✦ Drag the object or focus points
Image Dist (v)
Magnification
Nature
Optical Type
Focal Length (f) 100 mm
Object Distance (u) 200 mm
Object Height (h) 60 mm
Ray Visualization
CBSE Class 12 Physics

Ray Optics & Optical Instruments

Complete guide to spherical lenses, mirrors, and image formation principles

🎯 How to Use This Lab
1

Select Device

Choose convex lens, concave lens, concave mirror, or convex mirror from the top-right dropdown.

2

Adjust Parameters

Use sliders to change focal length (f), object distance (u), and object height (h). Ray diagram updates live.

3

Toggle Rays

Enable/disable parallel, central, and focal rays to understand light behaviour through lenses and mirrors.

4

Record & Analyze

Tap "Record Reading" to save observations. Switch to the Data tab to view tables and graphs.

📖 Essential Terminology

Optical Centre (C)

Central point of a lens through which rays pass without deviation. Used as origin in Cartesian sign convention.

Pole (P)

Geometric centre of a spherical mirror's reflecting surface. Origin for sign convention in mirror problems.

Principal Focus (F)

Where parallel rays converge (converging) or appear to diverge from (diverging) after refraction/reflection.

Focal Length (f)

Distance from optical centre/pole to principal focus. Positive for converging, negative for diverging systems.

Object Distance (u)

Distance of object from optical centre or pole. Always negative by new Cartesian sign convention.

Image Distance (v)

Distance of image from optical centre or pole. Positive for real images (lenses). Opposite sign for mirrors.

📐 New Cartesian Sign Convention

1. Origin Point

• For lenses: Optical Centre (C) is the origin
• For mirrors: Pole (P) is the origin

2. Direction of Light

• Light travels left to right (positive x-direction)
• All distances measured from the origin

3. Sign Rules

Horizontal: Along incident light → +ve, against → −ve
Vertical: Upward → +ve, downward → −ve

u is always negative. Real image: v > 0 (lens), v < 0 (mirror).

🧮 Lens & Mirror Formulas
Lens Formula
1/f = 1/v − 1/u
Convex & concave lenses
Mirror Formula
1/f = 1/v + 1/u
Concave & convex mirrors
Magnification
m = v/u = h′/h
|m|>1 magnified · |m|<1 diminished · m>0 erect · m<0 inverted
Power of a Lens
P = 1 / f(m)
Unit: Dioptre (D) · Convex → +P · Concave → −P
🔬 Image Formation Rules

Convex Lens

Object PositionImage PositionNature & Size
At infinityAt FReal, inverted, highly diminished
Beyond 2FBetween F and 2FReal, inverted, diminished
At 2FAt 2F (other side)Real, inverted, same size
Between F and 2FBeyond 2FReal, inverted, magnified
At FAt infinityReal, inverted, highly magnified
Between F and CSame side as objectVirtual, erect, magnified

Concave Mirror

Object PositionImage PositionNature & Size
At infinityAt FReal, inverted, highly diminished
Beyond CBetween F and CReal, inverted, diminished
At CAt CReal, inverted, same size
Between F and CBeyond CReal, inverted, magnified
Between F and PBehind mirrorVirtual, erect, magnified
💡 Real-World Applications

🔬 Microscopes

Two convex lenses (objective + eyepiece) to magnify microscopic specimens like cells and bacteria.

🔭 Telescopes

Convex lenses gather and magnify light from distant stars and planets.

📷 Cameras

Convex lenses focus light to form real, inverted images on sensor or film.

👓 Eyeglasses

Convex for hypermetropia, concave for myopia — adjusting focal length.

🚗 Vehicle Mirrors

Convex mirrors give wider field of view as side/rear-view mirrors.

🦷 Dental Mirrors

Concave mirrors used close-up give magnified, erect virtual images of teeth.

☀️ Solar Concentrators

Concave mirrors focus sunlight for solar cookers and power generation.

💡 Headlights

Concave mirrors with bulb at focus produce parallel beams for illumination.

Experimental Observations

# u (cm) v (cm) f (calc) Error %
📊
No observations yet.
Go to Simulation and tap "Record Reading".

Graph: 1/v vs 1/u