IB Physics SL Topic B.2 — Climate & the Greenhouse Effect Paper 1 & 2 Resonance Model · Enhanced Effect ~7 min read

The Greenhouse Effect

You now know which gases do the absorbing and roughly where. This page joins the dots: how a molecule actually captures infrared radiation, and why pumping more greenhouse gases into the atmosphere doesn’t just add a little warmth — it changes the whole energy balance.

📘 What you need to know

The Resonance Model of Warming

Picture the energy flow as a nightly cycle. During the day, ultraviolet and visible radiation from the Sun streams through the atmosphere almost untouched and is absorbed by the ground, oceans and vegetation. At night, that stored energy leaves the surface again as infrared radiation. Some of this infrared escapes straight through the atmosphere into space — but greenhouse gas molecules intercept the rest.

Because their natural frequency sits in the infrared region, these molecules don’t just absorb that energy passively — they begin to resonate, vibrating more vigorously and heating up. A hot, vibrating molecule doesn’t hold onto that energy forever: it re-emits infrared radiation of its own, scattered in every direction, including straight back down towards the surface it came from.

The more greenhouse gas there is in the atmosphere, the more of this returning radiation gets sent back down — so heat energy builds up in the surface–atmosphere system instead of draining away into space.

Why Infrared and Not Ultraviolet?

The reason greenhouse gases target infrared specifically comes down to molecular energy levels. High-frequency ultraviolet light carries enough energy to actually break chemical bonds within a molecule. Infrared light is far gentler — it doesn’t have enough energy to break bonds, but it does have exactly the right energy to set atoms within a molecule vibrating. Since a greenhouse gas’s natural vibrational frequency matches incoming infrared, that’s the wavelength range it absorbs and re-emits most efficiently.

GREENHOUSE EFFECT natural balance greenhouse gas layer EARTH’S SURFACE escapes re-emitted back downENHANCED GREENHOUSE EFFECT more greenhouse gas, more heat trapped thicker greenhouse gas layer EARTH’S SURFACE (warmer) less escapes more re-emitted back downgrey = incoming solar · orange = outgoing IR escaping to space · red = IR re-emitted back to the surface
A thicker layer of greenhouse gases absorbs and re-emits more outgoing infrared radiation back toward the surface, so less escapes to space and the surface warms further.

The Enhanced Greenhouse Effect

The greenhouse effect itself is not a problem — it’s the reason Earth is warm enough to support life at all. The concern is the enhanced greenhouse effect: human activity has been steadily increasing the concentration of greenhouse gases in the atmosphere, most notably carbon dioxide, which has climbed from around 280 parts per million before industrialisation to over 420 parts per million today. With more greenhouse gas molecules available to absorb and re-emit outgoing infrared radiation, less long-wave heat escapes the atmosphere overall, and average global temperatures have already risen by more than 1°C since pre-industrial times.

Quick recap: greenhouse gases absorb outgoing infrared because their natural frequency matches it, then re-emit it in all directions via resonance. More greenhouse gas concentration means more radiation sent back to the surface — that’s the enhanced greenhouse effect.
WE 1

Explain, in terms of molecular behaviour, why greenhouse gases absorb infrared radiation but not ultraviolet radiation.

Ultraviolet UV photons carry enough energy to break chemical bonds within a molecule, rather than being absorbed and re-emitted. Infrared IR photons don’t carry enough energy to break bonds, but they do match the natural vibrational frequency of greenhouse gas molecules. Matching frequency → resonance → absorption and re-emission of IR This is why greenhouse gases are selective: they respond strongly to infrared, not ultraviolet.
WE 2

Atmospheric CO₂ concentration has risen from about 280 ppm before industrialisation to around 420 ppm today. Calculate the percentage increase.

Step 1 — Find the change change = 420 − 280 = 140 ppm Step 2 — Express as a percentage of the original % increase = (140 ÷ 280) × 100 = 50% A 50% rise in CO₂ concentration is a major driver of the enhanced greenhouse effect.

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Up next: Energy Balance Problems — where we bring albedo, emissivity, the solar constant and the greenhouse effect together into full climate models and calculate exactly how much surface temperatures shift.

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