Because you need at least two coordinates to define the position of ANY object in a 2 dimensional coordinate system, . Your exact location on the Earth's surface requires BOTH latitude and Longitude, AND you can add altitude or depth as a third coordinate, AND TIME as a fourth coordinate to define your precise location in a FOUR dimensional coordinate system, that includes time.
"...A sphere is a two dimensional surface. Two coordinates are needed to define a point on its surface. The second coordinate used on the Earth is called Longitude. It is made up of a series of great circles running through both poles and set at right angles to the Equator. These circles are not parallel to each other. They are shown on the right sphere above.
Unlike Latitude which has two fixed points (the poles) and a fixed great circle (the Equator), Longitude has no natural zero. All lines of Longitude are identical. The zero line of Longitude is called the Zero Meridian or Prime Meridian. Its position must be decided by international agreement. ...
...The position of an object (like the Sun) is defined by two coordinates. Azimuth is measured clockwise from the North point. Altitude is measured from the horizon to the object. Both are measured in degrees.
Local coordinates are unique for each individual observer. As the Earth rotates on its axis, objects change their position in the sky relative to the observer. This means that the altitude and azimuth of an object change constantly. The altitude and azimuth of an object in the sky depends on
The location of the observer on the Earth
The time of day
The time of year (date)
In particular, the Sun rises from an easterly direction and crosses the Local Meridian. Sunrise is defined as the time when the centre of the Sun is on the horizon while it is moving above the horizon.
In the Northern Hemisphere, the Sun crosses the Meridian due South; in the Southern Hemisphere, the Sun crosses the Meridian due North. Local Solar Noon is the time when the Sun's centre is on the Meridian. The Sun is then at its highest altitude.
At the end of the day the Sun sets in a westerly direction. These motions of the Sun can be used for time keeping. A sundial measures the angle between the Sun and Meridian. The Sun appears to go around the Earth in a 24 hour period. This is a 360° circuit.
24 hours is equivalent to 360°, 1 hour is equivalent to 360 / 24 = 15°.
During a year, the Sun's motion across the sky also changes. This is because the Earth is moving around the Sun. This affects the altitude of the Sun at Noon. The following table shows the effect. ..."
http://www.krysstal.com/coordsystems.html
http://hyperphysics.phy-astr.gsu.edu/hbase/coord.html