Solar System from dust cloud
debris (solar nebula) 4.5 billion years ago due to big bang cosmic explosion 15
billion years ago – astrophysicists estimation
Solar nebula
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Rotating, disk shaped mass
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75 % H, 23% He
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Revolve about the centre with gravity concentrated
particles
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Sun is formed
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Outer disk region cooled & condensed, gas
interact chemically & collide with other particles form planets
Protoearth
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Bombarded by particles, heat energy trapped by new
accumulated layer of material
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Growing weight, compression, decomposition of
radioactive elements (uranium/thorium) raise temp.
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1st few hundred million yrs, interior
reach iron/nickel melting point, settle in centre of planet according to
density (density stratified, organized & differentiated layered system)
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Surface cool & solidify (thin crust)
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Oceans & atmosphere forms
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Parts: Solid inner core, Liquid outer core, Mantle,
Upper mantle, Crust
Lithosphere
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Thin rigid skin above mantle 1000°C
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Continental crust 25-90km, avr. 35km, Si Na K Al Ca O Mg Fe (2.8 g/cm3)
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Oceanic crust 5-10km, avr. 7km, Si Mg Fe O Ca
(3.0g/cm3)
Asthenosphere
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Weak, ductile, partially melted, hot, slowly flowing
(4.5 g/cm3)
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600km, Si Mg Fe O / Magnesium-iron silicates
Moho
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Chemical boundary between crust & mantle
(Andrija Mohorovicic discontinuity)
Lower mantle
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Rigid dense to core (5.5 g/cm3)
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1900km, Si Mg Fe O / Magnesium-iron silicates
Outer core
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Liquid, 3200°C, 2200km, 10 g/cm3
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Fe S
Inner core
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Solid, 5500°C, 1300km, 12 g/cm3
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Fe Ni
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