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A comprehensive set of vocabulary flashcards covering the major concepts from the lecture notes on the origin of the universe, formation of star systems, the solar system, Earth's subsystems, and Earth's history.
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Big Bang Theory
The universe started from a very small, hot state and expanded over time; the best explanation for the origin of the universe.
Steady State Theory
The universe is always expanding and matter is continuously created to form celestial bodies; the universe has no beginning or end in time.
Cosmic Inflation Theory
Rapid expansion of space-time; the early universe was a rapidly expanding bubble of pure vacuum energy.
Nebular Hypothesis
A star system formed from a rotating, hot gas cloud (nebula) that cooled, shrank, and formed a disk whose rings condensed into planets and satellites.
Planetesimal Theory
Debris from interactions near the Sun coalesced into solid bodies that became planets as they cooled.
Solar System
The Sun and all objects bound to it by gravity, including planets, moons, asteroids, and comets.
Terrestrial Planets
Also called Telluric planets; have solid surfaces and are mainly composed of silicate rocks and metals.
Jovian Planets
Also called Gas giants; primarily made of hydrogen and helium and lack solid surfaces.
Goldilocks Zone
The region around a star where conditions allow liquid water to exist on a planet’s surface.
Ozone Layer
High-altitude layer of ozone that shields living organisms from harmful ultraviolet radiation.
Moon’s Stabilization of Axial Tilt
Earth’s Moon helps stabilize the planet’s axial wobble, contributing to climate stability.
Water
Key element with neutral pH, high specific heat, good heat/conductive properties, and universal solvent; essential for life.
Energy
Key element representing the capacity to do work and drive biological and geological processes.
Time
Key element representing the temporal dimension over which Earth’s history and processes unfold.
Cycle
Key element referring to repeating processes in Earth’s systems (e.g., water cycle, carbon cycle).
Atmosphere (ATMO)
The gaseous envelope surrounding Earth.
Biosphere (BIO)
All living components that allow energy to circulate through ecosystems.
Hydrosphere (HYDRO)
All water on Earth, including oceans, rivers, lakes, groundwater, ice, and glaciers.
Geosphere (GEO)
Earth’s solid portions, including crust, mantle, and core.
Troposphere
Densest atmospheric layer; weather occurs here.
Stratosphere
Layer with ozone and strong horizontal winds.
Mesosphere
Coldest atmospheric layer.
Thermosphere
Hottest atmospheric layer; contains auroras.
Exosphere
Outermost layer of the atmosphere, fading into space.
Lithosphere
Crust and the rigid, upper part of the mantle.
Asthenosphere
Layer between the crust and mantle that is partially molten and deformable.
Mantle
Thick layer between crust and core; includes upper and lower mantle.
Core
Earth’s center; outer core is liquid, inner core is solid.
Mohorovičić Discontinuity (Moho)
Boundary between the crust and the mantle.
Gutenberg Discontinuity
Boundary between the lower mantle and the outer core.
Lehmann Discontinuity
Boundary between the outer core and the inner core.
Primordial Soup
Idea that life began from nonliving matter through simple organic compounds.
Deep-Sea Vents
Hypothesized origin sites for life on Earth, near hydrothermal vents in the deep ocean.
Panspermia
Idea that life on Earth began somewhere in the universe and was carried here by cosmic bodies.
James Hutton
Founder of modern geology; proposed Uniformitarianism—the present process shapes Earth’s history.
Charles Darwin
Developed the theory of natural selection and evolution; studied variation and adaptation.
Andrija Mohorovičić
Seismologist who proposed the boundary between Earth’s crust and mantle (Moho).
Beno Gutenberg
Seismologist who identified the boundary between the lower mantle and outer core (Gutenberg discontinuity).
Inge Lehmann
Seismologist who proposed the existence of a solid inner core (Lehmann discontinuity).
Alexander Oparin
Proposed the primordial soup theory in 1924 to explain the origin of life on Earth.
Stanley Miller
Co-created an experiment (Miller–Urey, 1952) that produced amino acids, supporting Oparin’s theory.
Harold Urey
Co-researcher on the Miller–Urey experiment; helped simulate early Earth conditions.
Catastrophism
Theory that catastrophic events (volcanoes, floods, earthquakes) caused mass extinctions and landform formation.
Uniformitarianism
Geologic processes occurring today also operated in the past, shaping Earth over long times.
Gradualism
Idea that Earth’s changes occur by small steps over long periods of time.