Reflection of Light
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Reflection of light is a fundamental phenomenon where light rays, upon striking a surface, return into the same medium. This interaction is governed by two primary laws: first, the angle of incidence is equal to the angle of reflection; and second, the incident ray, the reflected ray, and the normal to the surface at the point of incidence all lie in the same plane. This principle is crucial for u…
Quick Summary
Reflection of light is the bouncing back of light into the same medium after striking a surface. It's governed by two fundamental laws: the angle of incidence equals the angle of reflection (), and the incident ray, reflected ray, and normal all lie in the same plane.
Reflection can be specular (from smooth surfaces, forming clear images) or diffuse (from rough surfaces, scattering light and making objects visible from all angles). Plane mirrors form virtual, erect, laterally inverted images of the same size and at the same distance behind the mirror as the object is in front.
Spherical mirrors are curved: concave mirrors are converging, while convex mirrors are diverging. Key terms for spherical mirrors include pole (P), center of curvature (C), radius of curvature (R), principal axis, principal focus (F), and focal length (f).
The mirror formula, , relates object distance (), image distance (), and focal length (), while linear magnification () describes image size and orientation.
Strict adherence to the New Cartesian Sign Convention is crucial for accurate calculations.
Key Concepts
A plane mirror always forms a virtual, erect, and laterally inverted image. The image is located as far…
This convention is crucial for applying the mirror formula correctly. The pole of the mirror is the origin.…
For spherical mirrors, the focal length () is half of the radius of curvature (). This relationship, $f…
- Laws of Reflection:
* * Incident ray, reflected ray, normal are coplanar.
- Plane Mirror: — Virtual, erect, laterally inverted, same size, .
- Mirror Rotation (fixed incident ray): — Reflected ray rotates by .
- Number of Images (two mirrors at $\theta$): — (if even or symmetric odd), (if asymmetric odd), (if fraction).
- Spherical Mirrors: — Concave (converging, ), Convex (diverging, ).
- Focal Length: — .
- Mirror Formula: — (with New Cartesian Sign Convention).
- Magnification: — .
* : Erect, Virtual. * : Inverted, Real. * : Magnified; : Diminished; : Same size.
For mirror formula signs, remember 'U-V-F': Usually Unique (object is always real, so is negative). Very Variable (image can be positive or negative). Fixed For Form (focal length is negative for concave, positive for convex).