NDA Physics · Formula sheet
Light and Optics formulas
11 formulas, 3 reference tables and 37 common traps for NDA Physics Light and Optics, grouped by subtopic.
Reflection and Mirrors
Learn this subtopic in the notesSpherical mirrors — pole, focus, centre, and R = 2f
Focal length and radius of curvature
- focal length
- radius of curvature (= PC)
Mirror formula and magnification
- object distance (from pole)
- image distance (from pole)
- focal length (−ve concave, +ve convex)
- magnification (h'/h)
Common traps
Measure angles from the normal, not the surface
Virtual + erect + same-size — and only laterally inverted
Half your height — distance does not matter
R = 2f, so f = R/2 — not f = 2R
Object at F gives the image at infinity, not between F and P
Only inside F does a concave mirror give a virtual image
A convex mirror NEVER inverts
Sign convention is the whole game
Magnification sign tells you real vs virtual
Refraction, Speed of Light, and Total Internal Reflection
Learn this subtopic in the notesRefraction and Snell's law
Snell's law of refraction
- refractive indices of the two media
- angle of incidence (from the normal)
- angle of refraction (from the normal)
Refractive index — n = c/v
Refractive index and speed
- refractive index of the medium
- speed of light in vacuum (≈ 3 × 10⁸ m/s)
- speed of light in the medium
Total internal reflection and the critical angle
Critical angle
- critical angle (denser→rarer)
- refractive index of the denser medium (vs air)
Common traps
Frequency is the invariant — not speed or wavelength
Normal incidence still slows the light
Speed is the INVERSE of refractive index
Twinkling = refraction; blue sky / red sunset = scattering
TIR only goes denser → rarer
Both conditions, not just a big angle
Mirage is TIR, not simple reflection or dispersion
Lenses and the Lens Formula
Learn this subtopic in the notesLens formula and the sign convention
Lens formula
- object distance from optic centre (−ve for a real object)
- image distance from optic centre
- focal length (+ve convex, −ve concave)
Power of a lens — the dioptre
Power of a lens
- power (dioptre, D)
- focal length in METRES
Lens maker's equation
- refractive index of the lens material
- radii of curvature of the two faces (signed)
- focal length
Lenses in contact — powers add
Combination of thin lenses in contact
- powers of the individual lenses (D)
- power of the combination (D)
- focal length of the combination (m)
Lens magnification and image formation
Lens magnification
- magnification
- image distance
- object distance
Common traps
A concave lens has no real-image setting
Lens uses 1/v − 1/u; mirror uses 1/v + 1/u
Convert cm to metres before computing power
Sign the radii — convex faces are not both positive
Add powers, not focal lengths
Lens m = v/u (no minus); mirror m = −v/u
Prisms and Dispersion
Learn this subtopic in the notesCommon traps
Deviation is refraction, not reflection
Violet bends most because its speed in glass is LOWEST
Primary rainbow = ONE internal reflection (the inner bow)
The Human Eye and Optical Instruments
Learn this subtopic in the notesMicroscope and telescope
Telescope magnification (normal adjustment)
- focal length of the objective
- focal length of the eyepiece
Eye defects and their corrections
| Defect | Problem | Correction |
|---|---|---|
| Myopia (short / near-sightedness) | Cannot see DISTANT objects clearly; image of a distant object focuses BEFORE the retina; far point is finite | Concave (diverging) lens Myopia = sees near clearly, far blurred. Power P = −1/(far point in m). |
| Hypermetropia (long / far-sightedness) | Cannot see NEAR objects clearly; image focuses behind the retina | Convex (converging) lens |
| Presbyopia | Age-related loss of accommodation; both near and far affected | Bifocal lens |
| Cataract | Eye lens becomes cloudy/opaque | Surgery (lens replacement) — not a spectacle lensQ |
Common traps
The eye is a CONVERGING system, not a diverging one
Myopia → concave; hypermetropia → convex (don't swap)
Cataract is surgery, not a lens
Microscope wants a SHORT objective; telescope wants a LONG one
Newtonian telescope = mirrors only
Light Phenomena and the Electromagnetic Spectrum
Learn this subtopic in the notesThe electromagnetic spectrum
| Wave / band | Typical wavelength | Use / note |
|---|---|---|
| Radio waves | > 1 m | Longest wavelength; broadcasting, communication |
| Microwaves | mm to cm | Radar, microwave ovens; LONGER wavelength than light |
| Infrared | ~700 nm to 1 mm | Heat waves; absorbed strongly by water |
| Visible light | ≈ 400–700 nm | The only band the eye detects |
| Ultraviolet (UV) | ≈ 10–400 nm | Detects forgery in currency notes; higher energy than visibleQ |
| X-rays | ≈ 0.01–10 nm (≈ 1 Å) | Smallest wavelength of the common four; medical imaging X-ray ≈ 1 nm ≈ 1 Å — the standard tested value. Smallest wavelength among radio/UV/visible/X-ray. |
| Gamma rays | < 0.01 nm | Highest energy of all |
Colours of light and the spectrum
| Fact | Value |
|---|---|
| Primary colours of light | Red, Green, Blue (RGB) These ADD to white. Distinct from the primary pigments (paints). |
| Red + Green light gives | Yellow |
| Blue + Green light gives | Cyan |
| Red + Blue light gives | Magenta |
| Red + Green + Blue gives | White |
| First obtained sunlight's spectrum with a prism | Isaac NewtonQ |
| Order of colours in white light | VIBGYOR (Violet → Red) |
Common traps
Light speeds UP leaving a denser medium
Shorter wavelength = higher energy; UV beats visible
EM waves are NOT elastic and DO travel in vacuum
Sky/sunset colour = scattering; twinkling/early-sunrise = refraction
Primary colours of LIGHT are R, G, B — not R, Y, B
Only polarization proves transverse nature
The eye responds to the ELECTRIC field