Universe, Solar System & Earth Systems – Vocabulary Review

0.0(0)
studied byStudied by 0 people
GameKnowt Play
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
Card Sorting

1/79

flashcard set

Earn XP

Description and Tags

Vocabulary flashcards covering cosmology, solar-system formation, Earth structure, atmosphere, hydrosphere, biosphere, and related scientific terms to aid exam preparation.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

80 Terms

1
New cards

Creation Myth

A culture’s symbolic narrative describing the beginning of the world (e.g., the six-day Genesis account).

2
New cards

Big Bang Theory

Model proposed by Alexander Friedmann & Georges Lemaître describing a hot, dense origin of the universe that has expanded ever since.

3
New cards

Big Bang Singularity

The initial state of “nothingness” in which space, time, matter and energy were infinitely compressed.

4
New cards

Inflation (Cosmology)

A brief period of extremely rapid expansion immediately after the Big Bang, enlarging the universe from sub-atomic size.

5
New cards

Nucleosynthesis

Early Big-Bang process in which protons and neutrons fused to form light nuclei such as hydrogen and helium.

6
New cards

Recombination

Epoch when electrons bonded with nuclei to form neutral atoms, allowing photons to travel freely and ending the cosmic “Dark Ages.”

7
New cards

Inflationary Epoch

Stage when the universe grew from the size of an atomic nucleus to macroscopic proportions in a fraction of a second.

8
New cards

Radiation Era

Period dominated by photons; origin of the cosmic microwave background radiation.

9
New cards

Matter Domination

Era when matter (rather than radiation) controlled cosmic dynamics and lithium atoms first formed.

10
New cards

Strong Nuclear Force

Short-range, attractive force that binds protons and neutrons in atomic nuclei.

11
New cards

Electromagnetic Force

Long-range force of attraction or repulsion between charged particles; binds atoms.

12
New cards

Weak Nuclear Force

Short-range interaction responsible for radioactive decay and neutrino production.

13
New cards

Gravitational Force

Weak, long-range attractive force that governs the motion of planets, stars, and galaxies.

14
New cards

Cosmic Microwave Background (CMB)

Faint, uniform microwave radiation discovered by Penzias & Wilson, viewed as the afterglow of the Big Bang.

15
New cards

Hubble’s Law

Observation that galaxies are moving away from each other, implying universal expansion.

16
New cards

Light-Element Abundance

High proportions of H, He (and traces of Li, Be) predicted and observed as evidence for Big-Bang nucleosynthesis.

17
New cards

Descartes’ Vortex Theory

Early solar-system model in which whirlpool-like motions in a primordial fluid formed planets and satellites.

18
New cards

Buffon’s Collision Theory

Hypothesis that planets condensed from material pulled off the Sun by a passing comet.

19
New cards

Kant-Laplace Nebular Theory

Proposal that the solar system formed from a rotating gas-dust nebula collapsing under gravity.

20
New cards

Jeans-Jeffreys Tidal Theory

Idea that tidal forces ripped material from the Sun, which later condensed into planets.

21
New cards

Solar Nebular Theory

Modern model where interstellar gas and dust condensed into planetesimals, protoplanets, and finally the Sun and planets.

22
New cards

Planetesimal

Kilometer-scale body formed by dust collisions in the solar nebula; building block of planets.

23
New cards

Protoplanet

Large, gravitationally bound aggregation of planetesimals in the early solar system.

24
New cards

Cold Accretion Hypothesis

Concept that protoplanets formed from cool material gradually sticking together without initial melting.

25
New cards

Solar Wind

Stream of charged particles emitted by the young Sun, affecting planetary atmospheres and dust.

26
New cards

Terrestrial Planet

Inner, rocky planet composed mainly of silicate rock and metals (Mercury, Venus, Earth, Mars).

27
New cards

Jovian Planet

Outer gas-giant planet composed chiefly of hydrogen and helium (Jupiter, Saturn, Uranus, Neptune).

28
New cards

Dwarf Planet

Celestial body orbiting the Sun, massive enough for self-gravity to be spherical, but not having cleared its orbital neighborhood (e.g., Pluto).

29
New cards

International Astronomical Union (IAU)

Body that defines planetary nomenclature and classification standards.

30
New cards

Asteroid

Small, rocky, airless body orbiting the Sun; also called a minor planet.

31
New cards

Main Asteroid Belt

Region between Mars and Jupiter containing most known asteroids.

32
New cards

Near-Earth Asteroid (NEA)

Asteroid whose orbit brings it close to Earth, monitored for potential impact hazards.

33
New cards

Ceres

First discovered asteroid and also classified as a dwarf planet within the main belt.

34
New cards

Comet

Icy body that develops a glowing coma and tail when near the Sun due to sublimation of volatiles.

35
New cards

Kuiper Belt

Disc-shaped region beyond Neptune containing short-period comets and icy bodies; the solar system’s ‘final frontier.’

36
New cards

Oort Cloud

Hypothetical distant spherical shell of icy objects believed to be the source of long-period comets.

37
New cards

Accretion (Earth Formation)

Growth of Earth by gradual accumulation of centimeter-sized dust and kilometer-sized planetesimals.

38
New cards

Differentiation (Planetary)

Process where denser materials (Fe, Ni) sink to a planet’s core while lighter materials rise to form crust.

39
New cards

Inge Lehmann

Seismologist who discovered Earth’s solid inner core, identifying the Lehmann discontinuity.

40
New cards

Inner Core

Solid, metallic (Fe-Ni) central sphere of Earth with an estimated radius of ~1250 km.

41
New cards

Outer Core

Liquid Fe-Ni layer (~2300 km thick) whose convection generates Earth’s magnetic field.

42
New cards

Gutenberg Discontinuity

Boundary between Earth’s lower mantle and outer core marked by seismic wave changes.

43
New cards

Mohorovičić Discontinuity (Moho)

Seismic boundary separating Earth’s crust from the upper mantle.

44
New cards

Asthenosphere

Ductile, partially molten upper-mantle layer beneath the lithosphere that enables plate motion.

45
New cards

Lithosphere

Rigid outer shell of Earth comprising crust and uppermost mantle, broken into tectonic plates.

46
New cards

Plate Tectonic Theory

Framework explaining large-scale movement of lithospheric plates over the asthenosphere.

47
New cards

Pangaea

Supercontinent that existed during the late Paleozoic and early Mesozoic eras.

48
New cards

Divergent Boundary

Tectonic boundary where plates move apart, creating new crust (e.g., mid-ocean ridges).

49
New cards

Convergent Boundary

Tectonic boundary where plates collide, often forming mountains or subduction zones.

50
New cards

Transform Boundary

Plate boundary where plates slide horizontally past one another (e.g., San Andreas Fault).

51
New cards

Troposphere

Lowest atmospheric layer (surface to ~12 km) where weather occurs and temperature decreases with altitude.

52
New cards

Tropopause

Boundary between troposphere and stratosphere where temperature lapse rate stops.

53
New cards

Stratosphere

Atmospheric layer (12–50 km) where temperature rises with altitude due to ozone absorption.

54
New cards

Mesosphere

Middle layer (50–80 km) with decreasing temperature; meteors burn here.

55
New cards

Thermosphere

Upper layer (80–700 km) with rising temperatures; contains the ionosphere.

56
New cards

Ionosphere

Region of ionized gases within the thermosphere important for radio communication.

57
New cards

Exosphere

Outermost, thin atmospheric layer (above ~700 km) merging into space; hosts satellites.

58
New cards

Photodissociation

Splitting of water vapor by UV radiation, releasing oxygen in early atmosphere evolution.

59
New cards

Cyanobacteria

Photosynthetic microbes that produced Earth’s first significant oxygen via CO₂ + H₂O → glucose + O₂.

60
New cards

Hydrosphere

All of Earth’s water in liquid, solid, and vapor states, including oceans, lakes, and groundwater.

61
New cards

Salinity

Concentration of dissolved salts in water, expressed in parts per thousand (ppt).

62
New cards

Epipelagic Zone

Sunlit ocean layer (0–200 m) supporting most photosynthetic life.

63
New cards

Mesopelagic Zone

‘Twilight’ ocean layer (200–1000 m) with dim light and many migrating organisms.

64
New cards

Bathypelagic Zone

Midnight zone (~1000–4000 m) of total darkness and high pressure.

65
New cards

Abyssopelagic Zone

Deep-sea zone (4000–6000 m) of near-freezing waters and sparse life.

66
New cards

Hadalpelagic Zone

Deepest ocean trenches (>6000 m) hosting specialized organisms like tube worms.

67
New cards

Biosphere

Global sum of all ecosystems; the zone of life on Earth.

68
New cards

Edward Suess

Austrian geologist who coined the term “biosphere” in 1875.

69
New cards

Biota

The collective living organisms within the biosphere.

70
New cards

Gaia Hypothesis

Concept proposing Earth functions as a self-regulating, quasi-living system.

71
New cards

Climate

Long-term average of weather patterns in a region.

72
New cards

Biome

Major ecological community defined by climate and dominant vegetation.

73
New cards

Aquatic Biome

Biome encompassing freshwater and marine environments.

74
New cards

Desert Biome

Ecosystem with ≤50 cm annual rainfall, extreme temperatures, and drought-adapted life.

75
New cards

Taiga

Boreal forest biome with coniferous trees, long cold winters, and short summers.

76
New cards

Estuary

Partially enclosed coastal body where freshwater mixes with seawater, creating rich ecosystems.

77
New cards

Photic Zone

Upper ocean layer receiving sufficient light for photosynthesis.

78
New cards

Aphotic Zone

Ocean depths lacking enough light for photosynthesis.

79
New cards

Freshwater Ecosystem

Aquatic system of rivers, streams, lakes, ponds, or wetlands with low salinity.

80
New cards

Chaparral

Minor biome characterized by hot, dry summers and cool, moist winters; dominated by shrubs.