🌍 Simple Climate Model
Model Earth's global temperature using the zero-dimensional energy balance equation. Adjust solar constant, albedo, and greenhouse gas concentration to see how equilibrium temperature changes.
About Simple Climate Model
The zero-dimensional energy balance model (EBM) captures the essential physics of Earth's global mean temperature in one equation: at equilibrium, the absorbed solar power equals the emitted infrared power, so S₀(1−α)/4 = εσT⁴. Here S₀ ≈ 1361 W/m² is the solar constant, α is the planetary albedo (fraction of sunlight reflected), ε is the effective emissivity (reduced below 1 by greenhouse gases trapping outgoing infrared), σ = 5.67×10⁻⁸ W/m²K⁴ is the Stefan-Boltzmann constant, and T is the equilibrium temperature in Kelvin. Rearranging gives T_eq = [S₀(1−α)/(4εσ)]^(1/4). Despite its simplicity, this model correctly predicts that Earth's bare-rock temperature (~255 K) is raised to ~288 K by the greenhouse effect (ε < 1).
Adjust the solar constant, albedo, emissivity, and CO₂ multiplier to explore how the equilibrium temperature responds. Enable ice-albedo feedback to see how a cooler planet reflects more sunlight (higher α), further cooling the planet — a positive feedback that in extreme cases leads to a "Snowball Earth" state. The climate response curve plots T_eq against CO₂ multiplier for your current settings, showing the logarithmic relationship known as climate sensitivity.
Frequently Asked Questions
What is the energy balance model equation?
The equilibrium condition is S₀(1−α)/4 = εσT⁴. The left side is the average solar power absorbed per square metre of Earth's surface (dividing by 4 converts the cross-sectional disc area to the full sphere surface area). The right side is the outgoing longwave radiation per unit area, reduced by factor ε because greenhouse gases re-absorb and re-emit some of it. Solving for T gives T_eq = [S₀(1−α)/(4εσ)]^(1/4).
What is albedo and what values does Earth have?
Albedo (α) is the fraction of incident solar radiation that a surface reflects. Earth's average albedo is about 0.30 — fresh snow reflects 0.80–0.90, open ocean reflects only 0.06, and tropical forest about 0.12. Clouds contribute significantly, accounting for roughly half of Earth's total albedo. An increase in albedo from 0.30 to 0.35 would drop the equilibrium temperature by about 3°C, illustrating why Arctic ice loss (lowering α) is a positive feedback amplifying warming.
How does doubling CO₂ change the temperature in this model?
In this model, doubling CO₂ increases the effective emissivity ε by approximately 0.015, as coded in the co2ToEps function. The corresponding temperature rise (climate sensitivity) is approximately 3°C per CO₂ doubling — consistent with the IPCC's Equilibrium Climate Sensitivity (ECS) estimate of 2.5–4°C. The logarithmic dependence on CO₂ concentration means successive doublings produce equal temperature increments.
What is the ice-albedo feedback?
The ice-albedo feedback is a positive feedback loop: as temperature falls, more sea ice and snow accumulate, raising planetary albedo, which reduces absorbed solar energy, further cooling the planet. Conversely, warming melts ice, lowers albedo, absorbs more sunlight, and amplifies warming. This feedback is particularly strong in the Arctic, where sea-ice extent has declined about 13% per decade since satellite records began in 1979. In the model, enabling this feedback creates the possibility of runaway cooling to a Snowball Earth state if temperature drops below ~250 K.
What is climate sensitivity and why does it matter?
Climate sensitivity is the equilibrium global mean temperature increase caused by a doubling of atmospheric CO₂. The Equilibrium Climate Sensitivity (ECS) estimated from models and palaeoclimate data ranges from 2.5 to 4°C, with a best estimate around 3°C (IPCC AR6, 2021). A higher sensitivity means a given emissions pathway leads to more warming, and hence greater risk. Uncertainties in cloud feedbacks are the dominant source of uncertainty in ECS estimates.
What is the bare-rock (no-atmosphere) temperature of Earth?
Without any atmosphere — greenhouse effect or clouds — Earth's albedo would be roughly 0.11 (rock and ocean only), and emissivity ε = 1. The energy balance gives T ≈ 270 K (−3°C). With realistic no-GHG albedo of about 0.30 but ε = 1, T ≈ 255 K (−18°C). The greenhouse effect (ε < 1) raises this to the observed ~288 K (15°C), a warming of about 33°C attributable to water vapour, CO₂, methane, and other greenhouse gases.
What would happen to Earth's temperature if the Sun were 10% brighter?
A 10% increase in solar constant from 1361 to 1497 W/m² would increase T_eq ∝ S₀^(1/4). Multiplying 288 K by (1.1)^(1/4) ≈ 1.024 gives about 295 K (22°C), an increase of roughly 7°C. This is a "forcing" of about 3.4 W/m², comparable to a CO₂ tripling. Over Earth's history, the Sun has brightened by about 30% since the Archean eon (~4 billion years ago), yet the climate remained clement — a puzzle known as the Faint Young Sun paradox, likely resolved by higher CO₂ levels early in Earth's history.
What is the Stefan-Boltzmann law?
The Stefan-Boltzmann law states that a black body radiates power P = σT⁴ per unit area, where σ = 5.67×10⁻⁸ W/(m²·K⁴). A grey body with emissivity ε < 1 radiates P = εσT⁴. At Earth's current temperature of 288 K, this gives about 390 W/m² for a true black body, but because ε ≈ 0.78 due to greenhouse gases, only about 240 W/m² escapes to space — which must balance the absorbed solar flux of also ~240 W/m² at equilibrium.
How does this simple model differ from general circulation models (GCMs)?
This zero-dimensional EBM treats Earth as a single point with a uniform temperature — it has no geography, no ocean circulation, no seasonal cycle, and no atmospheric dynamics. General circulation models (GCMs) used by the IPCC divide Earth into a three-dimensional grid of millions of cells, solving fluid dynamics equations for atmosphere and ocean at resolutions of 10–100 km. GCMs capture regional patterns, precipitation changes, and cloud feedbacks that the EBM cannot, but the EBM correctly identifies the fundamental forcing-feedback framework that governs global mean temperature.
What is a "Snowball Earth" and how does the model show it?
Snowball Earth refers to episodes in Earth's history (~720 Ma and ~635 Ma) when the planet may have been almost entirely glaciated, with sea-ice extending to the tropics. In the energy balance model with ice-albedo feedback, if temperature drops below about 250 K the high-albedo ice state becomes self-sustaining — even at current solar forcing, the ice-covered planet reflects so much sunlight that it cannot warm. This hysteresis means escape from Snowball Earth requires a massive CO₂ build-up from volcanic outgassing over millions of years.
A zero-dimensional energy balance model — tune albedo, greenhouse effect and solar output to project temperature.
3D · Three.js / WebGL renderer · 60 FPS target · runs fully client-side, no install