Venus Earth Mars The surface temperature of Venus is around 460 C (890 degrees F ), the hottest average temperature in the Solar System. This is due.

Slides:



Advertisements
Similar presentations
CST Review Standard 4 Energy enters the Earth system primarily as solar radiation and eventually escapes as heat. Know the relative amount of incoming.
Advertisements

Micro meter = millionth of a meter Micro meter = m Visible light 0.4 m to 0.7 m.
There are all sorts of electromagnetic waves. The shorter the wavelength the higher the energy of the waves. The energy from the sun is mostly visible.
MODULE #1: Climate Change & Global Warming
Unit 4.2: Atmospheric Composition and Weather
Last Class How does variability in the earths physical structure affect the transformations of energy? - albedo of different spheres; clouds What is the.
Global Warming What determines the surface temperature of the Earth?
Heat Transfer, Greenhouse Effect, Ozone Layer Notes
Earth’s Climate System (part 1) climate system electromagenetic spectrum Earth’s radiation budget albedo greenhouse effect.
MET 12 Global Climate Change – Lecture 3
Chapter 22 Section 2 Review Page 560
Structure of Atmosphere From Cunningham & Cunningham, 2004, Fig. 9.1.
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
Solar Radiation and the Greenhouse Effect Earth Science Ms. Kurtzweil.
The Atmosphere.
Weather World Geography Notes 1.5. Atmosphere Atmosphere is a thin layer of gases This protects the surface from Temperature extremes (acts as insulation)
Greenhouse Gases and Energy Budget LP 3 1. What are the greenhouse gases? Where do they come from? How do they work? 2.
Greenhouse Gases and Energy Budget LP 3 1. What are the greenhouse gases? Where do they come from? How do they work? 2.
Lecture 3: The greenhouse effect. Other concepts from Lecture 2 Temperature Scales Forms of Heat Transfer Electromagnetic Spectrum Stefan-Boltzmann Law.
Handout (yellow) Solar Energy and the Atmosphere Standard 3 Objective 1 Indicators a, b, and c Standard 3 Objectives 1, 2, and 3 Workbook Pages 3,
the Natural Greenhouse Effect
Last Class – Global What transformations occur as energy flows through the earth system. Relationship between distance from the source and amount of energy.
Solar Energy & the Atmosphere
Aim: How is the earth's atmosphere similar to a greenhouse?
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
Solar and Terrestrial Radiation
Earth’s Changing Atmosphere. Main Topics Definition and Characteristics of the Atmosphere Changes to the Atmosphere composition Layers of the Atmosphere.
The Greenhouse Effect. Visible light from sun Earth radiates in IR.
The Atmosphere. Composition  Nitrogen  Oxygen  Other –Argon –Carbon Dioxide –Methane –Water Vapor  Atmospheric dust.
The Greenhouse Effect *The earth is similar to a greenhouse. The earth atmosphere acts like the glass in a greenhouse. *Sunlight streams through the.
The Greenhouse Effect Too much of a good thing?. Light from the sun is composed of many frequencies.
Case Studies of Important Scientific and Technological Issues Nature and Development of Science and Technology.
Greenhouse Gases and Energy Budget LP 3 1. What are greenhouse gases? Where do they come from? How do they work? 2.
Ch Solar Energy and the Atmosphere
The Greenhouse Effect. A lot of the light that comes from the sun, doesn’t make it to the surface of the earth.
11/14/2015 Global Warming Archer chapters 1 & 2 GEO 307 Dr. Garver.
Pre Test 1. True or False. Earths Surface tempature has been constantly changing in geological time. 2. How does earth exchange energy with the enviroment?
Chapter 3 Solar and Terrestrial Radiation. Driving Question How does energy flow into and out of the Earth-Atmosphere system? Law of Energy Conservation.
Mr. Fleming. The trapping of heat from the sun by gases in the Earth’s atmosphere. The major gas contributing to this process is Carbon dioxide gas.
The trapping of heat from the sun by gases in the Earth’s atmosphere. The major gas contributing to this process is Carbon dioxide gas. Greenhouse effect.
Topic 6. Without energy from the sun, conditions on Earth would be different. What is the energy that is radiated from the Sun? The energy that is radiated.
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
Lecture 3: Radiation and Earth’s Atmosphere EarthsClimate_Web_Chapter.pdfEarthsClimate_Web_Chapter.pdf, p. 1-5 For more advanced reading materials, please.
The Greenhouse Effect - Atomic level By Kaelin O’Hare.
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 2 “Greenhouse Effect: Earth and Venus” Dr. Eugene Cordero San Jose State University.
Incoming & Outgoing of Energy of the Earth. The Earth’s Energy Balance The Earth's average temperature remains fairly constant from year to year. Therefore,
Heat in the Atmosphere The sun’s energy is transferred to earth and the atmosphere three ways Radiation, Convection and Conduction.
The Atmosphere: Structure and Temperature
Greenhouse Effect Sun Earth’s Temperature Solar Energy Solar Energy Solar Energy Solar Energy.
The Greenhouse Effect. Natural heating of earth’s surface caused by greenhouse gases –CO 2 (Carbon Dioxide) –CH 3 (Methane) –N 2 O (Nitrous Oxide) –H.
Energy in the Earth System Big Ideas The climate system (and life on Earth ) is maintained by energy coming from the Sun (electromagnetic radiation). The.
CHAPTER 19 HEAT TRANSFER IN THE ATMOSPHERE. WHAT IS THE ATMOSPHERE? Earth’s atmosphere is heated by the transfer of energy from the sun. Some heat comes.
© 2014 Pearson Education, Inc. Chapter 16 The Oceans and Climate Change Greenhouse Effect.
Atmospheric gases allow sunshine to pass through but absorb heat that is radiated back from the surface of the earth. This acts as a blanket keeping heat.
Energy from the Sun Radiation is the transfer of energy by electromagnetic waves. Ninety-nine percent of the radiation from the Sun consists of visible.
3.1 Heat Transfer in the Atmosphere
The Greenhouse Effect.
Greenhouse effect The trapping of heat from the sun by gases in the Earth’s atmosphere. The major gas contributing to this process is Carbon dioxide gas.
Electromagnetic Radiation
Solar Energy and the Atmosphere
Energy from the Sun Sun’s energy travels 148 million km to Earth in only 8 minutes Earth receives less than one-billionth of the Sun’s energy Reaches Earth.
Unit 3 Notes Part 4: Greenhouse Effect
Earth's atmosphere reflects or absorbs some sunlight but allows most of the visible light pass through to Earth's surface. 4 ways the atmosphere affects.
17.2 Heating the Atmosphere
Earth's atmosphere reflects or absorbs some sunlight but allows most of the visible light pass through to Earth's surface. Atmosphere affects light in.
SOLAR BUDGET AND ALBEDO
The Greenhouse Effect and Global Warming
ELECTROMAGNETIC RADIATION
Albedo and Energy Balance
Presentation transcript:

Venus Earth Mars

The surface temperature of Venus is around 460 C (890 degrees F ), the hottest average temperature in the Solar System. This is due to a runaway Greenhouse Effect. The atmosphere of Venus is composed of : 97% CO2, 2% N2 and less than 1% of O2, H2O and CH4 (methane). Since CO2 is a major greenhouse gas, the radiation from the Sun is trapped in the atmosphere of Venus producing an extremely high surface temperature.

The surface temperature of Earth is around 15 degrees C (60 F). It is kept warm by the greenhouse effect. Water vapor is the most important greenhouse gas on Earth and Carbon dioxide (CO2) is second. Methane (CH4) Nitrous Oxide (N2O) Ozone (O3) and the CFCs are also relevant greenhouse gases. The dry atmosphere of Earth is composed of : 78% Nitrogen N2 21 % Oxygen O2 0.9 % Argon (Ar) Less than 0.1 % are the trace gases including CO2. The amount of water vapor in the atmosphere varies from between 0 and 4 %.

Mean Surface Temperature =-55 C. Unlike the Earth or Venus, the atmosphere of Mars is very thin, about 1% the mass of Earth's atmosphere. Similar Venus Its composition is 95% CO2, 3% N2, 2% Ar and less than 1% O2. James Lovelock (Gaia) suggested that the low abundance of CO2 in Earths Atmosphere and the relatively high abundance of O2 is suggestive of life.

Short wavelengths correspond to high photon energy Hot objects radiate more short wave length photons than cooler objects. UV photons have energies above Visible light IR photon energies are lower than visible light photons

The flux of radiation is also referred to as the radiation intensity. It is the amount of radiant energy passing through a surface area each second per unit area.

The Solar constant is 1365 W/m 2 This is the average solar energy that reaches the Earths upper Atmosphere if the sun is shining directly on a solar collector. If the collector is tilted a bit then the intensity is weaker since it is spread over a larger area.

Assume So=1000 W/m 2 What is S if r=2r o ?

Assume So=1000 W/m 2 What is S if r=2r o ?

Assume So=1000 W/m 2 What is S if r=.5r o ?

Assume So=1000 W/m 2 What is S if r=.5r o ?

T K =T C +273 T C =T K -273 T K = T C The mean temperature of Earth is 15 C. What is this on the absolute temperature scale? ( Kelvin scale)

Radiation Laws As temperature increases wavelength of maximum radiant intensity, max, increases. Weins Displacemnet Law. Sun Earth

Black Body =1.0

Stefan_Boltzman Radiation Law. As temperature increases total radiation output increases. Brightness = Intensity Energy leaving an object each sec per square meter As T double Brightness increases by ___??____ As T triples Brightness increases by _______

Radiation Laws As temperature increases total radiation output increases. Stefan_Boltzman Radiation Law. Brightness = Intensity Energy leaving an object each sec per square meter As T double Brightness increases by 16 As T triples Brightness increases by _81 times = 3x3x3x3__

30 % of sunlight incident on Earth is reflected back into space. I.e. Earths Albedo is 0.30 (30 %).

From K. Trenberth, J. Fasullo, and J. Kiehl, EARTHS GLOBAL ENERGY BUDGET BAMS 2009