Introduction to Earth Systems: Lesson 4


Earth Measure

 


Reading Assignment:

David Greenhood, Mapping, Chapter 1, 2, 3



NAVIGATION
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Reading Key Concepts Discussion More Links Exercises

 


Side Notes
Key Concepts

Links

 

 

 

 

 

 

 

 

 

Arcs and angles use the same units of measurement

These are the key concepts in this lesson. You should be able to define or describe them after you have read this lesson, finished the assigned reading and explored the links. You should also be able to do the exercises and answer the questions at the end of the lesson.
  • angle measure
  • arc length
  • radius -- arc length -- circumference relationships
  • rhumb lines
  • area on a sphere


Angle Measure

Depending on context, there are several systems of angle measure. In each case, there is a corresponding system for measure of circular arcs. The system of arc measure encountered most often in Earth measure is a consequence of the DMS (degrees-minutes-seconds) system described in Session 3. Corresponding to that, there is a DMS system of angle measure.

In the DMS system described in Session 3, every circle represents 360 degrees, i.e. can be divided into 360 arcs of equal length. The arc measure of any arc is a number of degrees occupied by the arc. Thus, for examples, a semi-circle has measure 180 degrees; a pair of perpendicular lines intersects at a 90 degree angle.

Corresponding to each circular arc, there is an angle with vertex at the center of the circle and that intersects the circle at the endpoints of the arc. This is a called a "central angle" for the circle. The measure of the angle is the same as the measure of the intercepted arc. For example, a 45 degree angle intercepts a 45 degree arc on any circle whose center is the vertex of the angle, and which intersects the sides of the angle.

 

 

 

 

 

 

  Arc length is different from arc measure

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Converting from DMS to decimal form

 

 

 

 

 

 

 

 

 

 

 

Relationship between north-south distance and latitude

 

 

 

 

 

 


Arc length

The units of length for an arc are linear units, e.g. meters, feet, kilometers. For a given central angle, larger circles correspond to greater arc lengths. To establish a relationship between measure of a central angle and corresponding arc length, we use an established relationship between the circumference of any circle and the diameter of that circle:
Circumference / diameter = Pi
(Pi is approximately 3.142, or 22/7)
or
Circumference = Pi * diameter
Since that ratio of circumference to diameter applies to all circles, it is helpful in making a formula that relates the DMS measure of an angle or arc to the length of the arc. Since, for any circle,
Diameter = 2 * radius,
We have
Circumference = 2 * radius * Pi
On any circle, the length of an arc is proportional to its measure, e.g. doubling the arc measure causes doubling of the arc length. And in particular,
(arc length)/circumference = (arc measure)/360
And so
Arc length
= circumference * (arc measure)/360
= 2 * Pi * radius * (arc measure)/360
= radius * (arc measure) * (Pi/180)
where arc measure is in the DMS system. For calculation relating angle measure to arc length and radius, we need first to express the DMS quantity in terms of degrees only because the formulas are in terms of degrees only. To do this we will convert minutes and seconds to fractions of a degree. Remember that
one degree = 60 minutes, and
one minute = 60 seconds. So
one second = 1/60 minute, and
one minute = 1/60 degree
Then, for example, to determine the length of an arc whose measure is 23° 15' 47", and which is part of a circle whose radius is 25 centimeters, we first write the measure in terms of degrees only:
23° 15' 47"
= 23° + 15 * 1/60 degrees+ 47 * 1/60 minutes
= 23° + 15 * 1/60 degrees+ 47 * 1/60 * 1/60 degrees
= (23 + 15/60 + 47/(60*60))°
which is approximately 23.263° Then
Arc length
= radius * (arc measure) * (Pi/180)
= 25 * 23.263 * Pi/180
which is approximately
25 * 23.263 * 3.142/180
or approximately
10.152
Since the radius is measured in centimeters, the arc length is approximately
10.152 centimeters
Relating this formula to Earth measure, the distance from the equator to a point at latitude 37° N can be calculated as follows:
Distance
= arc length
= (radius of Earth) * (arc measure) * (Pi/180)
which is approximately
(6370 kilometers) * (37 degrees) * 3.142/(180 degrees)
or approximately
4114.1 kilometers
Since in any circle the measure of any arc is the same as the measure of its central angle, we have a similar formula in terms of the central angle rather than the arc:
Arc length = radius * (central angle measure) * (Pi/180)
We have many occasions to measure length, on a plane or on a sphere. The examples above are intended to display rather straightforward relationships among arc length, arc measure and angle measure. In particular, many applications of Earth measure involve relationships between arc length and arc measure, i.e. relationships between distance and latitude or longitude.

 

 

 

 

Discussion of arc length.

 

 

 

 

Points on the same great circle are "collinear"

 

 

 

Sides of triangles are arcs of great circles.


Area

As in a plane, calculation of area on a sphere, especially for irregular shapes, is more difficult than is the case for distances along lines and other paths. In a plane, irregular shapes can be described or approximated in terms of mathematical functions; in other cases, methods for estimating area involve approximating the irregular shape as a polygon and calculating the area of the polygon.

Spherical triangle   On a sphere, we will use the spherical "triangle" as a primitive shape. A spherical triangle is defined by three points (vertices) that are not "collinear", i.e. not on the same great circle. The "sides" of the spherical triangle are great circle arcs whose endpoints are the vertices of the triangle. A general formula for areas of spherical triangles involves spherical trigonometry. Some special cases can be addressed through the formula for area of a sphere in terms of its radius:

Area of surface of a sphere = 4 * Pi * (radius)^2
(Note: 4 * Pi * (radius)^2 = 4 * Pi * radius * radius)
Then, for example, using 6370 kilometers as the radius of Earth, we can calculate the area of the Western Hemisphere. The area of the Western Hemisphere is half of the area of Earth. So
Area of the Western Hemisphere
= (1/2) * 4 * Pi * (6370)^2
= 2 * Pi * (6370)^2
which is approximately
2 * 3.142 * 6370 * 6370 square kilometers
or 254,985,000 square kilometers
As another example, note that for the spherical triangle whose vertices are
(0°N 45°W), (0°N 45°E) and the North Pole
the spherical triangle occupies one-eighth of the surface of Earth, so its area is approximately
(1/8) * 4 * Pi * (6370)^2 square kilometers
which is approximately
63,746,000 square kilometers.

 

 

 

 

 

 

 

 

 

 

 

 

About spherical triangles.

 

 

 

 

 

 

Paths of constant direction

 

 

 

 

 

 

 

 

 

Strategies for determining elevation

Rhumb lines

On Earth's surface, paths of constant direction are called "rhumb lines", or "loxodromes." In particular, travel along meridians is in constant direction, i.e. either due north or due south. And similarly, travel along parallels is in constant direction, either due east or due west. Other paths of constant direction are neither parallels nor great circles. For example, travel from a point on the Equator and bearing precisely north east, i.e. at an angle 45° with both due east and due north, will intersect each meridian at a 45° angle. Such a path will spiral through the Northern Hemisphere toward the North Pole.

Mercator Projection   One commonly-used projection of Earth to a plane is the Mercator projection. Such a projection, i.e. from a sphere to a plane, necessarily involves some distortion. The Mercator projection involves distortions of distance and shape, but it facilitates use of paths of constant direction. On a Mercator map, rhumb lines are actually line segments. Thus, for example, a line segment on the map from New York to London will describe a path that is in fact not a line or a great circle, but a path that intersects meridians at the same angle measure. Before the use of electronic aids for navigation across oceans, sailing along a rhumb line, by use of stars or magnetic compass, was an important option toward reaching one's destination.

Earth as spheroid

In sufficiently small regions, e.g. for a city map, Earth measure can be approximated as geometry of a plane. In larger regions, distances, areas and angle measures are accurate enough if Earth is regarded as a sphere. For still more accuracy, we work with approximations that reflect Earth's deviation from spherical shape. Hence the use of 6370 kilometers or 3960 miles only as approximations for an average radius of Earth. Earth's radius is greatest at the Equator, least at the poles. Estimated range is from 6357 km. to 6378 km. or from 3951 miles to 3964 miles.

Among other problems, irregularities in Earth's shape make difficult the determination of altitude. Traditional use of barometric pressure is subject to inaccuracies caused by atmospheric change. Use of electronic models aids in addressing problems in measurement caused by irregularities in Earth's shape. One strategy is the representation of portions of Earth's surface as parts of a spheroid, in this case a surface of revolution of an ellipse around its minor axis. There are many such full-scale models and they are used locally in measurement of altitude. Another strategy is the use of contours of equal gravitational attraction, called "geoids", which fill the role of mean sea level in Earth measure and, beyond that, bring us closer to the relationship between Earth's geometric center and its gravitational center.

Other coordinate systems

While the latitude-longitude (lat-lon) system has much historical support and is visually easy to comprehend, it also has an important disadvantage. The relationship between longitude and east-west distance varies according to latitude. For example, at the equator the arc length between 0° longitude and 30° E longitude is greater than the arc length between those longitudes at 45° N latitude.

One system designed to address this problem is the Universal Transverse Mercator projection. Its coordinate system is organized in terms of distances from the equator and from reference meridians. Units of measure for location and for distance are meters. Thus there is no unit conversion from map coordinates to linear units. While the complexity of the projection produces an unappealing image, application involving distances and areas on Earth's surface produce more consistency in results of calculation and of accuracy at various latitudes.


Links

Angle measure: postulates and theorems.

Dictionary of units of measurement.

Erathosenes' calculation of diameter of Earth


  TOP   Discussion


Exercises
  1. Assuming that Earth is a sphere and that its radius is 6370 kilometers, calculate the distance from the equator along any meridian to the North Pole?

     

  2. Assuming that the Moon is a sphere with radius 1000 miles, compare its area with that of Earth.

     

  3. Using the assumption in exercise (2.), calculate the circumference of the Moon, i.e. the length of any of its great circles.

     

  4. Calculate the area of the portion of the Eastern hemisphere that is bounded by the Greenwich meridian and the meridian with longitude 45°E.

     

  5. Given that the latitude of the city hall of San Francisco is 37° 46'N, calculate the distance of the city hall from the equator in nautical miles, in statute miles, and in kilometers.

     

  6. Assuming that the Moon is approximately 240,000 miles from Earth throughout its orbit, calculate the length of its orbit with respect to Earth. With respect to Earth's rotation about the Sun throughout a solar year, why is the Moon's path not a circle or an ellipse?

     

  7. Describe, in terms of place names, bodies of water, etc., the path on Earth occupied by a
    1. rhumb line from Los Angeles, California to Helsinki, Finland.
    2. great circle from Los Angeles to Helsinki

to  ANSWER/HINT PAGE

to  INDEX

 

 

 

 

 

 

 

 

Rhumb lines and the problem of constant direction

 

 

 

 

Spherical geometry


Materials developed by-
Wm. Rundberg
College of San Mateo
1700 West Hillsdale Blvd
San Mateo, Ca. 94402
650.574.6258
rundberg@smcccd.cc.ca.us