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Question #43229
The Question
A telescope has an objective lens of diameter and focal length . A thin transparent glass disk of thickness is placed immediately in front of the objective lens. The refractive index of the glass disk varies radially as , where is the radial distance from the optical axis, , and . The telescope is used to observe a distant star emitting light of vacuum wavelength . If the viewing screen is adjusted to the new focal plane to obtain the sharpest image, what is the linear diameter of the first dark ring (Airy disk) of the diffraction pattern?
Options
- A.
- B.
- C.
- D.
Check Your Answer
Correct Answer
Step-by-Step Solution
Explanation
How the Examiner Thinks
Multi-Concept_Bridge
Master problems that require linking physics and math concepts to solve complex competitive questions.
Concepts Behind This Question
Resolving Power Limits|Medium Dependency|Non-Uniform Dielectric Filling|Binomial Approximation
Why This Question Is Tricky
Common Mistakes
This question tests the student's ability to recognize that a non-uniform dielectric medium (gradient-index) introduces a spatially varying phase shift, effectively acting as a lens.
A common trap is to blindly apply the standard Airy disk formula using the original focal length, ignoring the wavefront curvature introduced by the profile.
Another trap is incorrectly scaling the wavelength to in the diffraction formula, failing to realize that the diffraction pattern forms in the air/vacuum after the light exits the thin disk, meaning the vacuum wavelength dictates the angular spread.
Quick Facts About This Question
Question Information
| Subject | Physics |
| Chapter | Ray Optics and Optical Instruments - Class 12 |
| Concept | Resolving Power Limits |
| Difficulty | 8 |
| Cognitive Load | 7 |
| Target Solve Time | 160 sec |
| Access | Free |