phenomenon

radiation pressure

The mechanical force exerted by light on surfaces it strikes, used here to synchronize vibrations.
5 related articles

Description

Radiation pressure is the mechanical force exerted by light or other electromagnetic radiation on a surface it strikes. Although light has no mass, it carries momentum, and when photons are absorbed or reflected, they transfer that momentum to the object. This pressure is minuscule in everyday life—sunlight exerts about 9 micronewtons per square meter—but it becomes significant in precision physics and space technology.

History

The concept was first proposed by Johannes Kepler in 1619 to explain why comet tails point away from the Sun, and was later derived from Maxwell's electromagnetic theory in the 19th century.

How it works

When a photon hits a surface, its momentum is transferred. If the surface is reflective, the photon bounces back, transferring twice the momentum compared to absorption. The cumulative effect of many photons produces a steady force. In optomechanics, this force can be used to cool or synchronize the vibrations of tiny mechanical resonators, effectively coupling light and motion.

In practice

Radiation pressure is used to manipulate microscopic objects in optical tweezers, to stabilize the orientation of spacecraft via solar sails, and to cool mechanical resonators in quantum experiments.

Fun fact

A solar sail the size of a football field would experience about 0.01 newtons of force from sunlight—enough to slowly accelerate a spacecraft over months.

Concept graph →

Related articles · 5

Optics2026-08-193 minarXiv:2608.19016
A Silicon Atom in the Dark: A Trap That Doesn't Glow
The laser beam in an optical tweezer is not just a spot of light but a force bag. A particle caught in it usually rolls toward the brightest point, like a ball into a dimple.
Plasma Physics2026-05-242 minarXiv:2605.25060express
Invisible Fire: How Plasma Cools by Emitting Light
Imagine a powerful hair dryer that blows not warm air but white-hot plasma, such devices are called plasma wind tunnels. They are used to test on Earth how a spacecraft will enter the atmosphere.
HEP Phenomenology2026-05-111 minarXiv:2605.11278express
Cosmic Hydrogen Catches Gravitational Waves
Hydrogen is the most common element. Its atoms are like antennas: they emit and absorb light at very specific frequencies. Einstein predicted that spacetime can ripple: these are gravitational waves.
HEP Phenomenology2026-03-071 minarXiv:2603.07010express
Cosmology2025-11-182 minarXiv:2511.14163express
Light Gets Even Lighter: New Upper Limit on Photon Mass
Fast radio bursts are brilliant cosmic flashes that, like a starting signal, set off a race of radio waves across the universe. Astronomers used them as a natural laboratory to test whether the photon, the quantum of light and the carrier particle of the electromagnetic interaction, has mass.