Thick Lens Back Vertex Power Calculator

Thick Lens Back Vertex Power Calculator

F₁ ÷ (1 − (t⁄n)F₁) + F₂, the exact form. A +9.40 / −4.70 lens 5.2 mm thick in polycarbonate is +5.00 D, not the +4.70 D its surfaces add to.

Surface powers + thickness → back vertex power

Reduced thickness
The TRUE power of the front surface, not the figure a lens measure clocks. A lens measure is calibrated for one index — usually 1.53 — so on any other material the clocked reading must be multiplied by (n − 1) ÷ 0.530 first. The two sources read for this page give that correction, and the figure in the result list above applies it to whatever you enter.
The true power of the back surface, which on a plus lens is negative. It enters the back vertex power unchanged: the thickness term acts on the FRONT surface only, because the back surface is where the vertex power is measured from and light reaches it last.
The axial thickness between the two surface vertices. A finished spectacle lens runs about 1 to 2 mm at the centre in minus and up to about 10 to 12 mm in high plus. The range here goes further so the page can show where the arithmetic breaks rather than printing nonsense: at a +60 D front surface and an index of 1.50 the back vertex power is undefined at 25 mm, and the page refuses beyond it.
The refractive index of the lens material. It enters only through the REDUCED THICKNESS, t divided by n: 5.2 mm of polycarbonate is worth 3.28 mm optically, so a higher index makes a given centre thickness matter less as well as needing less of it.
5.00D back vertex powerExample

Front +9.40 D, back −4.70 D, 5.2 mm centre thickness, polycarbonate at n = 1.586 — the published worked case

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Back vertex power, and the reduced thickness in it

F′v = F₁ ÷ (1 − (t⁄n)F₁) + F₂  ·  equivalently 1 ÷ (1⁄F₁ − t⁄n) + F₂, with t⁄n in metres
the reduced thickness
quoted: it “is simply the thickness, in the desired measurement … divided by the index of refraction”. 5.2 mm of polycarbonate is 3.28 mm reduced. That is the only way the thickness and the index enter the calculation at all, which is why a high-index material reduces the thickness effect twice over — once by needing less glass, and once by dividing by a bigger number
the procedure, as published
the source read works it step by step as plain text: the front surface’s focal length is 1 ÷ 9.40 = 0.106383 m; subtract the reduced thickness, 0.106383 − 0.00328 = 0.103103 m; invert, 1 ÷ 0.103103 = 9.70 D; then “adding the true power of the back surface”, +9.70 + (−4.70) = +5.00 D. The closed form at the top of this block is that same procedure in one line, and the proof behind this page asserts the two agree over a sweep of powers, thicknesses and indices
WHY ONLY THE FRONT SURFACE IS DIVIDED
back vertex power is measured FROM the back surface, so light has already crossed the thickness by the time it reaches the back surface and that surface’s power is added unchanged. Front vertex power is the mirror and divides the BACK surface instead. On the lens above the two are +5.00 D and +4.77 D, which is a quarter of a dioptre apart — and a prescription means the back vertex one
the approximation, and its error
the dispensing texts print the first-order expansion, F₁ + F₂ + (t⁄n)F₁², which the source read gives as “Deff = Df + Db + t(Df)²/n”. It is ALWAYS low, because the exact form is a geometric series whose later terms are all positive, and it is 0.009 D low on the lens above. It reaches 0.10 D at a +15.00 D front surface 8 mm thick and 0.33 D at a +20.00 D front surface 10 mm thick, so it is adequate for dispensing and not for lens design
the denominator is the shape factor
1 ÷ (1 − (t⁄n)F₁) is printed identically by three independent sources as the SHAPE FACTOR of spectacle magnification, and one of them works it at t = 4 mm, n = 1.50 and F₁ = +10.00 D to 1.027, which this page’s arithmetic reproduces as 1.0274. That three-way agreement is the corroboration this page rests on, because NO SOURCE READ FOR THIS BATCH PRINTED THE EXACT BACK-VERTEX EXPRESSION IN CLOSED FORM: four documents that should have carried it — two textbook chapters and two encyclopaedia articles — rendered their equations as images. What was read is the worked procedure, and this page reproduces its answer exactly. See spectacle magnification for the same term used the other way

Worked example

Front +9.40 D, back −4.70 D, 5.2 mm centre thickness, polycarbonate at n = 1.586 — the published worked case
Reduced thickness. 5.2 ÷ 1.586 = 3.279 mm, or 0.003279 m. The source read rounds it to 3.28 mm
Front surface focal length. 1 ÷ 9.40 = 0.106383 m
0.106383 − 0.003279 = 0.103104 m
1 ÷ 0.103104 = +9.699 D — the front surface seen from the back of the lens
Add the back surface. +9.699 + (−4.70) = +5.00 D, which is exactly the figure the published case reaches
What the thickness was worth. The two surfaces add to +4.70 D, so the thickness is worth +0.299 D — more than a quarter of a dioptre, on a lens whose thickness is 5 mm. That is why a plus lens cannot be specified by its surface powers
The approximation. 9.40 + (−4.70) + 0.003279 × 9.40² = 4.990 D, which is 0.0092 D low. Adequate here, and 0.33 D low on a +20.00 D front surface 10 mm thick
And the clocked curves. (1.586 − 1) ÷ 0.530 = 1.1057, so a lens measure calibrated for 1.53 would read these surfaces as +8.50 and −4.25 — which add to +4.25 D, three quarters of a dioptre below the real back vertex power. Two separate corrections, in the same direction
Where it refuses. Set the front surface to +60.00 D, the index to 1.498 and the thickness to 30 mm and no answer appears: 1 − (t⁄n)F₁ has gone negative, the front surface's focal point is inside the lens, and there is no back vertex power to report
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What the centre thickness is worth, and what the approximation misses

Front (D)Back (D)t (mm)nThin-lens sum (D)Exact BVP (D)Thickness worth (D)Approximation error (D)
+9.40−4.705.21.586+4.70+5.00+0.2990.0092
+15.000.008.01.498+15.00+16.30+1.3040.1043
+20.00−2.0010.01.67+18.00+20.72+2.7210.3259
+6.00−10.001.51.498−4.00−3.96+0.0360.0002
+2.00−8.001.21.74−6.00−6.00+0.0030.0000
0.00−6.002.01.586−6.00−6.000.0000.0000
Every figure is this page’s own arithmetic. The pattern is the one worth carrying away: on a PLUS lens the thickness is worth tenths or whole dioptres, while on a MINUS lens it is worth hundredths, because the thickness term acts on the front surface SQUARED and a minus lens has a flat front and a thin centre. The last row is the limit of that: a plano front surface makes the thickness worth exactly nothing.

Back vertex, front vertex and the thin-lens sum compared

QuantityValue on the default lensWhat it is for
Clocked surface sum, on a 1.53 lens measure+4.25 DNothing — it is a reading, not a power
True surface sum+4.70 DThe thin-lens approximation, and the starting point
First-order approximation+4.990 DWhat the dispensing texts print
BACK vertex power+5.00 DWhat a focimeter reads and a prescription specifies
FRONT vertex power+4.77 DThe neutralising power, used when verifying from the front
Equivalent powerNot computed hereA thick-lens property used in lens design, not dispensing
Four numbers for one lens, spread over three quarters of a dioptre, and only one of them is the prescription. The clocked sum is furthest out and is the one most easily arrived at by accident, because it needs no arithmetic. Equivalent power is named and not computed: no source read printed it as readable text, and this page does not print a formula it did not read.

A lens is not the sum of its surfaces, and on a plus lens the gap is a quarter of a dioptre

A thin lens has the power of its two surfaces added together. A real lens does not, because light diverging from the front surface’s focus has further to travel before it reaches the back surface, and the extra distance changes the vergence that arrives there. The quantity that captures it is the REDUCED THICKNESS, the centre thickness divided by the refractive index: 5.2 mm of polycarbonate behaves optically like 3.28 mm of air. The exact back vertex power is then the front surface power divided by (1 − (t⁄n)F₁), with the back surface power added unchanged.

Only the front surface is divided, and the reason is in the name. Back vertex power is measured from the back of the lens, so light has already crossed the glass by the time it meets the back surface and that surface acts on it directly. Front vertex power is the mirror image and divides the back surface instead, and the two are different numbers: on the lens this page opens with, +5.00 D and +4.77 D. A prescription, and a focimeter, mean the back vertex one.

The size of the effect is the useful half. On the published worked case reproduced here — a +9.40 front, a −4.70 back and 5.2 mm of polycarbonate — the surfaces add to +4.70 D and the real power is +5.00 D, so the thickness is worth +0.299 D. On a +15.00 D front surface 8 mm thick it is worth +1.30 D. On a minus lens it is worth almost nothing: a +6.00 front with a −10.00 back and a 1.5 mm centre moves by 0.036 D. The asymmetry is structural, because the term goes as the front surface power SQUARED and a minus lens has a flat front and a thin middle. That is also why the first-order approximation the dispensing texts print — F₁ + F₂ + (t⁄n)F₁² — is good enough for a workshop and not for a design: it is always low, by 0.009 D here and by 0.33 D on a +20.00 D front surface 10 mm thick.

Two honest notes about sources. The exact expression is printed in none of the documents read for this page; what was read is a continuing-education article that works the whole computation step by step in plain text, and this page reproduces its +5.00 D answer exactly. Four documents that should have carried the closed form rendered their equations as images instead. What corroborates the denominator is that three independent sources print 1 ÷ (1 − (t⁄n)F₁) as the shape factor of spectacle magnification, and one of them works it to a value this page reproduces to four decimal places. The second note is about the input: the figures a lens measure clocks are not surface powers unless the material happens to be index 1.53, and the correction — multiply by (n − 1) ÷ 0.530 — is worth more than the thickness term on a high-index lens. For the power a lens must have at a different distance from the eye rather than a different thickness, see vertex distance compensation.

Frequently asked questions

How do I calculate the back vertex power of a thick lens?

Divide the front surface power by (1 − (t⁄n)F₁), with the thickness in metres, then add the back surface power. Equivalently: take the front surface’s focal length, subtract the reduced thickness t⁄n, invert, and add the back surface. A +9.40 / −4.70 lens 5.2 mm thick at n = 1.586 is +5.00 D.

What is reduced thickness?

The centre thickness divided by the refractive index, which is the thickness the glass is worth optically. 5.2 mm of polycarbonate at 1.586 is 3.28 mm reduced. It is the only form in which the thickness and the index enter the calculation.

Why isn’t the lens power just the sum of its surface powers?

Because that is the thin-lens approximation and real lenses have thickness. On a plus lens the gap matters: a +9.40 / −4.70 lens 5.2 mm thick measures +5.00 D, not +4.70 D. On a minus lens it barely does, because the thickness term goes as the front surface power squared and a minus lens has a flat front and a thin centre.

What is the difference between back and front vertex power?

Which surface the thickness term divides. Back vertex power divides the front surface and adds the back one unchanged, because it is measured from the back of the lens; front vertex power does the reverse. On the lens above they are +5.00 D and +4.77 D. A prescription and a focimeter mean back vertex power.

Is F1 + F2 + (t/n)F1 squared accurate enough?

For dispensing, usually. It is the first-order expansion of the exact form and is always slightly LOW: 0.009 D low on a +9.40 / −4.70 lens 5.2 mm thick, 0.10 D low on a +15.00 D front surface 8 mm thick, and 0.33 D low on a +20.00 D front surface 10 mm thick. The exact form costs one division.

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References

  1. Musladin MG. Reduced Thickness. 20/20 Magazine continuing education, 2020mag.com, October 2023. (Works the back vertex power of a +9.40 / −4.70 lens, 5.2 mm thick, n = 1.586, step by step as plain text to +5.00 D; every step was recomputed here and the result reproduced exactly.)
  2. Optician’s Friend. Optics Study Guide. opticiansfriend.com. Accessed 10 October 2026. (The page states that its information may contain mistakes and should be independently verified, so every formula taken from it here is corroborated from a second source.)
  3. Open Exam Prep. Section 3.2: Lens Thickness, Magnification and Effective Power, ABO Advanced study guide. open-exam-prep.com. Accessed 10 October 2026.
  4. Aniseikonia, Binocular Vision Anomalies course notes hosted at umsl.edu/~garziar. University of Missouri-St. Louis. Accessed 10 October 2026.

Not medical advice. For healthcare professionals and education. Reference intervals vary by laboratory and assay — always use your own laboratory's. Never base a dose or a treatment decision on this page alone. Full disclaimer at calcengines.com/disclaimer/