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UNIT 2 GEOGRAPHICAL REVIEW: |
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A. INTRODUCTION
Overview
Do you know where the Ural Mountains are? the Atacama Desert? the East Pacific Rise? Your tour of Planet Earth will take you to many of its lesser-known reaches, and you will need a guide to help find your way. This unit can serve as such, and you should develop the habit of referring to it frequently throughout the course. It begins with a description of the major surface features of Earth: the continents and ocean basins. It then describes some of the rock types that you will encounter again and again in later units. Finally, a map of the world is keyed to every place and region name used throughout the book. A handy table enables you to look up any place name and find out where it is.
B. THE FACE OF THE EARTH
The picture beginning this chapter shows the familiar view of our planet from space: the deep blue of the oceans contrasting with the tan of the continents, spangled with white clouds and softened by the haze of the atmosphere. We are a very different kind of planet from the others in our solar system, and the strong contrast between continents and oceans is one of our most striking features.
The contrast is not only one of rock and water, though the visible presence of liquid water is unique in itself. The waters are gathered into oceans because these are the low points of the Earth's surface. Even if there were no water at all on Earth, the ocean basins would be remarkable features. In fact, the elevations of the rocky surface are dominated by two elevation ranges: that of sea level to 1,000 meters (3,300 feet) above it and that of 4,000 to 5,000 meters (13,000 to 16,400 feet) below sea level. Figure 2-1 shows graphically the distribution of elevations on Earth. The curve starts at the left at the highest elevations (8848 m or 29,030 ft at Mt. Everest) and proceeds to the lowest (11,000 m or 36,100 ft below sea level in the Mariana Trench). Each elevation is shown in direct proportion to the area of the Earth that stands at that elevation. Note how the two elevation ranges just cited mark the continental and oceanic platforms, which together account for the lion's share of the surface. The continental slope bridges these two elevations, while the extremes -- mountains and oceanic trenches -- take up only a tiny fraction of the available acreage.
HM 2-1:GLOBAL GEOGRAPHY--WORLD MAP |
If we look at a map of the world today, we can see it divided into two parts, land and water. The world's oceans make up about 71% or the earth's surface, compared with 29% made up by continents. On a world map the topography and bathymetry (underwater topography) is surprisingly consistent. On land most elevations are less than one kilometer above the sea surface. Of the total world's surface 20.8% is between 0 and 1 kilometer in elevation. The oceans also display surprising consistency. Most of the world's sea bottom is between 3 and 4 kilometers in depth. Of the total worlds surface 22.6% is between 3 and 4 kilometers below sea level. We have different terms for describing the continental geography. We call the region of continent, that is large land masses like North America or Australia, etc, that are above sea level the continental platform. That's because they are a platform above the surrounding ocean floor. Generally sea level goes up and down, so that the present day shore isn't a good indicator of where the continents begin and end. A better indicator is the continental shelf. This is defined as the sharp break between the relatively flat continental slope and the more steeply dipping continental slope.
HM 2-2 (A-G): GEOGRAPHY OF PLANET EARTH |
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| A | B | C | D | E | F | G |
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Earth is indeed a split-level planet. The liquid oceans are where they are because that is where there is room for their waters. In places, the oceanic waters lap onto the edges of the continents, forming shallow seas floored by continental, not oceanic, rocks. These are the continental shelves which in places like the Grand Banks off Newfoundland or the Falkland Banks near southern Argentina can extend hundreds of kilometers beyond the present-day shorelines.
As it happens, the rocks flooring the oceans and continents differ from one another, as we shall see in the Plate Tectonics unit. There, also, we shall investigate the reasons for this dichotomy of elevations. But before we can do that, we need to learn something about the rocky materials of the Earth's surface.
HM 2-3 (A-D): Three Dimensional Views--The Split Level Planet |
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| A | B | C | D |
INDIA |
Japan and the northwest Pacific basin |
Mariannes Trench system |
East Pacific Rise |
Figure 2-1 Hypsometric Diagram The curve shows the proportion of Earth's rocky surface that stands at each elevation. Areas are added cumulatively as you proceed from left to right. Adapted by permission of Smithsonian Institution Press from Continental Drift: The Evolution of a Concept, by Ursula B. Marvin. Figure 25, page 69. İSmithsonian Institution, Washington, D.C. 1973.
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HM 2-4 (A-C): REGION 1: PACIFIC BASIN |
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HM 2-5 (A-E): REGION 2: ATLANTIC BASIN |
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HM 2-6 (A-E): REGION 3: INDIAN OCEAN |
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C. ROCK TYPES
Rocks are divided into three varieties, based on their mode of origin: igneous, sedimentary, and metamorphic. Igneous rocks are produced by freezing of molten rock, which is called magma within the crust of the Earth, or lava when it erupts onto the surface.
Sedimentary rocks are formed when grains of sediment (mud, clay, sand, gravel, skeletal remains of plants and animals) are deposited by water, wind, or ice, or from low-temperature chemical precipitation, such as the precipitation of the mineral salt from evaporating water. Sedimentary rocks are classified on the basis of their texture, that is the size and shape of their mineral grains, and composition, both of the grains and the cement holding the sedimentary rock together. In the field, we generally identify sedimentary rocks on the basis of their grain size. Very fine grained sedimentary rocks are called siltstone or mudstones. Often these grains are so small they can only be seen with a hand magnifying lense. Sandstones have intermediate grain size, and the largest sedimentary rocks are called conglomerates or breccias depending on whether their large, pebble to block-sized, grains are rounded or angular. There is another class of sedimentary rock that is not mechanically deposited; instead it is chemically deposited. These are called limestones and evaporites. Evaporites are formed when salt-rich water dries, leaving behind a layer of salt and other crystals. Limestones are formed by the precipitation of calcium carbonate from sea water to form thick sediments of only this precipitated material.
All clastic sediment is derived from previously existing rocks. With time, these sediment grains may become lithified (made into rock) by burial, compaction, and cementation, often by precipitation of minerals that bind together the sediment grains into solid rock. Sandstones are formed from sandy deposits, shales from mud, and limestones from calcium-rich sediments -- often made up largely of the shells and skeletal remains of marine creatures large and small. Sedimentary rocks form a relatively thin veneer covering some three-quarters of Earth's surface but making up only about one-twentieth of the crust by volume.
Metamorphic rocks are any rocks that have been heated and/or squeezed to such an extent that their chemical and physical makeup are altered. Geologists noticed in the middle of the 1700s that in some regions sedimentary rocks would slowly change character over a region or near an igneous pluton or basalt dike. Sedimentary rocks where the original bedding was clear would become harder, and have a different orientation of fractures. This lead to the naming of a new class of rocks. Metamorphic in Greek simply means to change form. Today we define metamorphism as mineralogical changes that can be correlated with changes in heat or pressure. Metamorphic rocks are identified on the basis of their mineralogy and structure. The most common structure observed in these rocks is foliation. Foliation is a closely spaced layering observed in metamorphic rocks. If this layering is 1 mm or more thick and often very sinuous, this rock is called a gneiss. If the layering is finer, and generally more planer, this rock is a schist. From experimental studies it is known that different phases of some minerals exist under different heat and temperature conditions. Earth scientists have found that some minerals can only be made under specific conditions of heat and temperature. For example, the following reaction only occurs at temperatures of 500° C or slightly above.
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This is the reaction that takes chert and limestone and turns it into a new mineral called Wollastonite, and carbon dioxide gas. Wollastonite forms in a rock that has been heated under low pressure to at least this temperature. Such "Index Minerals," minerals of distinctive form and composition, are used to define "facies" of metamorphism. Metamorphic facies are defined as, any association of metamorphic rocks within which there is a constant correlation between thermal and chemical composition. The most important metamorphic facies, and the distinctive minerals that define them, are shown below.
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There are two main types of metamorphism. Contact metamorphism refers to changes close to an intruding igneous rock such as a pluton or dike. Regional metamorphism refers to metamorphism observed over a wide area. This type of metamorphism probably represents pressures and temperatures occurring in some region of the earth, since been uplifted to the earth's surface at a later date.
| HM 2-8: Laminated basin facies of Permian. Highway, 13 miles southwest of White City. Eddy County, New Mexico. |
Two important pressure and temperature environments of metamorphism are the blueschist and greenschist facies. The blueschist facies is only formed in low temperature, high pressure environments; greenschists only form in more intermediate pressures and temperatures. Blueschists and greenschists are given their respective names because of the distinctive blue and green minerals contained within them.
Igneous rocks are the primary rocks deep within the Earth. To be able to deal with them, you should understand a brief and simplified classification scheme, given in Figure 2-3. This scheme is based on the chemical composition of the rock (represented by the four vertical columns) and the texture of the rock (represented by the two horizontal rows).
The chemical classification is based on the abundance of certain minerals within the rock, especially silica (silicon dioxide, or SiO2). Rocks with a high silica content are termed felsic; those with a low silica content are termed mafic. Felsic rocks tend to be light in color and have a low density; mafic rocks are usually dark in color and have a higher density.
There is another chemical class of igneous rocks -- the ultramafic rocks. These make up much of the deeper part of the Earth, called the mantle, and in our classification scheme are found to the right of basalt and gabbro. They are dark in color and even denser than the mafic rocks. The rock type listed, peridotite, is only one of several different types of ultramafic rocks.
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The physical classification is based on the texture, or grain size within the rock. When a mass of magma cools slowly deep within the Earth, its atoms have time to aggregate into large grains of individual minerals: the rock becomes coarse-grained. On the other hand, lavas on the surface generally cool quickly, resulting in fine-grained rocks.
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Granites are familiar rocks, often used for decorative or memorial purposes. Its large grains give it a speckled appearance, and its overall color is often a light gray. Basalt, on the other hand, is a dark, nearly black rock that looks almost uniform in color. Only close inspection with a lens will reveal the small grains of the mostly dark minerals that constitute it. Andesite is a fine-grained rock of intermediate chemical composition. Rhyolite is a fine-grained rock whose chemical composition is very similar to that of granite, but differs from it in grain size.
Study Figure 2-3 and become familiar with the rocks shown in it. We shall refer especially to basalts, granites, andesites, and rhyolites in later units. Several centuries ago, Neptunists believed that all rocks were precipitated from a great ocean. In the later 1700s, however, experiments were done melting and recrystallizing rocks. These experiments showed that basalt could be formed by slowly allowing a liquid melt to cool, and that basalt is an igneous rock, that crystallized from a melt directly. Igneous rocks when they crystallize beneath the earth's surface are called intrusive rocks. This is because they intrude into other geological units. Extrusive rocks are igneous rocks that crystallize from a melt, but above the earth's surface. For example, a lava flow slowly cooling on the earth's surface forms an extrusive igneous rock. The discovery that basalt was an igneous rock solved the "heated basalt controversy," and effectively "sunk" the Neptunists.
Igneous rocks are classified by the relative abundance of certain key minerals, and whether they are of coarse or fine grained in mineral composition. Figure 2-3 shows how igneous rocks may be classified with respect to their mineral composition.
Granite, (density 2.7 g/cc), a common rock often found on continents, is classified as a coarse-grained, igneous, rock that contains the minerals quartz, K-feldspar and a few mafic minerals. Granite differs from a rock like basalt in two key respects. The first is that basalt is a fine-grained, igneous, rock and granite has coarse, or large, crystals. The second difference is that basalt, (density 2.9 g/cc), does not contain the minerals quartz or K-feldspar, but does contain mafic minerals pyroxene and olivine.
D. WHERE IS IT?
Figure 2-5 is a map of the world for your reference use. Marked on it are the features and localities mentioned throughout this text. Refer back to it often, and always be sure that you know where you are during our world travels.
| Virtual Geography--AVHRR satellite images of selected regions: | |
| Amazon Basin | This image shows regions of deforested and uncut rain forest in Brazil. |
| Arabia | This region marks a broad collision zone of the Arabian and Eurasian plates. Considerable earthquake activity in Iran and Iraq present significant geological hazards. |
| Australia | The northward motion of the Australia/India plate to the north has resulted in a collision zone marked by the mountainous Island of New Guinea. A portion of the Indonesian island arc is visible in the right hand portion of this image. |
| Baja Peninsula and the southwest United States. | This image shows the southwestern United States. The Basin and Range region is presently a broad region of diffuse spreading. Note the numerous high mountain ranges and downdropped basins. A larger scale image shows the Baja Peninsula. Can you find the San Andrea and Garlock faults? (Hint a LANDSAT image of the San Andreas and Garlock faults is presented in Unit 3). |
| Baltic Sea | Southern Sweden and Denmark border this portion of the Baltic Sea. As you can see this is a very narrow strait. Flow into the Baltic is highly complex. The Baltic Sea is especially vulnerable to industrial pollution. |
| Central America | This region marks a subduction zone between the Caribbean and Cocos plates. Before a convergence of the South America and North America plates, this portion of the Pacific Ocean was connected with the Caribbean sea. The uplift of central America separated currents in these two ocean bodies and has had a profound impact on the earth's climate. |
| England and Ireland | Early geological work showed that geological units in France could be correlated with those in southeastern England. |
| Eastern North America | In this AVHRR image, differences in vegetation are clearly seen. |
| Gibraltar, southern Spain and northern Africa | The topography in this region marks the collision of the Africa and Eurasian plates. Note the narrowness of the opening of the Mediterranean Sea with the Atlantic. |
| Mediterranean region near Italy | Volcanic activity in and near Italy is related to collision of the Africa plate with the southern margin of Eurasia. |
| Middle East | Note the abundant vegetation along the Nile. The Sinai Peninsula moves with the African plate. The plate tectonic boundary between this portion of the Africa plate and the Arabian plate is a transform fault system which is marked by the location of the Dead Sea (which is visible as a dark lake in this image). |
| New Guinea | New Guinea and Australia were connected by land during glacial low sea level events. The central mountains, which mark a collision zone, are more than 4,000 meters in height. |
| New Zealand | New Zealand consists of a subduction arc beneath the North Island, and a transform fault system (called the Alpine fault system) which runs through the middle portion of the South Island. Can you see the Alpine fault zone? |
| Southern Red Sea region and Afar triangle | Can you mentally place Arabia and Africa back together? Do they fit well together exactly? Check this higher resolution image first! |
Table 2-1 is the key to finding places on the map. The table lists all the features and localities alphabetically and by number. The location code takes you to the appropriate grid block on the map.
Two other important resources are provided for you in the glossary of geological terms and index at the end of this text. Use both liberally and you will find that you are getting far more out of the course.
Figure 2-5: WORLD INDEX MAP (Click on this image for full-size world map)
TABLE 2-1: WORLD INDEX
| Map # | Place Name | Location |
1 |
Adirondack Mountains, N.Y. | E-2 |
2 |
Afar Triangle | K-3 |
3 |
Africa | J-3 |
4 |
African Plate | J-4 |
5 |
Alaska | B-1 |
6 |
Alberta, Canada | D-2 |
7 |
Alcatraz Island | C-2 |
8 |
Aleutian Islands | B-2 |
9 |
Alexandria, Egypt | J-2 |
10 |
Allende, Mexico | D-3 |
11 |
Alps | J-2 |
12 |
Amazon Basin | E-4 |
13 |
Anatolian Fault | K-2 |
14 |
Anchorage, Alaska | C-1 |
15 |
Andes Mountains | E-4 |
16 |
Antarctic Circle | -6 |
17 |
Antarctic Plate | L-5 |
18 |
Antarctica | M-6 |
19 |
Appalachians | E-2 |
20 |
Arabian Peninsula | K-3 |
21 |
Arctic Circle | -1 |
22 |
Arctic Ocean | B-1 |
23 |
Argentina | E-5 |
24 |
Arizona | D-2 |
25 |
Asia | L-2 |
26 |
Aswan High Dam | K-3 |
27 |
Atacama Desert | E-5 |
28 |
Atlantic Ocean | F-2 |
29 |
Australia | N-4 |
30 |
Australian Plate | M-4 |
31 |
Azores | F-2 |
32 |
Baja California | D-3 |
33 |
Baltic Sea | J-2 |
34 |
Bangladesh | L-3 |
24 |
Barringer Crater, Arizona | D-2 |
35 |
Beaufort Sea | C-1 |
36 |
Benue Trough | J-3 |
37 |
Bering Strait | B-1 |
38 |
Bermuda | F-2 |
39 |
Birmingham, England | H-2 |
40 |
Black Forest, Germany | J-2 |
41 |
Black Sea | K-2 |
42 |
Bolivia | E-4 |
43 |
Boulder, Colorado | D-2 |
44 |
Brazil | F-4 |
45 |
Brisbane, Australia | N-5 |
46 |
Bushveld Igneous Complex, S.A. | J-4 |
47 |
Cairo, Egypt | K-2 |
48 |
Caledonian Mountains | H-2 |
49 |
Calgary, Alberta | D-2 |
7 |
California | C-2 |
50 |
Cambridge, England | J-2 |
51 |
Camp Century, Greenland | F-1 |
52 |
Campo del Cielo, Argentina | E-4 |
53 |
Canada | D-2 |
54 |
Canadian Shield | D-2 |
55 |
Cape Canaveral | E-3 |
56 |
Cape Hatteras | E-2 |
57 |
Cape Mendocino | C-2 |
58 |
Cape of Good Hope | J-5 |
59 |
Caribbean Sea | E-3 |
60 |
Caspian Sea | L-2 |
61 |
Central America | E-3 |
62 |
Charleston, South Carolina | E-2 |
63 |
Chesapeake Bay | E-2 |
27 |
Chile | E-5 |
64 |
China | M-2 |
65 |
Cincinnati, Ohio | E-2 |
66 |
Cocos Plate | D-3 |
67 |
Colombia River Plateau | D-2 |
43 |
Colorado | D-2 |
68 |
Congo River Basin | J-4 |
69 |
Cuba | E-3 |
70 |
Cyprus | K-2 |
71 |
Dead Sea | K-2 |
72 |
Death Valley | C-2 |
73 |
Deccan Traps, India | L-3 |
43 |
Denver, Colorado | D-2 |
50 |
Dover, England | J-2 |
74 |
Dresden, Germany | J-2 |
76 |
Dvina River | K-1 |
77 |
East African Rift | K-3 |
78 |
East Indies | M-4 |
79 |
East Pacific Rise | D-4 |
80 |
Equador | E-4 |
26 |
Egypt | K-3 |
81 |
El Chichon Volcano | D-3 |
82 |
Emperor Seamounts | A-2 |
39 |
England | H-2 |
50 |
English Channel | J-2 |
65 |
Erie, Pennsylvania | E-2 |
84 |
Ethiopia | K-3 |
85 |
Eurasian Plate | K-2 |
40 |
Europe | J-2 |
41 |
Euxine (Black) Sea | K-2 |
86 |
Falkland Banks | E-5 |
87 |
Falmouth, England | H-2 |
88 |
France | J-2 |
89 |
French Polynesia | B-4 |
90 |
Galapagos Islands | D-4 |
90 |
Galapagos Rift | D-4 |
91 |
Gary, Indiana | E-2 |
92 |
Georgia | E-2 |
40 |
Germany | J-2 |
93 |
Gibraltar | H-2 |
7 |
Golden Gate Bridge | C-2 |
94 |
Grand Banks | F-2 |
24 |
Grand Canyon National Park | D-2 |
95 |
Grand Canyon of the Yellowstone River | D-2 |
96 |
Great Basin | D-2 |
39 |
Great Britain | H-2 |
96 |
Great Salt Lake, Utah | D-2 |
97 |
Greenland | F-1 |
39 |
Greenwich, England | H-2 |
98 |
Gubbio, Italy | J-2 |
99 |
Gulf of Aden | K-3 |
100 |
Gulf of California | D-3 |
101 |
Gulf of Mexico | D-3 |
102 |
Hadrians Wall | H-2 |
103 |
Haicheng, China | N-2 |
104 |
Haiti | E-3 |
105 |
Hamburg, Germany | J-2 |
106 |
Hawaiian Islands | B-3 |
107 |
Herculaneum | J-2 |
108 |
Himalayas | L-3 |
109 |
Hiroshima, Japan | N-2 |
110 |
Homestake Gold Mine, South Dakota | D-2 |
106 |
Honolulu, Hawaii | B-3 |
111 |
Honshu, Japan | N-2 |
99 |
Horn of Africa | K-3 |
112 |
Hudson Bay | E-2 |
113 |
Iceland | H-1 |
67 |
Idaho | D-2 |
73 |
India | L-3 |
30 |
Indian Ocean | M-4 |
91 |
Indiana | E-2 |
30 |
Indo-Australian Plate | M-4 |
78 |
Indonesia | M-4 |
114 |
Indus River Valley | L-3 |
115 |
Ireland | H-2 |
98 |
Italy | J-2 |
111 |
Japan | N-2 |
111 |
Japan Sea | N-2 |
111 |
Japanese Archipelago, see Japan | N-2 |
111 |
Japanese Island Arc, see Japan | N-2 |
116 |
Java | M-4 |
117 |
Java Trench | M-4 |
118 |
Juneau, Alaska | C-2 |
119 |
Kansas | D-2 |
106 |
Kauai, Hawaii | B-3 |
120 |
Kenya | K-3 |
72 |
Kern County, California | D-2 |
39 |
Kew Botanical Gardens, London | H-2 |
106 |
Kilauea Volcano | B-3 |
113 |
Kirkjufell, Iceland | H-1 |
121 |
Kitt Peak, Arizona | D-2 |
116 |
Krakatoa | M-4 |
111 |
Kuroko Deposits, Japan | N-2 |
122 |
La Brea Tar Pits, California | D-2 |
91 |
LaPorte, Indiana | E-2 |
123 |
Lake Manicougan | E-2 |
123 |
Lake Mouchalagane | E-2 |
124 |
Lake Nayasa | K-4 |
125 |
Lake Tanganyika | K-4 |
106 |
Loihi Volcano | B-3 |
39 |
London, England | H-2 |
126 |
Long Valley, California | C-2 |
127 |
Los Alamos, New Mexico | D-2 |
122 |
Los Angeles, California | D-2 |
128 |
Madagascar | K-4 |
129 |
Maine Coast | F-2 |
130 |
Malaysia | M-3 |
126 |
Mammoth Lakes, California | C-2 |
123 |
Manicougan Crater | E-2 |
123 |
Manicougan River | E-2 |
131 |
Manila, Philippines | N-3 |
132 |
Mariana Trench | N-3 |
7 |
Marin Headlands | C-2 |
129 |
Marion, Massachusetts | F-2 |
133 |
Maritime Provinces, Canada | E-2 |
134 |
Martinique | E-3 |
129 |
Massachusetts | F-2 |
106 |
Maui | B-3 |
106 |
Mauna Loa Volcano | B-3 |
135 |
Mauritania | H-3 |
136 |
Mediterranean Basin | J-2 |
136 |
Mediterranean Sea | J-2 |
127 |
Mesa Verde National Park | D-2 |
137 |
Mesabi Range | D-2 |
138 |
Mesopotamia | K-2 |
24 |
Meteor Crater, Arizona | D-2 |
81 |
Mexico | D-3 |
55 |
Miami, Florida | E-3 |
139 |
Mid-Atlantic Ridge | F-3 |
71 |
Middle East | K-2 |
140 |
Midway Island | B-3 |
141 |
Minneapolis, Minnesota | D-2 |
141 |
Minnesota | D-2 |
142 |
Mississippi River | D-2 |
142 |
Missouri | D-2 |
72 |
Mojave Desert | C-2 |
49 |
Montana | D-2 |
143 |
Morocco | H-2 |
108 |
Mount Everest | M-3 |
144 |
Mount Huascaran, Peru | E-4 |
134 |
Mount Pelée | E-3 |
110 |
Mount Rushmore | D-2 |
145 |
Mount Saint Helens | C-2 |
124 |
Mozambique | K-4 |
146 |
Nagasaki, Japan | N-2 |
147 |
Namib Desert | J-4 |
148 |
Nantucket, Rhode Island | F-2 |
149 |
Nashville, Tennessee | E-2 |
150 |
Nazca Plate | D-4 |
119 |
Nebraska | D-2 |
108 |
Nepal | L-3 |
151 |
Netherlands | J-2 |
152 |
New Caledonia | A-4 |
129 |
New England | F-2 |
153 |
New Jersey | E-2 |
142 |
New Madrid, Missouri | D-2 |
127 |
New Mexico | D-2 |
154 |
New Orleans, Louisiana | D-3 |
153 |
New York City | E-2 |
153 |
New York State | E-2 |
155 |
New Zealand | A-5 |
94 |
Newfoundland | F-2 |
153 |
Niagara Falls | E-2 |
153 |
Niagara River | E-2 |
156 |
Niger River | J-3 |
156 |
Nigeria | J-3 |
111 |
Niigata, Japan | N-2 |
26 |
Nile River | K-3 |
157 |
Noranda District, Quebec | E-2 |
119 |
North America | D-2 |
119 |
North American Plate | D-2 |
28 |
North Atlantic | F-2 |
158 |
North Sea | J-2 |
159 |
Norway | J-1 |
160 |
Nova Scotia | F-2 |
106 |
Oahu | B-3 |
161 |
Ob River | L-1 |
65 |
Ohio | E-2 |
65 |
Ohio River | E-2 |
95 |
Old Faithful Geyser: See Yellowstone National Park | D-2 |
145 |
Oregon | C-2 |
162 |
Orinoco Tar Sands, Venezuela | E-3 |
159 |
Oslo, Norway | J-1 |
89 |
Pacific Ocean | B-4 |
89 |
Pacific Plate | B-4 |
163 |
Pakistan | L-3 |
153 |
Palisades, New York-New Jersey | E-2 |
88 |
Paris, France | J-2 |
164 |
Pechora River | K-1 |
153 |
Pennsylvania | E-2 |
165 |
Persian Gulf | K-3 |
144 |
Peru | E-4 |
144 |
Peru Desert | E-4 |
166 |
Peru-Chile Trench | E-4 |
131 |
Philippines | N-3 |
65 |
Pittsburgh, Pennsylvania | E-2 |
7 |
Point Arena | C-2 |
107 |
Pompeii | J-2 |
123 |
Quebec | E-2 |
114 |
Rajasthan Desert | L-3 |
168 |
Red Sea | K-3 |
153 |
Rhode Island | E-2 |
169 |
Rhone River | J-2 |
170 |
Rio Grande Rift | D-2 |
43 |
Rocky Mountains | D-2 |
171 |
Romania | J-2 |
85 |
Russia | K-2 |
172 |
Sahara Desert | J-2 |
173 |
Sahel Region | J-3 |
174 |
Saint Lawrence River | E-2 |
141 |
Saint Paul, Minnesota | D-2 |
175 |
Samos, Greece | J-2 |
72 |
San Andreas Fault | C-2 |
7 |
San Francisco, California | C-2 |
7 |
San Joaquin Valley, California | C-2 |
72 |
San Juan Bautista, California | C-2 |
176 |
Saomes | K-2 |
177 |
Sargasso Sea | E-2 |
178 |
Saskatchewan, Canada | D-2 |
20 |
Saudi Arabia | K-3 |
159 |
Scandinavia | J-1 |
48 |
Scotland | H-2 |
179 |
Seattle, Washington | C-2 |
180 |
Siberia | N-1 |
48 |
Siccar Point, Scotland | H-2 |
126 |
Sierra Nevada Mountains | C-2 |
67 |
Snake River Plain | D-2 |
181 |
Somalia | K-3 |
100 |
Sonora Desert | D-3 |
46 |
South Africa | J-4 |
44 |
South America | F-4 |
44 |
South American Plate | F-4 |
182 |
South Atlantic Ocean | F-5 |
62 |
South Carolina | E-2 |
110 |
South Dakota | D-2 |
183 |
South Magnetic Pole | N-6 |
184 |
South Pacific | B-5 |
93 |
Spain | H-2 |
134 |
St. Pierre, Martinique | E-3 |
93 |
Strait of Gibraltar | H-2 |
173 |
Sub-Saharan Africa | J-3 |
168 |
Sudan | K-3 |
47 |
Suez Canal | K-2 |
185 |
Sweden | J-1 |
11 |
Switzerland | J-2 |
78 |
Tambora, Indonesia | M-4 |
125 |
Tanganyika | K-4 |
186 |
Tangshan Area, China | M-2 |
187 |
Texas | D-2 |
188 |
Thailand | M-3 |
114 |
Thar Desert | L-3 |
153 |
Three-Mile Island, Pennsylvania | E-2 |
189 |
Tibet | L-2 |
153 |
Titusville, Pennsylvania | E-2 |
190 |
Tokyo, Japan | N-2 |
191 |
Tonga Trench | B-4 |
193 |
Tromso, Norway | J-1 |
70 |
Troodos Massif, Cyprus | K-2 |
194 |
Tropic of Cancer | -3 |
195 |
Tropic of Capricorn | -4 |
196 |
Tunguska River, Siberia | M-1 |
13 |
Turkey | K-2 |
119 |
U.S.A. | D-2 |
85 |
U.S.S.R.--Former Soviet Union (FSU) | K-2 |
119 |
United States | D-2 |
197 |
Ural Mountains | K-2 |
96 |
Utah | D-2 |
162 |
Venezuela | E-3 |
198 |
Vermont | E-2 |
113 |
Vestmannaeyjar, Iceland | H-1 |
107 |
Vesuvius | J-2 |
39 |
Wales | H-2 |
63 |
Washington, D.C. | E-2 |
67 |
Washington Scablands | D-2 |
179 |
Washington State | C-2 |
88 |
Western Europe | J-2 |
95 |
Wyoming | D-2 |
95 |
Yellowstone Caldera | D-2 |
95 |
Yellowstone Lake | D-2 |
95 |
Yellowstone National Park | D-2 |
199 |
Yenesey (Jenesei) River | L-1 |
200 |
Zimbabwe | J-4 |
For an interesting examination of the earth system check Calder (1991). Dotto (1991) give a wonderfully spectacular collection of views of Planet Earth taken from different Space Shuttle missions.
| Nigel Calder, Spaceship Earth, Viking Penguin Group, 1991. | |
| Lydia Dotto, Blue Planet, A Portrait of Earth, Harry N. Abrams, Incorporated (in association with the Smithsonian Instutition), 1991. | |
| Rand McNally and Company, Atlas of the World, Masterpiece Edition, Rand McNally, 1993. |
Every student should have access to a world atlas. One of the best of moderate cost is published by the National Geographic Society, Washington D.C.. Your college bookstore probably carries a small and inexpensive atlas by Rand McNally and Co. that will help you to find major cities and geographic features. Please ask your librarian regarding the location of your college’s map collection and explore these unique references.
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