Sigma Percentile
JEE Main 2019
LEVELJEE Main

Animated Solution for Physics - Optics: A concave mirror for face viewing has focal length of . The distance at which you hold the mirror from your face in order to see your image upright with a magnification of is

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Visualized Solution

\text{Visualizing the Setup}

\text{Magnification Sign Convention}

\text{Magnification Formula}

\text{Relation between } v \text{ and } u

\text{The Mirror Formula}

\text{Substituting Values}

\text{Algebraic Computation}

\text{Final Answer}

\text{The Way Forward}

The Sigma Insight: Spherical Mirror

Solution Diagram

The Magic of Concave Mirrors

Have you ever looked into a shaving mirror or a makeup mirror and marveled at how your face appears so much larger? This isn't just magic; it's the elegant physics of spherical mirrors at play. In this problem, we are tasked with finding the exact distance you need to hold a concave mirror to achieve a specific magnification. Let's dive into the mechanics of this fascinating phenomenon.

Analyzing the Setup

The problem states that the concave mirror has a focal length of . Because it is a concave mirror, we must apply the Cartesian sign convention, which tells us that the focal length is negative: .
We are also told that the image is upright and magnified times. In the realm of spherical mirrors, an upright image is always a virtual image. Virtual images are formed behind the mirror, and their heights are measured positively above the principal axis. Therefore, the magnification is strictly positive: .

The Master Equation

To find the object distance , we need to link the magnification to the mirror formula. We start with the magnification formula for spherical mirrors:
Substituting our known magnification, we get:
Rearranging this gives us a direct relationship between the image distance and the object distance:
This equation beautifully illustrates that the virtual image is formed behind the mirror at a distance five times greater than the object's distance in front of the mirror.

Final Calculation

Now, we bring in our heavy artillery—the mirror formula:
Let's carefully substitute our expression for and our known focal length :
To solve this, we find a common denominator on the left side:
Now, it's just a matter of simple algebra to isolate :
The negative sign is a reassuring confirmation of our sign convention—it simply means the object (your face) must be placed in front of the mirror.

Pro-Tip

The Speed Formula
While the step-by-step method is fantastic for building intuition, competitive exams demand speed. You can bypass finding entirely by using the combined magnification formula:
Let's plug in our values and watch the magic happen in one step:
Mastering these alternate forms will give you a significant edge in your physics journey!

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