Radiation Pressure
This definition page has been automatically generated. You can help ExoDictionary by expanding, updating, or correcting it. |
This autostub has not yet had its initial copyediting proof and may contain significant formatting and even factual errors. You can improve Exodictionary by cleaning up the page markup and verifying that the definition is correct and then removing this tag. |
This autostub has not yet had its initial categorization proof and may be categorized incorrectly. You can improve Exodictionary by removing inappropriate categories and then removing this tag. |
Radiation Pressure
r</sub>)</strong>
</dt>
Pressure exerted upon any material body by electromagnetic radiation incident
upon it. See Poynting-Robertson effect.
</dd>
This pressure is manifested whenever the electromagnetic momentum is
a radiation field is changes, and is exactly twice as great when the radiation
is reflected at normal incidence as it is when the radiation is entirely absorbed
at normal incidence. The magnitude of any radiation-pressure effect is directly
proportional to the intensity of the radiation, and is very small by most
standards. On a perfectly reflecting surface Pr = u/3 where u is
radiation density, the amount of radiative energy per unit volume in the space
above the surface. Radiation pressure has a perceptible effect on the orbit
of earth satellites, especially those with a large reflecting surface such
as Echo.
</dd>
References
This article is based on NASA's Dictionary of Technical Terms for Aerospace Use