Earth Science 11 – Review: Formation of Universe and Earth Concepts (Vocabulary Flashcards)

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Vocabulary flashcards covering formation of the universe, solar system, geologic time, Earth’s early history, planetary habitability, Earth’s subsystems and layers, and rock types with key processes.

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64 Terms

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Big Bang Theory

The widely accepted theory that the universe began ~13.8 billion years ago from a hot, dense singularity and has since expanded; evidence includes CMBR, redshift, and light-element abundances.

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singularity

A hot, dense point from which the universe originated in the Big Bang model.

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Cosmic Microwave Background Radiation (CMBR)

Faint radiation leftover from the early universe; key evidence for the Big Bang.

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Redshift

The apparent increase in wavelength of light from distant galaxies, indicating they are moving away and the universe is expanding.

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Abundance of light elements

Predominance of hydrogen and helium produced in the early universe, supporting Big Bang nucleosynthesis.

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Steady State Theory

Alternative to the Big Bang proposing the universe has no beginning or end, with continuous creation of matter to keep density constant.

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Inflation Theory

Extension of the Big Bang that explains a rapid, exponential expansion of the universe in a fraction of a second after its origin.

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Nebular Hypothesis

Kant and Laplace proposal that the Solar System formed from a collapsing nebula ~4.6 billion years ago, with the Sun at the center and planets forming from the disk.

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Sun

The central star of the Solar System around which the planets orbit.

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Mercury

Terrestrial planet; smallest; has little to no atmosphere.

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Venus

Terrestrial planet; hottest; thick atmosphere.

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Earth

Terrestrial planet; habitable; contains liquid water and life.

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Mars

Terrestrial planet; the Red Planet; thin atmosphere.

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Jupiter

Gas giant; largest planet; features the Great Red Spot.

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Saturn

Gas giant with a prominent ring system.

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Uranus

Ice giant with an extreme axial tilt; blue-green color from methane.

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Neptune

Ice giant with strong winds; farthest recognized planet in the notes.

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Asteroids

Rocky or metallic bodies mostly found in the asteroid belt.

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Meteoroids

Small space rocks that originate from comets or asteroids or other planets.

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Comets

Bodies composed of ice, rocks, and dust that develop tails when near the Sun.

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Kuiper Belt

Region beyond Neptune; source of short-period comets.

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Asteroid Belt

Region between Mars and Jupiter; source of asteroids.

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Oort Cloud

Distant region beyond the Kuiper Belt; source of long-period comets.

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Geologic Time Scale

Hierarchical system of time units used in geology: eon, era, period, epoch.

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Eon

Largest subdivision of geologic time; lasts hundreds of millions to billions of years.

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Era

Subdivision of an eon; lasts tens to hundreds of millions of years.

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Period

Subdivision of an era; lasts tens of millions of years.

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Epoch

Subdivision of a period; lasts millions of years.

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Hadean Eon

4.6–3.8 billion years ago; intense meteorite bombardment; formation of oceans and atmosphere; Theia impact forming the Moon.

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Archean Eon

3.8–2.5 billion years ago; methane-rich atmosphere with little oxygen; oceans; formation of continents; oldest rocks like stromatolites and apex chert.

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Proterozoic Eon

2.5 billion years ago to 542 million years ago; atmospheric oxygenation; origin and diversification of eukaryotic life; appearance of multicellular life.

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Phanerozoic Eon

Eon characterized by visible life; includes Paleozoic, Mesozoic, and Cenozoic.

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Paleozoic Era

Early life with marine shells, amphibians; reptiles appear; trilobites common.

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Mesozoic Era

Continents drifted; dinosaurs; major plant and animal changes; ends with mass extinctions.

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Cenozoic Era

Mountains uplifted; mammals rise; development of modern fauna and flora; Ice Ages; Homo genus appears.

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Goldilocks Zone

Habitable zone around a star where conditions may allow liquid water on a planet’s surface.

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Liquid water

Essential requirement for life as we know it; presence on a planet helps define habitability.

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Right distance to the Sun

Optimal solar distance to maintain liquid water and stable climate.

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Plate tectonics

Movement of Earth's lithospheric plates that recycles materials and shapes the crust.

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Right size

Sufficient planetary size to retain an atmosphere and sustain geologic activity.

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Right gravity

Gravity strong enough to hold an atmosphere and support life processes.

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Atmosphere

Layer of gases surrounding Earth; protects and sustains life.

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Moon (Luna)

Earth’s natural satellite influencing tides and climate stability.

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Magnetosphere

Magnetic field that shields the planet from harmful solar radiation.

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Energy

Sustaining energy input from the Sun to drive climate and life processes.

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Time

Sufficient time for chemical evolution and complex life to develop.

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Geosphere

The solid Earth: rocks, magma, and soil.

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Atmosphere (Earth layer)

Layer of gases surrounding the planet.

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Hydrosphere

All of Earth’s water: oceans, rivers, groundwater, etc.

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Biosphere

All living organisms on Earth.

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Crust

Outermost Earth layer; oceanic crust (5–10 km, basalt) is thinner; continental crust (30–70 km, granite) is thicker.

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Mantle

Largest Earth layer (up to ~2900 km); molten rock and convection currents; includes upper and lower mantle.

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Core

Earth’s center: outer core is liquid; inner core is solid.

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Mohorovičić discontinuity

Boundary between crust and upper mantle.

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Gutenberg discontinuity

Boundary between lower mantle and outer core.

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Lehmann discontinuity

Boundary between outer and inner core.

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Weathering

Natural breakdown of rocks and minerals on Earth’s surface into smaller pieces.

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Erosion

Movement of rock, soil, or sediment by wind, water, or ice after weathering.

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Magmatism

Movement or activity of magma; molten rock formed by melting existing rocks under high temperature/pressure.

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Igneous rocks

Rocks formed from cooling and solidification of molten material; extrusive (volcanic) or intrusive (plutonic).

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Sedimentary rocks

Rocks formed from accumulation and compression of sediments; often contain fossils.

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Lithification

Process by which sediments become sedimentary rocks via compaction and cementation.

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Metamorphic rocks

Rocks formed from pre-existing rocks transformed by heat or pressure.

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Metamorphism

Transformation of a parent rock into a new mineralogically/structurally different rock due to heat/pressure.