Weather, Climate, Atmospheric Science, and Astronomy Review

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Vocabulary practice flashcards covering weather, climate, atmospheric layers, astronomy, thermodynamics, and heat transfer based on lecture notes.

Last updated 2:29 PM on 9/11/26
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39 Terms

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Weather

Refers to the dynamic, constantly changing condition of the atmosphere at any particular time and place.

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Climate

Represents the accumulation of daily and seasonal weather events over a timeframe typically averaged across 3030 to 3535 years.

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Permanent Atmospheric Gases

Gases with constant concentrations in Earth's atmosphere, primarily nitrogen (78%78\%), oxygen (21%21\%), and argon (0.934%0.934\%).

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Variable Atmospheric Gases

Gases whose concentrations vary in the atmosphere, including carbon dioxide, methane, nitrous oxide, ozone, sulfur dioxide, and hydrogen.

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<p>Layers of the Atmosphere</p>

Layers of the Atmosphere

The five distinct thermal layers surrounding Earth: Troposphere, Stratosphere, Mesosphere, Thermosphere, and Exosphere.

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Exosphere

The outermost atmospheric layer with low density that functions like a space bridge where gas particles float and escape Earth's gravity.

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Thermosphere

The second-outermost layer of the atmosphere that absorbs high-energy X-rays and ultraviolet radiation from the Sun.

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Mesosphere

The third and middle layer of the atmosphere that shields Earth's surface from meteors and space debris.

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Stratosphere

The fourth layer of the atmosphere that shields Earth from harmful ultraviolet rays and serves as the altitude for airplane travel.

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Troposphere

The lowest layer of the atmosphere containing breathing air, water vapor, and most atmospheric mass where weather events occur.

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Meteorology

The study of the atmosphere and its phenomena, a term coined around 340 BC340\text{ BC} by Aristotle.

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RADAR

Acronym for Radio Detection and Ranging; a system that transmits radio/microwave signals and calculates speed, distance, and direction from returning echoes.

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Big Bang Theory

The widely accepted cosmological explanation stating that the universe originated about 13.7 billion13.7\text{ billion} years ago from an expanding tiny volume of hot mass.

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<p>Galaxies</p>

Galaxies

Systems of millions or billions of stars held together by gravitational attraction between gas and dust, categorized as spiral, elliptical, or irregular.

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Geocentric Theory

The theoretical model asserting that Earth was located in the center of the galaxy/universe and celestial bodies revolved around it.

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Heliocentric Theory

The theoretical model asserting that the Sun was in the center of the galaxy/solar system with planets revolving around it.

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Star Cluster

A group of stars, categorized as open or globular clusters, differing from galaxies because they exclusively contain stars.

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Terrestrial Planets

Inner planets with solid surfaces, which include Mercury, Venus, Earth, and Mars.

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Planetary Distance Table (AU)

Distances of planets from the Sun expressed in Astronomical Units: Mercury (0.390.39), Venus (0.720.72), Earth (11), Mars (1.521.52), Jupiter (5.25.2), Saturn (9.549.54), Uranus (19.219.2), and Neptune (30.0630.06).

<p>Distances of planets from the Sun expressed in Astronomical Units: Mercury ($$0.39$$), Venus ($$0.72$$), Earth ($$1$$), Mars ($$1.52$$), Jupiter ($$5.2$$), Saturn ($$9.54$$), Uranus ($$19.2$$), and Neptune ($$30.06$$).</p>
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Planetary Physical Characteristics Table

A tabular reference listing diameters in kilometers and distances from the Sun in kilometers for planets in the solar system.

<p>A tabular reference listing diameters in kilometers and distances from the Sun in kilometers for planets in the solar system.</p>
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Earth's Revolution

The orbital movement of Earth around the Sun taking 36514 days365 \frac{1}{4}\text{ days} (8,776 hours8,776\text{ hours}), ranging from 147,000,000km147,000,000\,km in January to 152,000,000km152,000,000\,km in July.

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Astronomical Unit (AU)

The average distance from the Earth to the Sun, approximately equal to 150,000,000km150,000,000\,km (1AU1\,AU).

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Earth's Rotation

The spin of Earth on its tilted axis taking 24 hours24\text{ hours}, causing day and night.

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Summer Solstice

Occurs on June 21st when the Sun is directly above 231223 \frac{1}{2}^\circ north latitude (Tropic of Cancer) in the Northern Hemisphere.

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Autumnal Equinox

Occurs on September 22nd when the Sun is directly above the equator, causing equal length of day and night.

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Greenhouse Effect

The mechanism where incoming solar energy absorbed by Earth is partially trapped by greenhouse gases in the atmosphere, keeping the planet warm.

<p>The mechanism where incoming solar energy absorbed by Earth is partially trapped by greenhouse gases in the atmosphere, keeping the planet warm.</p>
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Energy

The ability or capacity to do work on some form of matter.

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Temperature

A measure of the average speed of atoms and molecules in a substance.

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Density

The amount of mass packed into a given volume, defined mathematically as Mass/Volume\text{Mass}/\text{Volume}.

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Heat

Energy in the process of being transferred from one object to another due to a temperature difference between them.

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Kinetic Energy

The energy of motion possessed by an object, given by the formula KE=12mv2KE = \frac{1}{2} m v^2.

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Latent Heat

The heat energy required or hidden when a substance transforms from one phase state to another (such as melting, freezing, evaporation, sublimation, condensation, or deposition).

<p>The heat energy required or hidden when a substance transforms from one phase state to another (such as melting, freezing, evaporation, sublimation, condensation, or deposition).</p>
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Sensible Heat

Heat energy that can be felt or directly measured using a thermometer.

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Specific Heat

The heat required to raise the temperature of a unit mass of a substance by a given amount.

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Conduction

The transfer of heat from a warmer object to a colder object through direct molecular interaction.

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Convection

The transfer of heat by the mass movement of a fluid, such as liquids and gases.

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Advection

The transfer of heat or atmospheric properties by horizontally moving air.

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Radiation

The transfer of energy from the Sun or other sources through electromagnetic waves.

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Electromagnetic Spectrum

The complete range of radiation ordered by wavelength and energy, encompassing gamma rays, X-rays, ultraviolet, visible light (0.4μm0.4\,\mu m to 0.7μm0.7\,\mu m), infrared, microwave, and radio waves.

<p>The complete range of radiation ordered by wavelength and energy, encompassing gamma rays, X-rays, ultraviolet, visible light ($$0.4\,\mu m$$ to $$0.7\,\mu m$$), infrared, microwave, and radio waves.</p>