radiation pressure

American  

noun

Physics.

1. the pressure exerted on a surface by electromagnetic radiation or by sound waves.

---

radiation pressure Scientific  

1. Force per unit area exerted by waves or particles of radiation, especially photons. Though photons have no mass, they do have momentum, and can transfer that momentum to other particles upon impact. The amount of pressure exerted by a given amount of radiation depends on whether the radiation is absorbed or reflected. Radiation pressure is responsible for the Casimir effect; solar radiation pressure is exploited in the design of solar sails.

---

Etymology

Origin of radiation pressure

First recorded in 1900–05

Example Sentences

Dust can be pushed outward by radiation pressure from the central star, swept up by planets or planetesimals, or spiral inward and fall into the star.

From Science Daily

These are more powerful than run-of-the-mill supernovae, which occur when a star runs out of fuel and implodes with a sudden loss of radiation pressure akin to demolishing the supports holding up a roof.

From Scientific American

During the star-forming phases, the radiation pressure from the stars would blast out dust, making the galaxies appear bright and blue.

From Science Magazine

Solar radiation pressure is exceedingly weak, however, which is why practical solar sails must be so large.

From Scientific American

“I’m making an analogy to the Casimir effect, where you can push plates together with a noticeable radiation pressure from the vacuum,’’ he says.

From Literature