Textbook Notes (367,834)
Geography (263)
Chapter 1

# Chap 1 Earth and Earth Coords.docx

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School
Department
Geography
Course
Geography 2122A/B
Professor
Micha Pazner
Semester
Fall

Description
Determining Geodetic Latitude and Longitude - Oldest way is by using instruments o For observing positions of Celestial bodies, o Technique: establish celestial lines of position (east-west, north- south) by comparing the predicted positions of celestial bodies with their observed positions. - Sextant – tool used to measure the angle of a celestial body above the earth’s horizon. o Nautical navigators used to find their way using the moon, planets and stars, including our sun - Since Earth rotates on an axis defined by North and South poles, stars in the northern hemisphere’s night sky appear to move slowly in a circle centered on Polaris (the North Star). o Navigators need to only located Polaris to find North. - In Southern Hemisphere, latitude is harder to find because four stars are used to interpolate due south as there is no equivalent to Polaris over the South pole. Navigators use a small constellation called Crux Australis (the Southern Cross) o Finding South = more complicated because the Southern Cross is a collection of 5 stars that are part of the constellation Centaurus. th o 4 stars form cross, the 5 is dim = offset about 30 degrees below the center of the cross - The prime meridian at 0 degree longitude passes through Greenwich, England. Therefore, each hour difference between your time and that at Greenwich, called Greenwich mean time or GMT, is roughly equivalent to 15 degree of longitude from Greenwich o To determine geodetic longitude, compare you local time with Greenwich Mean Time and multiply by 15 degree of longitude for each hour of difference. - Before = difficult to determined longitude o 1762 – clock was portable enough and used accurate enough for longitude finding o Chronometer was set to Greenwich Mean Time before departing on a long voyage. o Longitude of distant local found by noting GMT at local noon (highest point of the sun in the sky, found with a sextant). The time difference was multiplied by 15 to find the longitude Properties of the Graticule - Circumference of the authalic and other spheres o Using spheres leads to simpler calculations, specially working with small-scale maps of countries, continents, or the entire earth. o The value of the earth’s spherical circumference used is called authalic sphere.  Authalic sphere is a sphere with the same surface area as a reference ellipsoid. o Other properties of oblate ellipsoid:  Rectifying sphere, is where the length of meridians from equator to pole on the ellipsoid equals one-quarter of the spherical circumference.  This sphere is a little over three-tenths of a percent larger in surface area than the WGS84 ellipsoid (authalic sphere).  The values are really close to each other, difference by less than two-tenths of a percent - Spacing of parallels o Important to know how to define distance as there may be different definitions for the words, i.e, what they mean. o There is a 15% difference in the number of statute and nautical miles per degree. o Statute miles are what we use for land distances in the United States. o Nautical miles are used worldwide for maritime and aviation purposes. o A Statute mile is about 1,609 meters and Nautical mile is 1,852 meters exactly (about 1.15 statute miles) o Original Nautical mile was defined as 1 minute of latitude measured north-south along a meridian. o Oblate ellipsoid are not spaced equally, but decrease slightly from pole to the equator. - Converging meridians - The precise spacing of meridans at a given latitude is found by: o 69.09 miles (111.20 Km) / deg. X cosine(latitude) o Example: at 45degree north or South of the equator, for example, cosine (45degree) = 0.7071. Therefore, the length of a degree of longitude is  69.09 x 0.7071 = 48.85 Statute miles (111.20 x 0.7071 = 78.63 km) - Great and Small circles o A great circle is the largest possible circle that could be drawn on the surface of the spherical earth. Its circumference is that of the sphere, and its center is the centere of the earth so that all great circles divide the earth into halves. o The prime meridian and the 180 deg. Meridian at the opposite side of the earth (called the antipodal meridian) form a great circle dividing the earth into eastern and western hemispheres.  A great circle is the shortest route between any two points on the earth and hence great circle routes are fundamental to long-distance navigation. o Any circle on the earth’s surface that intersects the interior of the sphere at any location other than the center is called a small circle. - Quadrilaterals - Quadrilaterals are areas bounded by equal increments of latitude and longitude, 10deg. By 10deg. - The equation cosine(latitude) gives the aspect ratio (with/height) of any quadrilateral. - A quadrilateral centered at 45deg N will have aspect ratio of 0.07071, whereas, 60deg. N = 0.5. [2:1 ratio] Graticule Appearance on Maps - Small-scale maps o World or continental maps such as globes and worldatlas sheets normally use coordinates based on an authalic sphere.  Reasons:  Before computers, it was easier to make them from spherical coordinates.  The difference in the plotted positions of spherical and corresponding geodetic parallels become negligible on maps that cover so much area.  The scale to a world wall map approx. 18 inches high and 36 inches wide - Large-scale maps o Parallels and meridians are shown in different ways on different types of maps.  Topographic maps in U.S and other countries have TICK MARKS showing the location of the graticule.  Ex:- U
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