Prentice Hall EARTH SCIENCE
Tarbuck Lutgens
◆
Chapter �1
Vocab
Antarctic Circle
Aphelion
Arctic Circle
Atmosphere
Autumnal equinox
Biosphere
Ecliptic
Galaxy
Geocentric model
Geology
Gregorian calendar
Habitable zone
Heliocentric model
Hydrosphere
Julian calendar
Lithosphere
Lunar calendar
Lunisolar calendar
Meteorology
Milky Way Galaxy
Oceanography
Penumbra
Perihelion
Solar Calendar
Solar Eclipse
Summer Solstice
Tropics
Umbra
Universe
Winter solstice
1.4 Earth System Science
What Is a System?
◆ Closed systems are self contained �(e.g., an automobile cooling system).
◆ Open systems allow both energy and matter to flow in and out of the system �(e.g., a river system).
◆ A system is any size group of interacting parts that form a complex whole.
1.4 Earth System Science
Earth as a System
◆ Earth is a dynamic body with many separate but highly interacting parts �or spheres.
◆ Earth science studies Earth �as a system that is composed of numerous parts, or subsystems.
1.4 Earth System Science
Earth as a System
◆ Sources of Energy
• Sun—drives external processes such as weather, ocean circulation and erosional processes
• Earth’s interior—drives internal processes including volcanoes, earthquakes and mountain building
1.1 What Is Earth Science?
◆ Encompasses all sciences that seek to understand
Overview of Earth Science
1.1 What Is Earth Science?
Overview of Earth Science
◆ Earth science includes
4. astronomy, the study of the universe
3. meteorology, the study of the atmosphere and the processes that produce weather
1. geology, the study of Earth
2. oceanography, the study of the ocean
1.1 What Is Earth Science?
Overview of Earth Science
Further specializations
1.1 What Is Earth Science?
Formation of Earth
◆ Most researchers conclude that Earth and the other planets formed at essentially the same time.
◆ Nebular Hypothesis
1.1 What Is Earth Science?
Formation of Earth
◆ Most researchers conclude that Earth and the other planets formed at essentially the same time.
◆ Nebular Hypothesis
1.1 What Is Earth Science?
Formation of Earth
• The nebula was composed mostly of hydrogen and helium.
◆ Nebular Hypothesis
• About 5 billion years ago, the nebula began to contract.
• It assumed a flat, disk shape with the protosun (pre-Sun) at the center.
1.1 What Is Earth Science?
Formation of Earth
• Inner planets begin to form from metallic and rocky clumps.
◆ Nebular Hypothesis
• Larger outer planets began forming from fragments with a high percentage of ices.
The Nebular Hypothesis
A
C
D
E
B
1.1 What Is Earth Science?
Formation of Earth
◆ Layers Form on Earth
• As Earth formed, the decay of radioactive elements and heat from high-velocity impacts caused the temperature to increase.
• Lighter rocky components floated outward, toward the surface.
• Gaseous material escaped from Earth’s interior to produce the primitive atmosphere.
1.1 Review
Explain how physical geology differs from historical geology.
Why is the earth called a dynamic planet.
How could meteorology be used to study other planets? Mars?
Mercury? Venus?
1.2 A View of Earth
1.2 A View of Earth
Earth's Major Spheres
1. Hydrosphere
• Ocean is the most prominent feature of the hydrosphere.
- Is nearly 71% of Earth's surface
- Holds about 97% of Earth's water
• Also includes fresh water found in streams, lakes, and glaciers, as well as that found underground
1.2 A View of Earth
Earth's Major Spheres
2. Atmosphere
• Thin, tenuous blanket of air
• One half lies below 5.6 kilometers (3.5 miles)
3. Biosphere
• Includes all life
• Concentrated near the surface in a zone that extends from the ocean floor upward for several kilometers into the atmosphere
1.2 A View of Earth
Earth's Major Spheres
4. Geosphere
• Based on compositional differences, it consists of the crust, mantle, and core.
- Crust—the thin, rocky outer layer of Earth.
- Mantle—the 2890-kilometer-thick layer of �Earth located below the crust.
- Core—the innermost layer of Earth, located beneath the mantle.
22.2 The Earth–Moon–Sun System
Motions of the Earth–Moon System
◆ Phases of the Moon
• The phases of the moon are the progression of changes in the moon’s appearance during the month.
• Lunar phases are a result of the motion of the moon and the sunlight that is reflected from its surface.
Phases of the Moon
22.2 The Earth–Moon–Sun System
Motions of the Earth–Moon System
◆ Lunar Motions
• The synodic month is based on the cycle of the moon’s phases. It lasts 29 1/2 days.
• The sidereal month is the true period of the moon’s revolution around Earth. It lasts 27 1/3 days.
22.2 The Earth–Moon–Sun System
Motions of the Earth–Moon System
• The difference of two days between the synodic and sidereal cycles is due to the Earth–moon system also moving in an orbit around the sun.
◆ Lunar Motions
• The moon’s period of rotation about its axis and its revolution around Earth are the same, 27 1/3 days. It causes the same lunar hemisphere to always face Earth.
Lunar Motions
22.2 The Earth–Moon–Sun System
Eclipses
◆ Solar eclipses occur when the moon moves in a line directly between Earth and the sun, casting a shadow on Earth.
◆ During a new-moon or full-moon phase, the moon’s orbit must cross the plane of the ecliptic for an eclipse to take place.
◆ Lunar eclipses occur when the moon passes through Earth’s shadow.
Solar Eclipse
Lunar Eclipse
Lunar Eclipse
Lunar Eclipse
Earth Moon Scale
22.3 Earth’s Moon
Lunar History
◆ The most widely accepted model for the origin of the moon is that when the solar system was forming, a body the size of Mars impacted Earth. The resulting debris was ejected into space, began orbiting around Earth, and eventually united to form the moon.
Formation of Earth’s Moon
22.3 Earth’s Moon
The Lunar Surface
• A crater is the depression at the summit of a volcano or a depression produced by a meteorite impact.
◆ Craters
• Most craters were produced by the impact of rapidly moving debris.
• Rays are any of a system of bright, elongated streaks, sometimes associated with a crater on the moon.
The Moon’s Surface
Mare Tranquillitatus
(Sea of Tranquility)
Mare Imbrium
(Sea of Rains)
Kepler
Crater
Copernicus
Crater
The Moon’s Surface
Earth’s Layered Structure
1.2 A View of Earth
Plate Tectonics
1.3 Representing Earth’s Surface
Determining Location
1.3 Representing Earth’s Surface
1.3 Representing Earth’s Surface
1.3 Representing Earth’s Surface
Maps and Mapping
◆ No matter what kind of map is made, some portion of the surface will always look either too small, too big, or out of place. Mapmakers have, however, found ways to limit the distortion of shape, size, distance and direction.
1.3 Mercator Map
Latitude and Longitude are parallel.
Shows true direction
1.3 Robinson Projection Map
Shows the whole earth, but is very distorted.
1.3 Conic Projection Map
Used to make weather and road maps. Shows relative little distortion of land masses.
1.3 Gnomonic Projection Map
Accurate distance and direction across the oceans
1.3 Polyheadral Projection Map
Shows distance and size/shape of land accurately, but is hard to navigate with
1.3 Representing Earth’s Surface
Topographic Maps
◆ Topographic maps represent Earth’s surface in three dimensions; they show elevation, distance directions, and slope angles.
1.4 Earth System Science
What Is a System?
◆ Closed systems are self contained �(e.g., an automobile cooling system).
◆ Open systems allow both energy and matter to flow in and out of the system �(e.g., a river system).
◆ A system is any size group of interacting parts that form a complex whole.
1.4 Earth System Science
Earth as a System
◆ Earth is a dynamic body with many separate but highly interacting parts �or spheres.
◆ Earth system science studies Earth �as a system that is composed of numerous parts, or subsystems.
1.4 Earth System Science
Earth as a System
◆ Sources of Energy
• Sun—drives external processes such as weather, ocean circulation and erosional processes
• Earth’s interior—drives internal processes including volcanoes, earthquakes and mountain building
1.4 Earth System Science
Earth as a System
◆ Humans are part of the Earth system.
◆ Consists of a nearly endless array of subsystems (e.g., hydrologic cycle)
1.4 Earth System Science
People and the Environment
◆ Environment
• Surrounds and influences organisms
1.4 Earth System Science
People and the Environment
◆ Resources
• Include water, soil, minerals, and energy
• Two broad categories
2. Nonrenewable—cannot be replenished in the near future (e.g., metals, fuels)
1. Renewable—can be replenished (e.g., plants, energy from water and wind)
1.4 Earth System Science
People and the Environment
◆ Population
• Population of the planet is growing rapidly
• Use of minerals/energy has climbed more rapidly than the overall growth of population
Growth of World Population
1.4 Earth System Science
Environmental Problems
◆ Caused by people and societies
• Urban air pollution
• Acid rain
◆ Caused by natural hazards
• Landslides
• Ozone depletion
• Global warming
• Earthquakes
◆ Local, regional, and global
6.1 Running Water
The Water Cycle
◆ Water constantly moves among the oceans, the atmosphere, the solid Earth, and the biosphere. This unending circulation of Earth’s water supply is �the water cycle.
Distribution of Earth’s Water
6.1 Running Water
The Water Cycle
◆ Processes involved in the cycle are
• infiltration—the movement of surface water into rock or soil through cracks and pore spaces
• transpiration—the release of water into the atmosphere from plants
• precipitation
• evaporation
• runoff
6.1 Running Water
Earth’s Water Balance
◆ Balance in the water cycle means the average annual precipitation over Earth equals the amount of water that evaporates.
The Water Cycle
6.1 Running Water
Rivers
6.1 Running Water
6.1 Running Water
1.5 What Is Scientific Inquiry?
Science
◆ Science assumes the natural world is
• consistent
• predictable
◆ Goals of science are
• to use the knowledge to predict
• to discover patterns in nature
1.5 What Is Scientific Inquiry?
Hypothesis and Theory
◆ An idea can become a
◆ Scientific Method
1.5 What Is Scientific Inquiry?
Science Methods
◆ Scientific knowledge is gained through
• following systematic steps
1. Collecting facts
• theories that withstand examination
2. Developing a hypothesis
3. Conducting experiments
4. Reexamining the hypothesis and accepting, modifying, or rejecting it