To solve this problem, we need to analyze how the images from the convex and plane mirrors can coincide.
Step 1: Determine the properties of the convex mirror.
Given:
For a convex mirror, the mirror formula is:
\(\frac{1}{f} = \frac{1}{v} + \frac{1}{u}\)
Substituting the given values:
\(\frac{1}{30} = \frac{1}{v} - \frac{1}{30}\)
Solving for \(v\):
\(\frac{1}{v} = \frac{1}{30} + \frac{1}{30} = \frac{2}{30}\)
Thus, \(v = 15 \, \text{cm}\)
This means the image formed by the convex mirror is virtual, upright, and located 15 cm behind the mirror.
Step 2: Analyze the image formation by the plane mirror.
The plane mirror forms an image that appears at the same perpendicular distance behind the mirror as the object is in front of it. If the image from the convex mirror coincides with the image formed by the plane mirror, they must be at the same location.
The virtual image from the convex mirror is at 15 cm behind it. For the images to coincide:
Let the distance between the two mirrors be \(D\) cm.
For the images to coincide:
\(D + D = 15 \, \text{cm}\)
Simplifying gives:
\(2D = 15 \, \text{cm}\)
\(D = 7.5 \, \text{cm}\)
Therefore, the distance between the two mirrors must be \(7.5 \, \text{cm}\).
Hence, the correct answer is 7.5 cm.
To solve this problem, we need to understand how the images formed by a convex mirror and a plane mirror can coincide.
Therefore, the correct answer is 7.5 cm.
Light from a point source in air falls on a spherical glass surface (refractive index, \( \mu = 1.5 \) and radius of curvature \( R = 50 \) cm). The image is formed at a distance of 200 cm from the glass surface inside the glass. The magnitude of distance of the light source from the glass surface is 1cm.
Consider the following statements:
A. The junction area of a solar cell is made very narrow compared to a photodiode.
B. Solar cells are not connected with any external bias.
C. LED is made of lightly doped p-n junction.
D. Increase of forward current results in a continuous increase in LED light intensity.
E. LEDs have to be connected in forward bias for emission of light.