Black Body Radiation
From ExoDictionary
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. |
Black Body Radiation
The electromagnetic
radiation emitted by an ideal black body;
it is the theoretical maximum amount of radiant energy of all wavelengths
which can be emitted by a body at a given temperature.
The spectral distribution of black-body radiation is described by Planck law
and the related radiation
laws. If a very tiny opening is made into an otherwise completely enclosed
space (hohlraum), the
radiation passing out through this hole when the walls of the enclosure have
come to thermal equilibrium at some temperature will closely approximate ideal
black-body radiation for that temperature.
References
This article is based on NASA's Dictionary of Technical Terms for Aerospace Use