The Physical Environment

                                                       
Contents | Glossary | Atlas |  Index | TPE Today | Blog | Podcast | Google Earth | Search

Essentials of Geography

Locational Systems

The fundamental work of a geographer begins by describing location. Locational reference systems have been created to accurately identify the location of earth phenomena.

Latitude and Longitude

Latitude/Longitude

Figure 1.31 The Geographic Grid: Latitude and Longitude (Courtesy The National Atlas)

Latitude and longitude comprises a grid system of lines encircling the globe and is used to determine the locations of points on the earth. Lines of latitude, also called parallels, run east - west. Latitude lines always run parallel to each other, and hence, they are always an equal distance apart. Latitude lines never converge or cross. equator

Figure 1.32 The Equator (Courtesy The National Atlas)

Lines of latitude measure distance north or south of the equator. The latitude of a particular location is the distance, measured in degrees, between that place and the equator along a meridian, or line of longitude. The equator is 0o latitude, and the North and South Poles are located at 90o north and 90o south latitude respectively. In other words, values for latitude range from a minimum of 0o to a maximum of 90o.

Measuring latitude

Figure 1.33 Measuring Latitude. (Courtesy The National Atlas)

If the earth were a perfect sphere (which it isn't), the distance, or the length, of 1o of latitude would be constant everywhere. In reality, the earth is slightly flattened at the poles, so the length of 1o of latitude at the poles is slightly more than at the equator. At the equator, the length of 1o of latitude is equal to 110.6 km (68.7 mi.) and at the poles, the length of 1o of latitude is equal to 111.7 km (69.4 mi.). For our purposes, we will assume the length of one degree of latitude is 111 km.

Longitude Figure 1.34 Longitude (Courtesy The National Atlas)

Lines of longitude, also called meridians, run north - south. Meridians are farthest apart at the equator, and converge at the North and South Poles. Lines of longitude measure distance east or west of the prime meridian. The longitude of a particular location is the distance along a parallel, measured in degrees, between that place and the prime meridian. The prime meridian passes through the old Royal Observatory at Greenwich, England, and is sometimes referred to as the Greenwich meridian. Since meridians are farthest apart at the equator and converge at the poles, the distance in kilometers (or miles) of 1o of longitude varies from a maximum at the equator, to a minimum at the poles. At the equator the approximate length of 1o is approximately 111 km (69 mi.). At 60o north and south latitudes, the length of 1o of longitude is approximately 55.5 km (34.5 mi.), or half what it is at the equator.

Figure 1.35 The prime meridian (Courtesy The National Atlas)

Prime MeridianThe prime meridian, which runs through Greenwich, England, is referred to as 0o longitude. Points are measured east or west of the prime meridian until one reaches the opposite side of the prime meridian, which is referred to as the International Date Line. This is considered 180o longitude, and is the highest value which longitude can take. In other words, values for longitude range from a minimum of 0o to a maximum of 180o.

An infinite number of parallels or meridians can be drawn on a globe. Thus, parallels and meridians exist for any point on the earth. Generally, only selected parallels and meridians are marked on maps and globes, and these are usually spaced equal distances apart. Parallels and meridians always intersect each other at right angles. In order to locate a particular point on the earth, a latitude and a longitude measurement is necessary. As stated above, these measurements are in degrees, but sometimes measurements smaller than degrees are necessary. In this case, minutes and seconds are used.

When we travel, we usually like to take the shortest route between two locations. If you pass a plane through the center of a sphere, the intersection of the plane and the surface of the sphere creates a great circle. Planes passing through any other part of a sphere without going through the center create small circles. An arc of a great circle is the shortest distance between two points on a sphere and therefore is the preferred route for planes traveling great distances, like crossing an ocean. The concept of great and small circles relates to meridians (longitude) and parallels (latitude). Meridians are half of a great circle (180o) whose ends are at the North and South poles. Parallels of latitude are  small circles, except for the equator which is a great circle. 

Great Circle

Figure 1.36 Great Circle
Source: Wikipedia

Small Circle


Figure 1.37 Small Circle
Source: Wikipedia

For more information about other locational systems, start "Digging Deeper Into Locational Systems: USPLS and UTM" or continue reading

Previous | Continue


    

Contents |Glossary | Atlas Index  |  Blog | Podcast | Google Earth | Search Updates | Top of page

About TPE | Who's Used TPE |  Earth Online Media

Please contact the author for inquiries, permissions, corrections or other feedback.

For Citation: Ritter, Michael E. The Physical Environment: an Introduction to Physical Geography.
Date visited.  https://www.earthonlinemedia.com/ebooks/tpe_3e/title_page.html

Michael Ritter (tpeauthor@mac.com)
Last revised 6/5/12

Help keep this site available by donating through PayPal.

paypal

Creative Commons License
This work is licensed under a Creative Commons Attribution-ShareAlike 4.0 International License..