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Physics

LAB: Determining Blackbody Emissivity

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Physics Lab

Thermodynamics and Quantum Mechanics

Goal: To Measure emissivity

Be sure that you play with the two student exercises so that you understand Planck's distribution formula.

Materials

Procedure

  1. Predict emissivity (amount of energy escaping through a side) for each side of the box in general terms: which side will emit the most energy? Which the least?
  2. Record the dimensions of the sides of your box.
  3. Create a data table for each set of measurements (you will need multiple tables, one for each temperature reading):
    T0 = val T0 +20°C = val T0 +40°C = val T0 +60°C = val T0 +80°C = val
    Calculated Flux
    White Side rev/min
    Metal Side rev/min
    Black Matte Side rev/min
    Black Glossy Side rev/min
  4. Set up the box as shown, with the lightbulb inside. Leave the lightbulb off.
  5. Place the box on your rotating table.
  6. Place the radiometer in a fixed distance from one side of the box, on a line normal to the center of the side.
  7. Record the ambient temperature T0 and calculate the Stefan-Boltzmann flux for that temperature; record this on the table under the temperature.
  8. Using the rotating table, turn each face to the radiometer and record the revolutions per minute (for at least 30 seconds) for each side OR your IR thermometer reading.
  9. Turn on the light bulb and let the temperature increase at least 20 °C (T0 + 20°C). Observe each side for at least 30 seconds and record the revolutions per minute.
  10. Repeat your measurements for T0 + 40°C, T0 + 60°C, T0 + 80°C, T0 + 100°C if possible.

Data Handling

  1. Plot the flux as a function of temperature.
  2. For each side, plot the revolutions/minute as a function of temperature.
  3. Discuss your results.

Report

  1. Describe your experiment in sufficient detail that another similarly equipped student could perform your tests.
  2. Include your assessment that the light bulb acts/doesn't act as a blackbody over various temperature ranges.