American kestrel vision: the science and the numbers
Falco sparverius · order Falconiformes · Birds: all the numbers
Their sharpest vision resolves 30.85 cycles per degree, against 63.75 for people in this dataset.[6][7] Their eyes cover about 292° with 27.5° seen by both eyes.[10]
- 30.85cycles per degree (sharpness)Measured
- 292°field of viewEstimated
The American kestrel (Falco sparverius) is a bird in the order Falconiformes. Its eyes belong to the vision type Raptor telephoto: four cone types, two foveas and very high sharpness. Measured in this species: sharpness, field of view, foveas and night vision. Measured core: measured values on at least 3 of the 6 dials.
This is a simulation built from published eye measurements, not what the animal experiences.
What kestrels see: colour receptors
What stands out
- Its sharpest vision resolves 30.85 cycles per degree: the finest stripe pattern it can tell apart from grey.
- Its eyes cover about 292° around the head, with 27.5° seen by both eyes at once.
- Activity pattern: diurnal.
The six dials
Evidence levels: how the tiers work. "Measured" means a value measured in this species; "Estimated" values come from a close relative or an eye-size formula. The last column gives the values for people from the same catalogue.
| Dial | Value | Evidence | Sources | People |
|---|---|---|---|---|
| Colour | Colour receptors 4 receptor classes: 417.5 nm (VS/SWS (violet)), 452 nm (SWS (blue)), 501 nm (MWS (green)), 570 nm (LWS (long)) receptor set of nearest measured relative Anas platyrhynchos (same class Aves) | Group default | [1][2] | Colour receptors: 3 receptor classes: 421.5 nm (VS/SWS (violet)), 532 nm (MWS (green)), 558.4 nm (LWS (long)) Measured (not re-verified)[2][3][4][5] |
| Sharpness | Acuity 30.85 cycles per degree median of 2 behavioural rows (method priority rule) | Measured | [6][7] | Acuity: 63.75 cycles per degree Measured[8][9] |
| Field of view | Binocular overlap 27.5° median of 2 rows (eyes-at-rest rows preferred) | Measured | [10][11] | Binocular overlap: 122.5° Measured[12][13] Total field of view: 200° Measured (not re-verified)[14] Blind area behind the head: 160° Derived[14] Eye placement: frontal Derived[12][13] |
| Total field of view 292° rule: total = 360 - blind area | Derived | [10] | ||
| Blind area behind the head 68° | Measured | [10] | ||
| Eye placement lateral frontal if binocular overlap >= 60 deg, else lateral | Derived | [10][11] | ||
| Binocular field, vertical extent 112.5°; elevation 90 deg (horizontal plane through the eyes); eyes at rest unless stated | Measured | [15] | ||
| Sharp zones (foveas) | Number of foveas 2 species-v1.csv text: 2 (central deep + temporal shallow) | Measured | [16][17] | Number of foveas: 1 Measured[18] Fovea type: fovea Measured[18] |
| Fovea type central fovea, temporal | Measured | [16][17] | ||
| Night vision | Activity pattern diurnal mode of 6 rows (of 6 rows): diurnal; not_nocturnal | Measured (not re-verified) | [19][20][21][22][23][24] | Activity pattern: diurnal Measured (not re-verified)[25][26][27][2][28][29][30][24] Pupil shape: vertical Group default[31][32] Reflective layer (tapetum): no Measured[33] Rods vs cones: cone-dominated Derived[25][26][27][2][28][29][30][24] Night sensitivity (optical, against people): S = 0.93 µm² sr, 1 times people (log10 ratio 0) Derived[34] |
| Rods vs cones cone-dominated nocturnal -> rod-dominated; crepuscular / cathemeral / mixed -> mixed; diurnal -> cone-dominated | Derived | [19][20][21][22][23][24] | ||
| Motion (flicker fusion) | Flicker fusion frequency 113.25 Hz median of 2 relatives in genus Falco: Falco peregrinus, Falco cherrug | Estimated | [35][36] | Flicker fusion frequency: 60 Hz Measured[37][38] |
All birds side by side: Birds: every measurement. Method: how we know what animals see.
Sources
- Lind et al. 2014
- Longcore 2023
- Kirwan
- Müller et al. 2009
- Thermal Activation and Photoactivation of Visual… 2004
- Caves et al. 2018
- Caves et al. 2024
- Kirk et al. 2004
- Veilleux et al. 2014
- Tyrrell et al. 2017
- Tyrrell et al. 2017
- Heesy 2004
- Heffner et al. 1992
- Campbell & Green 1965
- O'Rourke et al. 2010
- Rasys et al. 2024
- Potier et al. 2017
- Kopania et al. 2025
- Angielczyk et al. 2014
- Light conditions and the evolution of…
- Choiniere et al. 2021
- Wilman et al. 2014
- Schmitz et al. 2011
- Moura et al. 2024
- Anderson et al. 2017
- Borges et al. 2018
- Wilman et al. 2014
- Maor et al. 2017
- Jones et al. 2009
- Schmitz et al. 2011
- Banks et al. 2015
- Cervino et al. 2021
- Guareschi et al. 2025
- Brauburger et al. 2026
- Haarlem et al. 2026
- Lafitte et al. 2022
- Healy et al. 2013
- Inger et al. 2014
Every value cites its sources (all sources). Values were extracted from these works and converted (units, medians, derived values); changes are ours, and the listed sources do not endorse this site. Data: catalogue-v1, built 2026-09-29. Accuracy notes: how accurate is this? Method: how we know.