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Earth Science · ESS-013

The Greenhouse Effect

Two bottles under a lamp, one with extra CO₂. Which warms more, and why?

  • NGSS HS-ESS2-4
  • AP Environmental Science Unit 9
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About this lab

Compare heated gas-filled boxes and explore a separate atmosphere energy-balance model. High school students use the interactive 3D setup to select gases for the bench trial, set atmospheric carbon dioxide, toggle the model feedback setting, and inspect molecule-light combinations. Paired warming curves are presented with the apparatus's convection behavior, while the planet view records outgoing infrared energy and surface temperature. A molecular lens provides representative-wavelength interactions for the selected gas. These separate observations let the bench mechanism and atmosphere model be compared without treating their temperature curves as measurements of the same process. The experiment is aligned with NGSS HS-ESS2-4 and AP Environmental Science Unit 9.

The question behind the experiment

A tabletop temperature comparison and a planetary greenhouse model can involve different dominant mechanisms. This course deliberately investigates both so that a warmer gas-filled box is not treated as a complete explanation of climate. The open-box apparatus uses lamps and selected gases under a specified timing protocol. The planetary activity uses an energy-balance model. Keep their boundaries and scales separate before explaining a temperature difference, because the same visual outcome can arise through different combinations of radiation and convection.

Plan a useful comparison

Compare the air-filled and carbon-dioxide-filled boxes, then use argon as an additional control. In this particular apparatus, a heavy gas layer suppresses convection and accounts for much of the extra warming. Argon has similar heaviness without the modeled strong infrared absorption, making it useful for distinguishing those contributions. State that conclusion for the selected open boxes and timing interval. Do not extend it to every bottle demonstration or infer that planetary warming is explained mainly by a heavy gas physically holding down convection.

Connect the observation to the model

Use the molecular view to compare the representative wavelengths and gases in the course absorption table. Some vibrations change the electric dipole and support strong infrared absorption; others do not. Carbon dioxide, water vapor, methane, and ozone have different represented bands. The course distinguishes strong, weak, negligible, and unverified combinations rather than assigning a perfectly complete spectrum from a small selection. Keep the wavelength attached to a claim about absorption, since a gas can behave differently in infrared, visible, and ultraviolet comparisons.

Interpret the result carefully

In the planetary energy model, increased greenhouse forcing first reduces outgoing infrared relative to absorbed solar energy. The resulting imbalance changes temperature until the outgoing energy again balances the incoming energy under the selected model. Compare the transient response with the eventual equilibrium rather than treating a forcing value as the current warming itself. Climate feedback settings alter the response. Water vapor is represented as a feedback in this activity, so keep its role distinct from the externally selected forcing change that initiates the comparison.

Build an explanation from your evidence

The ozone comparison introduces another distinction: absorption and photochemical behavior at different wavelengths are not the same mechanism as greenhouse warming. Use the course's separate molecular and energy representations to explain each question. Report the model-form limitations of the tabletop calculation and the simplified planetary balance. Exact closure of an internal energy account checks the calculation but does not prove that the apparatus model reproduces every measured physical detail. A useful conclusion identifies which evidence comes from the box control, which from the molecular table, and which from the planetary model.

A reference case from this course

The planetary reference balance uses absorbed solar energy of about 240 W/m². This is an energy flux per surface area in the course's global model, not a lamp power or a box temperature. Retain the model boundary when comparing it with the tabletop activity, and distinguish an equilibrium energy balance from a transient energy imbalance.

Keep the investigation reproducible

Before changing the setup, write a prediction that names the measured quantity and the expected direction of change. Retain the original trial as a reference. Record the apparatus conditions, units, and whether you used Ideal or Real lab mode. If the selected activity includes seeded variation, keep the seed and run identity with the result so another comparison does not silently mix different conditions.

Separate the observation from its explanation. A reading or a counted object belongs in the evidence; the relationship you use to interpret it belongs in the reasoning. When a result differs from the reference case, check the settings and measurement procedure before deciding that the model relationship has failed. Describe a specific source of uncertainty and where it enters your calculation. Finish with a claim supported by the recorded comparison, and identify an additional trial that could distinguish your explanation from an alternative.

Continue the comparison

Inspect another climate feedback in Albedo & Ice Feedback, or connect dissolved carbon effects to Ocean Acidification. Keep each causal pathway and measured quantity distinct when explaining a shared change in atmospheric carbon dioxide.

Common questions

Standards alignment

  • NGSS HS-ESS2-4
  • AP Environmental Science Unit 9