Why this topic matters · 9 min read
Optics and Sound together form one of the most consistently tested physics areas in NDA GAT, contributing roughly 4-7 questions per paper. Optics covers reflection, refraction, lenses, mirrors, and optical instruments. Sound covers wave properties, Doppler effect, and resonance. NDA loves numerical questions on mirror and lens formulas, refractive index, and Doppler effect. Conceptual questions on total internal reflection, human ear, and sonar also appear frequently. Mastering these two topics together can easily fetch you 12-20 marks.
Reflection of Light and Mirrors
When light bounces off a surface, it follows two laws: angle of incidence equals angle of reflection, and both rays and the normal lie in the same plane. Curved mirrors (concave and convex) follow the mirror formula. Concave mirrors converge light and are used in torches, headlights, and shaving mirrors. Convex mirrors diverge light and always form virtual, erect, diminished images — used in rear-view mirrors.
- Concave mirror: center of curvature and focus are in front of mirror (real side)
- Convex mirror: always gives virtual, erect, diminished image regardless of object position
- Focal length f = R/2 where R is radius of curvature
- Sign convention: distances measured from pole; in front of mirror is negative
- Magnification m = -v/u; negative m means inverted image
Key formulas
Mirror Formula
1/f = 1/v + 1/u
When: Finding image distance or focal length for any spherical mirror
Magnification
m = -v/u = h_i/h_o
When: Finding size or nature (erect/inverted) of image
Focal Length from Radius
f = R/2
When: When radius of curvature is given instead of focal length
Worked examples
Object at 30 cm in front of concave mirror of focal length 10 cm. Using 1/f = 1/v + 1/u: 1/(-10) = 1/v + 1/(-30), so 1/v = -1/10 + 1/30 = -2/30, v = -15 cm. Image is real, in front of mirror.
A convex mirror has radius 40 cm, so f = +20 cm. Object at 30 cm in front. 1/v = 1/20 - 1/30 = 1/60... wait: u = -30, f = +20. 1/v = 1/20 + 1/30 = 5/60, v = +12 cm. Positive v means virtual image behind mirror.
Refraction and Snells Law
Refraction is bending of light when it travels from one medium to another due to change in speed. The refractive index n of a medium tells how much light slows down compared to vacuum. Denser medium (higher n) bends light toward the normal. This explains why a straw looks bent in water and why a pool looks shallower than it is.
- Refractive index n = speed of light in vacuum / speed in medium = c/v
- Higher n means slower light and more bending
- Apparent depth = Real depth / n (object in denser medium appears shallower)
- Total Internal Reflection (TIR) happens when light goes from denser to rarer medium beyond critical angle
- Critical angle C: sin C = 1/n (for medium to air)
- TIR applications: optical fibre, diamonds, mirages, periscopes
Key formulas
Snells Law
n1 sin(i) = n2 sin(r)
When: Finding angle of refraction or refractive index at any interface
Refractive Index
n = c/v = sin(i)/sin(r)
When: Comparing speed of light or angles between two media
Critical Angle
sin(C) = 1/n
When: Finding critical angle for TIR (medium to air)
Worked examples
Light goes from air to glass (n=1.5) at angle of incidence 30 degrees. sin(r) = sin(30)/1.5 = 0.5/1.5 = 0.333, so r = 19.5 degrees. Light bends toward normal as expected.
Critical angle for glass (n=1.5): sin C = 1/1.5 = 0.667, C = 41.8 degrees. Any angle beyond this causes total internal reflection.
Lenses and Optical Instruments
Convex (converging) lenses are thicker at center; concave (diverging) lenses are thinner at center. Lenses obey the thin lens formula similar to mirrors. Power of a lens in dioptres is the reciprocal of focal length in metres — a key concept for understanding spectacle prescriptions. When lenses are placed in contact, their powers simply add up.
- Convex lens: f is positive, can form real or virtual images depending on object position
- Concave lens: f is always negative, always forms virtual, erect, diminished image
- Power P = 1/f (in metres), unit is dioptre (D)
- Combined power: P = P1 + P2 for lenses in contact
- Human eye defects: Myopia corrected by concave lens; Hypermetropia by convex lens
- Microscope uses two convex lenses; Telescope objective is convex, eyepiece is convex
Key formulas
Lens Formula
1/f = 1/v - 1/u
When: Finding image position for any thin lens
Lens Power
P = 1/f(metres)
When: Converting focal length to power or for combined lens systems
Lens Makers Formula
1/f = (n-1)(1/R1 - 1/R2)
When: When radii of curvature of lens surfaces are given
Worked examples
Convex lens, f = 20 cm, object at 30 cm. u = -30, f = +20. 1/v = 1/20 + 1/(-30) = 1/20 - 1/30 = 1/60. v = +60 cm. Real, inverted image on other side.
Two lenses of powers +3D and -1D placed in contact. Net power = 3 + (-1) = +2D. Net focal length = 1/2 = 0.5 m = 50 cm.
Sound Waves and Properties
Sound is a longitudinal mechanical wave — it needs a medium to travel and cannot travel through vacuum. Particles vibrate parallel to the direction of wave propagation. Speed of sound in air at 0 degrees C is about 332 m/s and increases with temperature. Sound travels fastest in solids, then liquids, then gases — remember SLG (Solid Liquid Gas, fastest to slowest).
- Sound is longitudinal; light is transverse — key difference
- Speed in air at 0 C = 332 m/s; increases by 0.6 m/s per degree C rise
- Speed order: Solids greater than Liquids greater than Gases
- Frequency below 20 Hz = infrasound; above 20,000 Hz = ultrasound
- Resonance: when forced frequency equals natural frequency, amplitude becomes maximum
- Echo: reflected sound heard after 0.1 second minimum; minimum distance = 17 m from wall
Key formulas
Wave Speed
v = f x lambda
When: Relating frequency, wavelength and speed of any wave
Echo Distance
d = v x t / 2
When: Finding distance to reflecting surface using echo time
Speed vs Temperature
v_t = 332 + 0.6t m/s
When: Finding speed of sound at temperature t degrees Celsius
Worked examples
A sound echo returns in 2 seconds. Speed of sound = 340 m/s. Distance = 340 x 2 / 2 = 340 m.
Sound frequency 500 Hz, speed 340 m/s. Wavelength = 340/500 = 0.68 m.
Doppler Effect
The Doppler effect is the apparent change in frequency of sound (or light) when source and observer are in relative motion. If they move toward each other, apparent frequency increases (pitch rises). If they move away, frequency drops. Classic NDA question: a train approaches or moves away — find apparent frequency. Think of it like waves bunching up when source approaches you.
- Source approaching observer: frequency appears higher (wavelength shorter)
- Source moving away: frequency appears lower (wavelength longer)
- Observer moving toward source: frequency increases; moving away: decreases
- Doppler effect in light: blue shift (approaching), red shift (receding) — used in astronomy
- Used in RADAR, SONAR, speed guns, medical ultrasound
Key formulas
Doppler Formula
f_obs = f_source x (v + v_o) / (v - v_s)
When: Observer moving toward source (v_o positive) and source moving toward observer (v_s positive)
Source moving away
f_obs = f_source x v / (v + v_s)
When: Source receding from stationary observer
Worked example
Train of frequency 500 Hz moves toward stationary observer at 20 m/s. Speed of sound = 340 m/s. f_obs = 500 x 340/(340-20) = 500 x 340/320 = 531 Hz. Frequency increases as expected.
⚠ Common mistakes to avoid
- Sign convention errors in mirror and lens formulas: always measure u as negative when object is in front. Forgetting this flips the entire answer.
- Using f = R instead of f = R/2 for mirrors. The focal length is HALF the radius of curvature, not equal to it.
- Confusing concave and convex: students often mix which one converges. Remember Concave = Cave = hollow inward = converges light toward center.
- In Doppler formula, mixing up when to add or subtract velocities. Rule: motion that decreases distance increases frequency — use subtraction in denominator for source approaching.
- Forgetting that echo requires minimum 0.1 second gap between original and reflected sound, and minimum distance of about 17 m. NDA asks this as a conceptual trap.
🧠 Memory aids
- SLG for sound speed: Solids beat Liquids beat Gases. Like a soldier marches fastest on solid ground.
- For eye defects: My Convex (Myopia needs Concave lens). Hyper people are Far-sighted (Hypermetropia = Far = Convex lens corrects it).
- CONCAVE = CONverges = CONcentrates light. CONVEX = diVERGes = scatters (remember the X spreads out).
- Doppler: APPROACHING = frequency AMPLIFIES (both start with A). Receding = Reduces frequency (both R words).
🎯 NDA exam tips
- NDA typically asks 1-2 direct numerical questions on mirror or lens formula per paper. Practice plugging in sign convention correctly under time pressure — 30 seconds per question is the target.
- Conceptual questions on TIR, optical fibre, and why convex mirror is used in vehicles appear almost every year. These are easy guaranteed marks if you memorize the one-line reasons.
- Doppler effect questions usually give you a moving train scenario. They test the formula application, not derivation. Know the standard formula and which velocity goes in numerator vs denominator.
- Sound questions often test the boundary: infrasound vs ultrasound frequency limits, applications of ultrasound (SONAR, medical imaging), and echo conditions. These are purely factual and take under 20 seconds.
- In recent NDA papers (2021-2023), optical instruments like microscope magnification and telescope have appeared as single-line conceptual questions. Know which lens is objective and which is eyepiece, and that magnification of microscope is product of both lens magnifications.
Q1 · medium · AI-verified
A ray of light travels from air (refractive index = 1.0) to glass (refractive index = 1.5) at an angle of incidence of 60°. What is the angle of refraction?
- 30.0°
- 42.7°
- 45.0°
- 35.3°
Q2 · medium · AI-verified
In Young's double slit experiment, if the distance between slits is doubled while keeping other parameters constant, the fringe width will:
- Become half
- Become double
- Remain same
- Become four times
Q3 · medium · AI-verified
A ray of light passes from a denser medium to a rarer medium. If the angle of incidence is 30°, and refractive index of denser medium is √3, what is the angle of refraction in air?
- 60°
- 45°
- 30°
- 90°
Q4 · medium · AI-verified
A sound wave of frequency 340 Hz travels in air with velocity 340 m/s. What is the wavelength of the sound wave?
- 1 m
- 2 m
- 0.5 m
- 1.5 m
Q5 · medium · AI-verified
The intensity level of sound increases by 20 dB. By what factor does the intensity increase?
- 100
- 20
- 10
- 200