Unit 5 Flashcards

1
Q

What is the First Law of Thermodynamics? .

A

Energy cannot be created or destroyed, only transferred or transformed (conservation of energy). In climate science, this means Earth’s energy budget must balance: incoming solar radiation must equal outgoing radiation over the long term

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2
Q

What is the Second Law of Thermodynamics?

A

Energy naturally flows from regions of higher temperature to lower temperature, increasing entropy (disorder). This governs how heat is transferred within Earth’s climate system.

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3
Q

What is a blackbody object?

A

A blackbody is an idealized object that absorbs and emits all radiation perfectly at all wavelengths. The Sun and Earth approximate blackbodies.

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4
Q

What are sparkling surfaces? .

A

Sparkling surfaces (e.g., ice, snow, metals) have high reflectivity (albedo) and reflect most of the incoming radiation

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5
Q

What are clear surfaces? .

A

Clear surfaces (e.g., water, forests) have low reflectivity and absorb more energy

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6
Q

Why are high-albedo surfaces important?

A

High-albedo surfaces (e.g., polar ice) help regulate Earth’s temperature by reflecting sunlight.

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7
Q

What is temperature?

A

A measure of the average kinetic energy of molecules.

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8
Q

What is energy?

A

The capacity to do work (e.g., radiation, thermal energy).

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9
Q

What is the relationship between energy and wavelength?

A

Shorter wavelengths = higher energy (e.g., UV, X-rays); Longer wavelengths = lower energy (e.g., infrared, radio waves).

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9
Q

What is heat?

A

The transfer of thermal energy due to a temperature difference.

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10
Q

What does the Stefan-Boltzmann Law state?

A

E = σ T^4, where E is the total energy emitted, T is temperature, and σ is a constant. Hotter objects emit exponentially more energy.

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10
Q

What is shortwave radiation?

A

Emitted by hotter objects (e.g., the Sun) at high energy (visible & UV).

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11
Q

What is longwave radiation? .

A

Emitted by cooler objects (e.g., Earth) at lower energy (infrared)

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12
Q

What is Earth’s Greenhouse effect

A

Earth’s surface absorbs shortwave solar radiation and emits longwave infrared radiation. Greenhouse gases trap outgoing infrared radiation, warming the planet.

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12
Q

What are major greenhouse gases?

A

CO₂, CH₄, H₂O vapor, N₂O, O₃. They regulate Earth’s temperature by absorbing and re-emitting infrared radiation.

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13
Q

What is the Goldilocks Zone

A

Earth is just right for liquid water, but the greenhouse effect plays a key role.

14
Q

What is global radiative equilibrium?

A

With GHGs, a balanced climate with a stable temperature; without GHGs, Earth would be ~33°C colder.

15
Q

What are anthropogenic contributions to greenhouse gases?.

A

Human activities (fossil fuels, deforestation) increase CO₂, CH₄, and N₂O, enhancing the greenhouse effect and warming Earth.

15
Q

What is Global Warming Potential (GWP)?

A

GWP compares the warming effect of GHGs over time. CO₂ = baseline (1), CH₄ = ~28x CO₂ over 100 years, N₂O = ~265x CO₂.

16
Q

How do greenhouse gases interact with radiation?

A

They interact only with longwave radiation, absorbing and re-emitting it.

17
Q

What are the fates of incoming solar radiation?

A

Scattering (redirection by particles), Reflection (bounced back into space), Absorption (converted into heat).

17
Q

What is the global radiation budget?

A

Helps track energy flow (solar in, thermal out). Changes (e.g., GHGs, albedo shifts) can disrupt climate balance.

18
Q

What factors affect radiation distribution?

A

Latitude (equator gets more direct sunlight than poles), Clouds and aerosols (reflect or absorb energy), Seasonality (Earth’s tilt changes sunlight distribution).

19
Q

How does Earth’s orbit affect seasons?

A

Tilt (23.5°) determines seasons; Revolution around Sun causes variations in daylight length.

20
Q

What are the mechanisms of energy transfer?

A

Radiation (transfer via electromagnetic waves), Conduction (direct heat transfer via molecular contact), Convection (heat transfer via fluid movement).