Light: Part -2

🔭 Summary Note: Light – Spherical Mirrors & Lenses

In Light 2, here is a clear and concise summary note for the lesson “Light – Spherical Mirrors & Lenses”, ideal for SEE-passed students preparing for NEB Grade 11 Science entrance exams.


🪞 Spherical Mirrors

Light 2: Reflection through spherical mirror

🔹 Definition:

Spherical mirrors are parts of a sphere’s surface polished to reflect light.

🔸 Types:

  1. Concave Mirror (Converging): The Reflective surface is curved inward

  2. Convex Mirror (Diverging): The Reflective surface is curved outward


📌 Key Terms (Mirrors):

TermDescription
Pole (P)Centre of the mirror’s surface
Centre of Curvature (C)Centre of the sphere of which the mirror is a part
Radius of Curvature (R)Distance from pole to centre of curvature
Principal AxisLine joining the pole and the centre of curvature
Focus (F)Point where rays parallel to the axis converge (concave) or appear to diverge (convex)
Focal Length (f)Distance between pole and focus (f = R/2)

🔎 Image Formation by Concave Mirror (Rules):

  • Depends on the object’s position relative to F and C.

  • Image can be real/inverted or virtual/erect

  • Applications: torches, shaving mirrors, solar cookers


🔎 Image Formation by Convex Mirror:

  • Image is always virtual, erect, and diminished

  • Applications: rear-view mirrors in vehicles


📐 Mirror Formula:

1/f=1/v+1/u

Where:

  • f = focal length

  • v = image distance

  • u = object distance (sign conventions apply)


🔍 Spherical Lenses

Light 2: Refraction through Lenses

🔹 Definition:

Lenses are transparent materials bounded by two spherical surfaces.

🔸 Types:

  1. Convex Lens (Converging): Thicker at the centre

  2. Concave Lens (Diverging): Thinner at the centre


📌 Key Terms (Lenses):

TermDescription
Optical Centre (O)Centre point of the lens
Principal AxisA straight line passing through the optical centre
Focus (F)Point where rays converge (convex) or appear to diverge (concave)
Focal Length (f)Distance between the optical centre and the focus

🔎 Image Formation by Convex Lens:

  • Depends on the object’s position

  • Can be real/inverted or virtual/erect

  • Used in magnifying glasses, cameras, and spectacles

🔎 Image Formation by Concave Lens:

  • Image is always virtual, erect, and diminished

  • Used in spectacles for myopia


📐 Lens Formula:

1/f=1/v−1/u

Magnification (M)=Height of image/Height of object=v/u


⚙️ Sign Conventions (for Mirrors & Lenses):

  •  We should measure all distances from the pole (mirror) or the optical centre (lens)

  • Left side: negative, Right side: positive

  • We should always place the object on the left (u is negative)

🔍 You Can Also Read:

Light: Part -2

🔊 Sound

SEE Result: New Possibilities and Uncertainties for Students’ Future Careers in Nepal

How to Choose the Right Stream After SEE in Nepal

CDC

In conclusion, the concepts of reflection and refraction play a vital role in understanding how light behaves in different situations. As a result, students can now explain real-life phenomena such as mirages, rainbows, and optical illusions more clearly. In addition, Scientists and engineers widely apply these principles in instruments like mirrors, lenses, and optical fibres. Therefore, mastering them not only strengthens your foundation in physics but also prepares you for competitive entrance exams. So, you are now encouraged to revise key formulas, attempt MCQs, and explore practical examples to solidify your understanding.