A mirror sign audit checks each object and image distance against the sign convention across concave and convex rows, so the mirror equation closes consistently for each curvature. The arithmetic is exact only for the stated distances, focal lengths, and side/sign conventions in the ideal spherical-mirror model. Real measurements add alignment, mirror aberrations, finite aperture, thickness, screen/readout calibration, sign-convention bookkeeping, finite precision, and measurement uncertainty.
Concave and convex mirrors use the same reciprocal budget, but the focal-length sign changes where the image appears. Exact arithmetic here means exact results for the stated model inputs; measured inputs still carry uncertainty and significant-figure limits.
highlighted = computed this step
Concave mirrors can make real front images
Keep the concave focal length positive and move the object. The positive image distances are front-side real images, and the negative magnifications mark inversion.
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Changing mirror type changes the sign pattern
Hold the object distance fixed and compare a concave row with two convex rows. Convex focal lengths are negative, and the image distance stays negative in these checked rows.
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Convex mirrors keep upright virtual images
Hold the convex focal length fixed and move the object. The image distance remains negative, while positive magnification keeps the image upright.
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Mirror signs separate front and behind
For the mirror convention used here, positive image distance is a front-side real image. Negative image distance is a virtual image behind the mirror.