terrestrial planets: earth

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Terrestrial Planets: Earth Mercury Venus Earth Moon Mars Distance 1 AU Orbital Period 1 year Rotation Period 23.9 hours Radius (km) 6378 km Radius (R ) 1 R Mass (kg) 6.0x10 24 kg Mass (M ) 1 M Avg. Surface T 59 ̊F

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Page 1: Terrestrial Planets: Earth

Terrestrial Planets: Earth

Mercury Venus Earth Moon MarsDistance 1 AU

Orbital Period 1 year

Rotation Period 23.9 hours

Radius (km) 6378 km

Radius (R⊕) 1 R⊕Mass (kg) 6.0x1024 kg

Mass (M⊕) 1 M⊕

Avg. Surface T 59 ̊F

Page 2: Terrestrial Planets: Earth

Core: Iron & nickelliquid outer coresolid inner core

Mantle: Mostly Silicate RockSolid (upper mantle) Plastic (lower mantle)

Crust: Silicate Rock & MineralsSolid

Earth: Internal Structure

Trend?

Lithosphere: crust & uppermost mantle

Page 3: Terrestrial Planets: Earth

Differentiation•Denser materials in a liquid sink to the center

Gravity!why?

Implications?

• Planets were molten! (and hotter)

Page 4: Terrestrial Planets: Earth

Terrestrial Planets: Internal Structure

Core: Mantle: Crust:

Metallic, sometimes moltenSilicates & other rocksSilicates

highest densitymoderate densitylowest density

Back to beginning, Excerpt (15:40-18:30)

Page 5: Terrestrial Planets: Earth

Liquid Metal Core + Rotation = Magnetic Field

Planetary Magnetic Fields (B)

Warm planets act as electromagnets!

Current (moving charges) creates magnetic fields

Page 6: Terrestrial Planets: Earth

Liquid Metal Core + Rotation = Magnetic Field

Planetary Magnetic Fields (B)

Larger Liquid Metal Core ➝ Stronger Field

Faster Rotation ➝ Stronger Field

Page 7: Terrestrial Planets: Earth

Magnetic field protects us from the Solar Wind!!

Preserves our Atmosphere!

Page 8: Terrestrial Planets: Earth

Charged particles follow magnetic field lines.

Magnetic Fields on Earth - Create Aurorae!!

Page 9: Terrestrial Planets: Earth

Warm Planets...COOL OFF!Heat Escapes by

Convection in mantle

Conduction through lithosphere

Radiation from surface into space

Internal Heat Escaping Causes Geologic Activity!

Page 10: Terrestrial Planets: Earth

•Carries heat from interior of mantle (plastic) to base of lithosphere (solid)

Mantle Convection

•Solid Lithosphere Blocks Heat...

Page 11: Terrestrial Planets: Earth

...until the Lithosphere cracks!

Mantle Convection

Internal Heat Escaping Causes Geologic Activity: Plate Tectonics

Page 12: Terrestrial Planets: Earth

•Surface cracked into ~12 plates•Plates “float” on mantle •Motion causes geological features

Mantle Convection & Plate Tectonics

Tectonics (“building”): Creation of structures within lithosphere

Page 13: Terrestrial Planets: Earth

Plate Tectonics: Mountain Building

Ex: Himalayas (Indian➔Eurasian, 1cm/yr)

Convergent Plate Boundary - Plates Collide

Subduction:One plate pulled under another

Page 14: Terrestrial Planets: Earth

Ex: East African Rift Zone

Plate Tectonics: Rifts & ValleysDivergent Plate Boundary - Plates Move Apart

Page 15: Terrestrial Planets: Earth

Seafloor Spreading: Plates pull apart, lava seeps up and forms new crust

Plate Tectonics: Ocean Ridges/Seafloor Spreading

Ex: Mid Atlantic Ridge

Page 16: Terrestrial Planets: Earth

San Andreas Fault (Pacific & North American Plates)

Plates slip sideways few m/second!

Plate Tectonics: Earthquakes & Faults

2/27/10: Chilean Earthquake (Nazca/South American Subduction Zone)

1/12/10: Hatian Earthquake (Carribbean/North American Plates)

Page 17: Terrestrial Planets: Earth

Eruption of molten lava onto surface

Hotspot: Place where magma finds a path through the lithosphere

Volcanism (More Geologic Activity!)

Page 18: Terrestrial Planets: Earth

Plate motion over hotspots creates Island ChainsVolcanism on Earth

Kauai

Big Island

Page 19: Terrestrial Planets: Earth

Shaping Planetary Surfaces - 4 Main Processes

•(Plate) Tectonics•Volcanism

What else?

•Impact Cratering•Erosion

⧽Caused by HEAT!