17.2 – Heating the atmosphere – Part I

Slides:



Advertisements
Similar presentations
Prentice Hall EARTH SCIENCE
Advertisements

The Atmosphere: Structure and Temperature
17.2 Heating the Atmosphere
The Sun.
Energy Ability to do work Many different forms Conservation of energy (Law) Transformed: example: – Radiant to Thermal – Kinetic to Thermal (friction)
Chapter 22 Section 2 Review Page 560 #’s 1-9
16-1 Energy in Earth’s Atmosphere. (pages 542–545) 1
Thermal Energy. 1.Thermal Energy is the vibration or movement of atoms and molecules. 2.All matter has thermal energy because the atoms are always moving.
ENERGY FROM THE SUN Chapter 14.3 Pages Energy in the Atmosphere The sun is the source of ALL energy in our atmosphere. Three things that can.
Solar Energy and Heating the Atmosphere. Radiation Energy comes from the sun as radiant energy Radiation from the Sun can be visible (light) or invisible.
Earth Science 17.2 Heating the Atmosphere
Climate Long time, Large Area. Weather short term, small area.
Warm Up 3/6/08 More solar energy reaches the equatorial regions than the polar regions because the equatorial regions a. are covered by a greater area.
Solar Energy Heat and Light. Energy Can take many different forms –____________ –Heat –____________.
24.1 The Study of Light Electromagnetic Radiation
Structure of the Sun 24.3 The Sun  Because the sun is made of gas, no sharp boundaries exist between its various layers. Keeping this in mind, we can.
Introduction to Thermal Physics
Earth’s Energy Budget Ch ways heat can be transferred: Conduction Conduction Convection Convection Radiation Radiation.
Heat Transfer in the Atmosphere Essential Question: How is heat transferred in the atmosphere?
24.3 The Sun Structure of the Sun
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
Seconds Left: List & describe the three types of heat transfer.
Compare Radiation & Conduction (Part 2) Contrasting Case Activity 4b Weather & Water, Investigation 4.
Structure of the Sun 24.3 The Sun  Because the sun is made of gas, no sharp boundaries exist between its various layers.  Keeping this in mind, we can.
Conduction The transfer of energy as heat between particles collide within a substance or between two objects in contact Two objects of unequal temperature.
Monday April 18, 2011 (Atmospheric Heating; Video Flow Charts – The Atmosphere & Fossil Fuels)
HEAT TRANSFER Conduction, Convection and Radiation.
Structure of the Sun 24.3 The Sun  Because the sun is made of gas, no sharp boundaries exist between its various layers. Keeping this in mind, we can.
Chapter 22 Section 2 Handout
EARTH’S ENERGY. Energy from the Sun Nearly all of Earth’s atmosphere energy comes from the sun as electromagnetic waves. Most of the energy comes from.
Do Now: Based on the notes from last week, what is the difference between temperature and heat?
The Atmosphere: Structure and Temperature
17 Chapter 17 The Atmosphere: Structure and Temperature.
Weather and Climate Unit Investigative Science. * All materials are made of particles (atoms and molecules), which are constantly moving in random directions.
Warm-Up What would happen if there was no more ozone? What would happen if there was no more ozone? –We would die. What are the four layers of the atmosphere?
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
Heat and Energy Study Guide CH 3-2 for Quiz. What happens when objects with different temperatures come into contact with each other?  Energy will always.
TA12A –Teach About Heating Earth’s Air Use with BrishLab ES12A Done By: Coach – Period All This material is CC by StarMaterials.com.
Composition of the Atmosphere 14 Atmosphere Characteristics  Weather is constantly changing, and it refers to the state of the atmosphere at any given.
DO NOW: Heat Transfer. What type of heat transfer is shown?
1. Which of these features is a landform associated with karst topography? Sinkholes Streams Natural levees Deltas 2. What are the major environmental.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Heat Energy. What is Heat Energy? Heat Energy Heat Energy is the sum total of all of the energy of the particles of an object. Heat energytemperature.
I. WHAT IS TEMPERATURE? We don’t use the terms hot and cold often in science because they are relative terms: They could mean different things depending.
 The measure of the average kinetic energy of particles. Temperature doesn’t depend on the number of particles.
Do Now: In you notes, describe what happens to an object as heat (energy) is added to it. What changes take place, what happens to the molecules? With.
The Atmosphere: Structure & Temperature. Atmosphere Characteristics Weather is constantly changing, and it refers to the state of the atmosphere at any.
Heat Transfer How heat gets from one place to another.
Unit 3 Lesson 2 Energy Transfer
Explain where heat is “coming from” and “going to” in this picture.
The Atmosphere: Structure & Temperature
Heat in the Atmosphere.
What is Energy? Energy – the ability to do work
Unit 3 Lesson 2 Energy Transfer
Energy from the Sun The Sun’s energy gives us heat through conduction, convection, radiation The Sun’s energy also gives us light through electromagnetic.
17.1 Atmosphere Characteristics
(Discussion – Atmospheric Heating)
Chapter 17 The Atmosphere
Solar Radiation and the Atmosphere
Heating the Earth Investigation 4, Part 1
17.2 Heating the Atmosphere
Heating the Atmosphere
Atmospheric Heating Notes
17.2 Heating the Atmosphere.
17.2 Heating the Atmosphere
Heat and Temperature.
Energy transfer in the atmosphere
Unit 3 Lesson 2 Energy Transfer
Heat.
Solar Radiation and the Atmosphere
Presentation transcript:

17.2 – Heating the atmosphere – Part I

Do Now What is the difference between heat and temperature?

Do Now What is the difference between heat and temperature? Heat: Energy transferred from one object to another because of a difference in temperature. Temperature: is a measure of the average kinetic energy of the individual atoms or molecules in a substance.

Key Words Heat Mechanism Molecule Electromagnetic Spectrum Emit Absorb

Vocab Words Temperature Conduction Convection Radiation

Methods of Heat Transfer Three mechanisms of energy transfer as heat are conduction, convection, and radiation. All 3 happen at the same time in the atmosphere. They transfer energy between Earth's surface (both land and water) and the atmosphere. Conduction is the transfer of heat through matter by molecular activity. Convection is the transfer of heat by mass movement or circulation within a substance. Radiation is the transfer of energy (heat) through space by electromagnetic waves that travel out in all directions. Unlike conduction and convection, which need material to travel through, radiant energy can travel through the vacuum of space.

Laws Governing Radiation 4 laws govern radiation and help us better understand how the atmosphere is heated. All objects, at any temperature, emit radiant energy. Hotter objects radiate more total energy per unit area than colder objects do. The hottest radiating bodies produce the shortest wavelengths of maximum radiation. Objects that are good absorbers of radiation are good emitters as well.

Electromagnetic Waves The sun emits light and heat as well as the ultraviolet rays that cause a suntan. These forms of energy are only part of a large array of energy emitted by the sun, called the electromagnetic spectrum. Visible light is part of this spectrum, and the only part that we can see.

Group Activity Come up with an example, different from the book but similar to Figure 9 on page 483, and draw a picture with your description. Follow the directions to the Molecule Model Activity and then write how this activity helped you better understand energy transfer as heat.