Longitude


 
 
Longitude

Longitude, sometimes denoted by the Greek letter λ, describes the location of a place on Earth east or west of a north-south line called the Prime Meridian. Longitude is given as an angular measurement ranging from 0? at the Prime Meridian to +180? eastward and −180? westward. Unlike latitude, which has the equator as a natural starting position, there is no natural starting position for longitude. Therefore, a reference meridian had to be chosen. While British cartographers had long used the Greenwich meridian in London, other references were used elsewhere, including: Ferro, Rome, Copenhagen, Jerusalem, Saint Petersburg, Pisa, Paris, Philadelphia and Washington. In 1884, the International Meridian Conference adopted the Greenwich meridian as the universal prime meridian or zero point of longitude.

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Each degree of longitude is further sub-divided into 60 minutes, each of which divided into 60 seconds. A longitude is thus specified as 23° 27′ 30" E. For high accuracy, the seconds are specified with a decimal fraction. An alternative representation uses degrees and minutes, where parts of a minute are expressed as a decimal fraction, thus: 23° 27.500′ E. Degrees expressed as a decimal number is also used: 23.45833° E. Sometimes, the West/East suffix is replaced by a negative sign for West. Confusingly, the convention of negative for East is also sometimes seen. The preferred convention that East is positive is consistent with the right-handed x-axis in the Cartesian coordinate system.

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A specific longitude may then be combined with a specific latitude to give a precise position on the Earth's surface.

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As opposed to a degree of latitude, which always corresponds to about 111 km (69 mi), a degree of longitude corresponds to a distance from 0 to 111 km: it is 111 km times the cosine of the latitude, when the distance is laid out on a circle of constant latitude; if the shortest distance, on a great circle were used, the distance would be even a little less.

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Longitude at a point may be determined by calculating the time difference between that at its location and Coordinated Universal Time (UTC). Since there are 24 hours in a day and 360 degrees in a circle, the sun moves 15 degrees per hour (360?/24 hours = 15? per hour). So if the time zone a person is in is three hours ahead of UTC then that person is near 45? longitude (3 hours × 15? per hour = 45?). The word near was used because the point might not be at the center of the time zone; also the time zones are defined politically, so their centers and boundaries often do not lie on meridians at multiples of 15?. In order to perform this calculation, however, a person needs to have a chronometer (watch) set to UTC and needs to determine local time by solar observation or astronomical observation. The details are more complex than described here: see the articles on Universal Time and on the Equation of time for more details.

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A line of constant longitude is a meridian, and half of a great circle.

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East: :For other uses, see East (disambiguation)....

West: :This article refers to the cardinal direction; for other uses see West (disambiguation)....

Prime Meridian: The Prime Meridian is the meridian (line of longitude) passing through the Royal Greenwich Observatory, Greenwich, England; it is the meridian at which longitude is 0 degrees. It is often referred to as the Greenwich Meridian....


Longitude related Images and Photos (experimental)

Parallels of Longitude Relative to the Equator
Parallels of Longitude Relative to the Equator

~ Table of Content ~

Introduction
History of the measurement of longitude
Ecliptic latitude and longitude
Longitude on bodies other than Earth
See also
External links
 
FR: Longitude


 

~ Related Subjects ~

Meridian (2) - Greenwich (2) - Cosine (1) - Cartesian coordinate system (1) - England (1) - Great circle (1) - Washington (1) - Philadelphia (1) - Minutes (1) - 1884 (1) - Universal Time (1) - Chronometer (1) - Longitude (1) - Equation of time (1) - Royal Greenwich Observatory (1) -
 

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