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The Earth as a Terrestrial Planet

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Presentation on theme: "The Earth as a Terrestrial Planet"— Presentation transcript:

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

2 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 ( K) Inner core – solid ~ 7000K Why ? – differentiation of elements Rotating molten core produces magnetic field

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

4 Our Active Earth – Plate Tectonics or Continental Drift

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6 Consequences– earthquakes, volcanoes, mountain building

7 San Andreas Fault

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9 Caused by convective currents in mantle transfers heat to crust

10 The Earth at Night

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

12 Surface Features Craters Mare Highlands

13 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

14 Lunar rocks and soil samples

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


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