The Atmosphere is the layer of air surrounding the Earth

Similar documents
Atmosphere - Part 2. High and Low Pressure Systems

Atmosphere Weather and Climate

Space Atmospheric Gases. the two most common gases; found throughout all the layers a form of oxygen found in the stratosphere

10.1 TEMPERATURE, THERMAL ENERGY AND HEAT Name: Date: Block: (Reference: pp of BC Science 10)

Ocean s Influence on Weather and Climate

Investigating Planets Name: Block: E1:R6

Science 1206 Chapter 1 - Inquiring about Weather

Section 2: The Atmosphere

Clouds and Rain Unit (3 pts)

Chapter 4 Lesson 1: Describing Earth s Atmosphere

Name Period 4 th Six Weeks Notes 2013 Weather

Unit 2 Meteorology Test **Please do not write on this test** 5. El Nino & La Nina 6. Photosynthesis 7. Coriolis Effect 8.

Date Class Block. Science SOL Review 6 th grade material

Unit 3 Review Guide: Atmosphere

The Atmosphere - Chapter Characteristics of the Atmosphere

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Earth Science Chapter 16 and 17. Weather and Climate

according to and water. High atmospheric pressure - Cold dry air is other air so it remains close to the earth, giving weather.

Evolution of the Atmosphere

The order of the atmosphere layers. Unique characteristics of each layer. What do the temperatures do in each layer? Why is the temperature of the

I T A T I O N H B I T B T V A O C J K M R S A T M O S P H E R E

1. CLIMATOLOGY: 2. ATMOSPHERIC CHEMISTRY:

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

IV. Atmospheric Science Section

The Atmosphere. Composition of the Atmosphere. Section 2

The Atmosphere Made up of mainly two gases: Nitrogen 78% Oxygen 21% Trace Gases 1%

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings

Lesson Overview. Climate. Lesson Overview. 4.1 Climate

Atmosphere, Weather & Climate Review for Unit Assessment (Can be taken on Study Island Due Mon., 11/26/12)

Thermal / Solar. When air is warmed it... Rises. Solar Energy. Evaporation. Condensation Forms Clouds

Website Lecture 3 The Physical Environment Part 1

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

1 Characteristics of the Atmosphere

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

MASTERY ASSIGNMENT 2015

Unit 2: The atmosphere

Website Lecture 3 The Physical Environment Part 1

Chapter 15: Weather and Climate

Period 13 Solutions: Earth as an Energy System

Lithosphere: (Rocky Sphere) Solid, rocky, outer layer of the Earth. Includes the crust and part of the upper mantle. Lithosphere

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)

Climate versus Weather

AT 350 EXAM #1 February 21, 2008

student pretest Stewardship Project middle school (Grades 7-8)

Science Chapter 13,14,15

Planetary Atmospheres (Chapter 10)

Scholarship 2015 Earth and Space Science

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

10/31/2017. Calculating the temperature of earth (The greenhouse effect) IR radiation. The electromagnetic spectrum

Chapter 3 Packet. and causes seasons Earth tilted at 23.5 / 365 1/4 days = one year or revolution

Unit: Weather Study Guide

COMPOSITION OF THE ATMOSPHERE

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Atmospheric Basics Atmospheric Composition

,Solar Energy, Greenhouse effect, Convection.notebook October 31, 2016

Earth s Atmosphere. Atmospheric Composition 78% Nitrogen 21% Oxygen 1 % Argon, 0.03% Carbon dioxide, Water. Recall the Electro-Magnetic (EM) Spectrum

Earth Science final exam study guide (Semester 2)

3 Weather and Climate

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg )

The Earth. Overall Structure of Earth

CHAPTER 6 Air-Sea Interaction Pearson Education, Inc.

Climate Change Lecture Notes

The of that surrounds the Earth. Atmosphere. A greenhouse that has produced the most global. Carbon Dioxide

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

1. What is the phenomenon that best explains why greenhouse gases absorb infrared radiation? D. Diffraction (Total 1 mark)

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

Standard 3: Students will understand the atmospheric processes that support life and cause weather and climate.

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy.

Your web browser (Safari 7) is out of date. For more security, comfort and the best experience on this site: Update your browser Ignore

Weather is the of the Earth s atmosphere at a place and time. It is the movement of through the atmosphere o Energy comes from the

Tuesday, September 13, 16

Climate vs. Weather. Weather: Short term state of the atmosphere. Climate: The average weather conditions in an area over a long period of time

78% : component of atmosphere! 21% : 1% : Changes depending on origin of air: - originated over - originated over Ozone = O 3 Definition:

Carbon Cycling Internal

4-1 The Role of Climate

Atmosphere. Transfer in the Atmosphere

Earth s Atmosphere About 10 km thick

surrounds Earth and protects it somewhat from solar radiation. Like all other matter, air has weight,

5. In which diagram is the observer experiencing the greatest intensity of insolation? A) B)

2010 Pearson Education, Inc.

Module 11: Meteorology Topic 6 Content: Severe Weather Notes

3 Severe Weather. Critical Thinking

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

FCAT Review Space Science

Meteorology. I. The Atmosphere - the thin envelope of gas that surrounds the earth.

Background: What is Weather?

Energy Transfer in the Atmosphere

The Atmosphere and Atmospheric Energy Chapter 3 and 4

Unit 9. Atmosphere. Natural Science 1º ESO Antonio Jesús Moreno Quintero. Colegio Guadalete. Attendis.

MIDTERM PRACTICE EXAM ANSWERS

Name Team Period. Station #1 (drawing)

Section 13-1: Thunderstorms

Goal 2.5. The Atmosphere

Go With the Flow From High to Low Investigating Isobars

The surface of the ocean floor is as varied as the land. The five major oceans, from largest to smallest, are

Transcription:

The Atmosphere is the layer of air surrounding the Earth The gases in the atmosphere are important because: They block out dangerous rays from the sun, such as UV rays They stabilize the temperature across the Earth by retaining heat They include O2, which is essential for cellular respiration, and CO2, which is necessary for photosynthesis.

Atmospheric pressure is cause by gravity pulling down the particles of the atmosphere This is why atmospheric pressure decreases as you rise in the atmosphere. 99% of the particles is present in the first 30 km above the surface The atmosphere is considered to extend more than 10,000 km above the surface

Air is a mixture of gases, especially nitrogen and oxygen, that makes up the atmosphere 78% of air is Nitrogen 21% of air is Oxygen 1% of air is other gases Water only makes up a small portion of the air, but is still very important

Atmospheric circulation is the global-scale movement of the layer of air surrounding the Earth The hot air rises and the cooler air drops This is due to convection. Without this movement, the temperature difference between the equator and the poles would be much greater

An air mass is a large expanse of the atmosphere with relatively uniform temperature and humidity When two air masses collide, they do not simply combine The cooler air mass slides below the warmer and the warmer air mass rises

Where warm and cold air masses collide is referred to as a front Cold fronts occur when a mass of cold air meets a warm air mass As the warm air rises it cools quickly and condenses into clouds This produces puffy clouds called cumulus

A warm front is when a warm air mass meets a mass of cold air In this case, the warm air rises more slowly forming light clouds called nimbostratus On weather maps, cold fronts are represented by blue arrows and warm fronts are represented by red arrows

While most air masses move horizontally over the surface of the Earth, there is some vertical movement

An area of atmospheric circulation surrounding a high pressure center Clockwise for Northern hemisphere and counter-clockwise in the Southern hemisphere

An area of atmospheric circulation surrounding a low pressure center Counter-clockwise for Northern hemisphere and clockwise in the Southern hemisphere

Strong depressions sometimes form over warm waters of tropical oceans A huge spiral forms which can stretch up to 800 km across in diameter Winds can blow up to 360 km/h These storms can be called cyclones, hurricanes or typhoons depending on the region

Hurricanes have a characteristic eye in the center Typically they are between 30-65 km wide Can be as little as 3 km up to 670 km The eye is generally calm and without clouds The walls of the eye, the eyewall, are generally the tallest, strongest and most rainy parts of the hurricane

What are greenhouse gases? Mainly water vapour (H 2 O), Carbon Dioxide (CO 2 ), Methane (CH 4 ) and Nitrous Oxide (N 2 O) They are present in the atmosphere and they act as a type of insulation to retain the heat around the Earth. Without this effect, the Earth s average temperature would be -18 C

1- Most of the Sun s rays reach the Earth s surface and is absorbed by the ground 2- The heated ground sends infrared rays back into the atmosphere. A portion of the infrared rays pass through the atmosphere and are lost into space. 3- Greenhouse gases trap some of the rays and send them back to the Earth, further heating its surface

Over the last century, the levels of CO 2 have increased due to combustion of fossil fuels Human activities have increased the production of CO 2 by billions of tonnes which is having a big effect on the environment This is leading to climate change on the Earth

Methane, CH 4, has a 21 time greater effect on the greenhouse effect than CO 2, for the same volume CH 4 comes from the digestion in farm animals, and decomposition of garbage and waste N 2 O comes from the strong use of nitrogen rich fertilizers on farms

Wind Energy is the energy that can be drawn from the wind Wind turbines are huge machines which turn with the wind and produce electricity Wind is a renewable resource so wind turbines are considered to be environmentally friendly Wind turbines do have a few negatives though

People say that wind turbines ruin the natural beauty of the landscapes Wind is not a reliable source of power since the winds are not predictable Wind energy cannot be stored. Once the wind is gone, so is the electricity

The Sun and the Moon are the two bodies in our solar system which most affect us The Sun is vitally important because its energy provides us with light and heat The Moon exerts gravitational forces upon the Earth which explains the tides.

The Sun is composed 75 percent of Hydrogen and 25 percent Helium The temperature of the core reaches up to 15 million C due to nuclear Fission Hydrogen being made into Helium Light only takes 8 minutes to reach the Earth from the Sun The Earth is 150,000,000 km away from the Sun

Solar radiation contains all of the waves in the electromagnetic spectrum Only visible light, some infrared, and a small amount of UV light reach the surface of the Earth Due to the curvature of the Earth, the equator receives much more heat than the polar regions

The Earth receives enough energy in one hour from the sun to satisfy the world s energy requirements for a year. Solar energy is the energy that comes from the Sun in the form of radiation through the atmosphere Harnessing this energy is a huge challenge There are a few ways that we can harness the power of the Sun

Passive Heating Systems By positioning the house to take advantage of the Sun. Photovoltaic Cells When the material that makes up the cells is hit by light, electrons are set into motion. This causes a current which can be used to power small appliances or an entire house Solar Collectors These are sheets of glass which has copper pipes below it to absorb to heat up water or air for homes or water for a pool

The moon has been revolving around the Earth for billions of years Its average diameter is 3476km, which is roughly a quarter of the Earth The theory behind the origin of the Moon is that the Earth was struck by a meteor the size of Mars. This caused part of the Earth to explode The pieces reunited to form the Moon

The Moon not only rotates around the Earth, but also rotates on its own axis. These two movements are synchronised to that both rotations take the same amount of time (27.3 days)

Water masses on the side closest to the Moon are attracted to it As a result, they will swell, forming a slight bulge in the Moon s direction Also, the waters on the opposite side of the moon get pulled towards the moon as well.

Tidal energy is the energy obtained from the ebb and flow of the tides Works similarly to hydroelectric dam When the tide come in, it fills a huge basin The water remains there until the tide goes out again

The gate opens, releasing the basin of water to flow through the turbines The turbine is set into motion, generating electricity There are numerous advantages

Produces no greenhouse emissions Entirely renewable Perfectly reliable since meteorologists can predict the ebb and flow of tides

Building plants is complex and costly because they have to stand up to harsh conditions There are few suitable sites in the world for building this type of power plant There must be a tidal range of at least 5 meters