Mastery of ray optics and optical instruments is essential for CBSE board exams and competitive tests (JEE/NEET) because it links geometric reasoning with algebraic manipulation — students must analyse image formation, sign conventions, lens/mirror combinations and instrument design under varied arrangements. Problems in this chapter frequently require multi-step reasoning (ray tracing → applying lens/mirror formulas → interpreting final image parameters) and provide plentiful opportunities to score high marks.
Beyond routine formula use, the chapter tests conceptual understanding needed in competitive settings: dispersion and chromatic effects, resolving power, aberrations, and the behaviour of optical systems when immersed in different media or combined with other elements (slabs, mirrors, polarizers). Practising these topics builds the ability to interpret graphs/data, handle assertion–reason logic, and solve tricky quantitative problems under exam time pressure.
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10
Questions
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Marking Scheme
Q1. A thin convex lens of focal length forms a real, inverted image twice the size of the object. The object distance from the lens is:
Q2. Two thin convex lenses with focal lengths and are placed coaxially with a separation . The effective focal length of the combination (thin-lens approx.) is closest to:
Q3. A graph shows the refractive index of a glass exhibiting normal dispersion (monotonically decreasing with increasing wavelength ). A thin convex lens made of this glass is used in air. For monochromatic blue light () and red light () with , which statement about focal positions is correct?
Q4. Assertion (A): An achromatic doublet made of crown and flint glass can completely eliminate chromatic aberration for all wavelengths of the visible spectrum.
Reason (R): Achromatic doublets are designed so that the dispersions of the two lenses cancel for two chosen wavelengths; residual dispersion (secondary spectrum) remains for other wavelengths.
Q5. A convex lens of focal length is used as a magnifying glass. For an eye with least distance of distinct vision the angular magnifications when the final image is at infinity and when it is at the near point are and respectively. The ratio equals:
Q6. A thin converging lens of focal length forms a real image at distance when an object is at . A plane-parallel glass slab of thickness and refractive index is inserted between the object and the lens (slab adjacent to the object). Using the approximation that the slab shifts the apparent object toward the lens by , the image distance from the lens changes by approximately:
Q7. Two stars have an angular separation of (arcsecond). Using the Rayleigh criterion for a circular aperture at wavelength , the minimum diameter of the telescope objective required to just resolve them is closest to:
Q8. A plot of transmitted intensity vs analyzer angle for unpolarized incident light follows Malus’s law after the first polarizer. If unpolarized light of intensity passes through an ideal polarizer followed by an analyzer at angle relative to the polarizer, the transmitted intensity after the analyzer is:
Q9. Assertion (A): A parabolic reflector shows spherical aberration for parallel incoming rays close to the axis (paraxial rays).
Reason (R): Spherical aberration arises because spherical surfaces do not bring all parallel rays to the same focus; a parabolic reflector brings parallel rays to a single focus and thus removes spherical aberration for parallel rays.
Q10. A thin symmetric lens made of glass with refractive index has focal length when in air. It is now completely immersed in a liquid with refractive index . Using the lens-maker form and assuming the radii are unchanged, the new focal length (in the liquid) is approximately: