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Our Earth & Moon (Chapter 16)

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Page 1: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Our Earth & Moon

(Chapter 16)

Page 2: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for
Page 3: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Student Learning Objectives

• Compare and contrast interior structures of the Earth & Moon

• Describe surface features for our Earth & Moon

• State the theory for the origin of our moon.

Page 4: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

What do we know about the Earth?

Earth is a relatively small planet.

Oblate spheroid71% liquid water surface

The Earth is an active terrestrial planet.

7 main tectonic plates

Question: What is Pangea?

Page 5: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for
Page 6: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Fun Earth Facts• Travels through space at 660,000 miles per hour

• Weighs 6,588,000,000,000,000,000,000,000 tons

• Rotates more slowly in March than in September

• Rotates at an average speed of 283 mph

Page 7: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

If the oceans were evenly distributed over the entire surface of the Earth, the water would be approximately 2 miles deep at every point

Page 8: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Earth reflects an average of 30% of the sunlight that is incident upon the surface.

Earth Albedo= 0.306

Venus Albedo = 0.750

Planet Albedo

Page 9: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Practice: What does it mean for a planet to be in the habitable zone?

Planet Earth is composed primarily of metals.

Fe, O, Si, Mg

Earth is in the “Habitable Zone” (–60º F to +120º F)

Page 10: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Atmosphere

The greenhouse effect traps heat near the surface of Earth.

Global warming is the general increase in planet temperatures.

76% Nitrogen (N2)22% Oxygen (O2)2% Trace Gasses

Page 11: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Question: Is the greenhouse effect “bad”?

Page 12: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Practice

1) What contributes most to our greenhouse effect?

2) What common molecule increases albedo?

3) What is ozone and why is it important?

Page 13: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Earth’s Magnetic Field

The Earth is surrounded by a magnetic field, and the poles switch!

http://www.nasa.gov/topics/earth/features/2012-poleReversal.html

Page 14: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

The motion of ionized particles inside Earth's liquid core coupled with Earth’s rotation induces the magnetic field.

Page 15: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Solar particles interact with Earth's magnetic field.

Page 16: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for
Page 17: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

What causes the Aurora?

Solar particles hitair molecules

Molecules give off light(return to Ground state)

Air moleculesare “excited”

Page 18: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

How do we know the interior structure of the Earth?

Earthquake waves allow mapping of interior.

P waves travel through both solid and liquid matter

S waves travel through only solid matter

Page 19: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

P waves are compression waves. (Pressure Wave)

Longitudinal wave

S waves begin as a quick vibration. (Shear Wave)

Transverse wave

Page 20: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Earth’s 5 LayersSolid inner core

(iron and nickel)

Liquid Outer Core(convection currents)

Molten Mantle(solid rock flows)

&

Constantly changing surface

Page 21: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Earth’s Changing Outer Layers

Crust(plates floating on mantle)

Surface(shifting plates & weather result in continual change)

Page 22: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

The Moon is about 25,000 miles more distant at apogee than at perigee.

Harvest Moon

It would take an average of 135 days to drive to the moon at a speed of 70 mph

What are the characteristics of the Moon?

Page 23: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Image Credit: APOD

Page 24: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Fun Moon Facts• Earth-Moon distance is

an average of 239,000 miles or 0.00257 AU

• More than 100 spacecraft have been launched to explore the moon

Page 25: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

• If the Sun were as tall as a typical front door

– Earth would be the size of

a nickel

– The Moon would be the size of a pea

Page 26: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

The moon is a satellite of the Earth.

49 Moons would fit across the diameter of the Earth

Page 27: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

About Our Moon

Cool and Solid

3 Surface features

1/4 size of Earth-387 to 253 °F

Regolith

Page 28: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Highlands

Page 29: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Maria (craters filled with basalt)

Page 30: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

The moon is egg shaped with the large end pointed towards earth.

Page 31: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Practice

1) Why is the temperature range larger on the Moon than it is on Earth?

2) Compare the interior layers of the Earth and Moon. Are they relatively similar or very different?

Page 32: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

The Apollo Missions were 1963 – 1972.

July 20, 1969Neil Armstrong steps on Moon

Followed by Edwin Aldrin

Apollo 11 Mission

Page 33: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for
Page 34: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for

Giant Impact Theory

Earth was impacted by a Mars-size object after Earth had differentiated.

Earth tilt

Moon composition

Page 35: Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for