Calculate magnification from object and image distance, object and image size, microscope lens settings, or telescope focal lengths.
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Magnification Formula
The following equation is commonly used to calculate the magnification magnitude (absolute value) of a thin lens from the object and image distances.
|m| = \left|\frac{v}{u}\right| - Where |m| is the magnification magnitude (absolute value)
- v is the image distance (distance from the lens to the image)
- u is the object distance (distance from the lens to the object)
To calculate a magnification magnitude, divide the image distance by the object distance. Under common thin-lens sign conventions, the signed magnification is often written as m = −v/u (the negative sign indicates an inverted real image).
Magnification Definition
Magnification is a dimensionless quantity that describes image scaling. For linear (lateral) magnification, it is defined as the ratio of image height to object height: m = hi/ho. For a thin lens, this same magnification is related to distances by m = −v/u (or, in magnitude, |m| = |v/u|).
Magnification Example
How to calculate magnification?
- First, determine the distance of the object from the lens.
Using a measurement device, determine the total distance from the object to the lens.
- Next, determine the distance of the image formed by the lens.
As done in step 1, measure the total distance of the image formed by the lens.
- Finally, calculate the magnification.
Plug the values from steps 1 and 2 into the formula to calculate the magnification.
FAQ
Magnification is a dimensionless quantity that describes how large (or small) an image is compared with the object (for example, linear magnification is m = hi/ho). Magnification can be greater than 1 or less than 1, and the sign of m (if used) indicates image orientation.
A magnification value of 3, for example, means that the image is 3 times the size of the object (in linear dimensions).

