Light that has been deflected from its original path by particles or surfaces.Scattered light is light that has been deflected from its original trajectory by interactions with particles, molecules, or surfaces. This process is responsible for the blue color of the sky, the reddening of sunsets, and the diffuse glow around stars and galaxies. In astrophysics, scattered light carries information about the composition and structure of the scattering medium, from interstellar dust to the atmospheres of exoplanets.
The quantitative theory of scattering was developed by Lord Rayleigh in the 1870s, building on earlier work by James Clerk Maxwell on electromagnetism.
When light encounters a particle, its electric field induces oscillations in the particle's charges, which then re-radiate light in all directions. The intensity and angular distribution of this re-radiated light depend on the particle size relative to the wavelength, the refractive index, and the polarization. Rayleigh scattering dominates for particles much smaller than the wavelength, while Mie scattering applies to larger particles.
Used in remote sensing, atmospheric physics, and astronomy to probe the properties of dust clouds, planetary atmospheres, and even the cosmic microwave background.
The Tyndall effect — where a beam of light becomes visible when passing through a colloid — is a direct consequence of scattering and is why car headlights appear as cones in fog.

