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Geometrical Optics flash cards

Master Geometrical Optics through 97 NEET-level recall cards, systematically structured one idea at a time. Revise concept-wise, identify the areas where you need improvement, and focus your preparation with greater precision.

Geometrical Optics, question and answer

30 of this chapter's 97 cards, laid out open so you can read straight through. The remaining 67 are in the interactive deck, where the answer stays hidden until you commit to one.

  1. 1.State the laws of reflection.

    (1) The angle of incidence equals the angle of reflection (i=ri=r). (2) The incident ray, reflected ray and normal at the point of incidence all lie in the same plane.

    Hint: Two rules: angles + coplanarity.

  2. 2.What is the nature and size of the image formed by a plane mirror?

    Virtual, erect, laterally inverted, of the same size as the object, and located as far behind the mirror as the object is in front.

    Hint: Same size, equal distance behind.

  3. 3.By what angle does a reflected ray rotate if the mirror is rotated by angle θ\theta (incident ray fixed)?

    The reflected ray rotates by 2θ2\theta.

    Hint: Mirror turns θ\theta, ray turns double.

  4. 4.How many images are formed by two plane mirrors inclined at angle θ\theta?

    n=360θ1n=\dfrac{360}{\theta}-1 when 360θ\dfrac{360}{\theta} is even; for odd, n=360θ1n=\dfrac{360}{\theta}-1 if the object is off the bisector, or 360θ\dfrac{360}{\theta} if it is not an integer, take the nearest.

    Hint: 360/θ360/\theta then adjust.

  5. 5.Distinguish between a concave and a convex mirror.

    A concave mirror is a converging mirror (reflecting surface caves inward). A convex mirror is a diverging mirror (reflecting surface bulges outward).

    Hint: Concave converges.

  6. 6.What is the relation between focal length ff and radius of curvature RR of a spherical mirror?

    f=R2f=\dfrac{R}{2}; the focal length is half the radius of curvature.

    Hint: Focus is midway to centre.

  7. 7.State the mirror formula.

    1v+1u=1f\dfrac{1}{v}+\dfrac{1}{u}=\dfrac{1}{f}, where uu is object distance, vv image distance, ff focal length.

    Hint: 1/v+1/u=1/f1/v+1/u=1/f.

  8. 8.Define linear (transverse) magnification for a mirror.

    m=hh=vum=\dfrac{h'}{h}=-\dfrac{v}{u}, ratio of image height to object height.

    Hint: m=v/um=-v/u.

  9. 9.State the sign convention (Cartesian) used for mirrors and lenses.

    Distances are measured from the pole/optical centre; those measured along the incident light direction are positive, opposite are negative. Heights above the axis are positive, below negative.

    Hint: Incident direction positive.

  10. 10.For a concave mirror, what does a negative magnification indicate?

    A real, inverted image (image on the same side as the object).

    Hint: Negative mm → real & inverted.

  11. 11.What is the sign of ff for concave and convex mirrors?

    Concave mirror: ff negative. Convex mirror: ff positive (in the standard sign convention).

    Hint: Concave f<0f<0.

  12. 12.Where must an object be placed before a concave mirror to get a magnified real image?

    Between the focus FF and centre of curvature CC; the image forms beyond CC, real, inverted and enlarged.

    Hint: Between F and C.

  13. 13.What kind of image does a convex mirror always form?

    A virtual, erect, diminished image located between the pole and focus, for all real object positions.

    Hint: Always virtual, erect, small.

  14. 14.Why are convex mirrors used as rear-view mirrors in vehicles?

    They always form erect, diminished virtual images and provide a wider field of view.

    Hint: Wide view, erect small image.

  15. 15.Where is the image formed when an object is at the centre of curvature of a concave mirror?

    At CC itself; the image is real, inverted and of the same size as the object (m=1m=-1).

    Hint: Object at C → image at C, same size.

  16. 16.Define refraction of light.

    The bending of light as it passes from one transparent medium to another due to a change in its speed.

    Hint: Speed change bends light.

  17. 17.State Snell's law of refraction.

    n1sini=n2sinrn_1\sin i=n_2\sin r, or sinisinr=n2n1=1n2\dfrac{\sin i}{\sin r}=\dfrac{n_2}{n_1}={}_1n_2 (constant for a given pair of media).

    Hint: n1sini=n2sinrn_1\sin i=n_2\sin r.

  18. 18.Define absolute refractive index of a medium.

    n=cvn=\dfrac{c}{v}, the ratio of the speed of light in vacuum to its speed in the medium.

    Hint: n=c/vn=c/v.

  19. 19.How does refractive index relate to wavelength when light enters a denser medium?

    Frequency stays constant; speed and wavelength decrease. n=λvacλmedn=\dfrac{\lambda_{vac}}{\lambda_{med}}.

    Hint: λ\lambda shrinks, ff fixed.

  20. 20.What is lateral shift in refraction through a glass slab?

    The perpendicular displacement between the incident ray direction and the emergent ray; the emergent ray is parallel to the incident ray but laterally displaced.

    Hint: Parallel emergent ray, sideways shift.

  21. 21.Why does the emergent ray from a parallel-sided glass slab stay parallel to the incident ray?

    The refractions at the two parallel faces are equal and opposite, so the net angular deviation is zero (only a lateral shift remains).

    Hint: Equal & opposite bends cancel.

  22. 22.Why does a pool of water appear shallower than it really is?

    Because of refraction; real depth and apparent depth are related by n=real depthapparent depthn=\dfrac{\text{real depth}}{\text{apparent depth}}.

    Hint: Apparent depth = real/n.

  23. 23.Define critical angle.

    The angle of incidence in the denser medium for which the angle of refraction in the rarer medium is 9090^\circ.

    Hint: Refraction just grazes at 9090^\circ.

  24. 24.Relate critical angle CC to refractive index.

    n=1sinCn=\dfrac{1}{\sin C} (for a denser medium of index nn against vacuum/air).

    Hint: sinC=1/n\sin C=1/n.

  25. 25.State the two conditions necessary for total internal reflection.

    (1) Light must travel from a denser to a rarer medium. (2) The angle of incidence must exceed the critical angle.

    Hint: Denser→rarer and i>Ci>C.

  26. 26.Give two natural/technological examples of total internal reflection.

    Mirage, sparkle of diamonds, optical fibres, totally reflecting prisms in binoculars/periscopes.

    Hint: Mirage, diamond, optical fibre.

  27. 27.Why does a diamond sparkle brilliantly?

    Its very high refractive index gives a small critical angle (24.4\approx 24.4^\circ), so light undergoes repeated total internal reflection before emerging.

    Hint: High n, small critical angle.

  28. 28.How does an optical fibre guide light?

    By repeated total internal reflection at the core–cladding boundary, the core having a higher refractive index than the cladding.

    Hint: TIR down the core.

  29. 29.Why is a mirage seen on hot roads?

    Hot air near the ground is less dense (lower n); light from the sky bends and undergoes total internal reflection, creating an inverted watery image.

    Hint: TIR in hot rarer air.

  30. 30.State the equation for refraction at a single spherical surface.

    n2vn1u=n2n1R\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R}, where light travels from medium n1n_1 into n2n_2.

    Hint: n2/vn1/u=(n2n1)/Rn_2/v - n_1/u = (n_2-n_1)/R.

Open the interactive deck for the other 67 cards, with self-grading so the ones you keep missing come back.

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