The Earth as a Terrestrial Planet

Slides:



Advertisements
Similar presentations
Plate Tectonics What evidence do scientists have to support the fact that the Earth’s crust is continuously moving?
Advertisements

Astronomy 1010 Planetary Astronomy Fall_2013 Day-28.
Carbon Dating Used for determining the age of earth materials
Planet Earth.
Please Remember: Last day to withdraw without a grade is Feb. 27th.
Structure of the Earth Crust = solid outermost layer Mantle = middle layer Core = inner layer outer core = liquid inner core = solid.
4A Earth and Moon Our home and our nearest neighbor.
Planetary Geology. Layering of Terrestrial Worlds The process of differentiation separates materials with different densities Dense metals fall.
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.
Heat and Plate Tectonics
 Crust – Rocky surface of the earth  Mantle – A thick layer of rock above the Outer core  Outer Core – Molten lava  Inner Core – Very hot metal.
The Solar System.
Sponge: List the layers of the Earth’s atmosphere.
ASTR178 Other Worlds A/Prof. Orsola De Marco ts/ASTR178/
28 Sep 2000ASTR103, GMU, Dr. Correll1 Ch 05--Earth and Moon.
Lecture 22. Terrestrial Planets What are they like? Why? MercuryEarthVenusMars.
Natural Disasters Earth’s Internal Structure Introduction to Plate Tectonics Earth’s Energy Sources and Systems.
1A2 Geography 27 th January 2015 Objectives: To introduce students to the structure of the Earth’s interior, plate tectonics, and plate boundaries.
The Earth and Its Moon The Earth Solid inner core, liquid outer core atmosphere - 50km thick magnetosphere - charged particles caught in Earth’s magnetic.
Evidence for Early Earth. In order to think about the formation of Earth, there are some assumptions that must be made. Earth today is cooler than early.
Earth’s Internal Heat.
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.
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 6: Due Today, March 22. Smartworks Chapter 7: Due Friday, March st Quarter.
The Earth as a Terrestrial Planet Mass -- 6 x gm (6 x kg) Size -- diameter 12,756 km (eq.) Density – mean 5.5 gm/cm 3 Surface -- 71% water.
The Earth and it’s layers
GEOL3045: Planetary Geology Lysa Chizmadia Earth-Moon System Lysa Chizmadia Earth-Moon System.
Chapter 12 Earth’s Interior
Daily Review #1 What happens in radioactive decay? Define half-life.
Convection Current in the Mantle SAYRO PAW. The Four Layers of Earth Inner Core Outer Core Mantle Crust The inner core is the hottest layer in the Earth.
Plate Tectonics Understanding what causes the plates to move.
© Sierra College Astronomy Department Terrestrial Geology Basics.
Earth’s Structure Test Review Drill: Which part of the Earth creates the magnetic fields? How are they produced? Objective: SWBAT create a diagram of the.
November 14,  I will return your exams tomorrow. (Grades Look Good)  Pick up a textbook from the library  We will start Unit 3 today( Tectonic.
Notes: Earth/Moon Formation 3/11. 1.Explain the three sources of heat that contributed to the high temperature of the newly formed Earth. (p. 688). The.
The Geosphere. Changes occur on the Earth constantly: Molten rock flows from volcanoes Hurricanes batter beaches and change coastline Earthquakes shake.
Structure of the earth. Inner Core – This is in the centre of the earth where it is hottest. It is solid and consists of Iron and Nickel with temperatures.
Journey to the Center of Earth
Sponge: List the layers of the Earth’s atmosphere.
Earth Composition, Continental Drift and Plate Tectonics
Earth as a System Scientists divided this system into four parts:
The Earth Inside and Out
Plate Tectonics.
Chapter 6 Study Guide.
What is the Earth made of?
Plate Tectonics.
What is the Earth made of?
Jeopardy! Vocabulary 1 Misc. Erosion & Weathering Earth’s Interior
Connecting Planetary Interiors and Surfaces
Astronomy 340 Fall September 2005 Class #7.
Forces of Change With a partner, brainstorm a list forces that change the surface of our planet.
Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds
The Earth as a Terrestrial Planet
Plate Tectonics continental drift
The Geosphere.
EARTH OUR HOME IN SPACE.
A double ringed basin on Mercury image last week by the Messenger spacecraft during a swing past Mercury. Double and multiple ringed basins, although.
Geology.
Unit 1: Introduction to Earth Science part 3
Earth How We Know What We Know The Inside Volcanoes The Outside Drills
The Terrestrial Planets
Structure of the Earth.
Brief Summary.
Earth’s Internal Heat.
Earth Science Plate Tectonics Chapter 12.
The Moon.
Plate Tectonics Write on RIGHT Side.
The Terrestrial Planets
DO NOW Get out your notes from yesterday – “Origin of Our Solar System”. Get out Review #1 that was homework.
Crust mantle Outer core Inner core.
Presentation transcript:

The Earth as a Terrestrial Planet Mass -- 6 x 1027 gm (6 x 1024 kg) Size -- diameter 12,756 km (eq.) Density – mean 5.5 gm/cm3 Surface -- 71% water

Why ? – differentiation of elements Interior Crust Mantle Core Densities – crust < 3 gm/cm3 -- mantle 3.5 gm/cm3  ? Very dense core ~ 15 gm/cm3  Fe/Ni Outer core – molten (5000-7000K) Inner core – solid ~ 7000K Why ? – differentiation of elements Rotating molten core produces magnetic field

Age Dating of Earth Radioactive decay -- uranium, plutonium, thorium U238  Pb206 Th232  Pb208 using known half-life Rocks on Earth -- newly formed to ~ 3.5 - 4 x 109 yrs Oldest Moon rocks – 4.5 – 4.6 x 109 yrs

Our Active Earth – Plate Tectonics or Continental Drift

Consequences– earthquakes, volcanoes, mountain building

San Andreas Fault

Caused by convective currents in mantle transfers heat to crust

The Earth at Night

The Earth and Moon as a Double Planet Mmoon/Mearth = 0.012 (1/80th) Rmoon/Rearth = 0.27 (1/4th) Largest in Solar System

Surface Features Craters Mare Highlands

Origin of the Moon Sister planet – by fission Co-accretion – at same distance, same material Capture – not dynamically feasible Current theory – massive collision – computer modeling

Lunar rocks and soil samples

Age Dating Lunar rocks and soil samples Mare – 3.8 x 109 yrs Highlands – 4.3 – 4.6 x 109 yrs