Page authors: Richard E. Young, Michael J. Sweeney, Katharina M. Mangold, Inés Rosales
Vampyroteuthis infernalis is the only species known in the Vampyroteuthidae. The vampire squid is rather small, reaching a maximum of 21 cm ML (Hoving and Robison, 2012), and is very gelatinous; its consistency is that of a jellyfish. It occupies meso- to bathypelagic depths throughout the tropical and temperate regions of the world's oceans. The second pair of arms, apparently, is modified into retractile filaments that can extend to lengths up to eight times the total length of the animal, and they can be retracted into pockets between arms I and II (Hoving and Robison, 2012). The filaments appear to have a role in prey capture (Hunt, 1996), but in a novel fashion (see "Arms" next section). The vampire has black chromatophores with reddish-brown ones interspersed. [in most regions of the world's oceans, the black chromatophores dominate the general pigmentation, but off central California (e.g., the next two photographs) the reddish-brown cells dominate.] These chromatophores, however, have lost the muscles that enable the rapid color change seen in the chromatophores of other coleoids. A few normal coleoid chromatophores (i.e., chromatophore organs), however, are present on the vampire squid in the large, posterior photophores.

Figure. Two views of the same vampire squid showing some of their basic external features.© MBARI
The vampire sqid is a phylogenetic relict and possesses features of both octopodiforms and decapodiformes (most phylogenetic studies place it as an early branch of the Octopodiformes). In addition, it has many features that are probably adaptations to the deep-sea environment. Among these latter are the loss of the ink sac and most chromatophores organs, the development of photophores and the gelatinous consistency of the tissues.
A list of all nominal genera and species in the Vampyroteuthidae can be found below. The list includes the current status and type species of all genera, and the current status, type repository and type locality of all species and all pertinent references.
Danateuthis Joubin, 1929:375.
Hansenoteuthis Joubin, 1929:388.
Hymenoteuthis Thiele, 1916:4.
Melanoteuthis Joubin, 1912:1, figs 1-12.
Retroteuthis Joubin, 1929:383.
Vampyroteuthis Chun, 1903:88, text-fig.
Watasella Sasaki, 1920:168.
Melanoteuthis anderseni Joubin, 1931:170, figs 1-5.
Melanoteuthis beebei Robson, 1929:470, figs 1-8.
Vampyroteuthis infernalis Chun, 1903:88, text-fig.
Hansenoteuthis lucens Joubin, 1929:388, figs 17-23.
Melanoteuthis lucens Joubin, 1912:1, figs 1-12.
Cirroteuthis macrope Berry, 1911:589.
Watasella nigra Sasaki, 1920:168, pl 23 fig 1.
Retroteuthis pacifica Joubin, 1929:383, figs 13-16.
Danateuthis schmidti Joubin, 1929:375, figs 7-12.
Melanoteuthis schmidti Joubin, 1929:372, figs 3-6.
An octopodiform ...
Off California trawling data show most vampires between depths of 600-1100 m with peaks at 700-800 m and 900-1000 m, and with small individuals of less than 20 mm being most abundant at the deeper peak (Roper and Young, 1975). ROV observations in Monterey Bay, California suggest that the vampire occupies the oxygen minimum layer at depths of600-900 m with oxygen levels centered around 0.4 ml/l (Hoving and Robison, 2012).
Off Hawaii, 10 of 11 captures came from depths of 800-1200 m but little towing was done in deeper water. Two captures were from opening-closing nets at depths of about 800-950 m.
In the Atlantic at 18° N, 25° W, the vampire shows a peak distribution between 700 and 1200 m but without a clear size/depth pattern (Clarke and Lu, 1975).

Figure. Vertical distribution chart modified from Clarke and Lu, 1975.
In the figure, all captures were made with opening/closing trawls. Bars represent a capture and the bar length indicates the depth range of the trawl while open. Yellow bars indicate a daytime capture and blue bars a nighttime capture. Fishing effort between 1000-1250 m was about twice that between 1250 and 1500 m, and effort between 1000-1500 m was about 5 times that between 1500 and 2000 m and about the same as that between 500 and 1000 m.
Numerous records exists for captures in excess of 1200 m (e. g., see Roper and Young, 1975) from open nets. Unfortunately, due to the rather high probability of contamination from shallower depths, these records are of questionable value.
The vampire squid is broadly distributed throughout the depths of the world's tropical and temperate oceans. Some geographical variation has been noted. Young (1972) found that the beaks of vampire squid from the Pacific Ocean off California were distinctly smaller than those from vampires of the Gulf of Guinea in the Atlantic Ocean. He also noted differences in sucker size and gill size in vampires from these areas. Vampires from off Monterey, California have a predominance of reddish rather than black chromatophores.

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V. infernalis, sex ?, 13 mm GL, 1.0 mm LRL, Hawaiian waters. Photographs by R. Young |
V. infernalis, sex ?, ~40 mm ML, 2.2 mm LRL, Hawaiian waters. Photographs by R. Young. |
V. infernalis, sex ?, ML ?, 5.3 mm LRL, Hawaiian waters. Photographs by R. Young. |
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| Posterior Oblique View | ![]() |
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V. infernalis, sex ?, 13 mm GL, 1.0 mm LRL, Hawaiian waters. Photographs by R. Young |
V. infernalis, sex ?, ~40 mm ML, 2.2 mm LRL, Hawaiian waters. Photographs by R. Young. |
V. infernalis, sex ?, ML ?, 5.3 mm LRL, Hawaiian waters. Photographs by R. Young. |
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| Side View | ![]() |
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| Oblique View | ![]() |
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| Oblique View | ![]() |
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| “Top” view | ![]() |
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| Oral view | ![]() |
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| Front View | ![]() |
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| Posterior Oblique View | ![]() |
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Ventral view of an immature, female V. infernalis with the mantle cavity of cut open. Posteriorly the lining of the mantle cavity has been cut away to better view the visceral nucleus. Note that there is no abdominal septum, no ink sac, no anal flaps. The visceropericardial coelom (dark region surrounding the ventricle, stomach and caecum) is large. Posteriorly, in the ventral midline, the mantle muscle terminates on the conus of the gladius. The photograph on the right shows a mature female. The arrangement of the viscera looks very different. The gladius, with a small rostrum and a dark "apical organ", is visible because surrounding tissue has been removed.
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Figure. Vampyroteuthis infernalis.
Left - Ventral view, immature female, with the mantle cavity opened. Drawing by R. Young.
Right - The mantle cavity of a mature female. Photograph by R. Young.

Figure. View of a portion of the mantle cavity of V. infernalis. The stellate ganglion (arrow), a characteristic structure of cephalopods, appears as only a slight enlargement of a large mantle nerve. The nerve running toward the oviducal gland is the fin nerve. Photograph by R. Young.