Difficulty: Easy
Correct Answer: All of the above
Explanation:
Introduction / Context:
The thin-lens equation, written as 1/f = 1/u + 1/v, is used in geometrical optics to relate object distance u, image distance v, and focal length f. Surveying instruments (levels, theodolites, and telescopes) rely on this relation when forming images on cross-hair diaphragms. Knowing when this formula applies avoids errors in instrument design, adjustment, and basic optics questions in civil engineering exams.
Given Data / Assumptions:
Concept / Approach:
The thin-lens model assumes the principal planes coincide (negligible thickness) and rays make small angles with the axis (paraxial rays). Under these conditions, the simple reciprocal relation predicts image location and magnification accurately enough for most educational and field-calibration purposes. Off-axis points, high-aperture systems, or thick compound lenses need more advanced models (principal planes separated, nodal points, or matrix optics).
Step-by-Step Solution:
Verification / Alternative check:
For a simple telescope objective forming a sharp image on the diaphragm, predicted image distances closely match actual values for small apertures and modest fields, validating thin-lens use in most surveying optics questions.
Why Other Options Are Wrong:
Common Pitfalls:
Applying the formula to thick lenses without principal plane corrections; using skew-ray distances; expecting diffraction-limited predictions from a purely geometrical model.
Final Answer:
All of the above
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