Physics 30 Lesson 7: Optics – Curved Mirrors - Detailed Notes

Physics 30 Lesson 7: Optics – Curved Mirrors

Refer to Pearson pages 656 to 665.

I. Plane Mirrors – Revisited

  • Previous work on Reflection indicates that:

    • The image of an object in plane mirrors always exists within the mirror.

    • The image cannot be physically touched or projected since it does not exist outside the mirror.

  • Definitions:

    • Virtual Images: Images existing “inside” the mirror, not real objects.

    • Real Images: Images that can be projected onto a screen outside the mirror.

    • Example: Image produced by an overhead projector can be projected onto a screen.

II. Spherical Mirrors

  • Law of Reflection: For spherical mirrors, the law of reflection applies: θ<em>i=θ</em>r\theta<em>i = \theta</em>r (where θ<em>i\theta<em>i is the angle of incidence and θ</em>r\theta</em>r is the angle of reflection).

  • Normal Line: The normal line is defined as the radius of the sphere.

  • Types of Spherical Mirrors:

    • Converging (Concave) Mirrors:

    • Light rays reflect towards the focal point.

    • Behavior of parallel incident rays:

      • Rays parallel to the principal axis reflect toward a real focal point.

    • Diverging (Convex) Mirrors:

    • Light rays reflect away from the focal point.

    • Parallel incident rays reflect away from a virtual focal point.

  • Image and Object Spatial Terms:

    • A real image exists in actual space, allowing for physical interaction.

    • A virtual image exists only within the mirror (e.g., one’s reflection in a plane mirror).

III. Image Formation – Spherical Mirrors

  • Ray Diagrams:

    • Billions of light rays hit mirrors from objects. However, it is unnecessary to draw all these rays.

    • Three Key Rays to Determine Image Formation:

    1. Ray 1: The incident ray parallel to the principal axis reflects through (or away from) the focal point.

    2. Ray 2: The incident ray traveling through the focal point reflects parallel to the principal axis.

    3. Ray 3: The incident ray that passes through the center of curvature reflects straight back.

    • Factors Determining Image Formation:

    • Type of mirror (concave or convex)

    • Focal length (ff)

    • Distance from mirror to object (dod_o)

IV. Mirror Equations

  • Key Equations:

    • General Formulas:

    • 1f=1d<em>o+1d</em>i\frac{1}{f} = \frac{1}{d<em>o} + \frac{1}{d</em>i} (mirror equation)

    • M=h<em>ih</em>o=d<em>id</em>oM = \frac{h<em>i}{h</em>o} = -\frac{d<em>i}{d</em>o} (magnification)

    • Variable Definitions:

    • RR = radius of curvature of the mirror

    • ff = focal length

    • dod_o = distance from mirror to the object

    • did_i = distance from mirror to the image

    • hoh_o = height of object

    • hih_i = height of image

  • Image Characteristics:

    • Real images exist in real space and are always inverted.

    • Virtual images exist within the mirror and are always erect.

  • Sign Conventions:

    • ff:

    • (+) for concave mirror

    • (-) for convex mirror

    • dod_o: Always (+)

    • did_i:

    • (+) for real image

    • (-) for virtual image

    • hoh_o: Always (+)

    • hih_i:

    • (+) for virtual image

    • (-) for real image

V. Example Problems

Example 1: Converging Mirror
  • Given:

    • Height of object (hoh_o) = 5.0 cm

    • Distance from object to mirror (dod_o) = 60 cm

    • Radius of curvature (RR) = 80 cm

  • Analysis:

    • Focal length: f=R2=80cm2=40cmf = \frac{R}{2} = \frac{80cm}{2} = 40 cm

    • Using mirror formula:
      1f=1d<em>o+1d</em>i\frac{1}{f} = \frac{1}{d<em>o} + \frac{1}{d</em>i}

    • Calculate d<em>id<em>i : 1d</em>i=140160\frac{1}{d</em>i} = \frac{1}{40} - \frac{1}{60}
      di=+120cmd_i = +120 cm (real and inverted)

    • Height of image (h<em>ih<em>i): M=d</em>id<em>o=12060=2M = -\frac{d</em>i}{d<em>o} = -\frac{120}{60} = -2 h</em>i=Mho=25.0cm=10cmh</em>i = M \cdot h_o = -2 \cdot 5.0 cm = -10 cm

Example 2: Diverging Mirror
  • Given:

    • Height of object (hoh_o) = 5.0 cm

    • Distance from object to mirror (dod_o) = 60 cm

    • Radius of curvature (RR) = 80 cm

  • Analysis:

    • Calculate focal length as in Example 1: f=40cmf = -40 cm

    • Using mirror formula results in a virtual image:
      di=3.68cmd_i = -3.68 cm(virtual and erect)

    • Size of image: h<em>i=Mh</em>oh<em>i = M \cdot h</em>o (magnification calculated similarly)
      (1.32 cm)

Example 3: Object Size Consideration
  • An object produces an erect image 1/3 its size when placed 20 cm from the mirror.

  • Conjecture:

    • Mirror type is convex (diverging) since a virtual image cannot be larger than the object with concave.

  • Calculations:

    • do=20cmd_o = 20cm

    • di=6.67cmd_i = -6.67 cm

    • Using mirror equation to find focal length, results indicate a diverging mirror.

VI. Practice Problems

  1. **Concave Mirror:

    • Object height (5 cm) at distance 14 cm. A. Image distance = 7.8 cm; B. Image Description: real, inverted, smaller; C. Image size = -2.8 cm.**

  2. **Convex Mirror:

    • Object height (5 cm) at distance 14 cm. A. Image distance =-3.68 cm; B. Virtual, erect, smaller; C. Image size = 1.32 cm.**

  3. **Concave Mirror:

    • Object distance of 30 cm produces a quarter-sized image. A. Focal length = 6.0 cm.**

  4. Concave Mirror with erect image 80 cm and object distance 40 cm indicates a radius of curvature of 160 cm.

  5. Concave Mirror with inverted image at 120 cm, object at 40 cm yields a radius of curvature of 60 cm.

  6. Convex Mirror produces 20 cm distance and erect image 1/6 of size, with object distance 300 cm.

VII. Laboratory Activity – Concave Mirrors

Purpose:
  • To determine the focal length of a concave mirror.

Apparatus:
  • Construct a setup based on provided diagrams, ensuring proper material organization post-experiment.

Procedure:
  1. Place the object at around 60 cm in front of the concave mirror and record the object distance.

  2. Move a white screen until a sharp image appears. Record the image distance.

  3. Repeat to gather three different positions for accuracy.

Observations:
  • Create a data table to organize findings.

Analysis:
  1. Calculate focal lengths for each position, deriving an average.

  2. Illustrate scale ray diagrams for each observation detailing image formation.