmeridianen nn:Nullmeridianen pl:Południk zerowy pt:Meridiano de Greenwich ru:Гринвичский меридиан sq:Meridiani i Griniçit simple:Prime Meridian sk:Greenwichský poludník sr:Гринички меридијан sv:Nollmeridian tl:Punong Meridyano th:เส้นไพรม์เมอริเดียน tr:Baş meridyen uk:Гринвіцький меридіан vi:Kinh tuyến gốc zh:本初子午線This text is licensed under the Creative Commons CC-BY-SA License. This text was originally published on Wikipedia and was developed by the Wikipedia community.
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