IB Physics HL Climate & the Greenhouse Effect Paper 1 & 2 Global Warming ~10 min read

The Greenhouse Effect

You’ve met the greenhouse gases — now let’s watch them do their job. The greenhouse effect is how a thin blanket of gas keeps Earth warm and cosy instead of frozen solid. It’s a natural, helpful process. The problem starts when we pile on extra gas and the blanket gets too thick. That’s the enhanced greenhouse effect, and it’s what drives global warming.

📘 What you need to know

How the greenhouse effect works

Follow the energy on its journey. Sunlight comes in mostly as visible light and ultraviolet. The atmosphere is nearly see-through to visible light, so it passes straight down and is soaked up by the ground — warming the surface.

A warm surface can’t hold onto that energy, so it re-radiates it. But Earth is far cooler than the Sun, so it glows at much longer wavelengths: infrared. Now the greenhouse gases go to work. They absorb this outgoing infrared and re-emit it in all directions — so a good share is sent back down to the surface. Some still escapes to space, but the rest stays trapped in the surface–atmosphere system. The more greenhouse gas there is, the more infrared gets held back, and the warmer Earth becomes.

The one-line version: Short-wave sunlight comes in and warms the ground; long-wave infrared tries to leave; greenhouse gases catch it and send some back — so heat piles up.

Why is sunlight “short-wave” but Earth’s glow “long-wave”? There’s a tidy rule — Wien’s law — that says the hotter an object is, the shorter the wavelength it peaks at. Let’s use it to see the difference.

Wien’s displacement law λmax = (2.90 × 10−3) ÷ T
WE 1

The Sun’s surface is about 5800 K and Earth’s surface is about 288 K. Find the peak wavelength each one radiates at, and say which part of the spectrum that is. (Wien’s constant = 2.90 × 10−3 m K.)

Step 1 — the Sun (5800 K) λ = (2.90×10⁻³) ÷ 5800 λ ≈ 500 nm (visible) Step 2 — the Earth (288 K) λ = (2.90×10⁻³) ÷ 288 λ ≈ 10 μm (infrared) The hot Sun glows in visible light (short-wave); the cool Earth glows in infrared (long-wave). That’s exactly why the gases let sunlight in but trap Earth’s outgoing heat.

Why greenhouse gases in particular?

Not every gas traps heat — it comes down to how a molecule responds to different radiation. Think of pushing a child on a swing: push at the right rhythm and they swing higher; push at the wrong rhythm and nothing much happens.

ULTRAVIOLET high frequency too energetic — snaps bonds apartINFRARED lower frequency O C O matches its rhythm — vibrates & heats up
UV is high-frequency and energetic, so it can snap molecular bonds. Infrared has a lower frequency that matches a greenhouse-gas molecule’s natural rhythm — so the molecule resonates, vibrates harder, and heats up instead.

The enhanced greenhouse effect

Here’s the key idea to keep straight: the natural greenhouse effect is a good thing — without it Earth would be far too cold. The trouble is the enhanced greenhouse effect, where human activity pumps extra greenhouse gases into the air. A thicker gas blanket lets even less heat escape, so the planet warms up.

NATURAL greenhouse effect EARTH heat in balance temperature stays steadyENHANCED greenhouse effect EARTH more heat trapped Earth warms up
The pink band is the greenhouse-gas layer — thin on the left, thicker on the right. Orange = incoming sunlight, green = heat escaping to space, red = heat trapped and sent back. With a thicker, human-boosted layer, fewer green arrows escape and more red arrows stay — so the planet heats up.

The numbers back this up. Carbon dioxide has climbed by more than 100 ppm to reach about 420 ppm (2020), and average global temperatures have risen over 1 °C since pre-industrial times.

WE 2

Carbon dioxide has risen by about 100 ppm to reach 420 ppm. Estimate the percentage increase compared with its earlier level.

Step 1 — find the earlier level earlier = 420 − 100 = 320 ppm Step 2 — percentage increase = rise ÷ earlier × 100 = (100 ÷ 320) × 100 ≈ 31% A roughly one-third jump in CO2 — a big change for a gas that’s such a strong infrared absorber.

Most of this extra gas comes from things people do. You don’t need to memorise every source, but it helps to see the pattern:

Greenhouse gasMain human sourcesFormula
Carbon dioxideBurning fossil fuels, burning wood, deforestationCO2
MethaneDecaying organic matter — landfill, manure, cropsCH4
Nitrous oxideArtificial fertilisers, burning fossil fuelsN2O
Exam-favourite catch: the enhanced greenhouse effect increases the global average temperature and is caused by human activity. If a multiple-choice option says “decreasing” or “natural causes”, it’s wrong. Increase + human activity — that’s the pair to remember.
Sunlight in
short-wave
warms
surface
Earth emits
infrared
gases absorb
& re-emit down
Heat
accumulates
extra gas =
less escapes
Warming

🛠️ Explaining the greenhouse effect in an answer

  1. In: short-wave sunlight passes through the atmosphere and warms the surface.
  2. Out: the warm Earth re-radiates energy as long-wave infrared.
  3. Trap: greenhouse gases absorb the infrared and re-emit some of it back down.
  4. Why them: their natural frequency is in the infrared, so they resonate and heat up.
  5. Enhanced: more greenhouse gas → less heat escapes → temperature rises (human-caused).

💡 Top tips

⚠ Common mistakes

Quick recap: Short-wave sunlight warms the ground; Earth re-radiates long-wave infrared; greenhouse gases resonate with that infrared, absorb it, and send some back — keeping Earth warm. Adding extra gas (the enhanced effect) traps more heat, so global temperatures rise. It’s an increase, and it’s human-caused.
You can now tell the whole story: sunlight in, infrared out, gases trapping the difference — and how humans have tipped that balance. Next we make it quantitative in Energy Balance Problems, where we treat Earth and its atmosphere as bodies swapping radiation, and actually calculate how the temperature settles (and shifts).

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