High School

Modeling Energy Variations in Earth's Climate

NGSS Performance Expectation

HS-ESS2-4Use a model to describe how variations in the flow of energy into and out of Earth's systems result in changes in climate.

What This Standard Asks

The HS-ESS2-4 standard calls for an HS-ESS2-4 simulation to help students use a model to describe how variations in the flow of energy into and out of Earth's systems result in changes in climate. Rather than memorizing facts about climate change, the standard requires students to build mechanistic understanding: they must trace how imbalances in energy flow drive temperature change and climate patterns. The standard emphasizes modeling over observational data analysis, prioritizing students' ability to see and explain the causal chains within a dynamic system. An energy model that lets students adjust inputs and observe climate responses in real time is central to meeting this standard.

The Greenhouse Effect Simulation

The Greenhouse Effect simulation models how atmospheric gases trap outgoing heat. Students observe sunlight entering the model atmosphere, see it converted to infrared radiation at Earth's surface, and watch as greenhouse gas molecules absorb and redirect that radiation back downward. By adjusting the greenhouse gas concentration slider, students can trace the direct link between gas levels and temperature rise. This directly addresses the core of HS-ESS2-4: demonstrating that variations in energy out, specifically the amount of infrared radiation that escapes to space, create measurable changes in the model's climate state. The sim contains variation in a single parameter, gas concentration, allowing students to isolate that one factor and understand its effect clearly.

The Ice and Albedo Simulation

The Ice and Albedo simulation models Earth's energy balance through a feedback mechanism: as ice cover changes, the planet's reflectivity, or albedo, changes with it, altering how much solar energy the surface absorbs. Students can vary initial conditions such as polar ice extent or solar input and observe how the model responds to these changes. As ice melts, less solar radiation reflects back to space, so the surface absorbs more energy, causing further warming, which melts more ice. This reinforces the standard's focus on energy flow variations and introduces the concept of feedback loops, showing how small changes in one part of the system can amplify or dampen climate response. The two sims together let students explore both direct mechanisms (greenhouse gas absorption) and indirect mechanisms (albedo feedback).

A Class Period Using These Simulations

Begin with the Greenhouse Effect simulation. Students first predict what they expect to see when greenhouse gas levels increase, committing to a hypothesis before touching the model (predict phase). They then explore the simulation by adjusting gas concentration and observing temperature response, running multiple trials to build confidence in the pattern (explore phase). They explain the mechanism they observe, describing the path of energy through the model and why the outcome matches or contradicts their prediction (explain phase). The built-in assessment quiz checks their understanding with multiple-choice questions; results appear in your teacher dashboard in real time, allowing you to redirect instruction based on misconceptions or success. This four-phase cycle can fit in a standard 50-minute period and requires no setup beyond sharing a join code with students. You may follow with the Ice and Albedo simulation in a second period or extend the single class by comparing how the two mechanisms differ.

Try the simulations

Ice & Albedo: Earth's Energy Balance

Related resources

Ready to teach?

All simulations come with built-in standards-aligned questions and a live class dashboard. Share a join code and watch student thinking arrive in real time.