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CHEM3120 · Environmental and Analytical Chemistry

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Chapter 5 of 10 · CHEM3120

Atmospheric Chemistry & the Carbon/Nitrogen Cycles

Block 2 (Lectures 9-16) of CHEM3120 covers the atmosphere: the carbon and nitrogen cycles, the greenhouse effect and Earth's radiative energy balance (blackbody emission, Wien's law), photochemical smog and NOx, and CFCs and the ozone hole. The examinable calculations use formula-sheet relationships (Wien's law, Stefan-Boltzmann), and the mechanisms — why CO2 is an effective greenhouse gas, how HFCs are removed before reaching the stratosphere — appear as Part A short-answer.

In this chapter

What this chapter covers

  • 01Blackbody radiation: any body at T > 0 emits; the peak wavelength shortens as T rises
  • 02Wien's law λ_max · T = 2.898×10^6 K·nm; Earth's emission peaks in the infrared
  • 03Greenhouse effect: Earth's IR emission overlaps the CO2 bending-mode absorption
  • 04Why CO2 outweighs water vapour as a greenhouse gas near Earth's emission peak
  • 05Radiative energy balance and the IPCC picture; Stefan-Boltzmann q = 4πr²σT⁴
  • 06Photochemical smog: N2 + O2 → 2NO in engines (morning peak), O3 downstream at midday
  • 07Ozone and CFCs: HFC replacements removed in the troposphere by R-H + OH· → R· + H2O
  • 08Carbon and nitrogen cycles: nitrogen fixation, Haber-Bosch benefits and runoff drawbacks
Worked example · free

Wien's law: Earth's peak thermal emission and why CO2 matters

Q [3 marks]. Earth's mean surface temperature is about 288 K. Using Wien's law λ_max · T = 2.898×10^6 K·nm (from the exam formula sheet), find the wavelength at which Earth's thermal emission peaks, and use the result to explain why CO2 is an effective greenhouse gas. (3 marks)
  • +1Rearrange Wien's law for the peak wavelength: λ_max = (2.898×10^6 K·nm) ÷ T.
  • +1Substitute T = 288 K: λ_max = 2.898×10^6 ÷ 288 = 1.006×10^4 nm ≈ 10 µm — this lies in the infrared, not the visible.
  • +1Interpretation: Earth's emission peaks in the IR, overlapping the region where CO2 vibrational modes (its bending mode) absorb strongly, so CO2 intercepts outgoing IR and re-radiates it back — an effective greenhouse gas even though it is far less abundant than water vapour, because it absorbs where Earth radiates most.
λ_max ≈ 1.0×10^4 nm ≈ 10 µm (infrared). Because Earth's blackbody emission peaks in the IR near CO2's vibrational absorption, CO2 absorbs a large share of outgoing longwave radiation and re-emits it downward — the physical basis of its greenhouse effect. The Sun, being far hotter, peaks in the visible, so its incoming radiation passes through largely unabsorbed.
Sia tip — Wien's law is a one-line rearrangement, but watch the units: with T in K and the constant in K·nm the answer comes out in nm — divide by 1000 to reach µm. The physics mark is the overlap of Earth's IR peak with CO2 absorption, so always finish with that sentence.
Glossary

Key terms

Blackbody radiation
The thermal radiation emitted by any object at a temperature above absolute zero; hotter bodies emit more and peak at shorter wavelengths.
Wien's law
λ_max · T = 2.898×10^6 K·nm: the wavelength of peak emission is inversely proportional to absolute temperature. Cool Earth peaks in the IR; the hot Sun peaks in the visible.
Greenhouse effect
Absorption of Earth's outgoing infrared radiation by atmospheric gases (notably CO2 and water vapour) that then re-radiate energy downward, warming the surface.
Stefan-Boltzmann law
The total power radiated by a body scales as T⁴ (q = 4πr²σT⁴, σ = 5.67×10^-8 W m^-2 K^-4); the basis of Earth's radiative energy balance.
Nitrogen fixation
Conversion of atmospheric N2 into biologically accessible nitrogen oxides or hydrides; achieved industrially by the Haber-Bosch process, which boosts crop yields but whose runoff can cause algal blooms.
Photochemical smog
Air pollution in which NO from combustion (N2 + O2 → 2NO, peaking at morning rush hour) is processed photochemically to produce ozone downstream around midday.
FAQ

Atmospheric Chemistry & the Carbon/Nitrogen Cycles FAQ

Why is CO2 a more important greenhouse gas than water vapour, despite being less abundant?

Because of WHERE it absorbs. Earth's thermal emission peaks in the infrared near 10 µm (Wien's law at ~288 K), and CO2's vibrational modes absorb strongly in that region, so CO2 intercepts a large share of the outgoing longwave radiation. Water vapour absorbs more at shorter IR wavelengths where Earth radiates comparatively little, so per molecule near the emission peak CO2 is disproportionately effective.

How do CFC replacements avoid destroying stratospheric ozone?

The hydrofluorocarbon replacements keep a C-H bond, and that is the key. In the troposphere the hydroxyl radical attacks it, R-H + OH· → R· + H2O, breaking the molecule down before it can drift up to the stratosphere. The original CFCs had no such handle, survived to the stratosphere, and released chlorine that catalytically destroyed ozone.

Why does NO peak in the morning but ozone at midday?

NO is made thermally in hot engines, N2 + O2 → 2NO, so it tracks traffic and peaks at the morning rush hour. Ozone is not emitted directly; it forms downstream through sunlight-driven photochemistry acting on NOx and hydrocarbons, which takes time and needs strong sunlight, so O3 builds to a midday peak after the NO.

Can AI help me with the atmospheric-chemistry calculations in CHEM3120?

Yes. Sia can take you through a Wien's-law or Stefan-Boltzmann calculation step by step, check your unit conversions (nm to µm, K to power), and rehearse the mechanism answers — greenhouse overlap, CFC breakdown, smog timing — in the short-answer style. It explains the method and checks your reasoning; it does not do graded work for you, and University of Sydney academic-integrity rules apply.

Study strategy

Exam move

The atmosphere block mixes quantitative and conceptual marks, so prepare both. On the numbers, drill the formula-sheet relationships — Wien's law and Stefan-Boltzmann — as clean one-line rearrangements with careful units (K, nm, µm, W m^-2). On the concepts, rehearse the set-piece explanations: why CO2 outweighs water vapour near Earth's emission peak, how HFCs are removed by OH· before the stratosphere, and why NO peaks in the morning while O3 peaks at midday. Learn the nitrogen-fixation and Haber-Bosch trade-off (yield versus runoff) as a benefit/drawback pair. This is a large block spanning several lectures, so spread revision across the semester rather than cramming. Confirm the exam date, room and permitted materials on Canvas and the exam timetable.

Working through Atmospheric Chemistry & the Carbon/Nitrogen Cycles in CHEM3120? Sia is AskSia’s AI Chemistry tutor — ask any CHEM3120 Atmospheric Chemistry & the Carbon/Nitrogen Cycles question and get a clear, step-by-step explanation grounded in how CHEM3120 is taught and assessed. Read this chapter free, then take your hardest questions to Sia.

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