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Section ‘3’

Section ‘3’. Early Evolution of the Earth. ਃ 14 billion years ago, the Big Bang —an incomprehensibly large explosion that sent all matter of the universe flying outward at incredible speeds—occurred.

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Section ‘3’

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  1. Section ‘3’

  2. Early Evolution of the Earth ਃ 14 billion years ago, the Big Bang—an incomprehensibly large explosion that sent all matter of the universe flying outward at incredible speeds—occurred. ਃ The Earth system is powered by energy from two sources: energy from the sun and from the Earth’s interior. ਃ The nebular hypothesis proposes that the bodies of our solar system evolved from an enormous rotating cloud called the solar nebula. ਃMeteorites are the rocky and metallic pieces that remained in orbit. ਃ Planetisimals are large asteroid-size bodies which in a few tens of millions of years accreted into the four inner planets we, call MercuryVenus, Earth, and Mars.

  3. ਃ Formation of the solar system according to the nebular hypothesis: a. The birth of our solar system began as dust and gases (nebula) started to gravitationally collapse. b. The nebula contracted into a rotating disk that was heated by the conversion of gravitational energy into thermal energy. c. Cooling of the nebular cloud caused rocky and metallic material to condense into tiny solid particles. d. Repeated collisions cause the dust-size particles to gradually coalesce into asteroid-size bodies. e. Within a few million years these bodies accreted into the planets. ਃ The continental crust formed gradually over the last 4 billion years. The oldest rocks yet discovered are isolated fragments found in the Northwest Territories of Canada that dates about 4 billion years.

  4. Earth’s Internal Structure ਃ Three basic divisions of Earth’s interior: the iron-rich core, the primitive crust, and the mantle. ਃ Crust is the rocky outer skin and has two different types: - Continental crust: averages 35 to 40 km thick and consists of many rock types. The upper crust has an average composition of a graniticrock called granodiorite, it varies considerably from place to place. - Oceanic crust: roughly 7 km thick and composed of the dark igneous rock basalt. The rocks of the oceanic crust are younger and denser that continental rocks. ਃMantle is a solid, rocky shell that extends to a depth of about 2900 km. ਃPeridotite is the dominant rock type in the uppermost mantle and is richer in the metals magnesium and iron than the minerals found in either the continental or oceanic crust.

  5. ਃTwo types of mantle: - Upper mantle: extends from the crust-mantle boundary down to a depth of about 660 km. It is divided into three parts: ·Lithosphere: consists of the entire crust and uppermost mantle. It’s more than 250 km thick. ·Asthenosphere: beneath the lithosphere and has a depth of 350 km. ·Transition Zone: below asthenosphere and about 410 km to 660 km. - Lower mantle: 2,900 km deep.ਃ Core is composed of iron-nickel alloy with minor amounts of oxygen, silicon, and sulfur. The core is divided into two regions: -Outer core: is a liquid layer about 2,270 km thick. It’s the movement of metallic iron within this zone that generates Earth’s magnetic field. -Inner core: radius of 1,216 km. The iron in the inner core is solid due to the immense pressures that exist in the center of the planet.

  6. The Face of the Earth ਃ The two principal divisions of Earth’s surface: -Continents – the largest features can be grouped into two distinct categories: ·Mountain Belts – the most prominent topographic features of the continents. It was formed within the last 100 million years ·The stable interior – the interior of the continents (cratons) have been relatively undisturbed for the last 600 million years. -Ocean basins – If all water were drained from the ocean basins, a great variety of features would be seen and would be nearly as diverse as that on the continents. Three major topographically distinct units:

  7. ·Continental Margins – portion of the seafloor adjacent to major landmasses. It may include the continental shelf, continental slope, and the continental rise. ·Deep Ocean Basins – between the continental margins and oceanic ridges. ·Oceanic Ridges – broad elevated feature forms a continuous belt that winds for more that 70,000 km around the globe in a manner similar to the seam of a baseball.

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