Chapter 5: Earth and Its Moon We know the internal structure of the Earth and Moon by observing how Earthquake waves propagate through the interior. Compression.

Slides:



Advertisements
Similar presentations
LECTURE 9, SEPTEMBER 23, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT
Advertisements

The Living Earth Chapter Nine.
Survey of Astronomy Astro1010-lee.com Chapter 6 Our Living Earth.
The __-_____c Ridge is the largest tectonic feature on our planet. Mid-Atlantic 1.
Survey of Astronomy Astro1010-lee.com Chapter 6 Our Living Earth.
Clicker Questions Chapter 5 Earth and Its Moon Copyright © 2010 Pearson Education, Inc.
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
Earth Astronomy 311 Professor Lee Carkner Lecture 12.
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
Physics 202: Introduction to Astronomy – Lecture 9 Carsten Denker Physics Department Center for Solar–Terrestrial Research.
The Earth’s Structure. The Earth’s Lithosphere S and P Waves S and P waves travel at different speeds Both waves travel through sold material Only P.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 9 The Living Earth CHAPTER 9 The Living Earth.
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
Period 2. What is magnetic declination??? A) Magnetic declination is the angle between you and Earth when you are standing on a level surface. B) Magnetic.
The Living Earth. Industrial chemicals released into the atmosphere have damaged the ozone layer in the stratosphere.
Earth’s Magnetic Field The Magnetosphere And The Van Allen Belts.
Chapter 7.
Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide.
Chapter 20 Planet Earth.
© 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Chapter 5 Earth and Moon. What do you think? Will the ozone layer, which is now being depleted, naturally replenish itself? Does the Moon have a dark.
Sponge: List the six layers of the Earth.. Atmosphere A mixture of gases: N 2 78% O 2 21% Ar0.9% CO %
1. angular resolution ability to distinguish between two adjacent objects in the sky.
The Earth and Its Moon The Earth Solid inner core, liquid outer core atmosphere - 50km thick magnetosphere - charged particles caught in Earth’s magnetic.
Earth’s Moon  It takes 27.3 days for the moon to revolve around the Earth relative to a background star (sidereal month).  Because Earth also revolves.
Made by: Savannah Secrest Presented by: Bradford.
Sun, Moon, Earth, How do they work together to help life survive? Magnetosphere.
Chapter 7 Earth and the Terrestrial Worlds. Mercury craters smooth plains, cliffs.
In Nuclear fusion, four hydrogen atoms fuse together to form Helium and a lot of energy!
A Transitional Fossil 375 Ma fish: flat nose, beginnings of limbs “Missing link” between fish and life on land.
1 The Earth-Moon System The Earth’s Atmosphere Unique among terrestrial planets in its composition –78% Nitrogen (N 2 ) –21% Oxygen (O 2 ) –0.9% Argon.
The Earth-Moon System The Earth’s Atmosphere
Chapter 4: Earth and Moon. From the Earth, Venus appears as a white planet in the evening sky or the morning sky. From Mars, the Earth might appear as.
Have you ever wondered how a compass works? Compasses How many of you have used a compass before? Can you explain how it works?
Chapter 5 Earth and its Moon. The Earth Table 5-1 Some Properties of Earth and the Moon.
Magnetic Earth Chapter 1 Section 3 Pages Objective: Understand the Earth’s magnetic field and Compare magnetic and geographic poles. Compass:
Chapter 7 Earth. Mantle Two-part core Thin crust Hydrosphere (oceans) Atmosphere Magnetosphere Structure of Planet Earth.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 5 Earth and Its Moon.
Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for.
Lecture 17. Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12 th.
Earth’s Interior Jeopardy
The Earth’s Magnetic Field
Chapter 8 The Earth. How do we know that planet Earth really revolves and rotates? What is Aberration and what does it prove about the Earth? What is.
Universe Tenth Edition Chapter 9 The Living Earth Roger Freedman Robert Geller William Kaufmann III.
Earth Earth is the third planet from the sun. It has volcanoes like on Venus and Mars, craters like those found on Mercury, and swirling weather systems.
© Sierra College Astronomy Department Terrestrial Geology Basics.
Earth’s Magnetic Field Text 5.6 pp The Magnetosphere And The Van Allen Belts.
It comes in layers Just like the earth’s interior, the atmosphere is made of layers Troposphere Stratosphere Mesosphere Ionosphere.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
The Earth Famous picture Famous picture Oblateness of (demo) Oblateness of (demo) Average density is ~5.5 g/cm 3 Average density is ~5.5.
Alta High Astronomy Chapter 7 Earth: Our Home in Space.
Learning Targets I can explain how the Earth’s magnetic field protects from harmful radiation. The Sun Vocabulary Magnetosphere Gauss Declination.
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 7: Due Friday, March st Quarter Observing Nights: Tues & Thurs, March.
Sponge: List the six layers of the Earth.
© 2017 Pearson Education, Inc.
© 2017 Pearson Education, Inc.
Earth as a Magnet.
Earth’s Magnetic Field ~Magnetosphere
Earth’s Magnetic Field
Ch. 8: Earth as a Planet.
Goals Compare the Earth and the Moon and explain differences Describe the effects of gravity between the Earth and Moon Explain the greenhouse effect Discuss.
5.3 Atmospheres Troposphere is where convection takes place – responsible for weather.
Astronomy 04 The Solar System
Earth’s Magnetic Field
Planet Earth.
Earth: The Standard of Comparative Planetology
PLAYING THE MAGNETIC FIELD
Earth’s Magnetic Field
Round from pull of gravity over time
Presentation transcript:

Chapter 5: Earth and Its Moon We know the internal structure of the Earth and Moon by observing how Earthquake waves propagate through the interior. Compression and transverse waves can each travel through solids but only compression waves can travel through liquid. Therefore we know that at least part of the Earth’s core is liquid. Our information about the Moon is limited because there are few Moonquakes. We think the core is solid

Chapter 5: Earth and Its Moon Because the Earth has a liquid conducting core that rotates, electrical currents are set up which creates a strong magnetic field. Charged particles tend to spiral around magnetic field lines and get reflected when they become too strong. The Earth’s field is such that the solar wind particles are trapped in the Van Allen radiation belts Magnetosphere

Chapter 5: Earth and Its Moon Sometimes the reflection point occurs low in the atmosphere. As the charged particles slam into the atoms and molecules in the atmosphere they excite them and cause them to fluorescence. We call these events the Aurora. The Moon has no magnetic field.

Chapter 5: Earth and Its Moon Plate Tectonics The surface of the Earth consists of several plates which float on the molten interior. As these plates crash into each other they produce mountains. As they slide away from each other they produce trenches. The plates move about 2 cm/year

Chapter 5: Earth and Its Moon Origin of the Moon Video The giant impact theory best explains why the Moon is very much like the Earth’s mantel and contains very little nickel/iron. The creation and evolution of the Earth and Moon are closely related