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Solar – Radiometer

The Radiometer – also called lightmill – is an instructive, physical demonstration object that was invented about 100 years ago by the English physicist Crookes. This small physical-technical arrangement clearly shows how light is converted into mechanical energy.

 

 

The working princip of the solar radiometer:

Impeller inside the part evacuated glass ball

If warm light, ie sunlight, light of light bulbs or spotlights, meets with light in the spectrum of which the infrared component is present (but not cold light from fluorescent lamps) on the wing cross resting on a needle, this will turn depending on the intensity of the light source , In a particular method, a partial vacuum is generated in the glass ball, so that the air resistance is not stronger than the rotational force of the impeller generated by the light energy. The blackened surfaces of the wing cross absorb more light energy than the bright surfaces. Due to the warming of the air molecules, a much higher pressure is created on the dark areas than on the bright areas. This causes the constant rotation of the wing cross. (Brownian Molecular Theory). Depending on the light intensity, up to 3000 revolutions per minute should be achieved. (Source: Manufacturer of the Radiometer)

 

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