Chapter 1 Introduction to Planet “Earth”

Table of Contents

Overview

The world ocean is the most prominent feature on Earth.
Oceans cover 70.8% of Earth’s surface.
The origin and development of life on Earth are connected to the ocean.
The oceans have a long history on Earth.

Earth’s Oceans

Earth has one ocean.

It is divided into four principle oceans and one other.

  • Pacific Ocean
  • Atlantic Ocean
  • Indian Ocean
  • Arctic Ocean
  • Southern, or Antarctic, Ocean

Ocean Size and Depth

Pacific Ocean

  • World’s largest ocean
    • Accounts for more than half of Earth’s ocean space
  • World’s deepest ocean
  • Earth’s largest geographic feature
  • Named in 1520 by Ferdinand Magellan

Atlantic Ocean

  • Half the size of the Pacific Ocean
  • Shallower than the Pacific Ocean
  • Separates the Old World from the New World

Indian Ocean

  • Smaller than the Atlantic Ocean
  • Similar depth as the Atlantic Ocean
  • Primarily in the Southern Hemisphere

Arctic Ocean

  • Seven percent the size of the Pacific Ocean
  • Shallowest world ocean
  • Permanent layer of sea ice a few meters thick

Southern Ocean or Antarctic Ocean

  • Circumnavigates Antarctica
  • Is really the parts of the Pacific, Atlantic, and Indian Oceans that lie south of 50° S latitude

The Seven Seas

  • Smaller and shallower than oceans Salt water
  • Usually enclosed by land
    • Sargasso Sea defined by surrounding ocean currents
  • Directly connected to the ocean

Before the 15th century, Europeans considered the seven seas to be the following:

  1. Red Sea
  2. Mediterranean Sea
  3. Persian Gulf
  4. Black Sea
  5.  Adriatic Sea
  6. Caspian Sea
  7. Indian Ocean

Comparing Oceans to Continents

  • Average ocean depth is 3682 meters (12, 080 feet)
  • Average continental elevation is 840 meters (2756 feet)
  • Deepest ocean trench is the Mariana Trench at 11,022 meters (36,161 feet)
  • Highest continental mountain is Mt. Everest at 8850 meters (29,035 feet)

Early Exploration of the Oceans

  • Early “explorers” used boats to seek new fishing grounds for food.
  • The ocean facilitated trade and interaction between cultures.

Pacific Navigators

  • The peopling of the Pacific Islands required extensive travel in open boats and exceptional navigation skills.
  • It was difficult because islands are widely scattered

Pacific People

  • No written records exist of Pacific human history before the 16th century.
  • Archeological evidence suggests island occupation by people from New Guinea as early as 4000–5000 B.C.
  • Thor Heyerdahl sailed on a balsa raft – the Kon Tiki – to demonstrate migration of South Americans to Pacific Ocean islands.

European Navigators

  • Phoenecians – first from Western Hemisphere to develop navigation arts
  • Navigated circa 2000 B.C.
  • Explored Mediterranean Sea, Red Sea, and Indian Ocean
  • First circumnavigation of Africa
  • Greek Pytheas
  • Sailed northward using a simple method to determine latitude in 325 B.C.
  • Navigated using the North Star
  • Eratosthenes determined Earth’s

Europeans

  • Herodotus produced inaccurate world map around 450 B.C.
  • Claudius Ptolemy produced fairly accurate world map around 150 A.D.
    • Erroneously updated Eratosthenes’ original circumference estimation, later causing Christopher Columbus
  • to believe he had reached Asia

The Middle Ages

  • Arabs dominant navigators in the Mediterranean Sea
  • Traded extensively with East Africa, India, and Southeast Asia
  • Learned to use Indian Ocean monsoon winds for travel
  • Vikings explored North Atlantic Ocean
    • Settled Iceland and Greenland in 9th and 10th centuries A.D.
    • Leif Eriksson designated part of eastern Canada Vinland (now Newfoundland) in 995 A.D.
    • Greenland, Vinland settlements abandoned by 1450 A.D. due to climatic cooling

Viking Routes and Colonies

The Age of Discovery in Europe 1492–1522

  • Search for new Eastern trade routes by sea
    • Prince Henry the Navigator of Portugal sought trade routes around Africa.
    • Europeans explore North and South America.
      • Christopher Columbus was financed by the Spanish to find new trade routes to Asia.
      • Englishman John Cabot arrived in northeast North America in 1497.
  • Spaniard Ferdinand Magellan circumnavigated the globe.
    • Was killed on a Pacific Island in 1521
  • Juan Sebastian del Caño completed the circumnavigation in 1522.
  • Voyages paved the way for the Spanish to take gold from the Incas and Mayas.
  • Spain’s maritime dominance ended when England defeated the Spanish Armada in 1588.

Voyages of Columbus and Magellan

Voyaging for Science

  • The English wanted to retain maritime superiority.
  • Captain James Cook (1728–1779) undertook three scientific voyages.
    • Ships HMS Endeavour, Resolution,
    • Adventure
    • Mapped many islands in Pacific
    • Systematically measured ocean characteristics
    • Marine chronograph (longitude)

More high-technology tools available today

  • Sonar
  • Robotics
  • Computers
  • Satellites

Nature of Scientific Inquiry

  • Natural phenomena governed by physical processes
  • Physical processes similar today as in the past
  • Scientists discover these processes and make predictions.
  • Called the scientific method

The Scientific Method

Chapter 1 Introduction to Planet “Earth”
Chapter 1 Introduction to Planet “Earth”

Theories and Truth

  • Science never reaches absolute truth.
  • Truth is probable and based on available observations.
  • New observations yield scientific progress. In reality, scientists have no formal method.

Formation of Earth and the Solar System

  • Nebular hypothesis –
    • all bodies in the solar system formed from nebula
    • Nebula = cloud of gases and space dust
      • Mainly hydrogen and helium

Nebular Hypothesis

  • Gravity concentrates material at center of cloud (Sun).
  • Protoplanets form from smaller concentrations of matter (eddies).

Protoearth

  • Larger than Earth today
  • Homogeneous composition
  • Bombarded by meteorites
    • Moon formed from collision with large asteroid
  • Radioactive heat
    • Spontaneous disintegration of atoms
    • Fusion reactions
  • Heat from contraction (protoplanet shrinks due to gravity)
  • Protoearth partially melts
  • Density stratification (layered Earth)
Chapter 1 Introduction to Planet “Earth”
Chapter 1 Introduction to Planet “Earth”

Density Stratification

  • High density = heavy for its size
  • Early Earth experienced gravitational separation.
    • High-density materials (iron and nickel) settled in core.
    • Less dense materials formed concentric spheres around core.

Earth’s Internal Structure

  • Layers defined by
    • Chemical composition
    • Physical properties

Layers by Chemical Composition

  • Crust
    • Low-density, mainly silicate minerals
  • Mantle
    • Mainly iron (Fe) and magnesium (Mg) silicate minerals
  • Core
    • High-density, mainly iron (Fe) and nickel (Ni)

Layers by Physical Properties

  • Lithosphere
  • Asthenosphere
  • Mesosphere
  • Outer core
  • Inner core

Lithosphere

  • Cool, rigid shell
  • Includes crust and upper mantle
  • About 100 km
  • (60 miles) thick

Continental vs. Oceanic Crust

Oceanic CrustContinental Crust
Main rock typeBasalt (dark-colored igneous rock)Granite (light-colored igneous rock)
Density (grams per cubic centimeter)3.02.7
Average thickness8 kilometers (5 miles)35 kilometers (22 miles)

Asthenosphere

  • Relatively hot, plastic
  • Flows with high viscosity
    • Important for movement of lithospheric plates
  • Base of lithosphere to about 700 km (430 miles) deep.

Isostatic Adjustment

  • Vertical movement of Earth’s crust
  • Buoyancy of lithosphere on asthenosphere –
    • Less dense continental crust floats higher than denser oceanic crust.
  • Isostatic rebound – rising of crust formerly weighed down by glacier ice

Origin of Earth’s Atmosphere

  • Outgassing – occurred during density stratification
    • Water vapor
    • Carbon dioxide
    • Hydrogen
    • Other gases
  • Earth’s early atmosphere different from today

Origin of Earth’s Oceans

  • Outgassed water vapor fell as rain.
  • The first permanent oceans formed 4 billion years ago.
  • Salinity developed from dissolved rock elements.
    • Early acidic rain dissolved more crustal minerals than today.
Chapter 1 Introduction to Planet “Earth”
Chapter 1 Introduction to Planet “Earth”

Life’s Possible Ocean Origins

  • Earth’s earliest known life forms are 3.5-billion-year-old bacteria fossilized in ocean rocks.
  • These are the building blocks for life on early Earth.
  • There is no direct evidence of early Earth’s environment.

Oxygen

  • Humans require O2.
  • Ozone (O3) protects from ultraviolet radiation.
  • Early Earth had little free oxygen.
  • The lack of ozone may have helped originate life.

Stanley Miller’s Experiment

Organic molecules formed by ultraviolet light, electrical spark (lightning), and a mixture of water, carbon dioxide, hydrogen, methane, and ammonia.

Chapter 1 Introduction to Planet “Earth”
Chapter 1 Introduction to Planet “Earth”

Evolution and Natural Selection

  • Organisms adapt and change through time.
  • Advantageous traits are naturally selected. Traits are passed to the next generation.
  • Organisms adapt to environments.
  • Organisms can modify environments.

Plants and Animals Evolve

  • Heterotrophs
    • Very earliest life
    • Require external food supply
  • Autotrophs
    • Evolved later
    • Manufacture own food supply

First Autotrophs

  • Probably similar to modern anaerobic bacteria
    • Survive without oxygen
  • Chemosynthesis from chemicals at deep hydrothermal vents
  • Supports idea of life’s origins on deep ocean floor in absence of light

Photosynthesis and Respiration

  • Complex autotrophs developed chlorophyll.
  • This allowed the use of the Sun for photosynthesis.
  • Cellular respiration

Great Oxidation Event

  • 2.45 billion years ago
  • Increased oxygen and ozone eliminated the anaerobe food supply.
  • Light and oxygen kill anaerobes. Cyanobacteria adapted and thrived.

Changes to Earth’s Atmosphere

  • Photosynthetic organisms are responsible for life as we know it today.
  • Reduce CO2, increase O2 to 21%
  • High oxygen = biodiversity increase
  • Low oxygen associated with extinction events

Plants and Earth’s Environment

Age of Earth

  • Radiometric age dating
    • Spontaneous change/decay
    • Half-life
  • Earth is about 4.6 billion years old.

Radioactive Decay

Geologic Time Scale

NOTE-The content provided, which aligns with Essentials of Oceanography by Alan P. Trujillo and Harold V. Thurman (11th edition)

Reference: All images and content are taken from Essentials of Oceanography by Alan P. Trujillo and Harold V. Thurman, 12th Edition.

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