Snell's Law is a foundational principle in optics that governs the behavior of light as it moves from one medium to another. When a light ray encounters a boundary between two different transparent materials, it generally bends, or refracts, at an angle. This behavior can be precisely described by Snell's Law, which is mathematically represented as:
\[\begin{equation} n_1 \sin(\varphi_1) = n_2 \sin(\varphi_2)\end{equation}\]
Here, \(\varphi_1\) is the angle of incidence—this is the angle between the incident ray and an imaginary line called the normal, which is perpendicular to the boundary. Similarly, \(\varphi_2\) is the angle of refraction, which is the angle between the refracted ray and the normal. The variables \(n_1\) and \(n_2\) represent the indices of refraction for the first and second material, respectively.
- Understand the term 'normal': It is an imaginary line perpendicular to the boundary between two materials.
- Angle of incidence and refraction: These are measured from the normal, not the boundary.
- Implications of Snell's Law: It explains phenomena like bending of light in a pool and the formation of rainbows.
Snell's Law not only helps us understand why light bends, but it is also instrumental in calculating the extent of this bending, which is essential for designing optical devices such as lenses and telescopes.