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Earth Science Lecture Notes Review

Formation of the Moon

  • Early Theories:

    • Capture Hypothesis: Earth captured a small planet, which became the Moon.

    • Accretion Hypothesis: Earth and Moon formed together from the same accretion disc.

    • Collision (Giant Impact) Hypothesis: Current understanding is that a Mars-sized protoplanet (Theia) struck the Earth, creating a molten Earth and a debris field that coalesced to form the Moon.

Collision Theory (Giant Impact Theory)

  • Core Idea: The Moon formed from a collision between the Earth and another small planet, about the size of Mars.

  • Debris collected in orbit around Earth to form the Moon.

  • The colliding body is sometimes called Theia, named after the mythical Greek Titan, the mother of Selene (goddess of the Moon).

  • Analysis of lunar rocks (2016) suggests a direct hit, causing thorough mixing of both parent bodies.

Evidence Supporting Collision Theory

  1. The Moon is less dense than the Earth.

  2. Samples of rock from the Moon show that its surface was once molten.

  3. The Moon has a small iron core, like the Earth.

  4. Evidence outside the Solar System supports this theory.

  5. The collision theory fits with the theory of how the Solar system was formed.

  6. The composition of rocks on the Moon and the Earth are the same.

Evidence Contradicting Collision Theory

  1. The surface of the Earth doesn't appear to have ever been molten, while the collision would have caused the surface to melt.

  2. Venus has no moon, despite collisions being common in the early Solar System (scientists would expect Venus to have formed a moon the same way).

  3. The composition of rocks on the Moon would be more similar to Theia than rocks on Earth.

Nebulae

  • A nebula is a giant cloud of dust and gas, primarily hydrogen and helium, in space.

  • Nebulae originate from gas and dust thrown out by the explosion of a dying star, such as a supernova.

  • Other nebulae are regions where new stars are beginning to form and are called "star nurseries."

Examples of Nebulae

  • Orion Nebula (easily seen from the northern hemisphere)

  • Carina Nebula (easily seen from the southern hemisphere)

Stellar Nursery

  • An area of outer space within a dense nebula where gas and dust are contracting, resulting in the formation of new stars.

Star Formation

  • Stars form when clumps of hydrogen and other gases collapse under their own gravity.

  • As the collapse continues, the central clump grows stronger, and the gas heats up due to the conversion of gravitational potential energy into thermal energy.

  • When the temperature gets high enough, nuclear fusion ignites, forming a protostar.

  • The protostar emits enough energy to counterbalance its own gravitational pressure, and a cloud of material remains around the newly born star.

  • This cloud remnant is the protoplanetary disk, where planets may form around the star.

Star Birth

  • Stars are born from nebulae.

  • As the nebula gains mass, its gravitational forces build.

  • The inner part of the cloud heats up, becoming a protostar.

  • When the core heats up enough to cause nuclear fusion of hydrogen into helium, a star is born.

Forces Balancing Stars

  • Inward gravity of the star.

  • Outward push of pressure created by heat energy due to fusion reactions.

  • These two forces keep a star in equilibrium and hinder its collapse.

Tectonics

  • The continental drift hypothesis, proposed by Alfred Wegener, stated that the continents were assembled to form the supercontinent Pangaea and moved through time.

Evidence for Continental Drift

  • Fit of the continents.

  • Fossil evidence (similar fossils on different continents).

  • Ancient mountain ranges.

  • Past climate evidence (e.g., glaciers at the South Pole, swamps in tropical regions).

Plate Tectonics

  • Convection currents drive the movement of Earth's rigid tectonic plates in the planet's fluid molten mantle.

  • Where convection currents rise up towards the crust's surface, tectonic plates move away from each other in seafloor spreading.

Types of Tectonic Plate    s

  • Oceanic Plates:

    • Consist of oceanic crust called "sima" (silicon and magnesium).

    • Formed by divergent plate boundaries.

  • Continental Plates:

    • Consist of continental crust called "sial" (silicon and aluminum).

    • Formed primarily by convergent plate boundaries.

Volcanoes

  • A volcano is a feature in Earth’s crust where molten rock is squeezed out onto the Earth’s surface.

  • Molten rock is called magma beneath the surface and lava when it erupts from a volcano.

  • Volcanoes release lava, gases, ash, and solid rock.

Earth's Magnetic Field

  • Earth's magnetic poles have swapped approximately 200 times in the last 100 million years.