Discovering Near-Infrared Light: Reproducing Herschel's Experiment with a Thermal Camera

By Charles Xie

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We know substances of different colors absorb sunlight differently. Black absorbs the most and white absorbs the least. What about the absorption of light of different colors by the same kind of substance? We know sunlight is made of different colors (wavelengths) of light. Do different colors of sunlight have different heating effects when the sun shines on a surface? This inquiry led to the discovery of the invisible infrared light by Sir William Herschel in 1800.


Herschel's discovery of infrared light in 1800

Herschel set up an experiment in which sunlight was passed through a slit and then through a prism, forming a spectrum on his table. He arranged three thermometers in such a way that the central one could be placed at different points in the spectrum. The other two were positioned on either side, to act as controls. He discovered significant heating outside the red light, which is now known as infrared light (to be more precise, near-infrared light, or NIR light in short).

Reproducing Herschel's Experiment

With a thermal camera, we can now easily reproduce his experiment using a setup show as follows:


A very simple experimental setup (published in The Physics Teacher)

We do not need to use a slit to allow only a light beam to travel through a prism into a room like Herschel did to eliminate the effect of direct sunlight. We can just perform the experiment under the sun in an open space. The refracted light from the prism will cause extra heating on the surface of the dark paper that it shines on — in addition to the heating by the direct sunlight. The temperature difference between the additionally-heated area (part of which is illuminated by the rainbow) and the rest of the dark paper can be easily picked up by a thermal camera that typically has a temperature sensitivity of 0.1℃. Without the refracted light through the prism, a piece of dark paper exhibits a uniform temperature distribution on its surface when exposed under the sun (which can also be easily verified using a thermal camera).


Comparing the regular image and the thermal image of the warming on the dark paper


The temperature distribution in the horizontal direction

Click HERE for an interactive video on Telelab


The results above clearly show that the area outside the red light also warms up significantly, suggesting the existence of invisible light outside the red limit of the visible spectrum. (By comparison, the area outside the violet light does not warm up, meaning that this method cannot be used to detect the UV light.)

Important Notes

You may be wondering why there is a gap in our experiment as shown above (it is actually formed by two pieces of dark paper that do not touch each other). We deliberately created it for two reasons: 1) To ensure that the heat in the visible light area is not conducted through the paper to the infrared light area (so the rise of temperature can be solely attributed to the absorption of light — even though paper is not a good thermal conductor); and 2) To serve as a visual marker in the thermal image so that we can clearly see where the boundary between visible and infrared light is on the dark paper. The thermal image also confirms that the heat conduction was effectively impeded by the gap as it appears to be cooler than the adjacent areas.

It is also important to note that the wavelength of the infrared light that warms up the paper is known as the near-infrared (NIR), as opposed to the long-wave infrared (LWIR) detected by a thermal camera such as the FLIR ONE camera. The following image shows the locations of NIR and LWIR in the infrared spectrum.


Infrared spectrum (Image Credit: Edmund Optics)

That is to say, although we use a thermal camera in this experiment, what the device detects (the LWIR light) has nothing to do with the NIR light under investigation. What actually happens is that the dark paper absorbs the NIR light, which energizes its molecules. The molecules with higher kinetic energy then emit more LWIR thermal radiation that gets picked up by the thermal camera.

Conclusion

This experiment shows the incredible power of thermal imaging as a tool for scientific inquiry. While Herschel had only three thermometers to do his experiment, a thermal camera gives us tens of thousands of "thermometers." Through our Telelab platform, the experiment can be now be shared with anyone in the world — whether or not they have a thermal camera at their disposal — to rediscover what Herschel found more than 200 years ago!

Funded by the National Science Foundation, we are advancing the educational power of thermal imaging in collaboration with a consortium of colleges around the country.

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