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A geographic coordinate system ( GCS) is a spherical or geodetic coordinate system for measuring and communicating positions directly on Earth as latitude and longitude. [ 1] It is the simplest, oldest and most widely used of the various spatial reference systems that are in use, and forms the basis for most others.
In mathematics, a spherical coordinate system is a coordinate system for three-dimensional space where the position of a given point in space is specified by three real numbers: the radial distance r along the radial line connecting the point to the fixed point of origin; the polar angle θ between the radial line and a polar axis; and the ...
Geodetic coordinates P (ɸ,λ,h) Geodetic coordinates are a type of curvilinear orthogonal coordinate system used in geodesy based on a reference ellipsoid . They include geodetic latitude (north/south) ϕ, longitude (east/west) λ, and ellipsoidal height h (also known as geodetic height[ 1] ). The triad is also known as Earth ellipsoidal ...
ISO 6709, Standard representation of geographic point location by coordinates, is the international standard for representation of latitude, longitude and altitude for geographic point locations. The first edition ( ISO 6709:1983) was developed by ISO/IEC JTC 1 /SC 32. Later the standard was transferred to ISO/TC211, Geographic information ...
Informally, specifying a geographic location usually means giving the location's latitude and longitude. The numerical values for latitude and longitude can occur in a number of different units or formats: [2] sexagesimal degree: degrees, minutes, and seconds : 40° 26′ 46″ N 79° 58′ 56″ W
Longitude at right edge of map, in decimal degrees; Precision. Longitude: from West to East this map definition covers 0.1015 degrees. At an image width of 200 pixels, that is 0.0005 degrees per pixel. At an image width of 1000 pixels, that is 0.0001 degrees per pixel. Latitude: from North to South this map definition covers 0.056 degrees.
Ecliptic latitude or celestial latitude (symbols: heliocentric b, geocentric β ), measures the angular distance of an object from the ecliptic towards the north (positive) or south (negative) ecliptic pole. For example, the north ecliptic pole has a celestial latitude of +90°. Ecliptic latitude for "fixed stars" is not affected by precession.
Longitude at right edge of map, in decimal degrees; Precision. Longitude: from West to East this map definition covers 0.0984 degrees. At an image width of 200 pixels, that is 0.0005 degrees per pixel. At an image width of 1000 pixels, that is 0.0001 degrees per pixel. Latitude: from North to South this map definition covers 0.0784 degrees.