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latitude
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latitude, angular distance of any point on the surface of the earth north or south of the equator. The equator is latitude 0°, and the North Pole and South Pole are latitudes 90°N and 90°S, respectively. The length of one degree of latitude averages about 69 mi (110 km); it increases slightly from the equator to the poles as a result of the earth's polar flattening. Latitude is commonly determined by means of a sextant sextant, instrument for measuring the altitude of the sun or another celestial body; such measurements can then be used to determine the observer's geographical position or for other navigational, surveying, or astronomical applications.
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 or other instrument that measures the angle between the horizon and the sun or another celestial body, such as the North Star (see Polaris Polaris (pōlâr`ĭs) or North Star,
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). The latitude is then found by means of tables that give the position of the sun and other bodies for that date and hour. An imaginary line on the earth's surface connecting all points equidistant from the equator (and thus at the same latitude) is called a parallel of latitude. On most globes and maps parallels are usually shown in multiples of 5°. Because of their special meanings, four fractional parallels are also shown. These are the Tropic of Cancer (23 1-2°N) and the Tropic of Capricorn (23 1-2°S), marking the farthest points north and south of the equator where the sun's rays fall vertically (see tropics tropics, also called tropical zone or torrid zone, all the land and water of the earth situated between the Tropic of Cancer at lat. 23 1-2°N and the Tropic of Capricorn at lat. 23 1-2°S.
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), and the Arctic Circle Arctic Circle, imaginary circle on the surface of the earth at 66 1-2°N latitude, i.e., 23 1-2° south of the North Pole. It marks the northernmost point at which the sun can be seen at the winter solstice (about Dec.
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 (66 1-2°N) and the Antarctic Circle Antarctic Circle, imaginary circle on the surface of the earth at 66 1-2°S lat., i.e., 23 1-2° north of the South Pole. It marks the southernmost point at which the sun can be seen at the winter solstice (about June 22) and the northernmost point of the
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 (66 1-2°S), marking the farthest points north and south of the equator where the sun appears above the horizon each day of the year (see also midnight sun midnight sun, phenomenon in which the sun remains visible in the sky continuously for 24 hr or longer, occurring only in the polar regions. The midnight sun is due to the fact that the plane of the earth's equator is tilted about 23 1-2° to the plane of the
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). Parallels of latitude and meridians of longitude longitude (lŏn`jĭt
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 together form a grid by which any point on the earth's surface can be specified. The term latitude is also used in various celestial coordinate systems (see ecliptic coordinate system ecliptic coordinate system, an astronomical coordinate system in which the principal coordinate axis is the ecliptic , the apparent path of the sun through the heavens.
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).

The location north or south of the equator, measured in degrees from the equator, which is 0. The North Pole is plus 90 degrees, and the South Pole is minus 90 degrees. Degrees are further divided into minutes and seconds.

East/West Longitude
Longitude is the location east and west of the Greenwich prime meridian in London, measured in degrees from this reference point, which is 0. Europe is plus degrees to the east, and the Americas are minus degrees to the west.

To pinpoint a location on earth, the north/south latitude (y-axis) is combined with the east/west longitude (x-axis). For example, the Empire State Building in New York is expressed in degrees, minutes and seconds as follows:



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