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Vocabulary flashcards covering major terms and definitions from the provided Earth science and astronomy lecture notes.
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Galaxy
A gravitationally bound system of stars, stellar remnants, and interstellar gas and dust.
Elliptical Galaxy
Galaxy whose lines of equal brightness form concentric ellipses; lacks spiral arms.
Spiral Galaxy
Galaxy with spiral-shaped arms extending from a central nucleus, e.g., the Milky Way.
Irregular Galaxy
Grainy, highly irregular galaxy with no symmetry or defined nucleus.
Barred Spiral Galaxy
Spiral galaxy featuring a central bar-shaped structure of stars.
Planet
Large body that orbits a star and shines by reflected light.
Natural Satellite
Body that revolves around a planet and reflects starlight; e.g., the Moon.
Galilean Moons
The four largest moons of Jupiter discovered by Galileo: Io, Europa, Ganymede, Callisto.
Nebula
Interstellar cloud of dust and gas from which new stars form.
Quasar
Extremely luminous, distant active galactic nucleus.
Pulsar
Highly magnetized, rotating neutron star emitting periodic radio pulses.
Star
Self-luminous sphere of gas held by gravity; energy from nuclear fusion.
Protostar
Early stage star formed from collapsing nebular gas and dust.
Sirius
Brightest star system in Earth’s night sky.
Black Hole
Stellar remnant whose gravity is so strong that not even light escapes.
White Dwarf
Dense, Earth-sized, cooling remnant of a low-mass star.
Nova
Star that suddenly increases in brightness before fading.
Giant Star
Low-mass star swollen near the end of its life.
Supergiant Star
Very massive, luminous star nearing end of life; largest and brightest type.
Comet
Icy body that develops a glowing coma and tail when near the Sun.
Meteor
Visible streak of light from debris burning in a planet’s atmosphere.
Meteoroid
Rocky or metallic debris in outer space before it enters an atmosphere.
Meteorite
Fragment of meteoroid that survives passage through atmosphere and hits the ground.
Dark Matter
Unseen mass that exerts gravitational effects yet emits no detectable light.
Dark Energy
Mysterious form of energy thought to accelerate cosmic expansion.
Open Universe
Cosmic model where gravity is too weak to halt expansion, so it continues forever.
Closed Universe
Model in which gravity eventually reverses expansion, causing a Big Crunch.
Flat Universe
Universe whose expansion slows but never stops; overall spatial flatness.
Accelerating Universe
Currently accepted model where expansion speeds up due to dark energy.
Big Bang Theory
Idea that the universe began from an extremely hot, dense state and has been expanding.
Hubble’s Law
Relationship v = H₀d showing galaxy recessional velocity is proportional to distance.
Cosmic Microwave Background
Leftover thermal radiation from the Big Bang filling all space.
Singularity
Infinitely dense point that marks the universe’s beginning in Big Bang theory.
Inflation
Brief epoch of exponential cosmic expansion immediately after the Big Bang.
Planck Time
Earliest meaningful moment after the Big Bang (~10⁻⁴³ s).
Solar System
Sun and the bodies gravitationally bound to it, including planets, moons, and debris.
Terrestrial Planets
Rocky, high-density planets: Mercury, Venus, Earth, Mars.
Jovian Planets
Gas/ice giants with many moons: Jupiter, Saturn, Uranus, Neptune.
Mercury
Sun-skimming planet with no atmosphere; 88-day revolution.
Venus
Thick-atmosphere planet with retrograde rotation; brightest after Sun and Moon.
Earth
Only known habitable planet; possesses 1-atm atmosphere and one moon.
Mars
Thin-atmosphere ‘Red Planet’ featuring Olympus Mons and 687-day year.
Jupiter
Largest planet, 67 moons, hydrogen-helium atmosphere, Great Red Spot storm.
Saturn
Gas giant with prominent ring system and about 61 known satellites.
Uranus
Methane-blue ‘sideways planet’ whose axis is nearly parallel to its orbit.
Neptune
Distant ‘windy planet’ with Great Dark Spot and dynamic atmosphere.
Astronomical Unit (AU)
Average Earth-Sun distance, about 150 million km or 8.3 light-minutes.
Asteroid
Rocky or metallic minor body, mostly in belt between Mars and Jupiter.
Coma (Comet)
Bright, fuzzy sheath of gas and dust around a comet’s nucleus.
Halley’s Comet
Famous periodic comet visible from Earth roughly every 75–76 years.
Dwarf Planet
Solar-orbiting body too small to clear its orbit; e.g., Pluto, Eris.
Kuiper Belt
Region beyond Neptune containing icy bodies and dwarf planets.
Sun
Middle-aged G-type star; central energy source of the Solar System.
Core (Sun)
Innermost solar layer where nuclear fusion occurs.
Solar Envelope
Radiative and convective zones surrounding the Sun’s core.
Chromosphere
Reddish solar layer above photosphere visible during eclipses.
Photosphere
Visible ‘surface’ layer of the Sun where sunlight is emitted.
Corona
Outer, tenuous solar atmosphere seen as halo during total eclipse.
Sunspot
Dark, cooler patch on photosphere linked to magnetic activity.
Solar Flare
Sudden brightness flash ejecting energetic particles from the Sun.
Solar Wind
Stream of charged particles flowing outward from the Sun.
Aurora Borealis
Light display produced when solar wind particles interact with Earth’s magnetosphere.
Phases of the Moon
Regular changing illuminated shape: new, first quarter, full, third quarter, etc.
Solar Eclipse
Event where Moon passes between Sun and Earth, casting a shadow on Earth.
Lunar Eclipse
Event where Earth’s shadow falls on the Moon.
Spring Tide
Enhanced high-low tide range when Sun, Moon, Earth are aligned.
Neap Tide
Reduced tide range when Sun and Moon are at right angles to Earth.
Geocentric Model
Ancient view placing Earth at the center of the universe (Ptolemy).
Heliocentric Model
Model placing the Sun at the center of the Solar System (Copernicus, Galileo).
Nebular Hypothesis
Theory that planets formed from a collapsing rotating nebular cloud.
Vortex Theory
Descartes’ idea of whirlpool motions shaping planetary orbits.
Collision Theory (Buffon)
Hypothesis that a comet’s collision with the Sun produced planets.
Tidal Hypothesis
Jeans-Jeffreys idea that a passing star pulled material from the Sun to form planets.
Solar Nebular Theory
Modern refined nebular hypothesis involving a rotating disk and protostar.
Planetisimal Theory
Chamberlin & Moulton model where small solid bodies accreted into planets.
Lithosphere
Rigid outer layer consisting of crust and uppermost mantle.
Asthenosphere
Ductile upper mantle layer enabling plate movement.
Mesosphere (Earth)
Solid lower mantle beneath the asthenosphere.
Outer Core
Liquid iron-nickel layer generating Earth’s magnetic field.
Inner Core
Solid iron-nickel center formed by pressure freezing.
Mohorovičić Discontinuity
Boundary between Earth’s crust and mantle.
Continental Drift Theory
Wegener’s idea that continents moved from a supercontinent called Pangaea.
Plate Tectonics
Theory that Earth’s lithosphere is divided into moving plates.
Transform Boundary
Plate boundary where plates slide horizontally past each other.
Convergent Boundary
Boundary where plates collide, causing subduction or mountain building.
Divergent Boundary
Boundary where plates move apart, creating new crust at ridges.
Sea-Floor Spreading
Process of new oceanic crust forming at mid-ocean ridges and moving outward.
Earthquake
Sudden ground shaking caused by energy release along faults.
Focus (Hypocenter)
Point inside Earth where earthquake rupture starts.
Epicenter
Point on Earth’s surface directly above the focus.
P Wave
Fast compressional body wave traveling through solids, liquids, gases.
S Wave
Slower shear body wave traveling only through solids.
Love Wave
Surface wave causing horizontal ground motion; very destructive.
Rayleigh Wave
Surface wave producing rolling motion; causes strong shaking.
Richter Scale
Logarithmic scale measuring earthquake magnitude.
Modified Mercalli Scale
Scale ranking earthquake intensity based on observed effects.
Volcano
Mountain formed by accumulation of eruptive products around a vent.
Magma
Molten rock beneath Earth’s surface.
Lava
Magma that reaches the surface.
Composite Volcano
Steep-sided cone made of alternating lava and pyroclastic layers.