Physics and engineering

Mirror Conversion Calculator

Convert a spherical mirror specification among signed radius, focal length, optical power, curvature, f-number, and exact edge sag under one declared sign convention.

CURRENT MODEL

Choose the known mirror specification and aperture

Optics students, telescope makers, inspection technicians, and buyers translating a spherical mirror drawing or catalog specification before layout or fabrication.

Decision supportedDetermine whether radius, focal length, optical power, clear aperture, and spherical sag describe the same concave or convex surface.
Signed radius--
Signed focal length--
Optical power--
Surface curvature--
Working f-number--
Edge sag--

LIVE SPHERICAL SECTION

Signed mirror geometry

The live section changes curvature direction, focal-side marker, aperture chord, and sag annotation from the current mirror type and dimensions.

An optical fabrication specialist compares a polished spherical mirror blank with a radius gauge, aperture calipers, and a focal bench.
A drawing, radius gauge, aperture measurement, and focal bench describe different parts of the same spherical-mirror specification chain.
Spherical mirror specification ledgerExact current values; full precision is retained before display rounding
Spherical mirror specification ledger for the current inputs
QuantitySymbol or equationCurrent valueUnit

How to use

Translate one drawing value without losing sign or units

  1. Select concave or convex before entering a magnitude; that choice establishes the sign convention.
  2. Identify whether the known number is radius in millimetres, focal length in millimetres, or optical power in diopters.
  3. Enter the positive known magnitude rather than manually adding a negative sign for a convex mirror.
  4. Enter the actual clear aperture, not the outside diameter of the mirror blank or mount.
  5. Compare signed focal length and power with the geometric sag and f-number before transferring values to a drawing.
  6. Save the exact ledger with the surface identifier, coating side, datum, and measurement uncertainty.

Spherical-mirror fundamentals

Six distinctions behind a clean specification

Radius sign
Concave and convex surfaces can share a radius magnitude but focus on opposite signed sides.
Paraxial focus
Focal length equals half the radius only for rays sufficiently close to the optical axis.
Optical power
Power is reciprocal focal length in metres, so millimetres must be converted before inversion.
Clear aperture
The usable illuminated diameter may be smaller than the substrate or coating diameter.
F-number
The ratio |f|/D describes cone speed but does not alone establish image quality.
Spherical sag
Sag is a surface depth from the vertex plane, not focal distance or coating thickness.

Calculation method

Normalize radius first, then derive reciprocal and aperture quantities

The selected source value is converted to an unsigned radius magnitude. The mirror type then applies one sign to both radius and focal length. This prevents an unsigned catalog radius from being accidentally combined with a signed optical power.

F-number uses the absolute focal length because it describes geometry rather than convergence sign. Sag uses the sphere radius and aperture chord exactly; the square-root domain is checked before any result is shown.

Manufacturing datum

Radius metrology may reference a fitted sphere while sag is measured from a mechanical edge plane. Record both datums before comparing values.

Marginal-ray departure

A low f-number exposes stronger spherical aberration. The conversion is still geometrically correct, but the paraxial focus does not predict every ray intercept.

Power tolerance asymmetry

Because power is reciprocal focal length, symmetric millimetre tolerances become asymmetric diopter errors. Convert tolerance endpoints, not just the nominal value.

Detailed calculation process

Symbols, current substitution, intermediate quantities, and reconciliation

f = R/2; P = 1/f_m; C = 1/R_m; N = |f|/D; s = |R| - sqrt(R^2 - (D/2)^2)All conversions and sag calculations retain full precision. Signs and aperture validity are evaluated before display rounding.
Mirror conversion symbols and defaults
SymbolMeaningDefaultUnit
RSigned spherical radius+200mm
fSigned paraxial focal length+100 derivedmm
PReciprocal optical power10 derivedD
DClear aperture diameter25mm
NWorking f-number4 deriveddimensionless
sSpherical edge sag0.391007 derivedmm

    Waiting for valid inputs.

    Interpretation

    Use signed optics and unsigned fabrication geometry together

    A negative focal length or power identifies a diverging convex mirror; it does not imply a negative physical radius magnitude or sag depth. The f-number can compare cone speed between concave and convex specifications, while edge sag indicates whether the chosen aperture is practical on the declared sphere.

    Evidence and measurement

    Preserve the surface definition that made the conversion meaningful

    Record part number, mirror type, radius source and tolerance, wavelength if focal power was measured, clear-aperture definition, vertex and edge datums, coating side, temperature, instrument calibration, and whether radius came from interferometry, spherometry, or a drawing.

    Scope and limitations

    What a radius conversion cannot certify

    • Conic, aspheric, toroidal, freeform, or segmented surface sag
    • Spherical aberration, coma, astigmatism, scatter, or coating phase
    • Substrate edge thickness, mount interference, or bevel allowance
    • Radius tolerance, power uncertainty, or temperature sensitivity
    • Usable aperture after masking, obscuration, or incidence angle
    • Optical safety or finished-system image performance

    A rotationally symmetric spherical mirror in the paraxial focal-length convention. Concave radius and focal length are positive; convex values are negative. Edge sag is geometric and uses the unsigned sphere radius.

    Key terminology

    Mirror specification glossary

    Vertex
    Point where the optical axis meets the mirror surface.
    Center of curvature
    Center of the sphere from which the mirror patch is cut.
    Paraxial focal length
    First-order focus distance for rays close to the axis.
    Diopter
    Reciprocal metre unit of optical power.
    Clear aperture
    Diameter guaranteed to transmit or reflect the intended beam.
    Sagitta
    Axial depth of a curved surface relative to its aperture chord plane.

    Practical cases

    Two conversions with different engineering consequences

    Concave alignment mirror

    A 200 mm radius and 25 mm clear aperture yield a 100 mm paraxial focal length, 10 D power, f/4 geometry, and 0.391007 mm edge sag. The values form a coherent starting drawing.

    Convex inspection substitute

    A supplier offers a convex mirror by negative power while the assembly drawing lists radius magnitude. Converting both under one sign convention exposes whether the substitute diverges with the intended focal scale.

    Important note

    Specification equivalence is not optical acceptance

    Use this page to reconcile nominal first-order quantities. Approve a real mirror only with surface figure, roughness, coating, aperture, environmental, and system-level tolerance evidence.

    Frequently asked questions

    Why does a spherical mirror have f = R/2?

    For paraxial rays on a spherical mirror, the small-angle geometry places the focus halfway between the vertex and center of curvature. Marginal rays do not share exactly the same focus.

    Why is convex mirror power negative?

    This page uses the real-positive convention: a convex mirror has a virtual focus behind the surface, so signed focal length and reciprocal optical power are negative.

    Is mirror optical power measured in diopters?

    Yes when focal length is expressed in metres, P = 1/f has unit reciprocal metre, conventionally called the diopter.

    Does edge sag include coating thickness?

    No. Sag is the ideal spherical substrate geometry from vertex plane to the spherical edge at the entered clear aperture.

    Why can aperture not exceed twice the radius?

    The sag equation intersects a sphere. Beyond the sphere diameter the square-root radicand is negative, so no real spherical surface point exists.

    Can I use this for a parabolic telescope mirror?

    Only for the paraxial focal relation near the vertex. Parabolic sag differs from spherical sag and requires a conic-surface equation.

    Authority and follow-on work

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