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The Mirror Equation Calculator determines image properties for concave and convex mirrors using the mirror equation. Whether you are designing a reflecting telescope, analyzing a car side mirror, or studying for a physics exam, this tool computes image distance, magnification, and image characteristics instantly.
The mirror equation $$\frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i}$$ is mathematically identical to the thin lens equation but uses different sign conventions appropriate for reflected light. By selecting the mirror type and entering the focal length and object distance, you get a complete description of the image formed.
The mirror equation relates the focal length, object distance, and image distance for spherical mirrors:
$$\frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i}$$
Rearranging to solve for image distance:
$$d_i = \frac{f \cdot d_o}{d_o - f}$$
The sign conventions for mirrors differ from lenses:
The magnification is:
$$M = -\frac{d_i}{d_o}$$
For a concave mirror, the image properties depend on object position relative to the focal point and center of curvature. When the object is beyond the center of curvature (do > 2f), the image is real, inverted, and diminished. Between the center and focal point (f < do < 2f), the image is real, inverted, and magnified. Inside the focal point (do < f), the image is virtual, upright, and magnified — the principle behind makeup mirrors.
For a convex mirror, the image is always virtual, upright, and diminished regardless of object position. This wide-angle property makes convex mirrors ideal for security mirrors and vehicle side mirrors, which carry the warning "objects in mirror are closer than they appear."
The relationship between focal length and radius of curvature is $$f = \frac{R}{2}$$ for spherical mirrors under the paraxial approximation, where rays are close to and nearly parallel to the optical axis.
The signed focal length shows the effective focal length with the correct sign convention — positive for concave and negative for convex mirrors. The image distance tells you where the image forms: positive values mean a real image in front of the mirror, negative values mean a virtual image behind the mirror surface.
The magnification indicates both size and orientation. A magnification of −0.5 means the image is half-size and inverted. A magnification of +3 means the image is three times larger and upright (virtual). The image type description summarizes all these properties in plain language.
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Results
An object at 45 cm from a concave mirror with f = 15 cm (beyond 2f = 30 cm) produces a real inverted diminished image at 22.5 cm. M = −0.5 confirms the image is half the object size.
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A convex mirror with |f| = 20 cm produces a virtual image at −12 cm (behind the mirror) for an object at 30 cm. M = +0.4 means the image is upright and 40% of the object size.
The mirror equation is $$\frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i}$$ where f is the focal length, do is the object distance, and di is the image distance. It applies to both concave and convex spherical mirrors with appropriate sign conventions.
A concave mirror (f > 0) curves inward and can form both real and virtual images depending on object position. A convex mirror (f < 0) curves outward and always forms virtual, upright, diminished images. Concave mirrors are used in telescopes and shaving mirrors; convex mirrors are used in security and vehicle mirrors.
For a spherical mirror, the focal length is half the radius of curvature: $$f = \frac{R}{2}$$. This relationship holds under the paraxial approximation where light rays stay close to the optical axis.
A concave mirror produces a virtual image when the object is placed inside the focal point (do < f). The virtual image forms behind the mirror, is upright, and is magnified. This is the principle behind magnifying makeup mirrors.
Convex mirrors diverge reflected light, causing the reflected rays to appear to originate from a virtual focal point behind the mirror. The geometry ensures the virtual image is always closer to the mirror than the focal point, making it always smaller than the object but providing a wider field of view.
For objects near the optical axis (paraxial rays), the mirror equation works well for parabolic mirrors. Parabolic mirrors eliminate spherical aberration and are preferred for precision applications like telescope primaries. The equation breaks down for off-axis rays in spherical mirrors but remains accurate for parabolic shapes.
Roboculator Team
The Roboculator Team explains calculations, planning tools, and practical formulas in clear language for real-life situations.
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