Greenhouse effect
Teacher Guide

The atmospheric greenhouse effect

Why do planets have different temperatures even under the same Sun?

This is the teacher guide for this lesson. A student-focused guide to assist learners as they perform the activity is available.

View the student guide: The atmospheric greenhouse effect

What is the greenhouse effect? How do certain gases in our planetary atmosphere trap heat?

  • Infrared thermometer
  • Clear polyethylene sheets (0.002 inches, 0.005 inches, 0.01 inch thickness)
  • 12 popsicle sticks

In this hands-on lab, students investigate how atmospheric composition regulates planetary temperatures by modeling "optical thickness" using infrared thermometers and layers of polyethylene sheeting. By rotating through interactive stations—including PhET simulations and a physical demonstration of thermal radiation—students collect data to visualize how greenhouse gases trap heat. Teachers can use this Critical Conversations Guide (CCG) after the lesson to facilitate a discussion about how human actions and personal values connect to heat absorption and climate change.

  • Total time
    75–90 minutes (4 stations at 12–15 minutes per station, plus additional time for summary)
  • Education level
    Grades 6 - 10
  • Content Area
    physics, astronomy, atmospheric physics, earth & environmental science
  • Educational topic
    Radiative transfer, infrared radiation

When sunlight hits our atmosphere or the surface of the Earth, some of that energy is absorbed and later re-emitted as infrared radiation (heat). Unlike visible light, infrared light is absorbed efficiently by certain gases in the atmosphere, known as greenhouse gases, including carbon dioxide (CO2), methane (CH4), and water vapor (H2O).These gases allow incoming sunlight to pass through, but absorb outgoing infrared radiation, trapping heat in the atmosphere. This process keeps Earth warm enough to sustain life.

Mathematical model (optional)

Here is a schematic of the simplest model of greenhouse effect from Schneider and Novak (2024). An isothermal atmosphere with temperature Ta is in radiative equilibrium with an underlying surface with temperature Ts. The atmosphere is transparent to shortwave radiation but grey to longwave radiation, with a longwave emissivity. The surface absorbs and reflects shortwave radiation, with a shortwave albedo; it emits longwave radiation as a blackbody.

This graphic may be helpful for your students to see at the end of the lesson.
Key terms
  • Solar radiationAlso called shortwave radiation. Incoming light and energy originating from the sun. It is composed mainly of ultraviolet (UV), visible, and some infrared radiation.
  • Infrared radiation/infrared radiationA type of electromagnetic radiation with wavelengths longer than visible light that carries heat energy. Emitted by objects as heat, allowing us to measure the temperature of an object.
  • Greenhouse effectThe natural process by which certain gases in Earth's atmosphere trap heat radiating from the Earth toward space, keeping the planet warm.
  • Optical thicknessA measure of obstruction to radiation in a medium. A larger optical thickness allows less radiation to pass through.
Before the experiment
  • We invite you to watch a brief video demonstration of the developer conducting the experiment you’ll be facilitating with your students.

  • Create or have a set of students create an experimental structure for holding the plastic "atmosphere" layers using popsicle sticks like in the photo or other materials you may have like the activity developers used.

    1. Glue 4 popsicle sticks together into a square
    2. Glue 4 popsicle sticks as legs
    3. Glue another 4 popsicle sticks into a square for base of structure
    Fig. 1 - popsicle sticks glued together from materials in the kit. Glue in an offset fashion for best results.
    Fig. 2 - Structure made from tinker toys
  • Set up 4 stations as follows:

    1. Stations 1 and 2 include links to simulations and/or videos; if students are using physical worksheets, we recommend either setting up a computer with the simulation/video already pulled up at these stations or sharing those resources in an announcement to the class so they can access them easily on their own devices.
    2. Station 3: Infrared thermometer, popsicle stick tower, and plastic films. Teachers will be directly facilitating Station 3.
    3. Station 4: Independent research station. If students do not have their own devices such as Chromebooks, set up a computer that students can use to research information on the planets.
Setting up
  • Make a connection between what students learned in Activity 1 about types of light and infrared radiation. Describe IR radiation as heat or thermal radiation. Remind students this is what surfaces (in this case the hand) emit into the atmosphere.

  • Demonstrate how to properly use the infrared thermometer, showing how to point it (distance from the object), read values, and understand emissivity differences between different materials.

    a. Remind students that the thermometer measures surface infrared radiation, not air temperature.

    b. Remind students of safety when using the infrared thermometer.

During the experiment
Station 1: What is weather, climate, atmosphere?

Students will use a simulation and a video to understand weather, climate, and atmosphere. See student guide for more details.

Station 2: Molecules and light

Students will use Molecules and Light PhET simulation to understand how different molecules react when hit with different types of light from the electromagnetic spectrum. You may want to review information from Activity 1 if completed. If not, then review the electromagnetic spectrum. See student guide for more details.

Station 3 (teacher-led station): Why do planets have different temperatures even under the same Sun?

Students will test various thicknesses of plastic to mimic layers of the atmosphere and how heat is transferred through the layers. Have students:

  • Place a hand at the bottom of the popsicle structure, against the table, with their palm facing up.

  • Hold the thermometer just above the structure.

  • Take a temperature reading of their hand without any films in place.

  • Place the first (0.002 inch) thickness of plastic sheeting onto the popsicle stick structure. Make sure they handle the films with the edges only.

  • Check that each layer is smooth and laying evenly. This part of the experiment simulates the atmospheric “optical thickness”.

  • Hold the thermometer just above the plastic sheeting and take a measurement of the heat emitted from the hand through the sheeting.

  • Make sure the student’s hand is kept the same distance from the sheeting and the thermometer each time.

  • Record in the table below (also found in the student guide).

  • Repeat for each plastic thickness.

    Film thickness [inches]
    Temperature without film [Celsius]
    Temperature with film [Celsius]
  • If time allows, students may want to experiment with layering multiple films at once to get new thicknesses.

  • If time allows, different students can try measuring temperature with different hands.

  • Have students describe their observations in terms of atmospheric thickness, and relate that back to the greenhouse effect.

    Students will chart their data on the following graph as part of the discussion & conclusion section after the class comes back together.

Station 4: Atmosphere on different planets

Students will research different aspects of different planets’ atmospheres to see how optical thickness affects surface temperatures. Students will review the greenhouse effect and connect these ideas. If students are struggling to find good sources, offer this NASA webpage: https://science.nasa.gov/solar-system/planets/ ​​See student guide for more details.

Discussion and conclusion

Choose any or all of the discussion and conclusion prompts below. We’re aware that climate change can bring up a variety of perspectives and emotions in the classroom – see our Critical Conversations Guide for tips on how to facilitate an open dialogue surrounding these issues.

  • Have students graph their data from Station 3 using the chart provided.

  • Guide students to identify patterns. They should expect that more layers correspond to lower measured temperatures that eventually approach the room temperature, meaning less heat emitted from the palm can reach the thermometer.

  • Have students connect their data from Station 3 to the information they gathered about Mars, Venus, and Earth in Station 4, and match each layer from Station 3 with a planet in Station 4.

  • Help students define optical thickness based on their evidence, which is the idea that a thicker atmosphere absorbs and re-emits more infrared radiation to prevent heat from escaping efficiently.

  • Host a discussion on the definition of greenhouse effect. Have students connect the ideas of optical thickness with the greenhouse effect.

  • Have students connect greenhouse gases to the Molecules and Light simulation. They should observe that some molecules (greenhouse gases) allow visible light to pass through, but interact with/scatter infrared light.

  • Encourage students to come up with final conclusions supported by their data.

  • Help students brainstorm: What careers might involve studying how energy moves through the atmosphere or analyzing climate data, and what skills from this activity would be useful in those jobs?

Bonus Activity

Place the aluminum foil on the palm and let it warm up to reach the same temperature as the palm. Remind students that foil reflects more infrared light instead of emitting it. The measured temperature should therefore appear lower than for the plastic layers. Guide them to notice that the measured temperature should be lower and to connect this with low emissivity of reflective surfaces. Could this relate to how clouds or ice reflect sunlight in Earth’s atmosphere?

Real-world connections

  • Sign up for Physicists To-Go to have a scientist talk to your students.
  • Have students read and reflect on this year’s scientist profile on Eunice Newton Foote.

Credits

Developed by: Xiyue (Sally) Zhang, Patrick Arnott, Ph.D., Melodi Rodrigue, Ph.D., Megan Beckam, Ph.D., Sara Wilson – University of Nevada Reno

Piloted by: Thomas Binninger, Jacqueline Clarke, Nataliya Fletcher, Sandy Gady, Erin Martin, Vilma Orduna, Amy Truemper

Edited by: Rosie Durland – University of Utah
PhysicsQuest ©️ 2026 by American Physical Society is licensed under CC BY-NC 4.0

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