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Publié par
Date de parution
08 août 2012
Nombre de lectures
0
EAN13
9782764408902
Langue
English
Poids de l'ouvrage
60 Mo
Publié par
Date de parution
08 août 2012
Nombre de lectures
0
EAN13
9782764408902
Langue
English
Poids de l'ouvrage
60 Mo
THE VISUAL GUIDES
Understanding
The
Earth
QA INTERNATIONAL
Understanding
Planet
Earth
Publisher
Editorial Director
Executive Editor
Illustrations Editor
Art Director
Graphic Designer
Writers
Translator
Computer Graphic Artists
Page Layout
Researchers
Earth Reviewer
Copy Editor
Production
Prepress
Jacques Fortin
François Fortin
Serge D’Amico
Marc Lalumière
Rielle Lévesque
Anne Tremblay
Nathalie Fredette
Stéphane Batigne
Josée Bourbonnière
Claude Lafleur
Agence Science-Presse
Käthe Roth
Jean-Yves Ahern
Maxime Bigras
Patrice Blais
Yan Bohler
Mélanie Boivin
Charles Campeau
Jocelyn Gardner
Jonathan Jacques
Alain Lemire
Raymond Martin
Nicolas Oroc
Carl Pelletier
Simon Pelletier
Frédérick Simard
Mamadou Togola
Yan Tremblay
Lucie Mc Brearty
Véronique Boisvert
Geneviève Théroux Béliveau
Anne-MarieVilleneuve
Anne-Marie Brault
Kathleen Wynd
Jessie Daigle
Michèle Fréchet
Jafar Arkani-Hamed
Jane Broderick
Mac Thien Nguyen Hoang
Kien Tang
Karine Lévesque
The Visual Guide to Understanding Planet Earthwas created and produced by
QA International
e
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No part of this book may be reproduced or transmitted in any form or by any means,
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the Publisher.
The publisher acknowledges the financial support of the
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Development Program (BPIDP) for its publishing activities.
)3".
0rinted and bound inSlovakia.
10 9 8 7 6 5 4 3 2 1 10 20 30 40
www.qa-international.com
Understanding
Planet
Earth
QA INTERNATIONAL
4
28
26
24
22
20
18
Types of rocks
The life cycle of rocks
Mineral shapes
The minerals
Geomagnetism
Inside Earth
6 | Earth’s history16 | Earth’s structure
8The formation of Earth
10The geologic time scale
12Life emerges on the continents
14Our knowledge of geologic time
Ta b l e
30 | Tectonics
and volcanism
32
34
36
38
40
42
43
44
46
48
Plate tectonics
The fate of Pangaea
Continental drift
Volcanoes
Volcanism
Volcanic eruptions
Hot spots
Geysers
Earthquakes
Seismic waves
68
66
64
62
60
58
56
54
52
o f
The tides
Tsunamis
Waves
Ocean currents
Oceanic trenches and ridges
The ocean floor
The world ocean
The world’s rivers and lakes
Watercourses
50 | Water and oceans
c
87
86
84
82
80
78
76
75
74
72
o
Icebergs
Glacial erosion
Glaciers
Configuration of the coastline
Mountains of the world
How mountains are formed
Caves
Landslides
The cycle of erosion
Erosion
70 | The evolving landscape
n
t
e
122
120
118
116
114
112
111
110
n
t
Africa
Oceania
Asia
Europe
South America
North America
Antarctica
Configuration of the continents
88 | Representations108 | The continents
of Earth
90Terrestrial coordinates
92Cartographic projection
94 Cartography
96Cartographic conventions
98Physical and topographic maps
100Thematic maps
102Remote sensing
104Satellites and shuttles
106Time zones
s
124 | Glossary
126 | Index
128 | Photo credits
5
from a cloud of dust
Earth, born 4.6 billion years ago , did not always look like the planet that we know
increasingly
today. In fact, it has been changing constantly throughout its history, becoming
organized and complex
. This fascinating evolution is revealed through the rocks and fossils
that provide evidence of our planet’s early times.
Earth’s history
8
10
12
14
The formation of Earth
How it all started
The geologic time scale
Finding the origins of life
Life emerges on the continents
Increasingly complex organisms
Our knowledge of geologic time
Sources for dating
T h e f o r m a t i o n o f E a r t h
How it all started
Five billion years ago, the Solar System did not exist. There was only a huge
diffuse cloud of dust and gases turning slowly on itself. Over time, the Sun was
formed, followed by the nine planets,
including Earth, which formed
Earth’s history
like a snowball, by the
agglomeration of matter
around the original nebula.
0Q
W0
0E
R0
EMERGING FROM A CLOUD OF DUST
It all started 4.6 billion years ago, in one of
the spiral arms of the Milky Way. Impacted by
a shock wave that probably came from the
explosion of massive stars, a cloud of dust
(the solar nebula )ate rotn tobegaQ.
At the center of the cloud, matter became
increasingly dense, hot, and luminous.
It gave rise to an embryonic star, which
became the SunW.
Dust in the surrounding area began to
agglomerate. Small pebbles grew larger,
forming embryonic planets, or protoplanets,
a few kilometers in diameter E.
The protoplanets collided with each other
and agglomerated until they reached the size
of planetsveral th(seins retemolik dnasuo
diameter). Over hundreds of millions of years,
the emerging planets, including Earth, were
intensely bombarded by other rocky bodies
R.
LIFE ARISES FROM A BALL OF LAVA
When it was first formed, about 4.6 billion years ago, Earth was completely covered with an ocean of
burning lavacihtI .ktemo sreeddril kalerun horkcs—vel—qiiu d oceron rsu tr crithed net haT.
Little by little, the ocean of lava cooled. Pieces of crusta dnf oltadeo nthe surface of tenalp eh,tfoedrm
which was being intensely bombarded by meteorites and comets Y.
Over time, an early crust. The heformednest ,usva ylemetheorm to fted nnd aonirs achartnecnoc ,lekci
core, while the lighter elements (oxygen, silicon, aluminum, etc.) formed the crust U.
Earth was also host to intense volcanic activity, which led to the expulsion of light gases and liberated an
early atmosphereropav re demrof ; dsouclethrene trfll yidffs radicathat wa,destaw oc tnedn. ’s iAs tomayod
advent of rain allowed for the creation of lakes, rivers, and oceans. At the same time, the crust broke up and
formed continents I.
The presence of continents, oceans, and an oxygen-poor atmosphere resulted in the formation of more and
more complex molecules, which led to a remarkable phenomenon: lifehtraE retfa syearion billn a t ahoMer .
was born, life appeared in the oceans O!nesto th ontntine coaey t srme oegre aokew fil bonli .tIt eh not
0T
0Y
crater
continent
ocean
0O
0U
I0
meteorite
volcano
Earth’s history
T h e g e o l o g i c
t i m e s c a l e
Finding the origins of life
Since it came into being, 4.6 billion years ago, Earth has undergone numerous
transformations. In the beginning, it bore absolutely no resemblance to what we
Earth’s history
see today. The planet’s landscape changed very slowly: continents and oceans
formed, animal and plant species appeared and then were replaced by others.
10
To determine and date the major transformations of a world in perpetual change,
geologists have created a geologic time scale.
THE BEGINNINGS OF THE WORLD: AQUATIC LIFE
The Precambrian Period Qis the oldest and longest period in the
history of Earth. During this period, 4 billion years ago, the terrestrial
crust was formed, followed by the continents and oceans. Life
came into being 500 million years later, when the first
cellular organisms appeared, along with the first
bacteria and algae.
Precambrian
Q
In the Cambrian Period W, various groups
(4.6 b.y. to 570 m.y.)
of invertebrates evolved in the shallow
seas that covered much of Earth.
The first vertebrates appeared in the
following period, the Ordovician E.
There were also great quantities of
coral, sponges, and mollusks
such as cephalopods.
Cyanobacteria, colmymon
called blue-green algae, were
the first micro-organisms to
appear on Earth.
The trilobitewas an invertebrate
with an exoskeleton and a body
divided into three lobes.
m.y.: Millions of years ago
W
(570C–a5m0b5 rmia.yn.)
The brachiopodwas a marine
animal whose thin shell was
covered with grooves.
Calcareous concretions
formed by microscopic
algae, stromatolites,
more than 3 billion years
ago were evidence of the
first life forms.
The first vertebrates
were agnaths f,his
with no jaw.
E
Ordovician
(505–440 m.y.)<