The document summarizes key information about Earth's atmosphere:
1) Earth's atmosphere is composed of nitrogen (78%), oxygen (21%), and trace amounts of other gases like carbon dioxide and argon. It also contains water vapor, solid particles, and liquid droplets.
2) The atmosphere is divided into five main layers - troposphere, stratosphere, mesosphere, thermosphere, and exosphere - with varying temperature and air pressure profiles.
3) Air pressure decreases with increasing altitude as there are fewer gas molecules above Earth's surface to exert pressure downward. Atmospheric pressure is greater in the troposphere near Earth than in the exosphere.
The document is a lesson plan for teaching 7th grade science about Earth's atmosphere. It outlines the objectives of identifying and describing the 5 layers of the atmosphere, explaining how the layers are divided, discussing the composition of the atmosphere, and relating the importance of the atmosphere to humans. The lesson plan details preliminary activities, a motivation activity, presentation of new material through group work and discussions, and a concluding valuation section.
Meteorology-a student's report( a compilation of facts from books,internet,jo...John Allen Marilla
it is a summary of the topic about t6he atmosphere..... all information written are not words of the maker but are compilations only from various book,journal,internet sources... this makes learning about the atmosphere for freshmen easier,,,
Changes in the earth and its atmosphereSteve Bishop
The document summarizes changes to the Earth's core, mantle, crust, and atmosphere over time. It describes the theory of tectonic plates and how their movement causes earthquakes and volcanic eruptions. It explains how early theories of continental drift were rejected but later accepted when ocean floor investigations found evidence supporting plate tectonics. It also outlines how the atmosphere was initially composed of gases like carbon dioxide and methane, and how oxygen levels increased due to photosynthesis by plants and algae.
1. The document is a lesson plan about teaching students about the ozone layer and ozone depletion.
2. It outlines content that will be covered, including that the ozone layer is a region 18-55km above the Earth's surface that filters out ultraviolet rays, and that chlorofluorocarbons released by sprays and paints cause ozone depletion.
3. Activities are planned to help students understand the importance of the ozone layer and the consequences of ozone depletion, such as climate change and increased skin cancer rates, as well as ways to protect the ozone layer like reducing plastic use.
- The document discusses key features of Earth and the Moon, including their formation and interactions.
- It describes how plate tectonics leads to geological activity at plate boundaries like earthquakes and volcanoes.
- It also explains how tidal forces from the Moon cause Earth's ocean tides and how the Moon synchronously rotates to always show the same face to Earth due to tidal locking during its formation.
ATMOSPHERE ENVIRONMENT
PRESENTORS ::
>> Cuevas, Jennifer
>> Doble, Rogin
>> Gutierrez, Arlene
>> Marasigan, Debie Joy
>> Sibuan, Andrew
The Atmosphere Environment
This chapter discusses:
The significance of the Atmosphere
The composition of the Atmosphere
The layers of the atmosphere
The Atmospheric Circulation
Importance
Atmosphere – a thin layer of air that forms a protective covering around Earth.
It keeps Earth’s temperature in a range that can support life.
It also care for life-forms from some of the Sun’s harmful rays.
The Composition of Atmosphere
The Atmosphere** layer of gas that surrounds Earth more commonly known as “air”.
Atmosphere. How do you know its there
Is this “air” that surrounds us considered matter? Does it weigh anything? How do you know?
Think about it and decide on an answer.
Talk in groups with the person who sits by you
Be ready to tell the class what you decided and why.
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Dark matter and the habitability of planetsSérgio Sacani
This document discusses how dark matter annihilation could provide an energy source to maintain surface temperatures suitable for liquid water on some planets, making them potentially habitable even without being orbiting a star. It explains that while dark matter annihilation provides negligible heating for Earth, larger planets in regions with higher dark matter densities like dwarf galaxies could capture and annihilate dark matter at rates sufficient to habitability through liquid water, with this heating lasting trillions of years for some planets. The document then examines dark matter capture in Earth and super-Earth planets and calculates surface temperatures on planets in environments with high dark matter densities.
Here are the key points about heat and temperature scales:
1) Heat is the total amount of thermal energy in an object or system. Temperature is a measure of how hot or cold something is compared to a reference point.
2) Fahrenheit uses 32°F as the freezing point of water and 212°F as the boiling point. Celsius uses 0°C as the freezing point and 100°C as the boiling point. Kelvin uses 0K as absolute zero. Water freezes at 273.15K and boils at 373.15K.
3) Dew point is the temperature at which water vapor in air will condense into liquid water. Condensation occurs when air reaches saturation point and can hold no
The document is a lesson plan for teaching 7th grade science about Earth's atmosphere. It outlines the objectives of identifying and describing the 5 layers of the atmosphere, explaining how the layers are divided, discussing the composition of the atmosphere, and relating the importance of the atmosphere to humans. The lesson plan details preliminary activities, a motivation activity, presentation of new material through group work and discussions, and a concluding valuation section.
Meteorology-a student's report( a compilation of facts from books,internet,jo...John Allen Marilla
it is a summary of the topic about t6he atmosphere..... all information written are not words of the maker but are compilations only from various book,journal,internet sources... this makes learning about the atmosphere for freshmen easier,,,
Changes in the earth and its atmosphereSteve Bishop
The document summarizes changes to the Earth's core, mantle, crust, and atmosphere over time. It describes the theory of tectonic plates and how their movement causes earthquakes and volcanic eruptions. It explains how early theories of continental drift were rejected but later accepted when ocean floor investigations found evidence supporting plate tectonics. It also outlines how the atmosphere was initially composed of gases like carbon dioxide and methane, and how oxygen levels increased due to photosynthesis by plants and algae.
1. The document is a lesson plan about teaching students about the ozone layer and ozone depletion.
2. It outlines content that will be covered, including that the ozone layer is a region 18-55km above the Earth's surface that filters out ultraviolet rays, and that chlorofluorocarbons released by sprays and paints cause ozone depletion.
3. Activities are planned to help students understand the importance of the ozone layer and the consequences of ozone depletion, such as climate change and increased skin cancer rates, as well as ways to protect the ozone layer like reducing plastic use.
- The document discusses key features of Earth and the Moon, including their formation and interactions.
- It describes how plate tectonics leads to geological activity at plate boundaries like earthquakes and volcanoes.
- It also explains how tidal forces from the Moon cause Earth's ocean tides and how the Moon synchronously rotates to always show the same face to Earth due to tidal locking during its formation.
ATMOSPHERE ENVIRONMENT
PRESENTORS ::
>> Cuevas, Jennifer
>> Doble, Rogin
>> Gutierrez, Arlene
>> Marasigan, Debie Joy
>> Sibuan, Andrew
The Atmosphere Environment
This chapter discusses:
The significance of the Atmosphere
The composition of the Atmosphere
The layers of the atmosphere
The Atmospheric Circulation
Importance
Atmosphere – a thin layer of air that forms a protective covering around Earth.
It keeps Earth’s temperature in a range that can support life.
It also care for life-forms from some of the Sun’s harmful rays.
The Composition of Atmosphere
The Atmosphere** layer of gas that surrounds Earth more commonly known as “air”.
Atmosphere. How do you know its there
Is this “air” that surrounds us considered matter? Does it weigh anything? How do you know?
Think about it and decide on an answer.
Talk in groups with the person who sits by you
Be ready to tell the class what you decided and why.
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Weight of the atmosphere
Gases are in the atmosphere.
They are things we learned about in the periodic table: Nitrogen, Oxygen, Carbon Dioxide, Hydrogen
It is matter! Sound can travel through it.
Even though you can’t see them, Atoms make up gases.
Are some atoms bigger than others?
Are their atomic weights all the same?
Helium vs. Carbon Dioxide
Do you think of helium as light and floating or heavy and falling?
Do you think about Carbon Dioxide as light and floating or heavy and falling….think about the gas released from dry ice… does it go up or down?
Dark matter and the habitability of planetsSérgio Sacani
This document discusses how dark matter annihilation could provide an energy source to maintain surface temperatures suitable for liquid water on some planets, making them potentially habitable even without being orbiting a star. It explains that while dark matter annihilation provides negligible heating for Earth, larger planets in regions with higher dark matter densities like dwarf galaxies could capture and annihilate dark matter at rates sufficient to habitability through liquid water, with this heating lasting trillions of years for some planets. The document then examines dark matter capture in Earth and super-Earth planets and calculates surface temperatures on planets in environments with high dark matter densities.
Here are the key points about heat and temperature scales:
1) Heat is the total amount of thermal energy in an object or system. Temperature is a measure of how hot or cold something is compared to a reference point.
2) Fahrenheit uses 32°F as the freezing point of water and 212°F as the boiling point. Celsius uses 0°C as the freezing point and 100°C as the boiling point. Kelvin uses 0K as absolute zero. Water freezes at 273.15K and boils at 373.15K.
3) Dew point is the temperature at which water vapor in air will condense into liquid water. Condensation occurs when air reaches saturation point and can hold no
The document describes Earth's four main spheres - the lithosphere, hydrosphere, biosphere, and atmosphere. The lithosphere contains all of Earth's solid and liquid land, including the crust and layers below. The hydrosphere contains all of Earth's water, both liquid and frozen. Most is salty ocean water. The biosphere contains all living things on Earth, including microbes, plants and animals that form ecological communities. The atmosphere contains Earth's air and extends from the surface into space.
The document discusses the composition and structure of Earth's atmosphere. It is composed primarily of nitrogen, oxygen, and trace amounts of other gases. The atmosphere is divided into five layers - the troposphere, stratosphere, mesosphere, thermosphere, and exosphere - based on how properties like temperature and pressure change with altitude. Each layer has distinguishing characteristics, such as weather occurring in the troposphere and protective ozone existing in the stratosphere.
The document summarizes information about changes in the Earth's crust and atmosphere over time. It discusses how tectonic plates move due to convection currents in the mantle caused by radioactive processes in the core. Wegener's theory of continental drift proposed that the continents were once joined and have gradually moved apart, supported by matching fossil evidence. The early atmosphere was mostly carbon dioxide and water vapor with little oxygen, but it evolved over billions of years through volcanic outgassing and photosynthesis to today's composition of 78% nitrogen and 21% oxygen. The Miller-Urey experiment provided evidence that amino acids could have formed from simple gases in the early atmosphere.
The document provides an overview of Earth's atmosphere including:
- Its composition of nitrogen (78%), oxygen (21%), and trace amounts of other gases.
- It describes the layers of the atmosphere from lowest to highest - troposphere, stratosphere, mesosphere, thermosphere, and exosphere.
- Key topics covered include the nitrogen cycle, how pressure decreases with altitude, measuring pressure, atmospheric chemistry, and issues like acid rain, the greenhouse effect, and ozone depletion.
This document discusses the composition and structure of the atmosphere. It is composed of nitrogen, oxygen, and other gases. It has five layers: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. The document also discusses wind formation from air moving between high and low pressure areas, cloud formation through condensation, different types of precipitation, atmospheric pressure varying with altitude, and the importance of the atmosphere in regulating temperature and protecting the Earth. It concludes with discussing greenhouse effect, global warming caused by human activity, and atmospheric pressure.
The document summarizes the composition and structure of Earth. It is divided into four interconnected spheres: the atmosphere, hydrosphere, lithosphere, and biosphere. The atmosphere is composed primarily of nitrogen and oxygen and contains weather and protects the planet. The hydrosphere includes all water on Earth, both liquid and frozen. The lithosphere is the solid crust and interior of the planet. Finally, the biosphere contains all living organisms on Earth.
The document discusses various topics related to space including the universe, galaxies, the Milky Way galaxy, planets, stars, the solar system, the eight major planets, asteroids, Jupiter, Saturn, Uranus, Neptune, the Kuiper Belt, constellations like the Big Dipper, Ursa Major, Pegasus, Orion, and Cygnus, black holes, and comets. It provides descriptions of each topic with some key details like the immense size of the universe, components of galaxies, shapes and components of the Milky Way galaxy, definitions and compositions of planets and stars, an overview of the solar system and its planets, and characteristics of black holes and comets.
There are two basic groups of planets in the solar system - terrestrial and jovian. Terrestrial planets are small and rocky like Mercury, Venus, Earth, and Mars. Jovian planets are large and gaseous, consisting of Jupiter, Saturn, Uranus, and Neptune. Mars has the largest volcano and canyon in the solar system. Jupiter's clouds move in east-west bands and Saturn has a large ring system with gaps. Uranus and Neptune are similar in size and interior composition. Comets have long elliptical orbits and contain ice that evaporates when passing close to the sun. Meteoroids enter the atmosphere and burn up, appearing as meteors, with some larger pieces surviving
The document discusses three variable components of air: water vapor, aerosols, and ozone. Water vapor varies between 1-4% and is the source of clouds, precipitation, and latent heat. Aerosols are microscopic particles from natural and human sources that provide surfaces for water vapor to condense on, influencing cloud formation. Ozone is a form of oxygen with three atoms that absorbs harmful ultraviolet radiation in the stratosphere between 10-50 km above the surface.
The document provides an overview of a geography lesson on the interior of the Earth. It discusses various sources of evidence for the Earth's internal structure, including theories of the planet's origin, density and pressure measurements, temperature observations, and analysis of seismic wave behavior. Seismology is identified as the primary source of information, with discussion of how P, S, and L waves change speed and behavior when passing through the core, mantle, and crust.
The document provides information about the history and formation of Earth 4.54 billion years ago. It discusses Earth's atmosphere, composition, layers, facts, and natural phenomena like mountains, minerals, rocks, and volcanoes. The text also covers topics like meteoroids, global warming, the greenhouse effect, pollution, depletion of the ozone layer, and indications that the Earth is nearing its end. Suggested preventions include education programs, banning illegal dumping, raising awareness, and supporting green movements.
The document describes the composition and structure of Earth's atmosphere. It is divided into multiple layers based on chemical composition, thermal properties, and electromagnetic properties. The major layers from lowest to highest are: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. Each layer has unique characteristics such as varying temperature profiles and concentrations of different gases. The thermosphere and lower layers contain the ionosphere, where solar radiation ionizes gases to form a region that can reflect radio waves.
The document provides information about the history and formation of Earth 4.54 billion years ago, including five mass extinction events. It discusses Earth's atmosphere, composition, layers, facts, and natural phenomena like mountains, minerals, rocks, and volcanoes. The text also covers topics like the greenhouse effect, pollution, the ozone layer, depletion issues, and indications that the Earth is nearing an end unless preventative measures are taken.
• Earth, along with the other planets, is believed to have been born 4.5 billion years ago as a solidified cloud of dust and gases left over from the creation of the Sun.
• For perhaps 500 million years, the interior of Earth stayed solid and relatively cool, perhaps 2,000°F.
• The main ingredients were iron and silicates, with small amounts of other elements, some of them radioactive.
• As millions of years passed, energy released by radioactive decay—mostly of uranium, thorium, and potassium—gradually heated Earth, melting some of its constituents.
• The iron melted before the silicates, and, being heavier, sank toward the center.
• This forced up the silicates that it found there.
• After many years, the iron reached the center, almost 4,000 mi deep, and began to accumulate. No eyes were around at that time to view the turmoil that must have taken place on the face of Earth—gigantic heaves and bubblings on the surface, exploding volcanoes, and flowing lava covering everything in sight.
• Finally, the iron in the center accumulated as the core. Around it, a thin but fairly stable crust of solid rock formed as Earth cooled.
• Depressions in the crust were natural basins in which water, rising from the interior of the planet through volcanoes and fissures, collected to form the oceans. Slowly, Earth acquired its present appearance.
The document provides information about the history and formation of Earth 4.54 billion years ago, including major extinction events. It discusses Earth's atmosphere, composition, layers, and facts such as the presence of one natural satellite, the Moon. Graphics are included showing the relative sizes and distances of planets in the solar system. The document also covers mountains, minerals, rocks, volcanoes, meteoroids, and natural phenomena such as global warming, the greenhouse effect, ozone layer depletion, and indications of threats facing Earth. Prevention methods are mentioned.
The document discusses the composition and structure of Earth's atmosphere. It is composed primarily of nitrogen and oxygen, with smaller amounts of gases like carbon dioxide, argon, and methane. The atmosphere is divided into four layers - the troposphere closest to Earth's surface where weather occurs, the stratosphere above it where ozone absorbs UV light, the mesosphere where temperatures decrease with altitude, and the thermosphere where temperatures increase with altitude. The greenhouse effect describes how certain gases in the atmosphere trap heat radiating from Earth's surface, maintaining a climate suitable for life.
The document discusses the different spheres or layers of the Earth. It begins by describing the Earth and its color compared to other planets. It then discusses the four subsystems that make up Earth and flow of matter and energy between them. It identifies the layers of the Earth and differentiates between them. Finally, it discusses natural waters and the water cycle.
This document discusses the four subsystems that make up the Earth: the atmosphere, biosphere, geosphere, and hydrosphere. It provides descriptions of each subsystem, including what they are composed of and their key characteristics. The document also presents an activity that asks students to analyze the interactions between the different subsystems using the example of the Taal Volcano eruption.
The document discusses the composition and structure of Earth's atmosphere. It describes the different layers of the atmosphere, including the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. It explains how solar energy is transferred throughout the atmosphere using radiation, conduction, and convection. The document also mentions clouds and the water cycle.
The document discusses the key subsystems that make up the Earth system, including the atmosphere, hydrosphere, lithosphere, biosphere, and how they interact. It provides details on the composition and important processes of each subsystem. The atmosphere contains 78% nitrogen, 21% oxygen, and is responsible for heat redistribution and the hydrologic cycle. The hydrosphere covers 70% of the Earth as ocean water and freshwater. The lithosphere includes the crust and mantle, and plate tectonics shape the Earth's surface. The biosphere is the set of all life forms and the carbon cycle. Each subsystem interacts with the others, making life possible on Earth.
Here are the answers to your questions:
1) Heat is a form of energy that causes temperature change, while temperature is a measure of how hot or cold something is.
2) Fahrenheit measures temperature in degrees Fahrenheit (°F). Water freezes at 32°F and boils at 212°F. Celsius measures temperature in degrees Celsius (°C). Water freezes at 0°C and boils at 100°C. Kelvin measures temperature in kelvins (K) using the same increments as Celsius but water freezes at 273.15 K and boils at 373.15 K.
3) Dew point is the temperature at which water vapor in air condenses into liquid water. Condens
The document describes Earth's four main spheres - the lithosphere, hydrosphere, biosphere, and atmosphere. The lithosphere contains all of Earth's solid and liquid land, including the crust and layers below. The hydrosphere contains all of Earth's water, both liquid and frozen. Most is salty ocean water. The biosphere contains all living things on Earth, including microbes, plants and animals that form ecological communities. The atmosphere contains Earth's air and extends from the surface into space.
The document discusses the composition and structure of Earth's atmosphere. It is composed primarily of nitrogen, oxygen, and trace amounts of other gases. The atmosphere is divided into five layers - the troposphere, stratosphere, mesosphere, thermosphere, and exosphere - based on how properties like temperature and pressure change with altitude. Each layer has distinguishing characteristics, such as weather occurring in the troposphere and protective ozone existing in the stratosphere.
The document summarizes information about changes in the Earth's crust and atmosphere over time. It discusses how tectonic plates move due to convection currents in the mantle caused by radioactive processes in the core. Wegener's theory of continental drift proposed that the continents were once joined and have gradually moved apart, supported by matching fossil evidence. The early atmosphere was mostly carbon dioxide and water vapor with little oxygen, but it evolved over billions of years through volcanic outgassing and photosynthesis to today's composition of 78% nitrogen and 21% oxygen. The Miller-Urey experiment provided evidence that amino acids could have formed from simple gases in the early atmosphere.
The document provides an overview of Earth's atmosphere including:
- Its composition of nitrogen (78%), oxygen (21%), and trace amounts of other gases.
- It describes the layers of the atmosphere from lowest to highest - troposphere, stratosphere, mesosphere, thermosphere, and exosphere.
- Key topics covered include the nitrogen cycle, how pressure decreases with altitude, measuring pressure, atmospheric chemistry, and issues like acid rain, the greenhouse effect, and ozone depletion.
This document discusses the composition and structure of the atmosphere. It is composed of nitrogen, oxygen, and other gases. It has five layers: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. The document also discusses wind formation from air moving between high and low pressure areas, cloud formation through condensation, different types of precipitation, atmospheric pressure varying with altitude, and the importance of the atmosphere in regulating temperature and protecting the Earth. It concludes with discussing greenhouse effect, global warming caused by human activity, and atmospheric pressure.
The document summarizes the composition and structure of Earth. It is divided into four interconnected spheres: the atmosphere, hydrosphere, lithosphere, and biosphere. The atmosphere is composed primarily of nitrogen and oxygen and contains weather and protects the planet. The hydrosphere includes all water on Earth, both liquid and frozen. The lithosphere is the solid crust and interior of the planet. Finally, the biosphere contains all living organisms on Earth.
The document discusses various topics related to space including the universe, galaxies, the Milky Way galaxy, planets, stars, the solar system, the eight major planets, asteroids, Jupiter, Saturn, Uranus, Neptune, the Kuiper Belt, constellations like the Big Dipper, Ursa Major, Pegasus, Orion, and Cygnus, black holes, and comets. It provides descriptions of each topic with some key details like the immense size of the universe, components of galaxies, shapes and components of the Milky Way galaxy, definitions and compositions of planets and stars, an overview of the solar system and its planets, and characteristics of black holes and comets.
There are two basic groups of planets in the solar system - terrestrial and jovian. Terrestrial planets are small and rocky like Mercury, Venus, Earth, and Mars. Jovian planets are large and gaseous, consisting of Jupiter, Saturn, Uranus, and Neptune. Mars has the largest volcano and canyon in the solar system. Jupiter's clouds move in east-west bands and Saturn has a large ring system with gaps. Uranus and Neptune are similar in size and interior composition. Comets have long elliptical orbits and contain ice that evaporates when passing close to the sun. Meteoroids enter the atmosphere and burn up, appearing as meteors, with some larger pieces surviving
The document discusses three variable components of air: water vapor, aerosols, and ozone. Water vapor varies between 1-4% and is the source of clouds, precipitation, and latent heat. Aerosols are microscopic particles from natural and human sources that provide surfaces for water vapor to condense on, influencing cloud formation. Ozone is a form of oxygen with three atoms that absorbs harmful ultraviolet radiation in the stratosphere between 10-50 km above the surface.
The document provides an overview of a geography lesson on the interior of the Earth. It discusses various sources of evidence for the Earth's internal structure, including theories of the planet's origin, density and pressure measurements, temperature observations, and analysis of seismic wave behavior. Seismology is identified as the primary source of information, with discussion of how P, S, and L waves change speed and behavior when passing through the core, mantle, and crust.
The document provides information about the history and formation of Earth 4.54 billion years ago. It discusses Earth's atmosphere, composition, layers, facts, and natural phenomena like mountains, minerals, rocks, and volcanoes. The text also covers topics like meteoroids, global warming, the greenhouse effect, pollution, depletion of the ozone layer, and indications that the Earth is nearing its end. Suggested preventions include education programs, banning illegal dumping, raising awareness, and supporting green movements.
The document describes the composition and structure of Earth's atmosphere. It is divided into multiple layers based on chemical composition, thermal properties, and electromagnetic properties. The major layers from lowest to highest are: the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. Each layer has unique characteristics such as varying temperature profiles and concentrations of different gases. The thermosphere and lower layers contain the ionosphere, where solar radiation ionizes gases to form a region that can reflect radio waves.
The document provides information about the history and formation of Earth 4.54 billion years ago, including five mass extinction events. It discusses Earth's atmosphere, composition, layers, facts, and natural phenomena like mountains, minerals, rocks, and volcanoes. The text also covers topics like the greenhouse effect, pollution, the ozone layer, depletion issues, and indications that the Earth is nearing an end unless preventative measures are taken.
• Earth, along with the other planets, is believed to have been born 4.5 billion years ago as a solidified cloud of dust and gases left over from the creation of the Sun.
• For perhaps 500 million years, the interior of Earth stayed solid and relatively cool, perhaps 2,000°F.
• The main ingredients were iron and silicates, with small amounts of other elements, some of them radioactive.
• As millions of years passed, energy released by radioactive decay—mostly of uranium, thorium, and potassium—gradually heated Earth, melting some of its constituents.
• The iron melted before the silicates, and, being heavier, sank toward the center.
• This forced up the silicates that it found there.
• After many years, the iron reached the center, almost 4,000 mi deep, and began to accumulate. No eyes were around at that time to view the turmoil that must have taken place on the face of Earth—gigantic heaves and bubblings on the surface, exploding volcanoes, and flowing lava covering everything in sight.
• Finally, the iron in the center accumulated as the core. Around it, a thin but fairly stable crust of solid rock formed as Earth cooled.
• Depressions in the crust were natural basins in which water, rising from the interior of the planet through volcanoes and fissures, collected to form the oceans. Slowly, Earth acquired its present appearance.
The document provides information about the history and formation of Earth 4.54 billion years ago, including major extinction events. It discusses Earth's atmosphere, composition, layers, and facts such as the presence of one natural satellite, the Moon. Graphics are included showing the relative sizes and distances of planets in the solar system. The document also covers mountains, minerals, rocks, volcanoes, meteoroids, and natural phenomena such as global warming, the greenhouse effect, ozone layer depletion, and indications of threats facing Earth. Prevention methods are mentioned.
The document discusses the composition and structure of Earth's atmosphere. It is composed primarily of nitrogen and oxygen, with smaller amounts of gases like carbon dioxide, argon, and methane. The atmosphere is divided into four layers - the troposphere closest to Earth's surface where weather occurs, the stratosphere above it where ozone absorbs UV light, the mesosphere where temperatures decrease with altitude, and the thermosphere where temperatures increase with altitude. The greenhouse effect describes how certain gases in the atmosphere trap heat radiating from Earth's surface, maintaining a climate suitable for life.
The document discusses the different spheres or layers of the Earth. It begins by describing the Earth and its color compared to other planets. It then discusses the four subsystems that make up Earth and flow of matter and energy between them. It identifies the layers of the Earth and differentiates between them. Finally, it discusses natural waters and the water cycle.
This document discusses the four subsystems that make up the Earth: the atmosphere, biosphere, geosphere, and hydrosphere. It provides descriptions of each subsystem, including what they are composed of and their key characteristics. The document also presents an activity that asks students to analyze the interactions between the different subsystems using the example of the Taal Volcano eruption.
The document discusses the composition and structure of Earth's atmosphere. It describes the different layers of the atmosphere, including the troposphere, stratosphere, mesosphere, thermosphere, and exosphere. It explains how solar energy is transferred throughout the atmosphere using radiation, conduction, and convection. The document also mentions clouds and the water cycle.
The document discusses the key subsystems that make up the Earth system, including the atmosphere, hydrosphere, lithosphere, biosphere, and how they interact. It provides details on the composition and important processes of each subsystem. The atmosphere contains 78% nitrogen, 21% oxygen, and is responsible for heat redistribution and the hydrologic cycle. The hydrosphere covers 70% of the Earth as ocean water and freshwater. The lithosphere includes the crust and mantle, and plate tectonics shape the Earth's surface. The biosphere is the set of all life forms and the carbon cycle. Each subsystem interacts with the others, making life possible on Earth.
Here are the answers to your questions:
1) Heat is a form of energy that causes temperature change, while temperature is a measure of how hot or cold something is.
2) Fahrenheit measures temperature in degrees Fahrenheit (°F). Water freezes at 32°F and boils at 212°F. Celsius measures temperature in degrees Celsius (°C). Water freezes at 0°C and boils at 100°C. Kelvin measures temperature in kelvins (K) using the same increments as Celsius but water freezes at 273.15 K and boils at 373.15 K.
3) Dew point is the temperature at which water vapor in air condenses into liquid water. Condens
The document discusses the composition and structure of Earth's atmosphere. It notes that the atmosphere is a thin layer of air that forms a protective shield around Earth. It is made up of several gases, with nitrogen (78%) and oxygen (21%) being the most abundant. The atmosphere is divided into layers including the troposphere where weather occurs, the stratosphere which contains the ozone layer, and the ionosphere which reflects radio waves. The document also addresses how atmospheric gases allow life on Earth and describes phenomena like the greenhouse effect.
The document summarizes key aspects of the atmosphere and weather. It describes the main layers of the atmosphere, including the troposphere where weather occurs. It also explains that the atmosphere contains gases like nitrogen, oxygen, and water vapor. Greenhouse gases like carbon dioxide and methane trap heat in the atmosphere and contribute to the greenhouse effect. The document outlines factors that influence weather and issues like global warming from rising greenhouse gas levels.
Here are brief answers to the questions:
1. Temperature affects biological and chemical processes that are necessary to support life. Temperature must be within a certain range for liquid water and biological molecules to exist.
2. Liquid water is essential for life as we know it. It acts as a solvent and is necessary for biological and chemical reactions in living cells and organisms.
3. The atmosphere provides insulation from temperature extremes, protects from harmful radiation, provides gases like oxygen and carbon dioxide needed for life, and contributes to the greenhouse effect that helps regulate Earth's temperature.
4. Living organisms harness energy from the sun through photosynthesis or rely on chemical energy through chemosynthesis. This energy is used to power biological processes and
The document discusses the composition and evolution of Earth's atmosphere. It notes that nitrogen makes up 78% of the atmosphere, while oxygen is 21% and other gases like argon and carbon dioxide make up the remaining 1%. Earth originally had an atmosphere of hydrogen and helium that eventually escaped. Later, volcanoes released water vapor, carbon dioxide, and ammonia, forming a second atmosphere. Cyanobacteria introduced oxygen to the atmosphere between 3.3 to 2.2 billion years ago. The modern atmosphere of nitrogen and oxygen is considered the third atmosphere and has a composition influenced by biological and geological processes.
Characteristics Of The Atmoshere Q And Aaadeawscience
The document provides information about Earth's atmosphere including:
1) It describes the layers of the atmosphere from lowest to highest: troposphere, stratosphere, mesosphere, thermosphere, and exosphere.
2) It explains that the troposphere contains around 75% of the atmosphere and is where weather occurs.
3) It discusses how the stratosphere contains high levels of ozone which absorbs ultraviolet radiation from the sun.
The document discusses the four main spheres that make up the Earth's system - the geosphere, hydrosphere, biosphere, and atmosphere. It describes each sphere in detail, including what they contain and their interactions. The spheres - land, water, living things, and air - work together as a complex, interconnected system powered by both internal and external energy sources.
Earth system refers to Earth’s interacting physical, chemical, and biological processes.
The system consists of the land, oceans, atmosphere and poles.
It includes the planet’s natural cycles – the carbon, water, nitrogen, phosphorus, Sulphur and other cycles – and deep Earth processes.
Life too is an integral part of the Earth system
Reduce climate change
Ecological services generated by the living biosphere
Food production
Natural Resources
Earth is the third planet from the sun and the only known place in the universe to support life. It has liquid water, exists within the sun's habitable zone, and its atmosphere contains oxygen and protects it from radiation. Key factors that make Earth habitable include its distance from the sun, system of plate tectonics, size and protective moon. The four interacting spheres that comprise Earth's system are the atmosphere, biosphere, hydrosphere and geosphere.
1. The document discusses the four layers of Earth's atmosphere and how factors like temperature, pressure, wind, and moisture interact to cause weather.
2. It explains that the lowest layer, the troposphere, contains almost all of the atmosphere's mass and water and is where weather occurs.
3. The stratosphere contains the protective ozone layer. The thermosphere is where satellites orbit and temperatures can reach 2000 degrees Celsius.
4. Weather results from interactions of heat, air pressure, wind, and moisture. Unequal heating causes pressure differences that create wind, and wind circulations around the globe.
The document discusses the four major subsystems that make up the Earth system:
1) Geosphere - The solid portion of the Earth including the crust and lithosphere. The crust is the outermost solid layer and is composed of rocks and minerals.
2) Hydrosphere - The water on Earth, including oceans, seas, rivers, lakes, ice caps, groundwater and atmospheric water vapor.
3) Atmosphere - The envelope of air surrounding the Earth held in place by gravity.
4) Biosphere - The parts of the Earth system inhabited by life, from bacteria in the soil to trees in the forest. Together these subsystems interact as a single complex, self-regulating system known
Atmospheric Layers, Air Pressure, Weather Variablesrebelbrindley
The atmosphere is composed of several thin layers that surround the Earth. It is made up mostly of nitrogen and oxygen and protects life by trapping heat, providing breathable air, and blocking harmful radiation. Weather occurs in the lowest layer, the troposphere, where conditions vary daily. Climate describes average weather conditions over many years. Higher layers include the ozone-containing stratosphere, cooling mesosphere, and very thin thermosphere and exosphere at the top, where temperatures are extremely high despite low air density.
The document discusses the key components and layers of Earth's atmosphere. It describes how the atmosphere protects life on Earth by absorbing UV radiation, retaining heat through the greenhouse effect, and reducing temperature extremes. The main layers are the troposphere, stratosphere, mesosphere, thermosphere and exosphere, each with different properties and roles in regulating Earth's climate.
The document summarizes the four subsystems of Earth - the atmosphere, geosphere, hydrosphere, and biosphere. It describes the key characteristics of each subsystem, including their composition and interactions. Matter and energy flow between the subsystems, with the atmosphere serving as a protective blanket, the geosphere made up of Earth's solid surface, the hydrosphere encompassing all of Earth's water, and the biosphere defined as the zone in which living organisms exist.
The document discusses the four subsystems of Earth: the atmosphere, biosphere, geosphere, and hydrosphere. It provides descriptions of each subsystem and notes that they interact with one another, enabling Earth to sustain life. As an activity, students are tasked with listing terms from a passage that reflect each subsystem and arranging jumbled words related to the subsystems. The document emphasizes that the subsystems are interconnected and that human population growth and pollution threaten the planet. Students are encouraged to generate ideas for environmental protection.
This document appears to be a scavenger hunt checklist, as it contains blanks for a finder's time and date found, as well as 10 numbered lines for writing clues or locations found. The overall purpose seems to be tracking progress on solving a scavenger hunt or treasure hunt.
The document discusses different forms of energy including kinetic energy, potential energy, and chemical energy. It explains that energy can change forms through transformations but the total amount of energy stays the same. Examples are given of energy transformations, such as chemical energy in muscles changing to kinetic energy of motion when a person moves. Potential energy stored by raising an object can also change to kinetic energy if the object falls.
The Nook Color is a 7-inch Android tablet with an 8-hour battery life, 8GB internal storage plus micro SD support, Wi-Fi connectivity but no 3G or GPS. It has a 1024x600 screen resolution, weighs 15.8 ounces, and originally sold for $249 but can now be found for as little as $99.
The document outlines the Greek gods' family tree according to Hesiod's Theogony from 700 BCE. It begins with the primordial deities Chaos and includes Earth, Tartarus, Eros, Night, and Erebos. Their offspring were Sky and several personified concepts. The next generation comprised the Titans including Oceanus, Mnemosyne and Cronus. Cronus mated with Rhea and they produced the first six Olympians: Hestia, Demeter, Hera, Hades, Poseidon, and Zeus. Zeus went on to mate with several partners and father more prominent deities like Athena, Apollo, Artemis, Ares, and others. The twelve primary Olympians
The Theogony by Hesiod describes the origins and genealogies of the Greek gods. It begins by invoking the Muses, daughters of Zeus, to sing of the earliest beings - first came Chaos, then Gaia (Earth), Tartarus, Eros and others. Gaia bore Uranus (Sky) who covered her, and they produced the Titans including Kronos. Kronos overthrew his father Uranus with the help of his mother Gaia and her sickle. From Uranus' blood came Aphrodite. Night produced other offspring including Death. The poem continues recounting the origins and relationships between the major Greek divine figures.
Cells are the basic units of all living things, containing the necessary proteins, organelles and equipment to sustain life. They organize into tissues, systems and whole organisms. A cell's main purpose is to organize an organism's various parts, with each cell type performing different functions to allow organisms to grow, survive and develop complex structures like nervous systems and muscles.
This document provides a vocabulary lesson on nouns, adjectives, and verbs in Latin. It lists 6 nouns including "family", "fortune", and "earth". It also lists 4 adjectives such as "good" and "small". Finally, it presents 2 verbs like "they love/like" and "they carry".
1) The document discusses the connection between static electricity and cone-bearing trees. Cone-bearing trees secrete resin when their bark is broken, which hardens and seals wounds. This resin can fossilize over time to form amber.
2) Ancient Greeks noticed that amber could attract small bits of straw or ash when rubbed with wool or fur. They believed amber had magical properties related to this. The name they gave amber, "elektron", means "substance of the Sun".
3) By the 17th century, scientists had sparked curiosity about amber's properties. It was finally explained that amber produces static electricity when rubbed, transferring electrons between the objects.
1. Elijah McCoy developed the first automatic lubricating device in the 1870s to automatically oil train engines while running, avoiding the need to frequently stop trains to manually oil parts.
2. Modern automobiles have oil pumps that automatically circulate engine oil, allowing cars to travel long distances without stopping.
3. The document discusses how McCoy's invention helped connect train schedules to oil pumps by enabling trains to stay on schedule without frequent stops for oiling, paving the way for modern automatic lubrication systems in vehicles.
1. A 1600 Italian cobbler discovered a rock that glowed in the dark, leading to the discovery of fluorescent and phosphorescent substances that emit light when exposed to certain forms of energy.
2. In the 1850s, a scientist realized the fluorescent properties of substances could be used to create a new type of lighting, creating the first fluorescent light bulb by placing a fluorescent material inside a glass tube with an electric current.
3. Today, fluorescent light bulbs are widely used in places like offices, schools, and factories.
This document provides a vocabulary lesson on basic Latin words including nouns for water, island, forest, and road. It also lists verbs for "is" and "are" as well as the adverb for "not" and conjunctions for "and" and "but".
The Phoenicians were merchants and traders from an ancient civilization located in what is now Lebanon. They produced a purple-red dye and colonized areas throughout the Mediterranean for trade, including Syria, Cyprus, Libya, Tunisia, Italy, Algeria, Morocco and Spain. The Phoenicians developed one of the first alphabets, consisting of 22 letters, which was adopted in Babylon by the 15th century BCE and formed the basis for many modern scripts.
This document provides information about the connections between beverages, bottles, cans, and wildlife. It discusses:
1) How containers for beverages have evolved from clay jars and animal skins to glass bottles to metal cans. Cans became popular because they were stackable, non-breakable, and cooled drinks quickly.
2) The plastic six-pack yoke was invented to bind cans together for transport but unfortunately also bound and entangled thousands of birds, fish, and marine animals when released into the environment.
3) Today animals are still being harmed and sometimes killed by discarded plastic six-pack yokes and other plastic waste in the environment.
Protists and animals share some characteristics. Protists are classified into three main groups - plantlike, animal-like, and funguslike - based on their traits. Plantlike protists, called algae, contain chlorophyll and can photosynthesize. They include diverse organisms like diatoms, dinoflagellates, euglenoids, red algae, green algae, and brown algae. Algae are a primary food source in aquatic ecosystems and are important in producing oxygen.
The document summarizes how scientific methods were used to solve a problem at a veterinary clinic.
1) A veterinary technician noticed that two cats boarding at the clinic were scratching and developing skin sores. She wanted to determine what was causing the irritation.
2) She gathered information by observing the cats' behavior and contacting their owner. She formed a hypothesis that something in the cats' litter was irritating their skin.
3) She tested her hypothesis by conducting an experiment where she gave one cat litter with deodorant (the control) and the other litter without deodorant (the experimental). She analyzed the data and found the experimental cat's sores healed while the control cat's
Bulls played an important religious and symbolic role in Minoan culture. They are prominently depicted in Minoan art, especially at Knossos. One famous Minoan ritual possibly depicted is bull-leaping, where athletes demonstrate skill by vaulting and somersaulting over charging bulls. While some scholars doubt bull-leaping occurred, evidence from later French bull sports and Minoan art suggest it was a real ritual, though its purpose and meaning are still debated among scholars.
The document provides information on the Greek alphabet including:
1) A chart listing each letter of the Greek alphabet, its English name, and an example English word to demonstrate its pronunciation.
2) Additional details on diphthongs, breathing marks, accents, punctuation, syllables, and other diacritical marks used in Greek.
3) A link to practice the Greek alphabet online.
The document lists several ancient Mesopotamian civilizations including the Sumerians from 3500-1800 BCE, Akkadians from 2340-2125 BCE, Babylonians from 2300-538 BCE, Assyrians from 1170-612 BCE, Phoenicians from 1500-332 BCE, and Palestinians from 1170-612 BCE.
(1) Hesiod addresses the Muses and asks them to tell of Zeus and his power over mankind. He warns his brother Perses to avoid strife and work hard to store up food, rather than quarrel and listen to arguments in court.
(2) Zeus created Pandora to plague mankind as punishment for Prometheus stealing fire. He had Hephaestus craft her form and other gods endowed her with talents to deceive men. When Epimetheus accepted this "gift" from Zeus, it unleashed sickness and hardship upon humanity.
(3) Hesiod concludes by urging leaders to practice just rule, as the gods watch for injustice, and will punish whole cities for the sins
The Code of Hammurabi was carved on an eight foot tall black diorite monument that was found in 1901 in the Persian Mountains and is currently located in the Louvre Museum in Paris. It begins and ends with addresses to gods and contains laws numbered 1-282, though some sections are missing.
1. UNIT
4 Earth’s Air and Water
How Are
Air & Advertising
Connected?
278
2. I n the late 1800s, two scientists were studying
the composition of air when they discovered an
element that hadn’t been known before. They
named it “neon,” and soon this new element, rep-
resented by the chemical symbol Ne, had been
assigned a spot in the periodic table (right). It
took a few years for people to figure out some-
thing useful to do with neon! In 1910, a French
engineer experimented with passing an electrical
current through neon gas in a vacuum tube. The
result was a spectacular orange-red light. Neon’s
advertising possibilities were quickly realized, and
soon the first neon sign blazed on a boulevard in
Paris. Today, neon signs in a wide range of colors
advertise shops and services all over the world.
The other colors are made by mixing neon with
other gases and by using tinted tubes.
SCIENCE CONNECTION
NOBLE GASES Neon is one of six elements known as the noble gases. These
gases make up a tiny fraction of the atmosphere. Conduct research to find out
more about this group. What other gases belong to the group? What do they
all have in common? Why are they called “noble”? Create a chart that shows
when each of the noble gases was discovered and what distinctive characteris-
tics and uses it has.
3. 10 Atmosphere
W
hy is it difficult to breathe
at high elevations? Why
are some mountain peaks
permanently covered with snow?
These mountain climbers aren’t sup-
plementing oxygen just because the
activity is physically demanding. At
elevations like this, the amount of
oxygen available in the air is so small
that the climbers’ bodily functions
might not be supported. In this chap-
ter, you’ll learn about the composi-
tion and structure of the atmosphere.
You also will learn how energy is
transferred in the atmosphere. In
addition, you’ll examine the water
cycle and major wind systems.
What do you think?
Science Journal Look at the picture
below with a classmate. Discuss what
this might be. Here’s a hint: It “pops”
in thin air. Write your answer or best
guess in your Science Journal.
280
4. EXPLORE T
he air around you is made of billions of molecules.
These molecules are constantly moving in all
ACTIVITY directions and bouncing into every object in the room,
including you. Air pressure is the result of the billions
of collisions of molecules into these objects. Because
you usually do not feel molecules in air hitting you, do the activity below to
see the effect of air pressure.
Observe air pressure
1. Cut out a square of cardboard about
10 cm on a side from a cereal box.
2. Fill a glass to the brim with water.
3. Hold the cardboard firmly over the
top of the glass, covering the water,
and invert the glass.
4. Slowly remove your hand holding the
cardboard in place and observe.
Observe
Write a paragraph in your Science Journal describing what happened to the
cardboard when you inverted the glass and removed your hand. How does air
pressure explain what happened?
FOLDABLES
Reading &Study
& Study Making a Sequence Study Fold Make the following Foldable
Skills
to help you visualize the layers of Earth’s atmosphere.
1. Stack three sheets of paper in front of you so the short Exosphere
sides are at the top. Thermosphere
Mesosphere
2. Slide the top sheet up so that about four centimeters of Stratosphere
the middle sheet show. Slide the middle sheet up so Troposphere
that about four centimeters of the bottom sheet show. Earth's
3. Fold the sheets top to bottom to form six tabs and sta- Atmosphere
ple along the topfold. Turn the Foldable so the staples
are at the bottom.
4. Label the flaps Earth’s Atmosphere, Troposphere, Stratosphere, Mesosphere,
Thermosphere, and Exosphere, as shown.
5. As you read the chapter, write information about each layer of Earth’s atmosphere under the tabs.
281
5. SECTION
Earth’s Atmosphere
Importance of the Atmosphere
Earth’s atmosphere, shown in Figure 1, is a thin layer of air
s Identify the gases in Earth’s that forms a protective covering around the planet. If Earth had
atmosphere. no atmosphere, days would be extremely hot and nights would
s Describe the structure of Earth’s be extremely cold. Earth’s atmosphere maintains a balance
atmosphere. between the amount of heat absorbed from the Sun and the
s Explain what causes air pressure.
amount of heat that escapes back into space. It also protects life-
Vocabulary forms from some of the Sun’s harmful rays.
atmosphere ozone layer
troposphere ultraviolet radiation
ionosphere chlorofluorocarbon Makeup of the Atmosphere
Earth’s atmosphere is a mixture of gases, solids, and liquids
that surround the planet. It extends from Earth’s surface to
The atmosphere makes life on Earth
possible.
outer space. The atmosphere is much different today from what
it was when Earth was young.
Figure 1 Earth’s early atmosphere, produced by erupting volcanoes,
Earth’s atmosphere, as viewed contained nitrogen and carbon dioxide, but little oxygen. Then,
from space, is a thin layer of more than 2 billon years ago, Earth’s early organisms released
gases. The atmosphere keeps oxygen into the atmosphere as they made food with the aid of
Earth’s temperature in a range sunlight. These early organisms, however, were limited to layers
that can support life. of ocean water deep enough to be shielded from the Sun’s
harmful rays, yet close
enough to the surface to
receive sunlight. Eventu-
ally, a layer rich in ozone
(O3) that protects Earth
from the Sun’s harmful
rays formed in the upper
atmosphere. This protec-
tive layer eventually
allowed green plants to
flourish all over Earth,
releasing even more oxy-
gen. Today, a variety of
life forms, including you,
depends on a certain
amount of oxygen in
Earth’s atmosphere.
282 CHAPTER 10 Atmosphere
6. Gases in the Atmosphere Today’s
atmosphere is a mixture of the gases Argon
(0.93%)–
shown in Figure 2. Nitrogen is the most
Carbon
abundant gas, making up 78 percent of the dioxide–
atmosphere. Oxygen actually makes up (0.03%) 21% 78%
only 21 percent of Earth’s atmosphere. As Oxygen Nitrogen
Neon–
much as four percent of the atmosphere is
Helium–
water vapor. Other gases that make up Methane–
Earth’s atmosphere include argon and car- Krypton– – Trace 1%
bon dioxide. Xenon –
Hydrogen–
The composition of the atmosphere is
Ozone–
changing in small but important ways. For
example, car exhaust emits gases into the
air. These pollutants mix with oxygen and other chemicals in the Figure 2
presence of sunlight and form a brown haze called smog. This graph shows the percent-
Humans burn fuel for energy. As fuel is burned, carbon dioxide ages of the gases, excluding
is released as a by-product into Earth’s atmosphere. Increasing water vapor, that make up
energy use may increase the amount of carbon dioxide in the Earth’s atmosphere.
atmosphere.
Solids and Liquids in Earth’s Atmosphere In addition
to gases, Earth’s atmosphere contains small, solid particles such
as dust, salt, and pollen. Dust particles get into the atmosphere
when wind picks them up off the ground and carries them
along. Salt is picked up from ocean spray. Plants give off pollen
that becomes mixed throughout part of the atmosphere.
The atmosphere also contains small liquid droplets other
than water droplets in clouds. The atmosphere constantly moves Figure 3
these liquid droplets and solids from one region to another. For Solids and liquids can travel large
example, the atmosphere above you may contain liquid droplets distances in Earth’s atmosphere,
and solids from an erupting volcano thousands of kilometers affecting regions far from their
from your home, as illustrated in Figure 3. source.
On June 12, 1991, Mount Pinatubo in
the Philippines erupted, causing liquid
droplets to form in Earth’s atmosphere.
Droplets of sulfuric acid from volcanoes
can produce spectacular sunrises.
SECTION 1 Earth’s Atmosphere 283
7. Layers of the Atmosphere
What would happen if you left a glass of chocolate milk on
the kitchen counter for a while? Eventually, you would see a
lower layer with more chocolate separating from upper layers
with less chocolate. Like a glass of chocolate milk, Earth’s atmo-
sphere has layers. There are five layers in Earth’s atmosphere,
each with its own properties, as shown in Figure 4. The lower
Research Visit the layers include the troposphere and stratosphere. The upper
Glencoe Science Web site at atmospheric layers are the mesosphere, thermosphere, and exo-
science.glencoe.com sphere. The troposphere and stratosphere contain most of the air.
for more information about
layers of Earth’s atmosphere. Lower Layers of the Atmosphere You study, eat, sleep,
Communicate to your class and play in the troposphere, which is the lowest of Earth’s
what you learn. atmospheric layers. It contains 99 percent of the water vapor
and 75 percent of the atmospheric gases. Rain, snow, and clouds
occur in the troposphere, which extends up to about 10 km.
The stratosphere, the layer directly above the troposphere,
extends from 10 km above Earth’s surface to about 50 km. As
Figure 4 shows, a portion of the stratosphere contains higher
levels of a gas called ozone. Each molecule of ozone is made up
of three oxygen atoms bonded together. Later in this section you
will learn how ozone protects Earth from the Sun’s harmful rays.
Figure 4 Satellite Exosphere
Earth’s atmosphere is divided 500 km
into five layers. Which layer of the
atmosphere do you live in?
Space shuttle
Meteor trails
Thermosphere
85 km
Mesosphere
50 km
Ozone layer Stratosphere
Jet 10 km
Troposphere
284 Earth
8. Figure 5
During the day, the ionosphere
Day Night
absorbs radio transmissions. This
prevents you from hearing
distant radio stations. At night,
the ionosphere reflects radio
AM radio transmitter Radio waves waves. The reflected waves can
travel to distant cities.
Receiving antenna
ere
Ionosph
Boise
New Jersey
Upper Layers of the Atmosphere Beyond the strato-
sphere are the mesosphere, thermosphere, and exosphere. The
mesosphere extends from the top of the stratosphere to about
85 km above Earth. If you’ve ever seen a shooting star, you Figure 6
might have witnessed a meteor in the mesosphere. Wings help move aircraft in lower
The thermosphere is named for its high temperatures. This layers of the atmosphere. The
is the thickest atmospheric layer and is found between 85 km space shuttle can’t use its wings
and 500 km above Earth’s surface. to maneuver in the exosphere
Within the mesosphere and thermosphere is a layer of elec- because so few molecules are
trically charged particles called the ionosphere (i AHN uh sfir). present.
If you live in New Jersey and listen to the radio at night, you
might pick up a station from Boise, Idaho. The ionosphere
allows radio waves to travel across the country to another city, as
shown in Figure 5. During the day, energy from the Sun inter-
acts with the particles in the ionosphere, causing them to absorb
AM radio frequencies. At night, without solar energy, AM radio
transmissions reflect off the ionosphere, allowing radio trans-
missions to be received at greater distances.
The space shuttle in Figure 6 orbits Earth in the exosphere.
In contrast to the troposphere, the layer you live in, the exo-
sphere has so few molecules that the wings of the shuttle are
useless. In the exosphere, the spacecraft relies on bursts from
small rocket thrusters to move around. Beyond the exosphere is
outer space.
How does the space shuttle maneuver in the
exosphere?
SECTION 1 Earth’s Atmosphere 285
9. Atmospheric Pressure
Imagine you’re a football player running with
the ball. Six players tackle you and pile one on top
of the other. Who feels the weight more—you or
the player on top? Like molecules anywhere else,
atmospheric gases have mass. Atmospheric gases
extend hundreds of kilometers above Earth’s sur-
face. As Earth’s gravity pulls the gases toward its
surface, the weight of these gases presses down on
the air below. As a result, the molecules nearer
Earth’s surface are closer together. This dense air
exerts more force than the less dense air near the
top of the atmosphere. Force exerted on an area is
known as pressure.
Like the pile of football players, air pressure is
greater near Earth’s surface and decreases higher
in the atmosphere, as shown in Figure 7. People
find it difficult to breathe in high mountains
Figure 7 because fewer molecules of air exist there. Jets that fly in the
Air pressure decreases as you go stratosphere must maintain pressurized cabins so that people
higher in Earth’s atmosphere. can breathe.
Where is air pressure greater—in the
exosphere or in the troposphere?
Problem-Solving Activity
How does altitude affect air pressure?
tmospheric gases extend hundreds of
A kilometers above Earth’s surface, but the
molecules that make up these gases are
Air Pressure Changes with Altitude
1000
Pressure (millibars)
800
fewer and fewer in number as you go higher.
This means that air pressure decreases with 600
altitude. 400
Identifying the Problem 200
The graph on the right shows these 0
10 20 30 40 50
changes in air pressure. Note that altitude Altitude (km)
on the graph goes up only to 50 km. The
troposphere and the stratosphere are repre- Solving the Problem
sented on the graph, but other layers of the 1. Estimate the air pressure at an altitude of
atmosphere are not. By examining the 5 km.
graph, can you understand the relationship 2. Does air pressure change more quickly at
between altitude and pressure? higher altitudes or at lower altitudes?
286 CHAPTER 10 Atmosphere
10. Temperature in Atmospheric Layers
The Sun is the source of most of the energy on Earth. Before
it reaches Earth’s surface, energy from the Sun must pass
through the atmosphere. Because some layers contain gases that
Determining if air
easily absorb the Sun’s energy while other layers do not, the vari-
has mass
ous layers have different temperatures, illustrated by the red line
in Figure 8. Procedure
1. On a pan balance, find the
Molecules that make up air in the troposphere are warmed mass of an inflatable ball
mostly by heat from Earth’s surface. The Sun warms Earth’s sur- that is completely deflated.
face, which then warms the air above it. When you climb a 2. Hypothesize about the
mountain, the air at the top is usually cooler than the air at the change in the mass of the
bottom. Every kilometer you climb, the air temperature ball when it is inflated.
decreases about 6.5°C. 3. Inflate the ball to its
maximum recommended
Molecules of ozone in the stratosphere absorb some of the
inflation pressure.
Sun’s energy. Energy absorbed by ozone molecules raises the 4. Determine the mass of the
temperature. Because more ozone molecules are in the upper fully inflated ball.
portion of the stratosphere, the temperature in this layer rises Analysis
with increasing altitude. 1. What change occurs in the
Like the troposphere, the temperature in the mesosphere mass of the ball when it is
decreases with altitude. The thermosphere and exosphere are inflated?
the first layers to receive the Sun’s rays. Few molecules are in 2. Infer from your data
these layers, but each molecule has a great deal of energy. Tem- whether air has mass.
peratures here are high.
Temperature of the Atmosphere at Various Altitudes
Exosphere
500
Figure 8 Thermosphere
120 The division of the atmosphere
110
into layers is based mainly on dif-
ferences in temperature. Does the
100 temperature increase or decrease
90 with altitude in the mesosphere?
Altitude (km)
80 Mesosphere
70
60
50
Stratosphere
40
Highest concentration of ozone
30
20
10
Troposphere
0
-100 -80 -60 -40 -20 0 20 400 600 800
Temperature (ºC)
SECTION 1 Earth’s Atmosphere 287
11. The Ozone Layer
Within the stratosphere, about 19 km to 48 km above your
Algae are organisms that head, lies an atmospheric layer called the ozone layer. Ozone is
use sunlight to make their made of oxygen. Although you cannot see the ozone layer, your
own food. This process life depends on it.
releases oxygen to Earth’s The oxygen you breathe has two atoms per molecule, but an
atmosphere. Some scien- ozone molecule is made up of three oxygen atoms bound
tists suggest that growth is together. The ozone layer contains a high concentration of
reduced when algae are
exposed to ultraviolet ozone and shields you from the Sun’s harmful energy. Ozone
radiation. Infer what might absorbs most of the ultraviolet radiation that enters the atmo-
happen to the oxygen level sphere. Ultraviolet radiation is one of the many types of energy
of the atmosphere if that come to Earth from the Sun. Too much exposure to ultravi-
increased ultraviolet radia- olet radiation can damage your skin and cause cancer.
tion damages some algae.
CFCs Evidence exists that some air pollutants are destroying the
ozone layer. Blame has fallen on chlorofluorocarbons (CFCs),
chemical compounds used in some refrigerators, air conditioners,
and aerosol sprays, and in the production of some foam packaging.
CFCs can enter the atmosphere if these appliances leak or if they
and other products containing CFCs are improperly discarded.
Recall that an ozone molecule is made of three oxygen atoms
bonded together. Chlorofluorocarbon molecules, shown in
Figure 9, destroy ozone. When a chlorine atom from a
chlorofluorocarbon molecule comes near a molecule of ozone, the
ozone molecule breaks apart. One of the oxygen atoms combines
with the chlorine atom, and the rest form a regular, two-atom
molecule. These compounds don’t absorb ultraviolet radiation
the way ozone can. In addition, the original chlorine atom can
continue to break apart thousands of ozone molecules. The
result is that more ultraviolet radiation reaches Earth’s surface.
A. B. C.
Ultraviolet light Cl Cl O
breaks up CFC O O O
UV
molecule. light O
O The chlorine atom joins
Cl A released with an oxygen atom,
F chlorine atom breaks leaving behind a
Cl Cl up ozone (O3) molecule. molecule of oxygen (O2).
C
Figure 9 D. E. F.
Chlorofluorocarbon (CFC) mole- O Cl
cules were used in refrigerators O O
Cl O O
and air conditioners. Each CFC O
Released O
molecule has three chlorine A free oxygen Oxygen atoms chlorine atom
atoms. One atom of chlorine can atom breaks the rejoin to form a normal breaks up another
destroy approximately 100,000 chlorine-oxygen bond. oxygen (O2) molecule. ozone (O3) molecule.
ozone molecules.
288 CHAPTER 10 Atmosphere
12. October 1980 October 1988 October 1990 September 1999
Ozone Holes Each year, more Figure 10
than 1.3 million Americans develop These images of Antarctica were
skin cancer, and more than 9,500 die produced using data from a NASA
from it. Exposure to ultraviolet radiation can cause skin cancer. If satellite. The purple color shows
the ozone layer disappeared, skin cancer rates might increase. In how the ozone hole has grown
1986, scientists found areas in the stratosphere with extremely bigger over time.
low amounts of ozone. One large hole was found over Antarc-
tica. A smaller hole was discovered over the north pole. Figure 10
shows how the ozone layer has thinned and developed holes.
In the mid 1990s, many governments banned the produc-
tion and use of CFCs. Perhaps over time, the areas where the
ozone layer is thinning will recover.
Section Assessment
1. Earth’s early atmosphere had little oxygen.
How did oxygen come to make up 21 per-
6. Interpreting Scientific Illustrations Using
cent of Earth’s present atmosphere?
Figure 2, determine the total percentage of
2. List the layers of the atmosphere in order nitrogen and oxygen in the atmosphere. What
beginning at Earth’s surface. is the total percentage of argon and carbon
3. While hiking in the mountains, you notice dioxide? For more help, refer to the Science
that it is harder to breathe as you climb Skill Handbook.
higher. Explain why this is so. 7. Communicating The names of the atmo-
4. What are some effects from a thinning spheric layers end with the suffix -sphere a word
ozone layer? that means “ball.” Use a dictionary to find out
5. Think Critically During the day, the radio what tropo-, meso-, thermo-, and exo- mean.
only receives AM stations from a city near In your Science Journal, write the meaning of
you. At night, you are able to listen to an these prefixes and explain if the layers are
AM radio station from a distant city. appropriately named. For more help, refer to
Explain why this is possible. the Science Skill Handbook.
SECTION 1 Earth’s Atmosphere 289
13. Evaluating Sunscreens
W ithout protection, sun exposure can dam-
age your health. Sunscreens protect your
skin from ultraviolet radiation. In this activity, you
will draw inferences using the labels of different
sunscreens.
What You’ll Investigate
How effective are various brands of sunscreens?
Materials
variety of sunscreens of different brand names
Goals Sunscreen Assessment
s Draw inferences based on labels on sun-
Brand Name
screen brands.
SPF
s Compare the effectiveness of different sun-
screen brands for protection against the Sun. Cost per Milliliter
s Compare the cost of several sunscreen brands. Misleading Terms
Safety Precautions
Conclude and Apply
1. Explain why you need to use sunscreen.
Procedure 2. A minimum of SPF 15 is considered adequate
protection for a sunscreen. Sunscreens with
1. Make a data table in your Science Journal
an SPF greater than 30 are considered by
using the following terms: brand name, SPF,
government guidelines to be misleading
misleading terms, and cost per milliliter.
because sunscreens will wash or wear off.
2. The Sun Protection Factor (SPF) tells you how Evaluate the SPF of each brand of sunscreen.
long the sunscreen will protect you. For exam-
3. Considering the cost and effectiveness of all
ple, an SPF of 4 allows you to stay in the Sun
the sunscreen brands, discuss which brand
four times longer than if you did not use sun-
you consider to be the best buy.
screen. Record the SPF of each sunscreen on
your data table.
3. Calculate the cost per milliliter of each sun-
screen brand.
4. Government guidelines say that terms like Create a poster on the proper use of sun-
sunblock and waterproof are misleading screens, and provide guidelines for selecting
because sunscreens cannot block the Sun, and the safest product. For more help, refer to
they wash off in water. List the misleading the Science Skill Handbook.
terms in your data table for each brand.
290 CHAPTER 10 Atmosphere
14. SECTION
Energy Transfer
in the Atmosphere
Energy from the Sun
The Sun provides most of the energy on Earth. This energy
drives winds and ocean currents and allows plants to grow and s Describe what happens to the
produce food, providing nutrition for many animals. When energy Earth receives from the
Earth receives energy from the Sun, three different things can Sun.
s Compare and contrast radiation,
happen to that energy, as shown in Figure 11. Some energy is
conduction, and convection.
reflected back into space by clouds, atmospheric particles, and s Explain the water cycle.
Earth’s surface. Some is absorbed by the atmosphere. The rest is
absorbed by land and water on Earth’s surface. Vocabulary
radiation hydrosphere
conduction condensation
Heat convection
Heat is energy that flows from an object with a higher tem-
perature to an object with a lower temperature. Energy from the
Sun reaches Earth’s surface and heats objects such as roads, The Sun provides energy to Earth’s
atmosphere, allowing life to exist.
rocks, and water. Heat then is transferred through the atmo-
sphere in three ways—radiation, conduction, and convection, as
shown in Figure 12.
Figure 11
6% reflected by The Sun is the source of energy
the atmosphere for Earth’s atmosphere. Thirty-
five percent of incoming solar
radiation is reflected back into
space. How much is absorbed by
Earth’s surface and atmosphere?
25% reflected
from clouds 15% absorbed
by the
atmosphere
4% reflected from
Earth’s surface
50% directly or indirectly
absorbed by Earth’s surface
291
15. Radiation warms
the surface.
Cooler air pushes
warm air upward,
The air near creating a
Earth's surface convection current.
is heated by
conduction.
Figure 12 Radiation Sitting on the beach, you feel the Sun’s warmth on
Heat is transferred within Earth’s your face. How can you feel the Sun’s heat even though you
atmosphere by radiation, con- aren’t in direct contact with it? Energy from the Sun reaches
duction, and convection. Earth in the form of radiant energy, or radiation. Radiation is
energy that is transferred in the form of rays or waves. Earth
radiates some of the energy it absorbs from the Sun back toward
space. Radiant energy from the Sun warms your face.
How does the Sun warm your skin?
Conduction If you walk barefoot on a hot beach, your feet
heat up because of conduction. Conduction is the transfer of
energy that occurs when molecules bump into one another.
Specific heat is the amount
Molecules are always in motion, but molecules in warmer
of heat required to change
the temperature of a sub- objects move faster than molecules in cooler objects. When
stance one degree. Sub- objects are in contact, energy is transferred from warmer objects
stances with high specific to cooler objects.
heat absorb a lot of heat for Radiation from the Sun heated the beach sand, but direct
a small increase in temper- contact with the sand warmed your feet. In a similar way, Earth’s
ature. Land warms faster surface conducts energy directly to the atmosphere. As air
than water does. Infer
whether soil or water has a moves over warm land or water, molecules in air are heated by
higher specific heat value. direct contact.
Convection After the atmosphere is warmed by radiation or
conduction, the heat is transferred by a third process called con-
vection. Convection is the transfer of heat by the flow of mate-
rial. Convection circulates heat throughout the atmosphere.
How does this happen?
292 CHAPTER 10 Atmosphere
16. When air is warmed, the molecules in it move apart and the
air becomes less dense. Air pressure decreases because fewer
molecules are in the same space. In cold air, molecules move
closer together. The air becomes more dense and air pressure
increases. Cooler, denser air sinks while warmer, less dense air
rises, forming a convection current. As Figure 12 shows, radia- Modeling Heat
tion, conduction, and convection together distribute the Sun’s Transfer
heat throughout Earth’s atmosphere. Procedure
1. Cover the outside of an
empty soup can with black
The Water Cycle construction paper.
Hydrosphere is a term that describes all the water on Earth’s 2. Fill the can with cold water
surface. Water moves constantly between the atmosphere and and feel it with your fingers.
the hydrosphere in the water cycle, shown in Figure 13. 3. Place the can in sunlight for
1 h then pour the water
If you watch a puddle in the Sun, you’ll notice that over time over your fingers.
the puddle gets smaller and smaller. Energy from the Sun causes
Analysis
the water in the puddle to change from a liquid to a gas by a
1. Does the water in the can
process called evaporation. Water that evaporates from lakes, feel warmer or cooler after
streams, and oceans enters Earth’s atmosphere. placing the can in sunlight?
If water vapor in the atmosphere cools enough, it changes 2. What types of heat transfer
back into a liquid. This process of water vapor changing to a liq- did you model?
uid is called condensation.
Clouds form when condensation occurs high in the atmo-
sphere. Clouds are made up of tiny water droplets that can col- Figure 13
lide to form larger drops. As the drops grow, they fall to Earth as In the water cycle, water moves
precipitation, which completes the cycle by returning water to from Earth to the atmosphere
the hydrosphere. and back to Earth again.
Precipitation
Condensation
Evaporation
Runoff
SECTION 2 Energy Transfer in the Atmosphere 293
17. Sunlight Earth’s
Sunlight t
Atmosphere
Hea
Sunlight is Unique
On Earth, radiation
at
Sunlight
He
from the Sun can be
reflected into space, ab-
t
Hea
Heat
sorbed by the atmo-
Earth's sphere, or absorbed by
atmosphere land and water. Once it
is absorbed, heat can
be transferred by radi-
Figure 14 ation, conduction, or convection. Earth’s atmosphere, shown in
Earth’s atmosphere creates Figure 14, helps control how much of the Sun’s radiation is
a delicate balance between absorbed or lost.
energy received and energy lost.
What helps control how much of the Sun’s
radiation is absorbed on Earth?
Why doesn’t life exist on Mars or Venus? Mars is a cold, life-
less world because its atmosphere is too thin to support life or to
hold much of the Sun’s heat. Temperatures on the surface of
Mars range from 35°C to –170°C. On the other hand, gases in
Venus’s dense atmosphere trap heat coming from the Sun. The
temperature on the surface of Venus is 470°C. Living things
would burn instantly if they were placed on Venus’s surface. Life
on Earth exists because the atmosphere holds just the right
amount of the Sun’s energy.
Section Assessment
1. How does the Sun transfer energy to Earth?
2. How is Earth’s atmosphere different from 6. Concept Mapping Make a concept map that
the atmosphere on Mars? explains what happens to radiant energy that
3. How is heat transferred from the stove to reaches Earth. For more help, refer to the
the water when you boil a pot of water? Science Skill Handbook.
4. Briefly describe the steps included in the 7. Solving One-Step Equations Earth is about
water cycle. 150 million km from the Sun. The radiation
5. Think Critically What would happen to coming from the Sun travels at 300,000 km/s.
temperatures on Earth if the Sun’s heat How long does it take for radiation from the Sun
were not distributed throughout the to reach Earth? For more help, refer to the
atmosphere? Math Skill Handbook.
294 CHAPTER 10 Atmosphere
18. SECTION
Air Movement
Forming Wind
Uneven heating of Earth’s surface by the Sun causes some
areas to be warmer than others. Recall from Section 2 that s Explain why different latitudes on
warmer air expands, becoming less dense than colder air. This Earth receive different amounts of
causes air pressure to be generally lower where air is heated. solar energy.
s Describe the Coriolis effect.
Wind is the movement of air from an area of higher pressure to
s Locate doldrums, trade winds,
an area of lower pressure. prevailing westerlies, polar easter-
lies, and jet streams.
Heated Air Areas of Earth receive different amounts of radia-
tion from the Sun because Earth is curved. Figure 15 illustrates Vocabulary
Coriolis effect sea breeze
why the equator receives more radiation than areas to the north jet stream land breeze
or south. The heated air at the equator is less dense, so it is dis-
placed by denser, colder air, creating convection currents.
This cold, denser air comes from the poles, which receive less Wind systems determine major
radiation from the Sun, making air at the poles much cooler. The weather patterns on Earth.
resulting dense, high-pressure air sinks and moves along Earth’s
surface. However, dense air sinking as less-dense air rises does
not explain everything about wind.
Figure 15
Because of Earth’s curved surface, the Sun’s
rays strike the equator more directly than Near the poles,
North Pole
areas toward the north or south poles. the Sun's energy
strikes Earth at an angle, spreading
Suns Rays out the energy received over a larger
area than near the equator.
Suns Rays
Equator
Each square meter of
Suns Rays area at the equator
receives more energy from the Sun than
each square meter at the poles does.
South Pole
SECTION 3 Air Movement 295
19. Figure 16 N
The Coriolis effect causes moving
air to turn to the right in the
northern hemisphere and to the
left in the southern hemisphere.
Equ
ator
Actual path of wind
Path of wind
without Coriolis
effect
S
The Coriolis Effect What would happen if you threw a ball
to someone sitting directly across from you on a moving merry-
go-round? Would the ball go to your friend? By the time the ball
got to the opposite side, your friend would have moved and the
ball would appear to have curved.
Like the merry-go-round, the rotation of Earth causes mov-
ing air and water to appear to turn to the right north of the
equator and to the left south of the equator. This is called the
Coriolis (kohr ee OH lus) effect. It is illustrated in Figure 16.
The flow of air caused by differences in the amount of solar
radiation received on Earth’s surface and by the Coriolis effect
creates distinct wind patterns on Earth’s surface. These wind
systems not only influence the weather, they also determine
when and where ships and planes travel most efficiently.
Global Winds
How did Christopher Columbus get from Spain to the
Americas? The Nina, the Pinta, and the Santa Maria had no
Research Visit the
source of power other than the wind in their sails. Early sailors
Glencoe Science Web site at
discovered that the wind patterns on Earth helped them navi-
science.glencoe.com to
gate the oceans. These wind systems are shown in Figure 17.
learn more about global
Sometimes sailors found little or no wind to move their sail-
winds. Communicate to your
ing ships near the equator. It also rained nearly every afternoon.
class what you’ve learned.
This windless, rainy zone near the equator is called the dol-
drums. Look again at Figure 17. Near the equator, the Sun heats
the air and causes it to rise, creating low pressure and little wind.
The rising air then cools, causing rain.
What are the doldrums?
296 CHAPTER 10 Atmosphere
20. VISUALIZING
GLOBAL WINDS
Figure 17
he Sun’s uneven heating of Earth’s surface
T forms giant loops, or cells, of moving air.
The Coriolis effect deflects the surface winds
to the west or east, setting up belts of prevailing
winds that distribute heat and moisture around A WESTERLIES Near 30 ° north and south
the globe. latitude, Earth’s rotation deflects air from west
to east as air moves toward the polar regions.
In the United States, the westerlies move
weather systems, such as this one along the
Oklahoma-Texas border, from west to east.
60° N
Polar easterlies
Westerlies
30° N
Trade winds
B DOLDRUMS Along the
equator, heating causes air to
expand, creating a zone of low 0° Equatorial doldrums
pressure. Cloudy, rainy weather,
as shown here, develops almost
every afternoon.
Trade winds
30° S
Westerlies
C TRADE WINDS
Air warmed near 60°S
the equator travels Polar easterlies
toward the poles
but gradually cools
and sinks. As the air
flows back toward D POLAR EASTERLIES
the low pressure In the polar regions,
of the doldrums, cold, dense air sinks
the Coriolis effect and moves away from
deflects the surface wind to the west. Early sailors, the poles. Earth’s rota-
in ships like the one above, relied on these winds tion deflects this wind
to navigate global trade routes. from east to west.
SECTION 3 Air Movement 297
21. Surface Winds Air descending to Earth’s surface near 30°
north and south latitude creates steady winds that blow in tropi-
cal regions. These are called trade winds because early sailors
used their dependability to establish trade routes.
Between 30° and 60° latitude, winds called the prevailing
westerlies blow in the opposite direction from the trade winds.
Prevailing westerlies are responsible for much of the movement
of weather across North America.
Polar easterlies are found near the poles. Near the north
pole, easterlies blow from northeast to southwest. Near the
south pole, polar easterlies blow from the southeast to the
northwest.
Winds in the Upper Troposphere Narrow belts of strong
winds, called jet streams, blow near the top of the troposphere.
The polar jet stream forms at the boundary of cold, dry polar air
to the north and warmer, more moist tropical air to the south,
as shown in Figure 18. The jet stream moves faster in the winter
because the difference between cold air and warm air is greater.
The jet stream helps move storms across the country.
Jet pilots take advantage of the jet streams. When flying east-
ward, planes save time and fuel. Going west, planes fly at differ-
Figure 18 ent altitudes to avoid the jet streams.
A strong current of air, called the
jet stream, forms between cold,
polar air and warm, tropical air.
Local Wind Systems
Global wind systems determine the major weather patterns
Flying from Boston to Seattle for the entire planet. Smaller wind systems affect local weather.
may take 30 min longer than fly- If you live near a large body of water, you’re familiar with two
ing from Seattle to Boston. such wind systems—sea breezes and land breezes.
Cold air
Polar je
t stream
The polar jet stream Warm air
in North America usually is
found between 10 km and
15 km above Earth’s surface.
298 CHAPTER 10 Atmosphere
22. Warm Warm
air air
Cool air
Cool air Land breeze
Sea breeze
Sea Breezes Convection currents over areas where the land Figure 19
meets the sea can cause wind. A sea breeze, shown in Figure 19, These daily winds occur because
is created during the day because solar radiation warms the land land heats up and cools off faster
more than the water. Air over the land is heated by conduction. than water does. During the
This heated air is less dense and has lower pressure. Cooler, day, cool air from the water
moves over the land, creating a
denser air over the water has higher pressure and flows toward
sea breeze. At night, cool air
the warmer, less dense air. A convection current results, and
over the land moves toward the
wind blows from the sea toward the land. warmer air over the water, creat-
ing a land breeze.
How does a sea breeze form?
Land Breezes At night, land cools much more rapidly than
ocean water. Air over the land becomes cooler than air over the
ocean. Cooler, denser air above the land moves over the water, as
the warm air over the water rises. Movement of air toward the
water from the land is called a land breeze.
Section Assessment
1. Why do some parts of Earth’s surface,such
as the equator, receive more of the Sun’s
6. Comparing and Contrasting Compare and
heat than other regions?
contrast sea breezes and land breezes. For more
2. How does the Coriolis effect influence wind help, refer to the Science Skill Handbook.
circulation on Earth?
7. Using Graphics Software Use graphics soft-
3. Why does little wind and lots of afternoon ware and Figure 17 to draw the wind systems on
rain occur in the doldrums? Earth. Make a separate graphic of major wind cir-
4. Which wind system helped early sailors culation cells shown by black arrows. On another
navigate Earth’s oceans? graphic, show major surface winds. Print your
5. Think Critically How does the jet stream graphics and share them with your class. For more
help move storms across North America? help, refer to the Technology Skill Handbook.
SECTION 3 Air Movement 299
23. The Heat Is On
S ometimes, a plunge in a pool or lake on a hot summer day feels cool and refresh-
ing. Why does the beach sand get so hot when the water remains cool? A few
hours later, the water feels warmer than the land does. In this activity, you’ll explore
how water and land absorb heat.
Recognize the Problem
How do soil and water compare in their abilities to absorb and emit heat?
Form a Hypothesis
Form a hypothesis about how soil and water compare in their abilities to absorb and
release heat. Write another hypothesis about how air temperatures above soil and
above water differ during the day and night.
Safety Precautions
WARNING: Be careful when handling the
hot overhead light. Do not let the light or
its cord make contact with water.
Possible Materials
ring stand clear plastic boxes (2)
soil overhead light
metric ruler with reflector
water thermometers (4)
masking tape colored pencils (4)
Goals
s Design an experiment to compare
heat absorption and release for soil
and water.
s Observe how heat release affects
the air above soil and above water.
300
24. Test Your Hypothesis
Plan Do
1. As a group, agree upon and write 1. Make sure your teacher approves
your hypothesis. your plan and your data table before
2. List the steps that you need to take you start.
to test your hypothesis. Include in 2. Carry out the experiment as planned.
your plan a description of how you 3. During the experiment, record your
will use your equipment to compare observations and complete the data
heat absorption and release for table in your Science Journal.
water and soil.
4. Include the temperatures of the soil
3. Design a data table in your Science and the water in your measurements.
Journal for both parts of your exper- Also compare heat release for water
iment—when the light is on and and soil.Include the temperatures of
energy can be absorbed and when the air immediately above both of
the light is off and energy is released the substances. Allow 15 min for
to the environment. each test.
Analyze Your Data
1. Use your colored pencils and the 2. Analyze your graphs. When the
information in your data tables to light was on, which heated up
make line graphs. Show the rate of faster—the soil or the water?
temperature increase for soil and 3. Compare how fast the air temper-
water. Graph the rate of tempera- ture over the water changed with
ture decrease for soil and water after how fast the temperature over the
you turn the light off. land changed after the light was
turned off.
Draw Conclusions
1. Were your hypotheses supported or not? Explain.
2. Infer from your graphs which cooled faster—
the water or the soil. Make a poster showing the steps you
3. Compare the temperatures of the air above followed for your experiment. Include
the water and above the soil 15 minutes after graphs of your data. Display your poster in
the light was turned off. How do water and the classroom. For more help, refer to the
soil compare in their abilities to absorb and Science Skill Handbook.
release heat?
ACTIVITY 301
25. marsup al
nucleus organelle marsupial mantle element
ibosome primate sea otter hypertension jet
ici Science & Language Arts
and
or
wa Song of the Sky Loom1
no Brian Swann, ed.
me This Native American prayer probably comes from the
dRespond to the Reading Tewa-speaking Pueblo village of San Juan, New Mexico. The
og 1. Why do the words
Mother Earth and
poem is actually a chanted prayer used in ceremonial rituals.
ntu Father Sky appear on
Mother Earth
either side and above
Father Sky
m and below the rest of
the words?
we are your children
cai 2. Why does the song
use the image of a
With tired backs we bring you gifts you love
Then weave for us a garment of brightness
ha garment to describe
Earth’s atmosphere?
2
its warp the white light of morning,
ppu 3
weft the red light of evening,
fringes the falling rain,
atim
tim its border the standing rainbow.
ou Thus weave for us a garment of brightness
So we may walk fittingly where birds sing,
dig So we may walk fittingly where grass is green.
co Mother Earth Father Sky
aga
ga
ni
1
a machine or device from
which cloth is produced
2
threads that run lengthwise
he 3
in a piece of cloth
horizontal threads inter-
enc laced through the warp in a
piece of cloth
bre
oz
opo
poi 302 CHAPTER 10 Atmosphere
oem
26. m grat on compound d chotomous greenho
exoskeleton permafrost magmaMetaphor plat isotopes
cell
gym
Understanding Literature ma
Metaphor A metaphor is a figure of speech that com-
Linking Science
pares seemingly unlike things. Unlike a simile, a
and
ion
metaphor does not use the connecting words like or as.
the
For instance, in the song you just read, Father Sky is a
loom. A loom is a machine or device that weaves cloth.
Creating a Metaphor Write a
kid
The song describes the relationship between Earth and
sky as being a woven garment. Lines such as “weave for
four-line poem that uses a
metaphor to describe rain. You
us a garment of brightness” serve as metaphors for
how Mother Earth and Father Sky together create an
pro can choose to write about a gen-
tle spring rain or a thunderous
ign
atmosphere in which their “children,” or humans, can
rainstorm. Remember that a
metaphor does not use the words
thrive.
par like or as. Therefore,your poem
should begin with something like
the composition of Earth’s atmosphere. The atmo- zon
Science Connection In this chapter, you learned about
“Rain is ...” or “Heavy rain is ...”
sphere maintains the proper balance between the
mo
amount of heat absorbed from the Sun and the amount
orp
of heat that escapes back into space. You also learned
about the water cycle and how water evaporates from
Earth’s surface back into the atmosphere. Using
eta
etal
metaphor instead of scientific facts, the Tewa song con-
allo
veys to the reader how the relationship between Earth
and its atmosphere is important to all living things.
om
Career Connection Meteorologist oge
pro
Kim Perez is an on-air meteorologist for The Weather Channel, a
acc
national cable television network. She became interested in the
weather when she was living in Cincinnati, Ohio. There, in 1974, she
tab
witnessed the largest tornado on record. Ms.Perez now broadcasts
weather reports to millions of television viewers. Meteorologists
nol
study computer models of Earth’s atmosphere. These models help
them predict short-term and long-term weather conditions for the
eat
eath
United States and the world.
tem To learn more about careers in meteorology,
sol
sola
visit the Glencoe Science Web site at science.glencoe.com.
303 hav SCIENCE AND LANGUAGE ARTS
dim
27. Chapter 10 Study Guide
Section 1 Earth’s Atmosphere 4. Unlike the atmosphere on Mars or Venus,
1. Earth’s atmosphere is made up mostly Earth’s unique atmosphere maintains a
of gases, with some suspended solids and balance between energy received and energy
liquids. The unique atmosphere allows lost that keeps temperatures mild. This deli-
life on Earth to exist. cate balance allows life on Earth to exist.
2. The atmosphere is divided into five layers Section 3 Air Movement
with different characteristics. 1. Because Earth’s surface is curved, not all
3. The ozone layer areas receive the same amount of solar
protects Earth radiation. This uneven heating causes
from too much Cl
temperature differences at Earth’s surface.
F C
ultraviolet radia- 2. Convection currents modified by the
tion, which can Coriolis effect produce Earth’s global
Cl
be harmful. How Cl winds.
do chlorofluoro- 3. The polar jet stream is a strong current
carbon molecules of wind found in the upper troposphere.
destroy ozone? It forms at the boundary between cold,
polar air and warm, tropical air.
Section 2 Energy Transfer
in the Atmosphere 4. Land breezes
and sea breezes
1. Earth receives its energy from the Sun. occur near the
Some of this energy is reflected back into ocean. Why do
space, and some is absorbed. winds change
2. Heat is distributed in Earth’s atmosphere by direction from
radiation, conduction, and convection. day to night?
3. Energy from the Sun powers the water
cycle between the atmosphere and Earth’s
surface. Clouds form during which part
of the water cycle?
After You Read
FOLDABLES
Reading &Study
& Study Draw pictures on the front
Skills of your Foldable of things
that you might find in each
layer of Earth’s atmosphere.
304 CHAPTER STUDY GUIDE
28. Chapter 10 Study Guide
Complete the following cycle map on the water cycle.
Cooled
water vapor
condenses.
Energy from
the Sun evaporates
water.
Vocabulary Review Using Vocabulary
a. atmosphere i. jet stream The sentences below include terms that have
b. chlorofluorocarbon j. land breeze been used incorrectly. Change the incorrect terms
c. condensation k. ozone layer so that the sentence reads correctly.
d. conduction l. radiation 1. Chlorofluorocarbons are dangerous because
e. convection m. sea breeze they destroy the hydrosphere.
f. Coriolis effect n. troposphere
g. hydrosphere o. ultraviolet radiation 2. Narrow belts of strong winds called sea
h. ionosphere breezes blow near the top of the troposphere.
3. The thin layer of air that surrounds Earth is
called the troposphere.
Study Tip
4. Heat energy transferred in the form of
waves is called condensation.
Describe ways that you might design an experi-
ment to prove scientific principles. 5. The ozone layer helps protect us from the
Coriolis effect.
CHAPTER STUDY GUIDE 305
29. Chapter 10 Assessment
10. What are narrow belts of strong winds near
the top of the troposphere called?
Choose the word or phrase that best answers A) doldrums C) polar easterlies
the question. B) jet streams D) trade winds
1. What is the most abundant gas in the
atmosphere?
A) oxygen C) argon
B) water vapor D) nitrogen 11. Why are there few or no clouds in the
2. What causes a brown haze near cities? stratosphere?
A) conduction C) car exhaust 12. It is thought that life could not have existed
B) mud D) wind on land until the ozone layer formed about
3. Which is the uppermost layer of the atmo- 2 billion years ago. Why does life on land
sphere? require an ozone layer?
A) troposphere C) exosphere 13. Why do sea breezes occur during the day
B) stratosphere D) thermosphere but not at night?
4. What layer of the atmosphere has the most 14. Describe what happens when water vapor
water? rises and cools.
A) troposphere C) mesosphere 15. Why does air pressure decrease with an
B) stratosphere D) exosphere increase in altitude?
5. What protects living things from too much
ultraviolet radiation?
A) the ozone layer C) nitrogen
B) oxygen D) argon 16. Concept Mapping Complete the cycle con-
6. Where is air pressure least? cept map below using the following phrases
A) troposphere C) exosphere to explain how air moves to form a convec-
B) stratosphere D) thermosphere tion current: Cool air moves toward warm
7. How is energy transferred when objects are air, warm air is lifted and cools, and cool air
in contact? sinks.
A) trade winds C) radiation
B) convection D) conduction
8. Which surface winds are responsible for
most of the weather movement across the
United States?
Cool air is warmed
A) polar easterlies C) prevailing westerlies by conduction.
B) sea breeze D) trade winds
9. What type of wind is a movement of air
toward water?
A) sea breeze C) land breeze
B) polar easterlies D) trade winds
306 CHAPTER ASSESSMENT
30. Chapter 10 Assessment
17. Drawing Conclusions In an experiment, a
student measured the air temperature 1 m Test Practice
above the ground on a sunny afternoon and
again in the same spot 1h after sunset. The Each layer of Earth’s atmosphere has a
second reading was lower than the first. unique composition and temperature. The
What can you infer from this? four layers closest to Earth’s surface are
shown in the diagram below.
18. Forming Hypotheses Carbon dioxide in
the atmosphere prevents some radiation Thermosphere
from Earth’s surface from escaping to space. (85-500 km)
Mesosphere
Hypothesize how the temperature on Earth (50-85 km)
might change if more carbon dioxide were Stratosphere
released from burning fossil fuels. (10-50 km)
Troposphere
19. Identifying and Manipulating Variables (0-10km)
and Controls Design an experiment to find Oz
o
out how plants are affected by differing
ne
lay
amounts of ultraviolet radiation. In the
er
design, use filtering film made for car win-
dows. What is the variable you are testing? Earth
What are your constants? Your controls?
20. Recognizing Cause and Effect Why is the Study the diagram and answer the
inside of a car hotter than the outdoor following questions.
temperature on a sunny summer day? 1. In which part of the atmosphere is
ozone located.
A) Thermosphere C) Stratosphere
B) Troposphere D) Mesosphere
21. Poster Illustrate or find magazine photos 2. According to the diagram, how far
of convection currents that occur in every- does the mesosphere extend above
day life. Earth’s surface?
22. Experiment Design and conduct an experi- F) 10 km H) 50 km
ment to find out how different surfaces G) 85 km I) 60 km
such as asphalt, soil, sand, and grass absorb 3. What is the correct order of atmo-
and reflect solar energy. Share the results spheric layers that the space shuttle
with your class. goes through when landing on Earth?
A) Mesosphere C) Stratosphere
TECHNOLOGY Stratosphere Troposphere
Go to the Glencoe Science Web site at Troposphere Mesosphere
science.glencoe.com or use the B) Troposphere D) Mesosphere
Glencoe Science CD-ROM for additional Stratosphere Troposphere
chapter assessment. Mesosphere Stratosphere
CHAPTER ASSESSMENT 307