Great cormorant vision: the science and the numbers
Phalacrocorax carbo · order Suliformes · Birds: all the numbers
The great cormorant has four colour channels, including violet (405, 449, 504 and 567 nm).[1][2][3] Its sharpest vision resolves 12.45 cycles per degree, against 63.75 for people in this dataset.[7][8] Its eyes cover about 308° with 13° seen by both eyes.[15]
- 4colour receptor classesMeasured*
- 12.45cycles per degree (sharpness)Measured
- 308°field of viewMeasured*
The great cormorant (Phalacrocorax carbo) is a bird in the order Suliformes. Its eyes belong to the vision type Panoramic grain-eater and wader: four cone types, low to moderate sharpness and an almost all-round field of view. Measured in this species: colour, sharpness, field of view 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 the great cormorant sees: colour receptors
What stands out
- It has 4 colour receptor classes; people have 3.
- Its sharpest vision resolves 12.45 cycles per degree: the finest stripe pattern it can tell apart from grey.
- Its eyes cover about 308° around the head, with 13° 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: 405 nm (VS/SWS (violet)), 449 nm (SWS (blue)), 504 nm (MWS (green)), 567 nm (LWS (long)) measured in this species | Measured (not re-verified) | [1][2][3] | 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][4][5][6] |
| Sharpness | Acuity 12.45 cycles per degree median of 2 behavioural rows (method priority rule) | Measured | [7][8] | Acuity: 63.75 cycles per degree Measured[9][10] |
| Field of view | Binocular overlap 13° median of 1 rows (eyes-at-rest rows preferred) | Measured | [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 308° measured total field | Measured (not re-verified) | [15] | ||
| Sharp zones (foveas) | Number of foveas 1 median of 48 relatives in class Aves: Branta canadensis, Cardinalis cardinalis, Passerina cyanea, Zenaida macroura, Cyanocitta cristata, Junco hyemalis | Group default | [16][17][18] | Number of foveas: 1 Measured[19] Fovea type: fovea Measured[19] |
| Fovea type single central fovea (displaced dorso-temporally from retinal centre) | Group default | [16][17][18] | ||
| Night vision | Activity pattern diurnal mode of 3 rows (of 3 rows): diurnal; not_nocturnal | Measured (not re-verified) | [20][21][22] | Activity pattern: diurnal Measured (not re-verified)[23][24][25][2][26][27][28][22] Pupil shape: vertical Group default[29][30] Reflective layer (tapetum): no Measured[31] Rods vs cones: cone-dominated Derived[23][24][25][2][26][27][28][22] |
| Rods vs cones cone-dominated nocturnal -> rod-dominated; crepuscular / cathemeral / mixed -> mixed; diurnal -> cone-dominated | Derived | [20][21][22] | ||
| Motion (flicker fusion) | Flicker fusion frequency 88.5 Hz median of 17 relatives in class Aves: Bubo virginianus, Melopsittacus undulatus, Passer domesticus, Taeniopygia guttata, Columba livia, Calypte anna | Group default | [32][33][34][35][36] | Flicker fusion frequency: 60 Hz Measured[34][35] |
All birds side by side: Birds: every measurement. Method: how we know what animals see.
Sources
- Lind et al. 2014
- Longcore 2023
- Murphy et al. 2022
- 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
- Heesy 2004
- Heffner et al. 1992
- Campbell & Green 1965
- Pecsics et al. 2023
- Moore et al. 2017
- Potier et al. 2017
- Rodrigues et al. 2026
- Kopania et al. 2025
- Light conditions and the evolution of…
- Wilman et al. 2014
- 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
- Boström et al. 2016
- Haarlem et al. 2026
- Healy et al. 2013
- Inger et al. 2014
- Lafitte et al. 2022
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.