For a concave lens, the focal length \(f\) is negative. The formula for the image distance \(v\) formed by a lens is given by the lens equation: \[ \frac{1}{f} = \frac{1}{u} + \frac{1}{v} \] Where:
\(f\) is the focal length of the lens,
\(u\) is the object distance (distance from the lens to the point where the light beam converges),
\(v\) is the image distance (the distance at which the beam will converge after passing through the lens).
In this case, \(f = -16\) cm (since the lens is concave), and the object distance \(u = -12\) cm (since the beam converges at point P).
Substituting into the lens formula: \[ \frac{1}{-16} = \frac{1}{-12} + \frac{1}{v} \] Solving for \(v\), we get: \[ v = 48 \, \text{cm} \] Thus, the beam will converge at a distance of 48 cm from the lens.
A spherical mirror is a mirror which has been cut out of a spherical surface.
There are two kinds of spherical mirrors:
Concave mirrors are also called converging mirrors, because in these types of mirrors, light rays converge at a point after impact and reflect back from the reflective surface of the mirror.
The convex mirror has a reflective surface that is curved outward. Regardless of the distance between the subject and the mirrors, these mirrors are "always" virtual, upright and reduced.