Radiation pressure

A Crookes radiometer does not demonstrate radiation pressure. Instead, it demonstrates the pressure of hot air that is heated by the energy that light carries to a black surface.

Radiation pressure is the pressure exerted upon any surface exposed to electromagnetic radiation. If absorbed, the pressure is the energy flux density divided by the speed of light. If the radiation is totally reflected, the radiation pressure is doubled. This happens because the waves that make up electromagnetic radiation carry momentum with them and pass that momentum on when they reach a surface.

A Crookes radiometer appears to demonstrate the pressure of light, but instead it demonstrate the energy that light brings to a surface. The black side of each paddle absorbs most of the light's energy an causes the air near that surface to have a higher pressure. So, while a Crookes radiometer turns because of pressure, it is air pressure caused by the heat energy that light brings to the device.

Solar radiation at Earth

The solar radiation at Earth's distance from the Sun has an energy flux density of 1370 W/m², and more than half of this energy reaches surface. A calculation shows that this value of the flux would cause on an absorbing surface to experience 4.6 µPa of radiation pressure. A convenient way to compare the Sun's energy flux and radiation pressure is to imagine the pressure and energy deposited on one square meter:

Power = [math]\displaystyle{ P = \left(1370 \frac{W}{m^2}\right)\cdot \left(1 m^2\right) = 1371\, W }[/math] (or about 1.4 kilowatts.)

Force = [math]\displaystyle{ \left(4.6\times 10^{-6} \frac{N}{m^2}\right)\cdot \left(1 m^2\right) = 4.6\times 10^{-6}N = 4.6 \mu N }[/math]

To understand how small a micro-newton is, convert calculate how much mass you need on Earth to get that force using [math]\displaystyle{ \vec F=M\vec g }[/math]:

Mass = [math]\displaystyle{ \frac{F}{g}=\frac{4.6}{9.8}\times 10^{-6}\,kg=.00047 g }[/math] (or about ½ milligram.)

The difference between the energy flux and the pressure is like the difference between the heat coming through a large window and the weight of a very small mosquito.

Radiation Pressure Media

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  Force on a reflector results from reflecting the photon flux

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  Soviet ruble coin commemorating Lebedev's discovery

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  The Pillars of Creation clouds within the Eagle Nebula shaped by radiation pressure and stellar winds.

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  Star cluster Messier 92.

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  A protoplanetary disk with a cleared central region (artist's conception).

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  Comet Hale–Bopp (C/1995 O1). Radiation pressure and solar wind effects on the dust and gas tails are clearly seen.

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  In this optomechanical cavity, light is trapped and enhanced between two mirrors. One of the mirrors is attached to a spring and can move. The radiation pressure force of the light circulating in the cavity can damp or amplify the oscillation of the mirror on the spring.

• In this optomechanical system, the radiation pressure force is leveraged to detect a single protein molecule. Laser light interacts with a glass sphere: the radiation pressure force causes it to vibrate. The presence of a single molecule on the sphere disturbs that (thermal) vibration, and the disturbance in the sphere's motion can be detected in the oscillator spectrum on the left.

Further reading

• Demir, Dilek,"A table-top demonstration of radiation pressure",2011, Diplomathesis, E-Theses univie (http://othes.univie.ac.at/16381/)