Spherical Aberration Calculator
Enter the ray height and radius of curvature to approximate the longitudinal spherical aberration.
Result
How it is calculated
You enter the ray height h, the distance of an incoming ray from the optical axis, and the mirror's radius of curvature R. The tool applies the small-angle approximation LSA ≈ h² ÷ (4·R) and shows the result in millimetres, together with the working h² ÷ 4R. The paraxial focus of the mirror is at f = R ÷ 2, and the exact shift is (R/2)(1/cosθ − 1) with sinθ = h/R; the shortcut matches it closely for rays near the axis. Treat both inputs as millimetres and use the same unit for both. R must be above zero, h cannot be negative, and h must be smaller than R, since a ray at or beyond the mirror's edge does not hit the sphere; otherwise there is no result. Because the result grows with h², doubling the height makes the aberration four times larger.
Worked example
Consider a mirror with a radius of curvature of 2000 mm and a ray hitting it 100 mm from the axis. First h² = 100 × 100 = 10,000 and 4·R = 4 × 2000 = 8,000. Dividing gives 10,000 ÷ 8,000 = 1.2500 mm of longitudinal spherical aberration. Halving the ray height to 50 mm would give 2,500 ÷ 8,000 = 0.3125 mm, a quarter of the value, which shows why stopping down a mirror helps so much. The exact geometry gives about 1.252 mm for the first case, so the shortcut is very close here.
Common mistakes
- Entering the focal length where the radius is needed. For a spherical mirror the focal length is about half of R, so typing f in the R box makes the result twice too large.
- Using the mirror's full diameter as h. The formula needs the height of one ray above the axis, so for the edge of a 200 mm mirror use 100.
- Mixing units, such as h in inches and R in millimetres. The result then has no meaning and is still labelled mm.
- Trusting the shortcut for rays far from the axis. With h = 1000 on R = 2000 the tool gives 125 mm, while the exact geometry gives about 154.7 mm; and h equal to or above R shows no result.
- Taking the result as the exact blur size. It is the longitudinal shift of the focus along the axis; the blur seen on the sensor is a transverse quantity and is smaller.
About this calculator
Spherical aberration is an optical defect where light rays striking a spherical mirror or lens far from its center focus at a different point than rays near the center — the mirror simply can't bring every ray to one perfect focus. Longitudinal spherical aberration (LSA) measures how far along the optical axis that focus point shifts, approximated for a spherical mirror as LSA ≈ h² / (4·R), where h is the height of the ray from the axis and R is the mirror's radius of curvature.
This approximation is a standard tool in optics and telescope design: it's the reason amateur and professional telescope makers often favor parabolic mirrors over cheaper spherical ones for large apertures, and it's used to estimate image blur before deciding whether a design needs a corrector lens or a different mirror shape.
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