The Human Eye & the Colourful World

Cheat Sheet Β· CBSE Class X Β· Chapter 11

πŸ‘οΈ The Human Eye β€” Structure

Key: Eye = biological camera. Cornea+Lens = camera lens. Retina = film/sensor. Image: real, inverted, diminished.

πŸ” Power of Accommodation

Mechanism

ViewingCiliary MusclesLensFocal Length
Distant objectRelaxedThin (flat)Maximum
Near objectContractedThick (curved)Minimum
Remember: Contract β†’ Curved β†’ Close objects. Relax β†’ flat β†’ faR objects.

πŸ‘“ Defects of Vision & Corrections

DefectCan't SeeImage FormsCauseCorrectionLens Sign
Myopia
(Near-sighted)
Far objectsIn front of retinaElongated eyeball or excessive curvatureConcave lensβˆ’ve power
Hypermetropia
(Far-sighted)
Near objectsBehind retinaShort eyeball or weak curvatureConvex lens+ve power
Presbyopia
(Age-related)
Near objectsBehind retinaCiliary muscles weaken; lens loses flexibilityBifocal lens+ve (lower)
Mnemonics: Myopia = Minus lens. Hypermetropia = High (+ve) lens. Presbyopia = Progressive/Bifocal.

Key Formulas

P = 1/f (in metres)   Far point (myopia) = |f of concave lens|

1/f = 1/v βˆ’ 1/u (for calculating power of corrective lens)

πŸ”Ί Refraction Through a Prism

Key relationship: A = r₁ + rβ‚‚ and Ξ΄ = (i₁ + iβ‚‚) βˆ’ A

🌈 Dispersion of Light

Newton's Experiment

🌈 Rainbow Formation

RainbowAngleReflectionsColour Order (outside→inside)Brightness
Primary42Β°1 TIRRed β†’ VioletBrighter
Secondary51Β°2 TIRsViolet β†’ Red (reversed)Fainter

πŸ’« Scattering of Light

Rayleigh Scattering Law

Intensity of scattered light ∝ 1/λ⁴

Tyndall Effect

PhenomenonCauseKey Reasoning
Blue skyRayleigh scatteringBlue (short Ξ») scatters most β†’ reaches eyes from all directions
White cloudsMie scatteringLarge water droplets scatter all Ξ» equally β†’ white
Red sunset/sunriseRayleigh scatteringLong path β†’ blue scattered away β†’ only red/orange remains
Red danger signalsLeast scatteringRed (longest Ξ») β†’ least scattered β†’ travels farthest
Black sky on MoonNo atmosphereNo molecules β†’ no scattering β†’ sky is black

⭐ Atmospheric Refraction

Effects

PhenomenonExplanation
Twinkling of starsPoint source + varying refractive index β†’ apparent position shifts β†’ intensity fluctuates
Planets don't twinkleExtended source β†’ individual fluctuations average out
Advanced sunrise (+2 min)Refraction makes Sun appear above actual position
Delayed sunset (+2 min)Sun visible after crossing below horizon
Flattened Sun at horizonBottom edge refracted more than top β†’ vertical compression
Total extra daylight due to atmospheric refraction β‰ˆ 4 minutes/day (2 min sunrise + 2 min sunset).

πŸ“Š Wavelength & Colour Data

ColourWavelength (nm)FrequencyΞΌ in glassDeviation
Violet380–450HighestHighestMaximum
Indigo450–490↑↑↑
Blue490–520
Green520–565
Yellow565–590
Orange590–625↓↓↓
Red625–700LowestLowestMinimum
Remember: Ξ» increases Vβ†’R. Frequency increases Rβ†’V. Speed in glass increases Vβ†’R. All colours have same speed in vacuum (c = 3Γ—10⁸ m/s).

🧠 Exam Quick-Fire Facts

πŸ“ Important Numericals Pattern

Type 1: Power of Corrective Lens

P = 1/f  (f in metres)

Type 2: Combination of Lenses

P = P₁ + Pβ‚‚ + P₃ ...

Example

A person's far point is 80 cm. Find the power of corrective lens.

f = βˆ’80 cm = βˆ’0.8 m (concave lens for myopia)

P = 1/(βˆ’0.8) = βˆ’1.25 D

πŸ”‘ Key Differences

FeatureRayleigh ScatteringTyndall Effect
Particle sizeβ‰ͺ Ξ» (molecules)β‰ˆ Ξ» (colloidal)
DependenceStrong (∝ 1/λ⁴)Weaker λ dependence
ExampleBlue skyDusty room beam
FeaturePrimary RainbowSecondary Rainbow
Internal reflections12
Angle42Β°51Β°
IntensityBrighterFainter
Order (outside→in)Red → VioletViolet → Red