Radiation pressure

File:Crookes radiometer moving.gif

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

• Sail-Force1.gif

  Force on a reflector results from reflecting the photon flux

• 125-річчя з дня народження П. Н. Лебедєва.jpg

  Soviet ruble coin commemorating Lebedev's discovery

• Pillars of creation 2014 HST WFC3-UVIS full-res.jpg

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

• M92 arp 750pix.jpg

  Star cluster Messier 92.

• David A. Aguilar's Red Dwarf Stars.jpg

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

• Comet Hale-Bopp 1995O1.jpg

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

• 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.

Further reading

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