Earth's Energy Balance — the Physics of Climate
Climate is not meteorology. Where weather is the chaotic day-to-day state of the atmosphere, climate is the long-run energy budget of the planet — the balance between sunlight absorbed and infrared heat radiated to space. Starting from Stefan-Boltzmann radiation and a zero-dimensional energy balance model, we derive why Earth is 33 K warmer than it "should" be, how greenhouse gases shift the balance, and where tipping points come from.
1. Solar Radiation and Albedo
The Sun's luminosity is L☉ = 3.846 × 10²⁶ W. At Earth's mean orbital radius d = 1.496 × 10¹¹ m, the solar constant (total flux at the top of atmosphere) is:
The factor of 4 arises because the Sun illuminates a disk of area πR² but the planet radiates from its full sphere of 4πR². Albedo contributions: fresh snow ≈ 0.85, ocean ≈ 0.06, clouds ≈ 0.60 — clouds dominate the planetary mean.
2. Stefan-Boltzmann and the Effective Temperature
A blackbody radiates power proportional to T⁴. Setting emitted power equal to absorbed solar gives the effective radiating temperature Tₑ:
Earth's observed mean surface temperature is ~288 K (15°C). The difference of 33 K is the natural greenhouse effect — atmospheric gases absorb and re-emit outgoing infrared radiation, warming the surface above the bare blackbody prediction.
3. Zero-Dimensional Energy Balance Model
A 0D EBM treats the entire planet as a single well-mixed reservoir with heat capacity C:
By tuning ε ≈ 0.61 we recover T* = 288 K. Reducing ε (stronger greenhouse) increases T*. The EBM time constant is τ = C/λ where λ = dOLR/dT = 4σεT³ ≈ 3.3 W m⁻² K⁻¹ is the Planck feedback. With ocean mixed-layer heat capacity C ≈ 10⁸ J m⁻² K⁻¹, τ ≈ 30 yr.
4. Greenhouse Effect and Radiative Forcing
Greenhouse gases (CO₂, H₂O, CH₄, N₂O, O₃) absorb outgoing longwave radiation in specific spectral bands, reducing OLR for a given T. The resulting energy imbalance is the radiative forcing ΔF (W m⁻²):
Water vapour +
Warming increases atmospheric water vapour, a greenhouse gas itself — roughly doubling the CO₂ forcing. Largest positive feedback (~1.8 W m⁻² K⁻¹).
Lapse rate −
Tropics: moist adiabatic lapse rate causes upper troposphere to warm more than surface — upper layers radiate more, partially offsetting water vapour.
Ice-albedo +
Warming melts high-albedo ice → darker ocean/land absorbs more solar → more warming. Particularly strong in the Arctic.
Cloud −/+
Low clouds reflect solar (cooling) but also trap longwave (warming). Net cloud feedback ≈ +0.42 W m⁻² K⁻¹ — the most uncertain term.
5. Albedo-Temperature Feedbacks
To include ice-albedo feedback, α becomes a function of T. A simple parameterisation:
On Mars the ice-albedo feedback is strong enough that removing greenhouse forcing could tip it into a "snowball" state. On Venus a runaway greenhouse has locked the planet at 737 K.
6. Tipping Points and Bistability
With a non-linear α(T), the energy balance equation C dT/dt = F(T) can have multiple equilibria. Drawing the energy budget as a function of T reveals up to three fixed points: two stable (warm Earth, snowball Earth) and one unstable (between them).
Real Earth tipping elements include the West Antarctic Ice Sheet, Greenland Ice Sheet, Atlantic Meridional Overturning Circulation (AMOC), and Amazon dieback — each with their own threshold forcing and irreversibility timescale.
7. JavaScript EBM Simulation
// Zero-dimensional Energy Balance Model with ice-albedo feedback
const sigma = 5.67e-8; // Stefan-Boltzmann
const S0 = 1361; // W/m², solar constant
const C = 4e8; // J/(m²·K) mixed-layer heat capacity
function albedo(T) {
if (T < 263) return 0.62; // snowball
if (T > 293) return 0.28; // ice-free
return 0.62 + (0.28 - 0.62) * (T - 263) / (293 - 263);
}
function dTdt(T, eps, dForcing = 0) {
const ASR = S0 * (1 - albedo(T)) / 4;
const OLR = sigma * eps * T ** 4;
return (ASR - OLR + dForcing) / C;
}
function runEBM(T0, eps, dForcing, years = 500, dt = 3.15e7) {
// dt = 1 year in seconds
let T = T0;
const result = [{year: 0, T}];
const steps = years * 12; // monthly timesteps
const dtM = dt / 12;
for (let i = 1; i <= steps; i++) {
T += dTdt(T, eps, dForcing) * dtM;
if (i % 12 === 0) result.push({year: i / 12, T});
}
return result;
}
// Stable modern Earth
const modern = runEBM(288, 0.61, 0);
console.log('Equilibrium T:', modern.at(-1).T.toFixed(2), 'K');
// CO₂ doubling: +3.7 W/m² forcing
const co2x2 = runEBM(288, 0.61, 3.7);
console.log('ΔT for CO₂×2:', (co2x2.at(-1).T - 288).toFixed(2), 'K');
// Snowball Earth from modern state (increase albedo)
const snowball = runEBM(288, 0.61, -40); // −40 W/m² → triggers ice runaway
console.log('Snowball T:', snowball.at(-1).T.toFixed(2), 'K');
8. Hierarchy of Climate Models
- 0D EBM: Single temperature, energy balance only. Captures global mean and tipping points, ~5 parameters.
- 1D EBM (latitude): Adds meridional heat transport with a diffusion term κ∇²T. Resolves ice-line position and latitudinal gradients.
- 2D / EMIC: Earth Models of Intermediate Complexity — resolves ocean circulation and sea-ice but runs faster than full GCMs.
- GCM (CMIP6): Coupled atmosphere-ocean-land-ice models on 50–100 km grids, ~10⁷ DOF. Foundation of IPCC projections.
- km-scale models: AI-enhanced models (FourCastNet, Pangu-Weather) trained on ERA5 reanalysis achieve GCM-comparable forecasts 10 000× faster.