# Prime meridian

Not to be confused with Principal meridian.
Prime Meridian

A prime meridian is a meridian (a line of longitude) in a geographical coordinate system at which longitude is defined to be 0°. A prime meridian and its opposite in a 360°-system, the 180th meridian (at 180° longitude), form a great circle.

This great circle divides the sphere, e.g., the Earth, into two hemispheres. If one uses directions of East and West from a defined prime meridian, then they can be called Eastern Hemisphere and Western Hemisphere.

File:Atlas Cosmographicae (Mercator) 033.jpg
Gerardus Mercator in his Atlas Cosmographicae (1595) uses a prime meridian somewhere close to 25°W, passing just to the west of Santa Maria Island in the Atlantic. His 180th meridian runs along the Strait of Anián (Bering Strait)

A prime meridian is ultimately arbitrary, unlike an equator, which is determined by the axis of rotation—and various conventions have been used or advocated in different regions and throughout history.[1]

## History

File:Ptolemy-World Vat Urb 82.jpg
Ptolemy's 1st projection, redrawn under Maximus Planudes around 1300, using a prime meridian west of Africa

The notion of longitude was developed by the Greek Eratosthenes (c. 276 BC – c. 195 BC) in Alexandria and Hipparchus (c. 190 BC – c. 120 BC) in Rhodes and applied to a large number of cities by the geographer Strabo (64/63 BC – c. 24 AD). But it was Ptolemy (c. AD 90 – c. AD 168) who first used a consistent meridian for a world map in his Geographia.

Ptolemy used as his basis the "Fortunate Isles", a group of islands in the Atlantic which are usually associated with the Canary Islands (13° to 18°W), although his maps correspond more closely to the Cape Verde islands (22° to 25° W). The main point is to be comfortably west of the western tip of Africa (17.5° W) as negative numbers were not yet in use. His prime meridian corresponds to 18° 40' west of Winchester (about 20°W) today.[2] At this time the chief method of determining longitude was by using the reported times of lunar eclipses in different countries.

File:Worldmap 1529-Ribero.jpeg
Diogo Ribeiro's map of 1529, now in the Vatican library

Ptolemy’s Geographia was first printed with maps at Bologna in 1477 and many early globes in the sixteenth century followed his lead. But there was still a hope that a "natural" basis for a prime meridian existed. Christopher Columbus reported (1493) that the compass pointed due north somewhere in mid-Atlantic and this fact was used in the important Tordesillas Treaty of 1494 which settled the territorial dispute between Spain and Portugal over newly discovered lands. The Tordesillas line was eventually settled at 370 leagues west of Cape Verde. This is shown in Diogo Ribeiro's 1529 map. São Miguel Island (25.5°W) in the Azores was still used for the same reason as late as 1594 by Christopher Saxton, although by this time it had been shown that the zero deviation line did not follow a line of longitude.[3]

File:Atlas Ortelius KB PPN369376781-006av-006br.jpg
1571 Africa map by Abraham Ortelius, Cabo Verde prime meridian

In 1541, Mercator produced his famous forty-one centimetre terrestrial globe and drew his prime meridian precisely through Fuertaventura (14°1'W) in the Canaries. His later maps used the Azores, following the magnetic hypothesis. But by the time that Ortelius produced the first modern atlas in 1570, other islands such as Cape Verde were coming into use. In his atlas longitudes were counted from 0° to 360°, not 180°W to 180°E as is common today. This practice was followed by navigators well into the eighteenth century.[4] In 1634, Cardinal Richelieu used the westernmost island of the Canaries, Ferro, 19° 55' west of Paris, as the choice of meridian. Unfortunately, the geographer Delisle decided to round this off to 20°, so that it simply became the meridian of Paris disguised.[5]

In the early eighteenth century the battle was on to improve the determination of longitude at sea, leading to the development of the chronometer by John Harrison. But it was the development of accurate star charts principally by the first British Astronomer Royal, John Flamsteed between 1680 and 1719 and disseminated by his successor, Edmund Halley that enabled navigators to use the lunar method of determining longitude more accurately using the octant developed by Thomas Godfrey and John Hadley.[6] Between 1765 and 1811, Nevil Maskelyne published 49 issues of the Nautical Almanac based on the meridian of the Royal Observatory, Greenwich. "Maskelyne's tables not only made the lunar method practicable, they also made the Greenwich meridian the universal reference point. Even the French translations of the Nautical Almanac retained Maskelyne's calculations from Greenwich—in spite of the fact that every other table in the Connaissance des Temps considered the Paris meridian as the prime." [7]

In 1884, at the International Meridian Conference held in Washington, D.C., 22 countries voted to adopt the Greenwich meridian as the prime meridian of the world. The French argued for a neutral line, mentioning the Azores and the Bering Strait but eventually abstained and continued to use the Paris meridian until 1911.

## List of prime meridians on Earth

Locality GPS longitude Meridian name Comment
Bering Strait 168°30′ W
• Bering Strait offered 1884 as possibility for a "neutral prime meridian" by Pierre Janssen at the International Meridian Conference [8]
Washington, D.C. 77°03′56.07″ W (1897) or 77°04′02.24″ W (NAD 27) or 77°04′01.16″ W (NAD 83) New Naval Observatory Meridian
Washington, D.C. 77°02′48.0″ W, 77°03′02.3″, 77°03′06.119″ W or 77°03′06.276″ W (both presumably NAD 27). If NAD27, the latter would be 77°03′05.194″ W (NAD 83) Old Naval Observatory Meridian
Washington, D.C. 77°02′11.56258″ W (NAD 83), 77°02′11.55880″ W (NAD 83), 77°02′11.57375″ W (NAD 83) White House Meridian
Washington, D.C. 77°00′32.6″ W (NAD 83) Capitol meridian
Philadelphia 75° 10′ 12″ W [9][10]
Rio de Janeiro 43° 10′ 19″ W [11]
Fortunate Isles / Azores ~ 25° 40′ 32″ W Used until the Middle Ages, proposed as one possible neutral meridian by Pierre Janssen at the International Meridian Conference[12]
El Hierro (Ferro),
Canary Islands
18° 03′ W,
later redefined as
17° 39′ 46″? W
Ferro Meridian [13]
Tenerife 16° 38' 22" W Tenerife meridian Rose to prominence with Dutch cartographers and navigators after they abandoned the idea of a magnetic meridian[14]
Lisbon 9° 07′ 54.862″ W [15]
Madrid 3° 41′ 16.58″ W [15]
Greenwich 0° 00′ 05.3101″ W Greenwich meridian Airy Meridian[16]
Greenwich 0° 00′ 05.33″ W United Kingdom Ordnance Survey Zero Meridian Bradley Meridian[16]
Greenwich 0° 00′ 00.00″ W IERS Reference Meridian
Paris 2° 20′ 14.025″ E Paris meridian
Brussels 4° 22′ 4.71″ E [15]
Antwerp 4° 24′ E Antwerp Meridian [citation needed]
Amsterdam 4° 53′ E through the Westerkerk in Amsterdam; used to define the legal time in the Netherlands from 1909 to 1937[17]
Bern 7° 26′ 22.5″ E [citation needed]
Pisa 10° 24′ E [9]
Oslo (Kristiania) 10° 43′ 22.5″ E [9][10]
Florence 11°15′ E Florence Meridian used in the Peters projection, antipode of a line running through the Bering Strait
Rome 12° 27′ 08.4″ E meridian of Monte Mario Used in Roma 40 Datum [18]
Copenhagen 12° 34′ 32.25″ E Rundetårn[19]
Naples 14° 15′ E [12]
Stockholm 18° 03′ 29.8″ E at the Stockholm Observatory[15]
Warsaw 21° 00′ 42″ E Warsaw Meridian [15]
Oradea 21° 55′ 16″ E [20]
Alexandria 29° 53′ E [21]
Saint Petersburg 30° 19′ 42.09″ E Pulkovo Meridian
Great Pyramid of Giza 31° 08′ 03.69″ E 1884 [22]
Jerusalem 35° 13′ 47.1″ E [10]
Mecca 39° 49′ 34″ E see Mecca Time Approximately 59° east of Greenwich [23]
Ujjain 75° 47′ E Used from 4th century CE Indian astronomy and calendars.[24]
Kyoto 136° 14′ E Used in 18th and 19th (officially 1779-1871) century Japanese maps. Exact place unknown, but in "Kairekisyo" in Nishigekkoutyou-town in Kyoto, then the capital.[citation needed]
~ 180 Opposite of Greenwich, proposed 13 Oct 1884 on the International Meridian Conference by Sandford Fleming [12]

## International prime meridian

In October 1884 the Greenwich Meridian was selected by delegates (forty-one delegates representing twenty-five nations) to the International Meridian Conference held in Washington, D.C., United States to be the common zero of longitude and standard of time reckoning throughout the world.[25]

### Prime meridian at Greenwich

File:Prime meridian.jpg
Markings of the prime meridian at the Royal Observatory, Greenwich.

The modern prime meridian, based at the Royal Observatory, Greenwich, was established by Sir George Airy in 1851.[26]

The position of the Greenwich Meridian has been defined by the location of the Airy transit circle ever since the first observation was taken with it by Sir George Airy in 1851.[26] Prior to that, it was defined by a succession of earlier transit instruments, the first of which was acquired by the second Astronomer Royal, Edmond Halley in 1721. It was set up in the extreme north-west corner of the Observatory between Flamsteed House and the Western Summer House. This spot, now subsumed into Flamsteed House, is roughly 43 metres to the west of the Airy Transit Circle, a distance equivalent to roughly 0.15 seconds of time.[16] It was Airy's transit circle that was adopted in principle (with French delegates, who pressed for adoption of the Paris meridian abstaining) as the Prime Meridian of the world in 1884.[27][28]

All of these Greenwich meridians were located via an astronomic observation from the surface of the Earth, oriented via a plumb line along the direction of gravity at the surface. This astronomic Greenwich meridian was disseminated around the world, first via the lunar distance method, then by chronometers carried on ships, then via telegraph lines carried by submarine communications cables, then via radio time signals. One remote longitude ultimately based on the Greenwich meridian using these methods was that of the North American Datum 1927 or NAD27, an ellipsoid whose surface best matches mean sea level under the United States.

### IERS Reference Meridian

Satellites changed the reference from the surface of the Earth to its center of mass around which all satellites orbit regardless of surface irregularities. The first satellite navigation system, TRANSIT, selected in the 1960s as its reference meridian on an Earth-centered ellipsoid the longitude on the NAD27 ellipsoid of its development laboratory halfway between Washington, D.C. and Baltimore, Maryland. These identical numeric longitudes at a location remote from Greenwich caused 0° of longitude on an Earth-centered ellipsoid to be 5.3" east of the astronomic Greenwich prime meridian through the Airy transit circle. At the latitude of Greenwich, this amounts to 102.5 metres. This was officially accepted by the Bureau International de l'Heure (BIH) in 1984 via its BTS84 (BIH Terrestrial System) that later became WGS84 (World Geodetic System 1984) and the various ITRFs (International Terrestrial Reference Systems).

Due to the movement of Earth's tectonic plates, the line of 0° longitude along the surface of the Earth has slowly moved toward the west from this shifted position by a few centimetres; that is, towards the Airy transit circle (or the Airy transit circle has moved toward the east, depending on your point of view) since 1984 (or the 1960s). With the introduction of satellite technology, it became possible to create a more accurate and detailed global map. With these advances there also arose the necessity to define a reference meridian that, whilst being derived from the Airy transit circle, would also take into account the effects of plate movement and variations in the way that the Earth was spinning.[29] As a result, the International Reference Meridian was established and is commonly used to denote Earth's prime meridian (0° longitude) by the International Earth Rotation and Reference Systems Service, which defines and maintains the link between longitude and time. Based on observations to satellites and celestial compact radio sources (quasars) from various coordinated stations around the globe, Airy's transit circle drifts northeast about 2.5 centimetres per year relative to this Earth-centered 0° longitude. Circa 1999 the international reference meridian (IRM) passed 5.31 arcseconds east of Airy's meridian or 102.5 metres (336.3 feet) at the latitude of the Royal Observatory, Greenwich, London.[30][31][32][33] It is also the reference meridian of the Global Positioning System operated by the United States Department of Defense, and of WGS84 and its two formal versions, the ideal International Terrestrial Reference System (ITRS) and its realization, the International Terrestrial Reference Frame (ITRF).[30][31][32] A current convention on the Earth uses the opposite of the IRM as the basis for the International Date Line.

#### List of places

On Earth, starting at the North Pole and heading south to the South Pole, the IERS Reference Meridian passes through:

Co-ordinates
(approximate)
Country, territory or sea Notes
90°0′N 0°0′E﻿ / ﻿90.000°N 0.000°E{{#coordinates:90|0|N|0|0|E|type:waterbody name=North Pole

}}

Arctic Ocean
81°39′N 0°0′E﻿ / ﻿81.650°N 0.000°E{{#coordinates:81|39|N|0|0|E|type:waterbody name=Greenland Sea

}}

Greenland Sea
72°53′N 0°0′E﻿ / ﻿72.883°N 0.000°E{{#coordinates:72|53|N|0|0|E|type:waterbody name=Norwegian Sea

}}

Norwegian Sea
61°0′N 0°0′E﻿ / ﻿61.000°N 0.000°E{{#coordinates:61|0|N|0|0|E|type:waterbody name=North Sea

}}

North Sea
45|N|0|0|E|type:country name=United Kingdom

}}

United Kingdom From Tunstall in East Riding to Peacehaven
50°47′N 0°0′E﻿ / ﻿50.783°N 0.000°E{{#coordinates:50|47|N|0|0|E|type:waterbody name=English Channel

}}

English Channel
19|N|0|0|E|type:country name=France

}}

France From Villers-sur-Mer to Gavarnie
41|N|0|0|E|type:country name=Spain

}}

Spain From Cilindro de Marboré to Castellón de la Plana
39°56′N 0°0′E﻿ / ﻿39.933°N 0.000°E{{#coordinates:39|56|N|0|0|E|type:waterbody name=Mediterranean Sea

}}

Mediterranean Sea Gulf of Valencia
52|N|0|0|E|type:country name=Spain

}}

Spain From El Verger to Calpe
38°38′N 0°0′E﻿ / ﻿38.633°N 0.000°E{{#coordinates:38|38|N|0|0|E|type:waterbody name=Mediterranean Sea

}}

Mediterranean Sea
50|N|0|0|E|type:country name=Algeria

}}

Algeria From Stidia to Algeria-Mali border near Bordj Mokhtar
50|N|0|0|E|type:country name=Mali

}}

Mali
59|N|0|0|E|type:country name=Burkina Faso

}}

Burkina Faso
6|N|0|0|E|type:country name=Togo

}}

6|N|0|0|E|type:country name=Ghana

}}

57|N|0|0|E|type:country name=Togo

}}

36|N|0|0|E|type:country name=Ghana

}}

Ghana From the Togo-Ghana border near Bunkpurugu to Tema
Passing through Lake Volta at 7°48′N 0°0′E﻿ / ﻿7.800°N 0.000°E{{#coordinates:7|48|N|0|0|E|type:waterbody_region:GH
name=Lake Volta

}}

5°37′N 0°0′E﻿ / ﻿5.617°N 0.000°E{{#coordinates:5|37|N|0|0|E|type:waterbody name=Atlantic Ocean

}}

Atlantic Ocean Passing through the Equator at 0°0′N 0°0′E﻿ / ﻿0.000°N 0.000°E{{#coordinates:0|0|N|0|0|E|type:landmark name=Equator

}}

60°0′S 0°0′E﻿ / ﻿60.000°S 0.000°E{{#coordinates:60|0|S|0|0|E|type:waterbody name=Southern Ocean

}}

Southern Ocean
54|S|0|0|E|type:country name=Antarctica

}}

Antarctica Queen Maud Land, claimed by Norway

## Prime meridian on other planetary bodies

"Prime meridian (planets)" redirects here. It is not to be confused with Central meridian (planets).

As on the Earth, prime meridians must be arbitrarily defined. Often a landmark such as a crater is used; other times a prime meridian is defined by reference to another celestial object, or by magnetic fields. The prime meridians of the following planetographic systems have been defined:

• The prime meridian of the Moon lies directly in the middle of the face of the moon visible from Earth and passes near the crater Bruce.
• The prime meridian of Mars is defined by the crater Airy-0.
• The prime meridian of Venus passes through the central peak in the crater Ariadne.[34]
• Two different heliographic coordinate systems are used on the Sun. The first is the Carrington heliographic coordinate system. In this system, the prime meridian passes through the center of the solar disk as seen from the Earth on 9 November 1853, which is when Richard Christopher Carrington started his observations of sunspots.[35] The second is the Stonyhurst heliographic coordinates system.
• Jupiter has several coordinate systems because its cloud tops—the only part of the planet visible from space—rotate at different rates depending on latitude.[36] It is unknown whether Jupiter has any internal solid surface that would enable a more Earth-like coordinate system. Scientific Astronomer uses System II coordinates, based on the mean atmospheric rotation of the north and south Equatorial belts. System III coordinates use Jupiter's magnetic field.
• Titan, like the Earth's moon, always has the same face towards Saturn, and so the middle of that face is 0 longitude.

## Footnotes

1. ^ Prime Meridian, geog.port.ac.uk
2. ^ Norgate 2006
3. ^ Hooker 2006
4. ^ e.g. Jacob Roggeveen in 1722 reported the longitude of Easter Island as 268° 45' (starting from Fuertaventura) in the Extract from the Official log of Jacob Roggeveen reproduced in Bolton Glanville Corney, ed. (1908), The voyage of Don Felipe Gonzalez to Easter Island in 1770-1, Hakluyt Society, p. 3, retrieved 13 Jan 2013
5. ^ Speech by Pierre Janssen, director of the Paris observatory, at the first session of the Meridian Conference.
6. ^ Sobel & Andrewes 1998, pp. 110–115
7. ^ Sobel & Andrewes 1998, pp. 197–199
8. ^
9. ^ a b c Hooker (2006), introduction.
10. ^ a b c Oct. 13, 1884: Greenwich Resolves Subprime Meridian Crisis, WIRED, 13 October 2010.
11. ^ Atlas do Brazil, 1909, by Barão Homem de Mello e Francisco Homem de Mello, published in Rio de Janeiro by F. Briguiet & Cia.
12. ^ a b c https://www.gutenberg.org/files/17759/17759-h/17759-h.htm
13. ^ Ancient, used in Ptolemy's Geographia. Later redefined 17° 39′ 46″ W of Greenwich to be exactly 20° W of Paris. French "submarin" at Washington 1884.
14. ^ A.R.T. Jonkers; Parallel meridians: Diffusion and change in early modern oceanic reckoning, in Noord-Zuid in Oostindisch perspectief, The Hague, 2005, p. 7. Retrieved 2 February 2015.
15. Bartky, Ian R. (2007), One Time Fits All: The Campaigns for Global Uniformity, p. 98, retrieved through GoogleBooks, 6 May 2014.
16. ^ a b c
17. ^ Invalid language code.Eenheid van tijd in Nederland (Unity of time in the Netherlands), Utrecht University website, retrieved 28 August 2013.
18. ^ Grids & Datums - Italian Republic, asprs.org, Retrieved 10 December 2013.
19. ^ meridian, article from Den Store Danske Encyklopædi
20. ^ Oradea, Tourism office website, retrieved 3 February 2015.
21. ^ The meridian of Ptolemy's Almagest.
22. ^
23. ^ Maimonides, Hilchot Kiddush Hachodesh 11:17, calls this point אמצע היישוב, "the middle of the habitation", i.e. the habitable hemisphere. Evidently this was a convention accepted by Arab geographers of his day.
24. ^ Burgess c. 2013
25. ^ "International Conference Held at Washington for the Purpose of Fixing a Prime Meridian and a Universal Day. October, 1884. Protocols of the proceedings". Project Gutenberg. 1884. Retrieved 30 November 2012.
26. ^ a b Greenwich Observatory ... the story of Britain's oldest scientific institution, the Royal Observatory at Greenwich and Herstmonceux, 1675-1975 p.10. Taylor & Francis, 1975
27. ^ . McCarthy, Dennis; Seidelmann, P. Kenneth (2009). TIME from Earth Rotation to Atomic Physics. Weinheim: Wiley-VCH. pp. 244–5.
28. ^ ROG Learing Team (23 August 2002). "The Prime Meridian at Greenwich". Royal Museums Greenwich. Royal Museums Greenwich. Retrieved 14 June 2012.
29. ^
30. ^ a b History of the Prime Meridian -Past and Present
31. ^ a b IRM on grounds of Royal Observatory from Google Earth Accessed 30 March 2012
32. ^ a b The astronomic latitude of the Royal Observatory is 51°28'38"N whereas its latitude on the European Terrestrial Reference Frame (1989) datum is 51°28'40.1247"N.
33. ^ Guinot, B., 2011. Solar time, legal time, time in use. Metrologica 48, S181–S185.
34. ^ "USGS Astrogeology: Rotation and pole position for the Sun and planets (IAU WGCCRE)". Retrieved 22 October 2009.
35. ^
36. ^ "Planetographic Coordinates". Retrieved 2009-06-19.

## References

• Burgess, Ebenezer (1860), "Translation of the Surya-Siddhanta", Journal of the American Oriental Society (e book) 6, Google (published c. 2013), p. 185