Bridge Width Reference Chart

The printed 14 to 24 mm band drawn as a ladder: what each stamped bridge does to the lens centres, to decentration and to the front's width at a fixed 52 mm lens, the two guessing rules crossed into four combinations, and the five whole millimetres no mirror rule reaches. Print it or keep it on your phone.

1. What the middle figure measures

The middle figure of a stamped trio, in three lines.
   
What it measures The gap between the two lenses, read at the openings the lenses sit in. A boxing-system reference dated 10 June 2026 defines the figure as the shortest distance between the nasal edges, and that is the number that lands in the middle of a temple arm — the aperture figure, not the rim figure.
What it is not The bridge opening, and not a measurement of your nose. Three published instructions place the ruler on three different boundaries — across the inside faces of the two rims, which includes the rim walls, and between the openings the lenses sit in, which excludes them. What separates the two readings is a pair of rim walls, a quantity no page in this family prints.
What else decides fit Two quantities no frame prints: the thickness of the frame at the ridge and the curvature the front carries. A wearer's account names them beside the stamped figure, which is why a 17 mm bridge can fit where a 20 mm one will not, and why one buyer reports frames from 17 to 24 mm that all fit.

2. The printed band, as a ladder

distance between lens centres, mm 66 68 70 72 74 76 14 16 18 20 22 24 1.5 2.5 3.5 4.5 5.5 6.5 decentration per eye, mm inward, at a 63 mm pupillary distance what the mirror rules return: 16 to 21 mm
One published band run against one lens width. Rows are the printed adult bridge sizes, 14 to 24 mm; the lens is held at 52 mm, which is the width a retailer's own worked example uses. Column two is 52 plus the bridge, column three is column two minus 63 mm and halved, column four is two lenses plus the bridge, and column five adds the 20 mm pair allowance. The rows are arithmetic, not stock items.
Bridge, as stamped Distance between lens centres Decentration per eye at 63 mm Hinge to hinge Front, at the 20 mm allowance
14 mm (0.55 in)66 mm (2.60 in)1.5 mm (0.06 in) inward118 mm (4.65 in)138 mm (5.43 in)
16 mm (0.63 in)68 mm (2.68 in)2.5 mm (0.10 in) inward120 mm (4.72 in)140 mm (5.51 in)
18 mm (0.71 in)70 mm (2.76 in)3.5 mm (0.14 in) inward122 mm (4.80 in)142 mm (5.59 in)
20 mm (0.79 in)72 mm (2.83 in)4.5 mm (0.18 in) inward124 mm (4.88 in)144 mm (5.67 in)
22 mm (0.87 in)74 mm (2.91 in)5.5 mm (0.22 in) inward126 mm (4.96 in)146 mm (5.75 in)
24 mm (0.94 in)76 mm (2.99 in)6.5 mm (0.26 in) inward128 mm (5.04 in)148 mm (5.83 in)

The allowance is this site's own number and only the last column contains it: at 12 mm for the pair the same six fronts read 130 to 140 mm (5.12 to 5.51 in) instead of 138 to 148, and not one other figure in the table moves. Column three steps 1 mm (0.04 in) per eye for every 2 mm of bridge, because halving the excess of a sum is what the formula does. Against the two ceilings in print, column three clears the 5 mm (0.20 in) figure in four rows, the 4 mm (0.16 in) end in three, and the 3 mm (0.12 in) end in two — the 14 and 16 mm bridges. The 14 to 24 mm band is 10 mm wide while the published 40 to 60 mm lens band is 20 mm wide.

3. The two guessing rules, crossed

Two published rules that ask for a mirror and no tool, crossed. Column three is the set of whole millimetres both rules allow at once. The four source windows are 16 to 18 mm (0.63 to 0.71 in) and 19 to 21 mm (0.75 to 0.83 in) against 14 to 18 mm (0.55 to 0.71 in) and 18 mm or more.
What the bridge reads against the pupils What the nose is rated The window both rules allow together
At or below the pupils Narrow 16 to 18 mm (0.63 to 0.71 in) — three whole millimetres, and the only wide agreement available.
At or below the pupils Broad 18 mm (0.71 in) — the two windows touch at exactly one whole millimetre.
Above the pupils, or wider than average Narrow Nothing — 19 to 21 mm and 14 to 18 mm do not overlap by a single millimetre.
Above the pupils, or wider than average Broad 19 to 21 mm (0.75 to 0.83 in) — and this is the window that lands highest on the ladder above.

The empty cell is the finding, and it is internal to one page: the source that supplies the nose-width rule also supplies the pupil-height rule, in the same list of steps, so a bridge that reads above the pupils with a narrow nose is left holding two instructions that cannot both be followed. The pupil rule, applied to the printed band, can only ever return six whole millimetres — 16, 17, 18, 19, 20, 21 — so five of the eleven integers the same pages publish, 14, 15, 22, 23 and 24 mm, are unreachable by the most-reprinted fitting instruction in this family. The nose-width rule can reach the 14 and 24 ends, and it overlaps its own two bands at 18 mm without saying what to do there. Run through the ladder above at a 52 mm lens, the low window costs 2.5 to 3.5 mm (0.10 to 0.14 in) of decentration per eye and the high window 4.0 to 5.0 mm (0.16 to 0.20 in).

4. What the band does against the published lens band

Multiply the two published bands instead of picking from them: a lens from 40 to 60 mm and a bridge from 14 to 24 mm produce lens-centre distances from 54 to 84 mm (2.13 to 3.31 in). That is a space 30 mm wide, and every combination in it is inside the adult ranges as printed.

Three ceilings dropped onto that space at the worked-example distance of 63 mm (2.48 in).
Ceiling Sums admitted Of the printed 30 mm Left outside
5 mm53 to 7319 mm11 mm, all of it at the wide end
4 mm—16 mm14 mm
3 mm—12 mm18 mm — three fifths of the space

Where the 3 mm reading's 18 mm of exclusion sits is not symmetrical: 3 mm of it is at the narrow end and 15 mm at the wide end. The narrowest combination in print — a 40 mm lens and a 14 mm bridge, 54 mm between centres — is not safe just because it is small: at 63 mm it puts each lens 4.5 mm (0.18 in) outward, which clears the 5 mm reading and fails both ends of the tighter band.

5. Your own numbers

6. Two stages, not one

  1. Get a band from the mirror and treat its width as roughly 3 mm — the whole of the low window's span, and about the gap between the two published windows' edges.
  2. Then let the sum move the band. The frame you buy has to keep its lens centres close enough to your own distance that a laboratory is willing to cut the order, and that constraint is a two-line subtraction.
  3. Treat the number as a coordinate, not a fit guarantee. A bridge taken off an old frame identifies a position on a front; the object that occupied it has been discarded, and the two quantities that decide the rest of the fit are printed nowhere.