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Page 1: Announcements

Announcements

• 7 people have still not joined the class on Astronomy Place. Once you join, all your previous submissions appear in your grade.

• Planet Assignment 5, due Wed. March 3, – Astronomy Place tutorial “Surface Temperature of

Terrestrial Planets”

• Star Assignment 1, due Wed. March 3– READ chapter 15, do Angel quiz

• Planet Project 6, due Wednesday March 17– Global Warming internet project

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Announcement

• Wednesday– Finish planets– Begin the Sun, Read chapter 15– If nice, view Moon, Stars & Planets from the

BPS roof

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Earth’s Plate Motion

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Objectives:

• Compare the Atmospheres of the terrestrial planets. Describe and explain the differences in composition & energy balance.

• Describe and explain the Greenhouse Effect. Describe the processes contributing to global warming of Earth.

• Describe how Earth’s climate is exceptional compared to Mars & Venus.

• Describe the factors that effect long term climate change.

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Planets as Homes for Life

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A tale of three planets

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Thought Question

What does a planet need to support life?

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Thought Question

What does a planet need to support life?

Write down your thoughts on the activity paper, along with your full name & student ID. When you are done pass them to the aisle for collection for credit.

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What does a planet need to support life?

• Source of Energy• Elements - C, N, O, Ca, Fe, etc.• Liquid Water• Temperature

between freezing and boiling of water

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Source of Energy

A Star (the Sun)

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Elements

• 3rd generation Star or later– Earlier generations produce the elements

heavier than H & He needed to form planets. Recall: probability of planet formation increases with increasing Iron abundance

– Elements such as C, N, O, Ca, Fe needed for life, as we know it

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Origin of water?

• Water in rocks, originally from planetesimals, like icy comets formed far from Sun

• Volcanoes OUTGAS Water (H2O) and Carbon Dioxide (CO2) from rocks into the atmosphere.

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Volcano

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How Much was Outgassed?

• Earth & Venus outgassed similar amounts of H2O and CO2

– Can tell because have similar amounts of Nitrogen today

• Mars, being smaller, probably outgassed less.

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How much was Lost?

• Mars, being smaller, although colder, lost more atmosphere

• Venus & Earth large, lost little atmosphere

• Venus became very hot, water evaporated. H2O molecules in atmosphere broken apart by solar UV radiation, hydrogen easily escaped.

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Role of Planetary SIZE

Larger Planets heat more and cool slower -> have thinner rigid lithospheres -> more volcanic & tectonic activity -> produce more atmosphere More Massive Planets -> stronger gravity

-> more difficult for atmosphere to escape.-> retain more atmosphere

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Terrestrial Planets

• Moon & Mercury - no atmosphere– too small

• Venus : Earth : Mars = 90 : 1 : 0.01– Why Earth so much less than Venus

• Venus & Mars, CO2 (98%)

• Earth, N2 (77%), O2 (21%)

– What happened to Earth’s CO2?

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What happened to Earth’s CO2?CO2 dissolves in oceansbecomes locked inRocks.

Venus hasno oceans.

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What determines a planet’s surface temperature?

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QuickTime™ and aTIFF (Uncompressed) decompressor

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743 K (470 C)(878 F)

223 K (-50 C)(-58 F)

288 K ( 15 C)( 59 F)

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Surface Temperature of Planets

Determined by balance between- Heating by absorbing visible sunlight and- Cooling by radiating infrared light to space

Since Temperature does not change much, on average,

Amount of energy lost to space =Amount of energy gained from Sun

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The energy emitted by a planet in infrared light equals the amount of sunlight energy it absorbs

Conservation of energy

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Heating by Absorbing Sunlight

Farther from the Sun -> less sunlight hits the planet

Sunlight spreads out

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Heating by Absorbing Sunlight

Earth’s atmosphere reflects 1/3 of the sunlight falling on it

More reflection -> Less Heating

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Thought Question

What kind of shirt is cooler on a sunny summer day?

A. White shirtB. Black shirt

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Earth’s atmosphere absorbs most kinds of light before it reaches the ground.

Heating by Absorbing Sunlight

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Cooling by Radiating Infrared Light

• Heat must leave Earth

• Surface Temperature of Earth ~ 300 K, peak emission is in infrared

• Energy is conserved: Amount of heat emitted = amount of heat absorbed or temperature changes

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Expert Model

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Expert Model II

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Simple Model

Carbon Dioxide Blanket

The hot temperatures may be due to a buildup of carbon dioxide in the atmosphere, caused by the burning of fossil fuel, and by the shrinking of the world's forests. Result: a blanket over the planet that keeps in the heat. (Susan Spencer, CBS News, 1999)

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Why does Temperature Rise?

More insulation ->

Temperature rises to still get rid of the same amount of heat (Recall: Hotter -> Brighter)

Radiate more energy, same fraction gets through, = larger total amount escapes

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No Greenhouse Temp Actual Temp. Warming

Venus -43 C 470 C 513 C

Earth -17 C 15 C 32 C

Moon 0 C 125 C (day) ---175 C (night)

Mars -55 C -50 C 5 C

(from Table 11.2)

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How is human activity affecting Earth’s climate?

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The Global Carbon Cycle - 1990sUnits Gt C and Gt C y-1

Atmosphere

Fossil Deposits6.363

91.7

60

90

3.2

Plants

Soil

Oceans

750

500

2000

39,000

About 16,0001.6

…are leading to a build up of CO2

in the atmosphere.

Fossil emissions ...

…and land clearing in the tropics...

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Burning Fossil FuelsCO2 BuildupCO2 Traps Heat = InsulatesTemperature RisesNegative Consequences

The Causal Chain of Global Warming

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CO2 Concen-tration

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Indicators of the Human Influenceon the Atmosphere during the Industrial Era

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Increased CO2 is causing global warming

Global Warming

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What can and should we do?

We are responsible for managing our Earth prudently!

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Confusions

• Originally, surfaces were heated by bombardment, interiors by differentiation and radioactive decay. Now surface is heated by sunlight.

• More craters on small planets because their lithosphere became solid quickly, while heavy bombardment was still occurring.

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Confusions

• Force of gravity is proportional to both masses, so objects with less mass feel a smaller force.

• Atmosphere’s pressure is due to its particles colliding. When put more molecules in a balloon there are more particles to collide -> more pressure.

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Global Warming Projectdue Wednesday March 17

• Sample 4 web sites taking different positions on whether Global Warming is occurring & whether people are responsible.

• For each site, evaluate the science - Is it good or poor?

• Criteria?


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