1. Chapter 7 Earth and the Terrestrial Worlds

2. Mercury craters smooth plains, cliffs

3. Venus volcanoes few craters Radar view of a twin- peaked volcano

4. Mars some craters volcanoes riverbeds?

5. Moon craters smooth plains

6. Earth volcanoes craters mountains riverbeds

7. Why have the planets turned out so differently, when they formed at the same time from nearly the same materials?

8. Our Goals for Learning Why is Earth geologically active? What processes shape Earth’s surface? How does Earth’s atmosphere affect the planet? 7.1 Earth as a Planet

9. Why is Earth geologically active?

10. Short answer: the Earth is big enough to still have a hot interior. So what do we know about the interior of the Earth and why is it hot?

11. Internal Structure, by density lithosphere

12. Internal structure, by rock strength The lithosphere is the cool rigid rock that forms a planet’s outer layer: the crust and some of the mantle. The lithosphere “floats” on the lower layers.

13. The thickness of the lithosphere controls many geologic processes

14. Internal Structure of the Terrestrial Planets

15. Sources of Internal Heat 1)Gravitational potential energy of accreting planetesimals 2)Differentiation 3)Radioactivity

16. Why do water and oil separate? A.Water molecules repel oil molecules electrically. B.Water is denser than oil, so oil floats on water. C.Oil is more slippery than water, so it slides to the surface of the water. D.Oil molecules are bigger than the spaces between water molecules.

17. Why do water and oil separate? A.Water molecules repel oil molecules electrically. B.Water is denser than oil, so oil floats on water. C.Oil is more slippery than water, so it slides to the surface of the water. D.Oil molecules are bigger than the spaces between water molecules.

18. Differentiation Layers controlled by density Highest density on the bottom (sinks) Gravity sorts materials by density. Differentiation converts gravitational potential energy to heat.

19. What cools off faster? A.A grande-size cup of Starbucks coffee B.A teaspoon of capuccino in the same cup.

20. What cools off faster? A.A grande-size cup of Starbucks coffee B.A teaspoon of capuccino in the same cup.

21. What cools off faster? A.A big terrestrial planet. B.A tiny terrestrial planet.

22. What cools off faster? A.A big terrestrial planet. B.A tiny terrestrial planet. Why?

23. Heat Drives Geological Activity Convection: hot rock rises, cool rock falls. 1 cycle takes 100 million years on Earth.

24. A large planet… Is still warm inside Has a convecting mantle Has a thinner, weaker lithosphere Has molten rock nearer the surface …which makes it more geologically active

25. Comparing the Planets Which planets have the most and least geological activity?

26. Planetary magnetic fields Moving charged particles create magnetic fields. So can a planet’s core if it is electrically conducting, convecting, and rotating

27. Earth’s Magnetosphere Earth’s magnetic fields protects us from charged particles from the Sun The charged particles can create aurorae (“Northern lights”)

28. How do we know what is inside the Earth? A.We can drill deep inside the Earth. B.We can use optical fibers to see deep inside the Earth. C.X-ray machines allow us to view the inside of the Earth. D.Seismic waves generated by earthquakes probe the Earth’s interior.

29. How do we know what is inside the Earth? A.We can drill deep inside the Earth. B.We can use optical fibers to see deep inside the Earth. C.X-ray machines allow us to view the inside of the Earth. D.Seismic waves generated by earthquakes probe the Earth’s interior.

30. What processes shape Earth’s surface?

31. 1)Impact cratering 2)Volcanism 3)Tectonics 4)Erosion

32. Impact Cratering

33. Moon must be hit as often as Earth. Where are Earth’s craters? Erased by tectonic activity and erosion. The more craters, the older the surface

34. Volcanism Molten rock rises when it is: Less dense than its surroundings. Squeezed by its surroundings. Pushed by expanding trapped gas (water vapor, CO 2, N 2, H 2 S, SO 2 )

35. Volcanism Erases other geologic features Provides gas for our atmosphere Provides water for our oceans

36. Why doesn’t Mars have as much volcanic activity as Earth? A.It’s too far from the Sun, so it cooled off faster. B.It’s smaller than the Earth, so it cooled off faster. C.It might, we just haven’t seen them erupt yet.

37. Why doesn’t Mars have as much volcanic activity as Earth? A.It’s too far from the Sun, so it cooled off faster. B.It’s smaller than the Earth, so it cooled off faster. C.It might, we just haven’t seen them erupt yet.

38. Tectonics and Plate Tectonics Tectonics: any surface reshaping from forces on the lithosphere Plate tectonics: pieces of lithosphere moving around on mantle Responsible for mountains, earthquakes, volcanoes Only Earth has plate tectonics. Internal Heat Required!

39. Erosion Wearing down of geologic features by wind, water and ice (weather) Important on Earth - why?

40. How does Earth’s atmosphere affect the planet ?

41. How does Earth’s atmosphere affect Earth? 1)Erosion 2)Protection from radiation 3)Changes the surface temperature: greenhouse effect 4)Allows the existence of liquid water at the surface

42. Radiation Protection X-ray light absorbed very high in the atmosphere. Ultraviolet light absorbed by ozone (O 3 )

43. The Greenhouse Effect

44. How does the greenhouse effect alter surface temperature?

45. Earth’s atmosphere absorbs light at most wavelengths.

46. Greenhouse effect: Certain molecules let sunlight through but trap escaping infrared photons (H 2 O, CO 2, CH 4 )

47. A Greenhouse Gas Any gas that absorbs infrared Greenhouse gas: molecules with 2 different types of elements (CO 2, H 2 O, CH 4 ) Not a greenhouse gas: molecules with single or 2 atoms of the same element (O 2, N 2 )

48. Greenhouse Effect: Bad? The Earth is much warmer because of the greenhouse effect than it would be without an atmosphere…but so is Venus.

49. What have we learned? Why is Earth geologically active? Internal heat drives geological activity, and Earth retains plenty of internal heat because of its relatively large size for a terrestrial world. This heat causes mantle convection and keeps Earth’s lithosphere thin, ensuring active surface geology. It also keeps part of Earth’s core melted, and the circulation of this molten metal creates Earth’s magnetic field.

50. What have we learned? What processes shape Earth’s surface? The four major geological processes are impact cratering, volcanism, tectonics, and erosion. Earth has experienced many impacts, but most craters have been erased by other processes. We owe the existence of our atmosphere and oceans to volcanic outgassing. A special brand of tectonics— plate tectonics—shapes much of Earth’s surface. Ice, water, and wind drive rampant erosion on our planet.

51. What have we learned? How does Earth’s atmosphere affect the planet? Two crucial effects are (1) protecting the surface from dangerous solar radiation— ultraviolet is absorbed by ozone and X rays are absorbed high in the atmosphere— and (2) the greenhouse effect, without which the surface temperature would be below freezing.