Depth of field by subject distance#
28 mm at f/11 on full frame (36×24 mm), circle of confusion 30 µm. “Background blur” is the size of an out-of-focus light at infinity as a percentage of frame width.
| Focus distance | Near limit | Far limit | Total DoF | Front / behind | Background blur |
|---|---|---|---|---|---|
| 30.0 cm (0.98 ft) | 26.9 cm | 33.9 cm | 7.0 cm | 44% / 56% | 0.73% |
| 50.0 cm (1.64 ft) | 41.7 cm | 62.4 cm | 20.7 cm | 40% / 60% | 0.42% |
| 75.0 cm (2.46 ft) | 57.5 cm | 1.08 m | 50.2 cm | 35% / 65% | 0.27% |
| 1.00 m (3.28 ft) | 71.0 cm | 1.69 m | 98.3 cm | 30% / 70% | 0.20% |
| 1.50 m (4.92 ft) | 92.6 cm | 3.94 m | 3.02 m | 19% / 81% | 0.13% |
| 2.00 m (6.56 ft) | 1.09 m | 11.8 m | 10.7 m | 8% / 92% | 0.10% |
| 3.00 m (9.84 ft) | 1.33 m | ∞ | ∞ | — | 0.07% |
| 4.00 m (13.1 ft) | 1.50 m | ∞ | ∞ | — | 0.05% |
| 5.00 m (16.4 ft) | 1.62 m | ∞ | ∞ | — | 0.04% |
| 7.00 m (23.0 ft) | 1.78 m | ∞ | ∞ | — | 0.03% |
| 10.0 m (32.8 ft) | 1.92 m | ∞ | ∞ | — | 0.02% |
| 15.0 m (49.2 ft) | 2.05 m | ∞ | ∞ | — | 0.01% |
| 20.0 m (65.6 ft) | 2.13 m | ∞ | ∞ | — | 0.01% |
| 30.0 m (98.4 ft) | 2.20 m | ∞ | ∞ | — | 0.01% |
| 50.0 m (164 ft) | 2.27 m | ∞ | ∞ | — | 0.00% |
| 100 m (328 ft) | 2.32 m | ∞ | ∞ | — | 0.00% |
Try other settings#
28 mm at other apertures (subject at 3 m)#
Other focal lengths at f/11#
Same lens settings on other formats#
When to use it#
At f/11, a 28 mm lens on full frame is a natural choice for landscapes and architecture where front-to-back sharpness matters. Focused at 3 m you get everything to infinity; for maximum front-to-back sharpness focus at 2.40 m and everything from 1.20 m to infinity will be acceptably sharp.
See also the f/11 aperture guide.
Frequently asked questions#
What is the depth of field of a 28mm lens at f/11?
On full frame, focused at 3 m, it is infinite (beyond the hyperfocal distance); at 1 m it is 98.3 cm.
What is the hyperfocal distance for 28mm f/11?
2.40 m (7.89 ft) on full frame. Everything from 1.20 m to infinity is acceptably sharp.
Last updated October 03, 2026 · How we calculate · Sources