1. Our Earth & Moon (Chapter 16)

3. 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.

4. What do we know about the Earth?  Earth is a relatively small planet.  Oblate spheroid  71% liquid water surface  The Earth is an active terrestrial planet.  7 main tectonic plates Question: Question: What is Pangea?

6. 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

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

8.  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

9. Practice: 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)

10. Atmosphere  The greenhouse effect traps heat near the surface of Earth.  Global warming is the general increase in planet temperatures. 76% Nitrogen (N 2 ) 22% Oxygen (O 2 ) 2% Trace Gasses 76% Nitrogen (N 2 ) 22% Oxygen (O 2 ) 2% Trace Gasses

11. Question: Question: Is the greenhouse effect “bad”?

12. Practice 1)What contributes most to our greenhouse effect? 2)What common molecule increases albedo? 3)What is ozone and why is it important?

13. 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

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

15.  Solar particles interact with Earth's magnetic field.

17. What causes the Aurora? Solar particles hit air molecules Molecules give off light (return to Ground state) Air molecules are “excited”

18. 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

19.  P waves are compression waves. (Pressure Wave) Longitudinal wave  S waves begin as a quick vibration. (Shear Wave) Transverse wave

20. Earth’s 5 Layers Solid inner core (iron and nickel) Liquid Outer Core (convection currents) Molten Mantle (solid rock flows) & Constantly changing surface

21. Earth’s Changing Outer Layers Crust (plates floating on mantle) Surface (shifting plates & weather result in continual change)

22.  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?

23. Image Credit: APOD

24. 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

25. 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

26.  The moon is a satellite of the Earth. 49 Moons would fit across the diameter of the Earth

27. About Our Moon  Cool and Solid  3 Surface features 1/4 size of Earth -387 to 253 °F Regolith

28. Highlands

29. Maria (craters filled with basalt)

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

31. 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?

32.  The Apollo Missions were 1963 – 1972. July 20, 1969 Neil Armstrong steps on Moon Followed by Edwin Aldrin Apollo 11 Mission

34. Giant Impact Theory  Earth was impacted by a Mars-size object after Earth had differentiated. Earth tilt Moon composition