LEVELJEE Main
Visualized Solution
The Sigma Insight: Refraction at Spherical Surface
Analyzing the Setup
Imagine a spherical surface that acts as a boundary between two different media: air on one side and glass on the other. The problem tells us that the center of curvature of this surface lies inside the glass. This means if we are looking from the air, the glass surface bulges outwards towards us—it's a convex refracting surface.
We place a point object in the air. Light rays from travel through the air, hit the spherical surface, and refract into the glass to form a real image . The line connecting the object and the image passes through the pole of the spherical surface. We are given a beautiful symmetry: the distance from the pole to the object () is exactly equal to the distance from the pole to the image (). Let's call this unknown distance .
The Master Equation
To solve any problem involving refraction at a single spherical surface, we rely on the master equation:
Here, is the refractive index of the medium where the incident rays originate (air, so ), and is the refractive index of the medium where the refracted rays travel (glass, so ). The terms , , and represent the object distance, image distance, and radius of curvature, respectively.
Applying the Sign Convention
The most critical step in optics is applying the Cartesian sign convention correctly. We take the pole as our origin . The direction of incident light (from left to right) is taken as positive.
1. Object Distance (): The object is in the air, to the left of the pole. Therefore, .
2. Image Distance (): The real image forms in the glass, to the right of the pole. Therefore, .
3. Radius of Curvature (): The center of curvature is in the glass, to the right of the pole. Therefore, the radius is .
Final Calculation
Now, let's substitute these values into our master equation:
Notice how the two negative signs in the second term cancel each other out:
Since the denominators on the left side are the same, we can simply add the numerators:
Finally, solving for , we get:
Thus, the distance is exactly .
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