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What is the formula for magnification?

Published in Optics Formula 3 mins read

The formula for magnification is M = Hi/Ho = -Di/Do. This equation relates the magnification to both image and object heights, as well as image and object distances.

Understanding the Magnification Formula

The magnification formula is a fundamental concept in optics and is used to determine how much larger or smaller an image appears compared to the actual object. The formula is derived from the principles of similar triangles in geometric optics. Let's break down each component:

  • M (Magnification): Represents the total magnification of the image. A positive M indicates an upright image, while a negative M indicates an inverted image.
  • Hi (Height of the Image): This is the size of the image formed by the optical system.
  • Ho (Height of the Object): This refers to the actual size of the object being viewed.
  • Di (Distance of the Image): Represents the distance between the lens (or mirror) and the image.
  • Do (Distance of the Object): This is the distance between the lens (or mirror) and the actual object.

Detailed Explanation and Applications:

The magnification formula has two main parts:

  1. M = Hi/Ho: This part of the formula shows how magnification relates to the size of the image (Hi) compared to the size of the object (Ho).

    • If M > 1, the image is larger than the object.
    • If M < 1, the image is smaller than the object.
    • If M = 1, the image is the same size as the object.
    • If M is negative, it means the image is inverted
  2. M = -Di/Do: This part relates magnification to the distances of the image (Di) and the object (Do) from the lens or mirror.

    • The negative sign is present because real images formed by lenses are inverted.
    • By utilizing both sides of the formula we can also say that Hi/Ho = -Di/Do

Examples of Practical Applications

  • Microscopes: Microscopes use lenses to magnify extremely small objects. The magnification is calculated to ensure clear visibility of the microscopic structures.
  • Telescopes: Telescopes gather light and use lenses or mirrors to magnify distant objects, enabling us to observe celestial bodies.
  • Cameras: The lenses in cameras magnify the image onto the sensor to allow for photographic recording.

Important Considerations

  • Sign Conventions: The negative sign in the M = -Di/Do portion of the equation is critical for determining the orientation of the image. Real images (formed by converging lenses and concave mirrors) are inverted and have a negative Di. Virtual images (formed by diverging lenses and convex mirrors) are upright and have a positive Di.
  • Lens/Mirror Properties: The type of lens or mirror used will also affect the magnification and type of image created.

Understanding this formula is crucial for anyone working with optical instruments or involved in the study of optics.

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