Science: Light – Reflection and Refraction

Introduction to Light and Visibility

  • Visibility of Objects:     - Objects in a dark room are invisible. They become visible upon lighting up the room.     - During the day, sunlight facilitates vision.     - An object reflects light that falls onto it. When this reflected light is received by the human eye, it enables vision.     - For transparent media, light is transmitted through it, allowing us to see through the medium.
  • Common Optical Phenomena:     - Image formation by mirrors.     - The twinkling of stars.     - The beautiful colors of a rainbow.     - Bending of light by a medium (refraction).
  • Nature of Light Propagation:     - Based on common observations (like sharp shadows of opaque objects), light is traditionally thought to travel in straight lines, known as a ray of light.     - Diffraction of Light: If an opaque object on the path of light is very small, light tends to bend around it instead of traveling in a straight line. This suggests light has wave-like properties.     - Quantum Theory: In the early 20th century, it was discovered that light also acts like a stream of particles when interacting with matter. Modern quantum theory reconciles these by stating light is neither purely a 'wave' nor a 'particle' but possesses characteristics of both.

Reflection of Light

  • Definition: A highly polished surface, such as a mirror, reflects the majority of the light falling on it.
  • Laws of Reflection:     - (i) The angle of incidence is equal to the angle of reflection (i=ri = r).     - (ii) The incident ray, the reflected ray, and the normal to the mirror at the point of incidence all lie in the same plane.     - These laws apply to all reflecting surfaces, including plane and spherical surfaces.
  • Image Properties in a Plane Mirror:     - The image is always virtual and erect.     - The size of the image is equal to the size of the object.     - The distance of the image behind the mirror is equal to the distance of the object in front of it.     - The image is laterally inverted.

Spherical Mirrors: Definitions and Terms

  • Spherical Mirror: A mirror whose reflecting surface is a part of a hollow sphere.     - Concave Mirror: The reflecting surface is curved inwards (faces toward the center of the sphere).     - Convex Mirror: The reflecting surface is curved outwards.
  • Crucial Terminology:     - Pole (P): The center of the reflecting surface of a spherical mirror. It lies on the surface of the mirror.     - Centre of Curvature (C): The center of the sphere of which the mirror's reflecting surface is a part.         - In a concave mirror, CC lies in front of the reflecting surface.         - In a convex mirror, CC lies behind the reflecting surface.     - Radius of Curvature (R): The radius of the sphere of which the reflecting surface is a part. The distance PCPC equals RR.     - Principal Axis: A straight line passing through the pole (PP) and the center of curvature (CC). It is normal to the mirror at its pole.     - Principal Focus (F):         - For a concave mirror: The point on the principal axis where rays parallel to the axis converge after reflection.         - For a convex mirror: The point on the principal axis from which rays parallel to the axis appear to diverge after reflection.     - Focal Length (f): The distance between the pole (PP) and the principal focus (FF).     - Aperture: The diameter of the circular outline of the reflecting surface of the spherical mirror.
  • Relationship between R and f:     - For mirrors with small apertures, the radius of curvature is twice the focal length:     - R=2fR = 2f

Image Formation by Concave Mirrors

  • Summary of Image Characteristics (Table 9.1):     - Object at Infinity: Image at Focus FF. Nature: Real and inverted. Size: Highly diminished, point-sized.     - Object Beyond C: Image between FF and CC. Nature: Real and inverted. Size: Diminished.     - Object At C: Image at CC. Nature: Real and inverted. Size: Same size.     - Object Between C and F: Image beyond CC. Nature: Real and inverted. Size: Enlarged.     - Object At F: Image at Infinity. Nature: Real and inverted. Size: Highly magnified.     - Object Between P and F: Image behind the mirror. Nature: Virtual and erect. Size: Enlarged.
  • Rules for Ray Diagrams:     - (i) A ray parallel to the principal axis passes through the focus (FF) after reflection (concave) or appears to diverge from it (convex).     - (ii) A ray passing through the focus (FF) emerges parallel to the principal axis after reflection.     - (iii) A ray passing through the center of curvature (CC) is reflected back along the same path because it strikes the surface normally.     - (iv) A ray incident obliquely at the pole (PP) is reflected obliquely, following the laws of reflection (i=ri = r).
  • Uses of Concave Mirrors:     - Used in torches, search-lights, and vehicle headlights to produce powerful parallel beams.     - Used as shaving mirrors to see a larger image of the face.     - Used by dentists to see large images of teeth.     - Large concave mirrors are used in solar furnaces to concentrate sunlight for heat.

Image Formation by Convex Mirrors

  • Summary of Image Characteristics (Table 9.2):     - Object at Infinity: Image at focus FF behind the mirror. Nature: Virtual and erect. Size: Highly diminished, point-sized.     - Object Between Infinity and Pole (P): Image between PP and FF behind the mirror. Nature: Virtual and erect. Size: Diminished.
  • Uses of Convex Mirrors:     - Primarily used as rear-view (wing) mirrors in vehicles.     - Advantages: They always provide an erect image and have a much wider field of view because they are curved outwards, allowing drivers to see more traffic than a plane mirror would.

New Cartesian Sign Convention

  • When dealing with reflection by spherical mirrors, the following conventions are used:     - (i) The object is always placed to the left of the mirror (light travels from left to right).     - (ii) All distances parallel to the principal axis are measured from the pole (PP), which is the origin.     - (iii) Distances measured in the direction of incident light (along +x+x axis) are positive; distances measured against incident light (along x-x axis) are negative.     - (iv) Distances measured perpendicular to and above the principal axis (+y+y axis) are positive.     - (v) Distances measured perpendicular to and below the principal axis (y-y axis) are negative.

Mirror Formula and Magnification

  • Mirror Formula:     - Represents the relationship between object distance (uu), image distance (vv), and focal length (ff).     - 1v+1u=1f\frac{1}{v} + \frac{1}{u} = \frac{1}{f}
  • Magnification (m):     - Defined as the ratio of the height of the image (hh') to the height of the object (hh).     - m=hhm = \frac{h'}{h}     - Also related to distances: m=vum = -\frac{v}{u}
  • Interpretation of Magnification:     - A negative sign for mm indicates a real image.     - A positive sign for mm indicates a virtual image.

Numerical Examples (Mirrors)

  • Example 9.1 (Convex Mirror):     - Given: R=+3.00mR = +3.00\,m, u=5.00mu = -5.00\,m.     - Focal length: f=R2=+1.50mf = \frac{R}{2} = +1.50\,m.     - Using 1v=1f1u=11.5015.00=11.50+15.00=6.507.50\frac{1}{v} = \frac{1}{f} - \frac{1}{u} = \frac{1}{1.50} - \frac{1}{-5.00} = \frac{1}{1.50} + \frac{1}{5.00} = \frac{6.50}{7.50}.     - v=+1.15mv = +1.15\,m (image is behind the mirror).     - m=vu=1.155.00=+0.23m = -\frac{v}{u} = -\frac{1.15}{-5.00} = +0.23.     - Result: Image is virtual, erect, and smaller by a factor of 0.23.
  • Example 9.2 (Concave Mirror):     - Given: h=+4.0cmh = +4.0\,cm, u=25.0cmu = -25.0\,cm, f=15.0cmf = -15.0\,cm.     - Using 1v=1f1u=115.0125.0=275\frac{1}{v} = \frac{1}{f} - \frac{1}{u} = \frac{1}{-15.0} - \frac{1}{-25.0} = -\frac{2}{75}.     - v=37.5cmv = -37.5\,cm (screen should be placed in front).     - h=vu×h=37.525.0×4.0=6.0cmh' = -\frac{v}{u} \times h = -\frac{-37.5}{-25.0} \times 4.0 = -6.0\,cm.     - Result: Image is real, inverted, and enlarged.

Refraction of Light

  • Definition: When light travels obliquely from one transparent medium to another, its direction of propagation in the second medium changes. This is due to the change in the speed of light.
  • Common Observations:     - Bottom of a water tank appears raised.     - Letters under a glass slab appear raised.     - A pencil partially immersed in water appears bent at the air-water interface.     - A lemon in water appears larger when viewed from sides.
  • Refraction through a Rectangular Glass Slab:     - Light bends towards the normal when entering from a rarer medium (air) to a denser medium (glass).     - Light bends away from the normal when entering from a denser medium (glass) to a rarer medium (air).     - The emergent ray is parallel to the incident ray but shifted laterally.
  • Laws of Refraction:     - (i) The incident ray, the refracted ray, and the normal to the interface at the point of incidence all lie in the same plane.     - (ii) Snell’s Law: The ratio of the sine of the angle of incidence to the sine of the angle of refraction is a constant for a given pair of media and color of light.     - sin(i)sin(r)=constant\frac{\sin(i)}{\sin(r)} = \text{constant}

The Refractive Index

  • Definition: The constant in Snell's Law is the refractive index of the second medium relative to the first (n21n_{21}).
  • Basis in Light Speed:     - n21=Speed of light in medium 1Speed of light in medium 2=v1v2n_{21} = \frac{\text{Speed of light in medium 1}}{\text{Speed of light in medium 2}} = \frac{v_{1}}{v_{2}}
  • Absolute Refractive Index (n):     - Refractive index relative to vacuum/air.     - nm=cvn_{m} = \frac{c}{v} (where c=3×108m/sc = 3 \times 10^{8}\,m/s).
  • Optical Density:     - A medium with a higher refractive index is 'optically denser'.     - Light travels slower in an optically denser medium and faster in an optically rarer medium.
  • Refractive Index Table (Table 9.3 highlights):     - Air: 1.00031.0003     - Water: 1.331.33     - Crown Glass: 1.521.52     - Diamond: 2.422.42 (highest optical density listed).

Spherical Lenses

  • Lens: A transparent material bound by two surfaces where at least one is spherical.
  • Types of Lenses:     - Convex (Converging) Lens: Thicker at the middle than at the edges. Converges parallel rays of light.     - Concave (Diverging) Lens: Thicker at the edges than at the middle. Diverges parallel rays of light.
  • Key Terms:     - Centres of Curvature (C1,C2C_{1}, C_{2}): The centers of the spheres forming the lens surfaces.     - Optical Centre (O): The central point of a lens. Ray passing through OO suffers no deviation.     - Principal Foci (F1,F2F_{1}, F_{2}): Foci on both sides of the lens where parallel rays converge (convex) or appear to diverge from (concave).     - Focal Length (f): Distance from the optical center to the principal focus.     - Aperture: The effective diameter of the circular outline of the lens.

Image Formation by Lenses

  • Convex Lens Image Summary (Table 9.4):     - At Infinity: At focus F2F_{2}. Nature: Real and inverted. Size: Highly diminished.     - Beyond 2F1: Between F2F_{2} and 2F22F_{2}. Nature: Real and inverted. Size: Diminished.     - At 2F1: At 2F22F_{2}. Nature: Real and inverted. Size: Same size.     - Between F1 and 2F1: Beyond 2F22F_{2}. Nature: Real and inverted. Size: Enlarged.     - At Focus F1: At Infinity. Nature: Real and inverted. Size: Highly magnified.     - Between F1 and O: On the same side as object. Nature: Virtual and erect. Size: Enlarged.
  • Concave Lens Image Summary (Table 9.5):     - Always produces a virtual, erect, and diminished image regardless of object position.

Lens Formula, Magnification, and Power

  • Lens Formula:     - 1v1u=1f\frac{1}{v} - \frac{1}{u} = \frac{1}{f}
  • Magnification (m):     - m=hh=vum = \frac{h'}{h} = \frac{v}{u}
  • Power of a Lens (P):     - The degree of convergence or divergence of light rays. It is the reciprocal of focal length in meters.     - P=1fP = \frac{1}{f} (where ff is in meters).     - Unit: Dioptre (DD). 1D=1m11\,D = 1\,m^{-1}.     - Signs: Convex lens power is Positive (+); Concave lens power is Negative (-).
  • Combination of Lenses:     - Net power P=P1+P2+P3+P = P_{1} + P_{2} + P_{3} + \dots     - Used in cameras, microscopes, and telescopes to increase magnification and sharpness.

Numerical Examples (Lenses)

  • Example 9.3 (Concave Lens):     - Given: f=15cmf = -15\,cm, v=10cmv = -10\,cm.     - Using 1u=1v1f=110115=130\frac{1}{u} = \frac{1}{v} - \frac{1}{f} = \frac{1}{-10} - \frac{1}{-15} = -\frac{1}{30}.     - u=30cmu = -30\,cm.     - m=vu=1030=+0.33m = \frac{v}{u} = \frac{-10}{-30} = +0.33 (virtual, erect, 1/3 size).
  • Example 9.4 (Convex Lens):     - Given: h=+2.0cmh = +2.0\,cm, f=+10cmf = +10\,cm, u=15cmu = -15\,cm.     - Using 1v=1f+1u=110+115=130\frac{1}{v} = \frac{1}{f} + \frac{1}{u} = \frac{1}{10} + \frac{1}{-15} = \frac{1}{30}.     - v=+30cmv = +30\,cm.     - m=vu=3015=2m = \frac{v}{u} = \frac{30}{-15} = -2.     - h=m×h=2×2.0=4.0cmh' = m \times h = -2 \times 2.0 = -4.0\,cm.     - Result: Real, inverted, enlarged (double size).

Questions & Discussion

  • Focus of Concave Mirror: The point on the principal axis where rays parallel to the axis meet after reflection.
  • Focal Length Calculation: If R=20cmR = 20\,cm, f=10cmf = 10\,cm. If R=32cmR = 32\,cm, f=16cmf = 16\,cm.
  • Concave Mirror Image: To get an erect and enlarged image, the object must be between the pole and the focus.
  • Vehicle Rear-View Mirrors: Convex mirrors are used because they provide erect images and a wider field of view.
  • Refractive Index Meaning: "Refractive index of diamond is 2.42" means the speed of light in diamond is 12.42\frac{1}{2.42} times the speed of light in air/vacuum.
  • Lens Materials: Materials like clay cannot be used for lenses as they are not transparent.
  • Plane Mirror Magnification: m=+1m = +1 means the image is the same size as the object and is virtual and erect.
  • Refraction Logic: When entering water from air obliquely, light bends towards the normal because water is optically denser than air.