The refraction of light through a single spherical surface is governed by the formula for refraction at a spherical surface, given by:
\[
\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}
\]
Where:
- \( n_1 \) and \( n_2 \) are the refractive indices of the media (in this case, \( n_1 = 1 \) for air and \( n_2 = 1.5 \) for glass),
- \( u \) is the object distance (the distance of the point source \( S \) from the spherical surface),
- \( v \) is the image distance (the distance of the image formed),
- \( R \) is the radius of curvature of the spherical surface.
Given:
- Radius of curvature \( R = 2 \, \text{cm} \),
- The object is placed in air, so \( n_1 = 1 \),
- The refractive index of glass \( n_2 = 1.5 \).
Substituting these values into the formula:
\[
\frac{1.5}{v} - \frac{1}{u} = \frac{1.5 - 1}{2}
\]
\[
\frac{1.5}{v} - \frac{1}{u} = \frac{0.5}{2} = 0.25
\]
Thus, the image will be formed at a distance \( v \) from the spherical surface. To find the position and nature of the image, the value of \( u \) (object distance) must be specified, as it determines the final image location.
The ray diagram would show light rays entering the spherical surface from the object at a distance \( u \), refracting and converging at the image point \( v \).