To determine the location of an image formed by a spherical mirror (concave or convex) using a ray diagram, we rely on the principles of reflection. The image is formed at the point where the reflected rays actually intersect (for real images) or appear to diverge from (for virtual images).
While using multiple rays can help confirm the image location and characteristics, only two reflected rays are fundamentally necessary to pinpoint the image's position. The intersection point of these two rays defines where the image is formed.
The point where these two reflected rays (or their extensions) intersect is the location of the image.
Every point on the object emits rays in all directions. By selecting two specific, predictable rays (like the ones described above, or others like a ray hitting the pole or passing through the focus), we can trace their paths after reflection. Since geometry dictates that two intersecting lines define a unique point, the intersection of just two reflected rays is sufficient to locate the image corresponding to the point from which those rays originated on the object.
Which one of the following telescopes contains only mirrors?
The correct relation between the radius of curvature R and focal length f of a spherical mirror is
Spherical mirror formula relating an object distance ‘u’, image distance ‘v’ and focal length of mirror ‘f’ may be applied to a plane mirror when
The image of an object formed by a plane mirror is
The image we see in plane mirror is