Geographic Grid System

A bisected sphere Geography is about spatial understanding, which requires an accurate grid system to determine absolute and relative location. Absolute location is the exact x- and y- coordinate on the Earth. Relative location is the location of something relative to other entities. For example, when you use your GPS in your smart phone or car, say Google Maps, you put in an absolute location. But as you start driving, the device tells you to turn right or left relative to objects on the ground: "Turn left on exit 202" is relative to the other exit points. Or if you give directions to your house, you often use relative locations to help people understand how to get to your house.

Great and Small Circles

Much of Earth's grid system is based on the location of the North Pole, South Pole, and Equator. The poles are at the ends of an imaginary line running from the axis of Earth's rotation. The plane of the equator is an imaginary horizontal plane that cuts the earth into two equal halves. This brings up the topic of great and small circles. A great circle is any circle that divides the earth into two equal halves. It's also the largest circle that can be drawn on a sphere. The line connecting any points along a great circle is also the shortest distance between those two points. Examples of great circles include the Equator or the line that divides the earth into day and night (called the circle of illumination). Any two opposing meridians of longitude (such as 0 degrees and 180 degrees) also form a great circle. Small circles are circles that cut the earth, but not into equal halves. Examples of small circles include all lines of latitude except the equator, including the Tropic of Cancer, Tropic of Capricorn, the Arctic Circle, and the Antarctic Circle.

Two globes showing longitude and latitude. Latitude lines show north–south positioning on the earth. The equator is a latitudinal line. Longitude lines show east–west positioning.

Latitude and Longitude

Latitude is an angular measurement north or south of the equator. So 30 degrees north means that a point is 30 degrees north of the equator. Latitude is also expressed in degrees, minutes, and seconds. There are 360 degrees in a circle, 60 minutes ( ' ) in a degree, and 60 seconds ( " ) in a minute. When you use Google Earth, the coordinate locations are in this degrees/minutes/seconds format. Latitude varies from 0 degrees (equator) to 90 degrees north and south (the poles).  A line connecting all points of the same latitude is called a parallel, because the lines run parallel to each other. The only parallel that is also a great circle is the equator. All other parallels are small circles. The following are the most important parallels:

  • Equator, 0 degrees
  • Tropic of Cancer, 23.5 degrees N
  • Tropic of Capricorn, 23.5 degrees S
  • Arctic Circle, 66.5 degrees N
  • Antarctic Circle, 66.5 degrees S
  • North Pole, 90 degrees N (infinitely small circle, or a point)
  • South Pole, 90 degrees S (infinitely small circle, or a point)


Latitude is also sometimes described as zones of latitude. Some of these zones of latitude include:

  • Low latitude—generally between the equator and 30 degrees N
  • Midlatitude—between 30 degrees and 60 degrees N and S
  • High latitude—latitudes greater than about 60 degrees N and S
  • Equatorial—within a few degrees of the equator
  • Tropical—within the tropics (between 23.5 degrees N and 23.5 degrees S
  • Subtropical—slightly pole-ward of the tropics, generally around 25-30 degrees N and S
  • Polar—within a few degrees of the North or South Pole


Two globes showing longitude and latitude. Latitude lines show north–south positioning on the earth. The equator is a latitudinal line. Longitude lines show east–west positioning. Longitude is the angular measurement east and west of the Prime Meridian (image on the right). Like latitude, longitude is measured in degrees, minutes, and seconds. Lines connecting equal points of longitude are called meridians. But unlike parallels, meridians do not run parallel to each other. Rather they are farthest apart from each other at the equator and merge toward each other (converge) toward the poles. The problem with longitude is that there isn't a natural baseline like the equator is for latitude. For over a hundred years, countries used their own "prime meridian" which proved problematic for trade. But in 1883 an international conference in Washington D.C. was held to determine a global prime meridian. After weeks of debate, the line of longitude that runs through the Royal Observatory at Greenwich, England was designated as the prime meridian (also called the Greenwich Meridian) for the world. So today, longitude starts at the prime meridian and measures east and west of that line.

Located mostly at or near 180 degrees from the Prime Meridian in the Pacific Ocean is the International Date Line. This line determines where the new day begins in the world. Because of this, the International Date Line is not actually a straight line, but rather it follows national borders so that a country isn't divided into two separate days. If you look at the map below, the International Date Line is to the right in a dark, black line. Note how it is drawn to make sure countries or island groups are not divided by the International Date Line.

Standard Timezones of the world. Timezones are, in general, divided by longitudinal lines.

Time Zones

This is also a good place to take a look at time zones around the world. If you refer to the map above, you can see the different time zones in various colors. Since the earth rotates 360 degrees in a 24 hour period, the earth rotates 15 degrees every hour, creating 24 time zones. In an ideal world, each time zone would follow lines of longitude every 15 degrees (7.5 degrees in each direction from the center of the time zone). To avoid dividing cities or countries into different time zones, however, time zone boundaries have been adjusted, so the actual time zones vary greatly in shape and width. Greenwich, England was chosen in 1883 as the starting point of time worldwide. The reason was because at the time, England was the world's superpower, both militarily and economically, so the meridian that ran through Greenwich became zero degrees or the prime meridian. Because of the earth’s rotation in reference to the prime meridian, locations east of the new meridian meant time was ahead while locations west of the meridian were behind in time in reference to Greenwich, England. Ultimately, when we combine parallels and meridians, we end up with a geographic grid that allows us to determine precise absolute locations on the planet.

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