Present-day ecosystems host a huge variety of organisms that interact and transfer mass and energy via a cascade of trophic levels. When and how this complex machinery was established remains largely unknown. Although exceptionally preserved biotas clearly show that Early Cambrian animals had already acquired functionalities that enabled them to exploit a wide range of food resources, there is scant direct evidence concerning their diet and exact trophic relationships. Here I describe the gut contents of Ottoia prolifica, an abundant priapulid worm from the middle Cambrian (Stage 5) Burgess Shale biota. I identify the undigested exoskeletal remains of a wide range of small invertebrates that lived at or near the water sediment interface such as hyolithids, brachiopods, different types of arthropods, polychaetes and wiwaxiids. This set of direct fossil evidence allows the first detailed reconstruction of the diet of a 505-million-year-old animal. Ottoia was a dietary generalist and had no strict feeding regime. It fed on both living individuals and decaying organic matter present in its habitat. The feeding behavior of Ottoia was remarkably simple, reduced to the transit of food through an eversible pharynx and a tubular gut with limited physical breakdown and no storage. The recognition of generalist feeding strategies, exemplified by Ottoia, reveals key-aspects of modern-style trophic complexity in the immediate aftermath of the Cambrian explosion. It also shows that the middle Cambrian ecosystem was already too complex to be understood in terms of simple linear dynamics and unique pathways.
Citation: Vannier J (2012) Gut Contents as Direct Indicators for Trophic Relationships in the Cambrian Marine Ecosystem. PLoS ONE 7(12): e52200. https://doi.org/10.1371/journal.pone.0052200
Editor: Andrew A. Farke, Raymond M. Alf Museum of Paleontology, United States of America
Received: August 11, 2012; Accepted: November 12, 2012; Published: December 26, 2012
Copyright: © 2012 Jean Vannier. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Funding: The author’s research is supported by ANR (Agence Nationale de la Recherche) grants (ORECO and RALI) and by the European Assemble Project (2010, Sven Lovén Centre for Marine Sciences at Kristineberg, Sweden). ANR website at: www.agence-nationale-recherche.fr, ASSEMBLE (Association of European Marine Biological Laboratories): www.assemblemarine.org. The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.
Competing interests: The author has declared that no competing interests exist.
The study of exceptionally preserved Cambrian biotas [e.g., Burgess Shale , , Chengjiang , , Sirius Passet – and Emu Bay Shale – has led to accurate reconstructions of the anatomy, lifestyles –, visual properties , and even behaviors ,  of early animals. However, information is lacking concerning their interactions within the food chain and their diet. The functioning of the Cambrian ecosystem has mainly been addressed through a combination of indirect fossil evidence supported by modern analogues . Typically, the feeding types (e.g. predation vs. particle-feeding) and strategies (sediment-eating vs. carnivory) of most Cambrian animals have been inferred from the morphofunctional analysis of their food-gathering apparatuses/limbs – and digestive systems . The predatory habit of anomalocaridids, for example, is supported by evidence from their frontal appendages, mouth apparatus – and sophisticated eyes , but there is no direct evidence of what organisms they actually preyed upon. Mechanical models using finite element analysis  and recent studies of the oral cone  contradict the view that anamolocaridids were durophagous predators able to perform strong biting motions and to inflict wounds on hard exoskeletons , , . The contents from coprolites  provide a degree of trophic resolution but cannot be tied to particular predators although some coprolites composed entirely of crushed skeletal elements from the Cambrian of California, Utah, Canada (Burgess Shale) and Australia  may have been produced by arthropods with robust gnathobasic appendages such as Sidneyia . Rare fossil associations  and trace fossils  have suggested possible hunting or scavenging behaviors but these relationships require quantification. Qualitative and quantitative analyses of the communities from the Burgess Shale ,  and the Maotianshan Shale – have provided detailed information on the diversity of ecological types and the presumed organization of the early and middle Cambrian ecosystems but do not tell us about the exact trophic links between species. Recent theoretical models  have predicted strong similarities between the trophic organization of Cambrian food webs and modern ones but lack detailed testing by fossil evidences. By contrast, the analysis of gut contents presented here and exemplified by the priapulid worm Ottoia prolifica from the middle Cambrian Burgess Shale provides direct and detailed evidence for trophic relationships and new insights both into the actual diet and feeding behavior of Cambrian animals. The case of priapulids reveals the potential of a source of information that has long been considered as relatively limited and anecdotal , . A noticeable exception though is S. Conway Morris’ comprehensive work  on the priapulid worms from the Burgess Shale in which the gut contents of Ottoia are first described. This pioneer work is important in that it led to the concept of Ottoia as an iconic Cambrian predator and formed the basis of my study. My results also invite reassessment of the function and the complexity of Cambrian marine food webs where animals, for the first time in their history, played a major role in the transfer of mass and energy. The interpretations here also challenge the notion of strict feeding regimes and linear food chain and provide support for a marine trophic web where energy flow circulated via multiple animal interactions and parallel pathways , as it does in present-day ecosystems.
Materials and Methods
Our fossil material comes from two stratigraphic horizons in the middle Cambrian Burgess Shale Member: 1) the Walcott Quarry Member, characterized by fossiliferous, finely laminated, calcareous, siltstones and silty graphitic mudstones, typically with a weathered horizontally-banded appearance; and 2) the slightly younger Raymond Quarry Member, characterized by grey, greenish and brown layered blocky-slaty mudstone , , –. The Ottoia specimens kept in the collections of the National Museum of Natural History, Smithsonian Institution, Washington D.C. (USNM), all come from excavations at Walcott’s original site (the so-called Phyllopod Bed within the Walcott Quarry Member). Those from the Royal Ontario Museum (ROM) collections, Toronto, were collected from both the Raymond and Walcott Quarry Members (RQ, RT and WQ, WT numbers respectively) in successive seasons of excavations and talus picking (RT, WT) between 1975 and 2000 by Royal Ontario Museum parties led by D. Collins. Altogether more than 2,600 specimens of Ottoia prolifica were examined, only a small percentage had preserved gut contents (Fig. 1, Table S1). The recent priapulid Priapulus caudatus was collected from the Gullmar fjord near the Sven Lovén Centre for Marine Sciences at Kristineberg, Sweden and from near The White Sea Biological Station “Kartesh” (WSBS), Russia. Digital photography (with polarizing filters to increase contrast of anatomical features), scanning electron microscopy and Energy-dispersive X-ray spectroscopy (EDX) analysis were used to study the morphology and chemical composition of the fossil and Recent material. The global chronostratigraphic subdivision of the Cambrian System is currently in the process of ratification by the International Union of Geological Sciences (IUGS). The Burgess Shale Formation belongs to Series 3, Stage 5 (see recent provisional chart ). For convenience, I maintain usage of “middle Cambrian” for this formation.
The pie diagrams illustrate differences in the diet of Ottoia from the Raymond Quarry (RQ+RT) and the Walcott (WQ+WT) Quarry. Hyolithids dominate in the gut contents from the Raymond Quarry followed in decreasing order by brachiopods, agnostids, trilobites, bradoriids, ASE (presumed wiwaxiids), SLE (presumed polychaetes) and trilobites. In the Walcott Quarry, three almost equally represented groups (SLE, hyolithids and ASE) are prevalent, followed by bradoriids, trilobites, agnostids and brachiopods. (1) guts containing skeletal fragments and/or undetermined material and a variable proportion of sediment; (2) guts containing skeletal elements or fragments that belong to animal species present in the Burgess Shale biota; (3) guts containing elements that belong to a single species (e.g. only hyolithid skeletal elements). Empty guts generally appear as a colored or reflective strip running axially from the pharynx to the anus. ASE, almond-shape elements (presumed wiwaxiid sclerites); RQ, RT, collection specimens from the Raymond Quarry and talus (Royal Ontario Museum); SLE, setae-like elements (presumed polychaete chaetae); USNM, collection specimens from the National Museum of Natural History, Smithsonian Institution, Washington D.C.; WQ, WT, collection specimens from the Walcott Quarry and talus (Royal Ontario Museum). Raw data in Table S1.
This research does not involve human participants. I obtained permission to study the Burgess Shale fossil collections from the Royal Ontario Museum (ROM,Toronto) and the Smithsonian National Museum of Natural History (USNM, Washington D.C.) from Jean-Bernard Caron and Douglas Erwin, respectively. The majority of specimens were studied in the ROM and the USNM. A small number of them were obtained on loan and returned.
Gut Content Analysis
As with the majority of non-biomineralizing fossils from the Burgess Shale, Ottoia prolifica is preserved as compressed aluminosilicate and carbonaceous films ,  (Fig. 2). Ottoia resembles Recent priapulids ,  (Fig. 3) in having a retractile introvert armed with hooks and an invaginable pharynx lined with small teeth, two features of key-importance in locomotion and feeding . The gut of Ottoia appears as a colored or reflective strip of constant width (1.4 to 2.3 mm in specimens 60–100 mm long ) running axially from the pharynx to the anus. It is either straight, sinuous or looped. EDX elemental mapping reveals anatomical partitioning of the gut with elevated C, Fe and P that probably reflects its organic-rich original composition and early diagenetic mineralizations in pyrite, apatite or calcite (Fig. 4). More than 50% of the studied specimens possess empty guts (Fig. 1) and about 20% display three-dimensionally preserved gut contents (GC) that preferentially concentrate in the posterior half of their digestive tract. GC typically occur as compacted ribbon-like features or fragmented blobs containing skeletal elements (e.g. hyolithid conchs, brachiopod valves), smaller debris of uncertain origin, and sediment. Thin section, SEM and EDX analyses do not show any significant compositional difference between GC and the aluminosilicate host rock, except from being enriched in organic matter (Fig. 5). Furthermore, acritarchs and sponge spicules found in comparable quantities in GC and the host rock  confirm that Ottoia ingested sediment.
from the middle Cambrian Burgess Shale. A, ROM 61780a, high concentration of complete specimens. B–D, ROM 61759, ROM 61752 and ROM 61757, complete specimens. E, F, ROM 61751 and ROM 61765, details of anterior part. G, ROM 61760, details of introvert bearing curved scalids. H, I, ROM 61769 and ROM 61764, details of posterior part showing bursa and posterior hooks. Abbreviations: a, anus; an, trunk annulation; bu, bursa; gu, gut; in, introvert; m, mouth; ph, posterior hook; pt, pharyngeal teeth; px, pharynx; px(e), everted pharynx; px(i), inverted pharynx; sc, scalid; tr, trunk. Scale bar: 1 cm for A–D and 5 mm for E–I.
A, B, general view of a live specimen in sea water and simplified section through body showing major anatomical features. C, section through pharynx (sclerotized pharyngeal teeth in orange; introvert removed. D, F, frontal view of a slightly everted pharynx showing pentagonal pattern of pharyngeal teeth around mouth opening and details of pharyngeal teeth. E, G, scalid rows along bulbous introvert and details of scalids (tip perforated). H–J, feces of Priapulus caudatus filled with compacted undigested material and enclosed by a transparent membrane, bundles of undigested polychaete chaetae and undetermined gut contents (mainly sediment and detritus of various origin). D–G, I, J, are scanning electron micrographs of dessicated specimens. Abbreviations: a, anus; an, trunk annulation; bu, bursa; ca, caudal appendage; cc, coelomic cavity; fc, feces contents; fm, feces membrane; go, gonads; gu, gut; in, introvert; m, mouth; pm, pharyngeal muscles; pt, pharyngeal tooth; px, pharynx; rm, retractor muscle; sc, scalid; sr, scalid row; tr, trunk. Scale bar: 1 cm for A, B; 5 mm for C; 500 µm for D, E, H; 200 µm for F; 100 µm for G; 10 µm for I; 5 µm for J.
from the middle Cambrian Burgess Shale. The mapping reveals anatomical partitioning of the gut, with elevated C, Fe and P that probably reflects its organic-rich original composition and early diagenetic mineralizations in pyrite, apatite or calcite. A–E, ROM 61758b. A, B, general view under normal and polarized light (white arrow to indicate mapped area). C, D, back scattered image of gut showing patches of carbonaceous film; this film is interpreted as remains of the gut wall, rather than gut contents. E, elemental mapping. Abbreviations: a, anus; cf, carbonaceous film; gc, gut content; gu, gut; m, mouth. Scale bar: 1 cm for A, B; 5 mm for E; 1 mm for C; 20 µm for D.
from the middle Cambrian Burgess Shale Formation. A–D, USNM 196195, three-dimensionally preserved gut contents, general view and thin section; gut material (C) is easily distinguished from the matrix (D) by its brown colour due to high organic content. Crystals (in white) are not specific to the gut and are observed elsewhere in the matrix though smaller and less concentrated; they are interpreted as sponge spicules . E, F, ROM 61755a, isolated fragment of gut content seen in transverse section. G, H, ROM 61754, gut contents showing small skeletal fragments and undetermined elements embedded in sediment. I, J, ROM 61755a, transverse section through upper part of gut content; the uppermost thin layer possibly represent the gut wall. K, ROM 61755b, thin carbonaceous film overlying gut contents, possibly representing the gut wall. gc, gut contents; se, sediment; sf, skeletal fragment; ue, undetermined element. A–D, courtesy L. Wilson (see also ). A, G are light photographs; B and D were taken in transmitted light; E, F, H-K are scanning electron micrographs (K, back-scattered image). Scale bar: 5 mm for A; 2 mm for G; 500 µm for B, H; 100 µm for C, D; 50 µm for K; 10 µm for E, I; 5 µm for F; 2 µm for J.
The most frequent animal in Ottoia’s GC (Fig. 1, Tables 1, 2, 3, 4 and Table S1) is the hyolithid Haplophrentis carinatus ,  characterized by a mineralized exoskeleton with a pointed conch, an operculum and a pair of curved appendages called helens; Figs. 6A–H, 7). It occurs in 48% of GC that have identifiable elements (Fig. 1). The number of conchs varies from 1 to exceptionally 6; 82% of hyolithid-bearing GC have only 1 or 2 conchs; 62% of the conchs are ca. 3–6 mm long and 0.6–3 mm wide (Table 1). Hyolithids in GC are 3D-preserved and show no visible trace of physical breakdown or chemical dissolution, the conch and the operculum being sometimes connected (Fig. 6D). The very rare presence of helens within GC, either attached or detached from the conch, suggests that the majority of hyolithids became partly disarticulated as they entered the digestive tract of the worm (e.g. by the muscular contractions of pharynx). Helens may have been weakly attached in life, which may account for the low percentage (ca. 7%; ) of fully articulated hyolithids in the fossil assemblages. Hyolithid conchs show a remarkably consistent orientation with 77% of them pointing towards the mouth of Ottoia. This indicates that hyolithids were preferentially grasped and drawn into the gut by their anterior side, where they probably offered a stronger grip point to the pharyngeal teeth of Ottoia.
A–C, ROM 61747, with 4 hyolithid shells (Haplophrentis carinatus), their apex pointing anteriorly. D, ROM 61767, hyolithid with operculum and conch in connexion. E, F, ROM 61749, hyolithid conch and a pair of disarticulated helens. G, ROM 61774, hyolithid conch and disarticulated operculum. H, USNM 202777, hyolithid conch within the posteriormost part of the gut (bursa everted). I–K, ROM 61779 with two brachiopods (Micromitra burgessensis) in posterior gut. L, M, ROM 61775 with complete agnostid arthropod (Ptychagnostus praecurrens) within the anterior gut. N, O, ROM 61777 with a trilobite pygidium (Ehmaniella burgessensis) inside the gut. P, ROM 61785 with a trilobite cephalon (E. burgessensis). Abbreviations: a, anus; ag, agnostid; an, trunk annulation, ANT, anterior; ase, almond-shape element; br, brachiopod; br1, br2, from anterior, brachiopod 1 and 2; bu, bursa; ce, cephalon; co, hyolithid conch; gc, gut content; gu, gut; gw, gut wall; h1–h4, from anterior, hyolithid 1 to 4; he, helen; in, introvert; m, mouth; op, hyolithid operculum; ph, posterior hook; POST, posterior; pt, pharyngeal teeth; py, pygidium; tr, trunk. Scale bar: 1 cm for A, I, L; 5 mm for B, C, E, H, M; 2 mm for K; 1 mm for D, F, G, J, N–P.
from the middle Cambrian Burgess Shale. A, ROM 61753a, showing 3 hyolithids preserved with their opercule. B–E, ROM 61782, with 5 hyolithid shells (Haplophrentis carinatus) within the gut, their apex pointing anteriorly; general view and details. F–H, USNM 196381, with 6 hyolithid shells within the gut. I, USNM 188604, with 3 hyolithids (h3 close to the anus). Abbreviations: ANT, anterior; an, trunk annulation; co1–co3, hyolithid conch 1 to 3; gc, gut content; gu, gut; he, helen; h1–h6, from anterior, hyolithid 1 to 6; op1–op3, hyolithid operculum 1 to 3; lo, loop; ph, posterior hook; POST, posterior; tr, trunk. Scale bar: 1 cm for B, F, H, I; 5 mm for A, C–E; 2 mm for G.
Articulate brachiopods (Table 2) are represented in GC by Micromitra burgessensis , ,  characterized by a very distinctive lozenge-like reticulated pattern (Figs. 6I–K, 8A–F) and, possibly Diraphora , , , although much more rarely. The best-preserved specimens of Micromitra burgessensis (not in GC) are fringed with long and delicate setae which indicates that the animal did not live buried in the sediment  but more likely at the water sediment interface.
from the Middle Cambrian Burgess Shale. A–D, USNM 196204, with articulate brachiopod, possibly Diraphora bellicostata , , . E, ROM 61756, with the inarticulate brachiopod Micromitra burgessensis , ,  and undetermined gut contents. F, ROM 61750 with Micromitra burgessensis and a hyolithid. G, H, ROM 61770 with agnostid (possibly Pagetia bootes , ), general view and close-up. I, J, ROM 61783 with complete agnostid and hyolithid. Abbreviations: ag, agnostid; an, trunk annulation; ANT, anterior; br, brachiopod; ce, cephalon; gc, gut contents; gu, gut; h, hyolithid; op, operculum of hyolithid; ph, posterior hook; POST, posterior; py, pygidium. All light photographs. Scale bar: 1 cm for A, G; 2 mm for B–F, H–J.
Arthropod skeletal elements (Table 3) are frequent, represented mainly by agnostids, small trilobites and bradoriids (Figs. 6L–P; 8G–J). The agnostids Ptychagnostus praecurrens ,  and possibly Pagetia bootes ,  occur as mainly disarticulated exoskeletal elements (anterior and posterior shields, thoracic segments), except for one complete specimen found within the anterior-most section of the gut just behind the pharynx (Fig. 6L, M). The trilobite Ehmaniella ,  is represented by isolated cephalons, pygidia and disarticulated thoracic segments (Figs. 6N–P, 9A–E). The bradoriid Liangshanella burgessensis  is a tiny arthropod capped by a dorsally folded shield. Although extremely abundant in the Burgess Shale biota , L. burgessensis is a rare element in GC (Fig. 9F, G). Indeterminate bivalved arthropods different from bradoriids also occur as shield-like folded features (Fig. 9I, J). In addition to these readily identifiable undigested remains are setae-like (SLE) and almond-shape (ASE) skeletal elements.
from the middle Cambrian Burgess Shale. A, B, ROM 61785, showing gut contents with a trilobite cephalon (probably Ehmaniella burgessensis , ). C, D, ROM 61761, with contents containing trilobite remains (e.g. thoracic segments). E, USNM 196425, with gut contents containing possible trilobite remains. F, G, ROM 61776, with bradoriid arthropod  in anterior part of gut. H, I, ROM 61778, with possible shields of bivalved arthropods in posterior gut, general view and detail. J, ROM 61771, with possible shields of bivalved arthropods. Abbreviations: ANT, anterior; ba, bivalved arthropod (shield); bd, bradoriid; ce, cephalon; gc, gut contents; gu, gut; ph, posterior hook; POST, posterior; px(e), everted pharynx; tr, trilobite; ts, thoracic segment. All light photographs (J, whitened with ammonium chloride). Scale bar: 1 cm for A–C; 5 mm for F; 2 mm for D, E, G; 1 mm for I, J.
(d) Setae-like elements (SLE).
SLE generally occur as large concentrations of straight or slightly curved 3D-preserved cylindrical elements (Fig. 10). Their size (length and diameter 50–950 and 17–55 µm, respectively; Fig. 11) is not consistent with a sponge origin (Figs. 11, Fig. S1). Most sponges occurring in the same horizon or associated with Ottoia on the same bedding plane ,  have monaxial needle-like elements (diameter between 10 and 20 µm) usually tightly clustered to form tracts or tufts. Pirania has strong radial spicules (length >7 mm and diameter >100 µm). No cross-shaped or rayed structure typical of hexactinellid (e.g. Protospongia) or stem-group calcareous (e.g. Eiffelia) sponges was found in SLE. That SLE are arthropod setae is unlikely because of the lack of tergites, shields or appendages associated with them. SLE are interpreted as the chaetae of the polychaete worm Burgessochaeta setigera ,  (Figs. 10G–J, 11) that effectively co-occurs with Ottoia (Table 5). Supporting evidence comes from the high number of chaetae in Burgessochaeta (>1000 attached to more than 20 pairs of biramous parapodia), their size range (diameter 30–90 µm) and frequent groupings in bundles (Fig. 10B–E). The size of SLE is consistent with Ottoia feeding on juveniles of Burgessochaeta (Fig. 11). Polychaete chaetae are frequent in the feces of Recent priapulid worms such as Priapulus (Fig. 3I).
A–D, ROM 61755b, general view, accumulations and details of SLE in gut. E, ROM 61772b, SLE in gut. F, ROM 61746a, SLE in cross section, preserved in aluminosilicate. G–I, Burgessochaeta setigera (Polychaeta; , ); G, ROM 56967 complete specimen with numerous chaetae on parapodia; H, ROM 56968a(1), ROM 56968a(1), decayed specimen; I, ROM 56968a(2), chaetae on parapodia. J, ROM 56969a, bundle of chaetae (compare with C). Abbreviations: ANT, anterior; bd, possible bundle of SLE; cf, carbonaceous film; ch, chaetae; gc, gut content; gu, gut; pa, parapodium; POST, posterior. Scale bar: 1 cm for A, G; 1 mm for E, H–J; 500 µm for B; 100 µm for D; 20 µm for F.
,  and sponge spicules. The diameter of most spicules of sponges occurring in the same horizons as Ottoia ranges between 10 and 20 µm and is lower than that of most SLE. Interpolation (up right diagram) suggests that SLE are undigested chaetae of small individuals of Burgessochaeta, possibly between 5 and 10 mm long. Size distribution of chaetae (blue) and SLE (red) lengths are given for three well-preserved Burgessochaeta specimens (A–C) and one Ottoia gut content (number 4). Diagonella (bottom left) is a typical sponge in the Burgess Shale biota. Abbreviations: ANT, anterior; BL, body length; bo, body; ch, chaetae; CL, chaeta length; pa, parapodium; POST, posterior; sp, spicule. 1, ROM 61786b; 2, ROM 61787; 3, ROM 61772b; 4, ROM 61755; 5, ROM 61788; 6, ROM 61789; 7, ROM 61746. A, ROM 56968a; B, ROM 56968b; C, ROM 56967; D, ROM 56968b; E, ROM 56969a.
(e) Almond-shape elements (ASE).
ASE (Table 4) have a consistent almond shape, are slightly convex, and bear at least 6 ribs parallel to their margins (Fig. 12). They typically occur in GC as aligned elements (N = 1 to 12; 34% over 9; Table 1) often overlapping each other. Their length varies from 1.5 to 6 mm (63% between 2 and 3.5 mm). More than 88% of ASE point towards the anus of Ottoia - i.e. - the opposite direction of hyolithid shells in GC (compare with Figs. 6A–H, 7). The only skeletal elements comparable in size, shape and ornament with ASE are the scale-like sclerites of wiwaxiids, especially those of Wiwaxia corrugata ,  (Fig. 12J) that co-occurs with Ottoia (Table 5). The relatively low number of ASE in GC, the absence of typical spiny and crescentic elements, and the average size of Wiwaxia (>20 mm vs. gut diameter of Ottoia <3 mm) is not consistent with wiwaxiids being ingested whole by Ottoia. More likely it suggests that Ottoia fed on decaying wiwaxiids by ingesting lumps of soft tissues where small sclerites were still attached. The consistent orientation of ASE in GC may be explained by both the unidirectional imbricated pattern of the Wiwaxia scleritome  and also by capture constraints (see hyolithids). The cannibalistic behavior of Ottoia based on a single poorly preserved specimen  is not confirmed here although this behavior clearly remains plausible (see recent priapulid worms such as Priapulus; ). I re-examined this specimen (USNM 198922). The spinules and proboscis hooks that are assumed to be present within its gut are most probably preservational artefacts or due to the chance juxtaposition of two ill-preserved Ottoia specimens as suggested by L. Wilison . Gut contents from the Raymond Quarry are largely dominated by hyolithids, whereas SLE (assumed polychaetes), hyolithids and ASE (assumed wiwaxiids) prevail in GC from the Walcott Quarry (Fig. 1). This suggests that Ottoia was not dependent on one particular food source but could adapt its diet with local food availability.
. A–C, G, H, ROM 61768, general views, and details of ASE (bulbous feature in G is an artefact due to mineralization). D, ROM 61763b with aligned ASE. E, ROM 61773a, with ASE and other skeletal elements. F, ROM 61781a, three aligned ribbed ASE. I, ROM 61745b, isolated ASE within gut. J, ROM 61747, Wiwaxia corrugata ,  with sclerites in situ. K, L, ROM 56965, W. corrugata, ribbed sclerite and general view of decayed specimen. Abbreviations: a, anus; ANT, anterior; ase, almond-shape element; gc, gut content; m, mouth; ma, mouth apparatus; POST, posterior; scs, scale-like sclerite; se, skeletal element; sps, spine-like sclerite. Scale bar: 5 mm for A–C, J, L; 2 mm for D, E, K; 1 mm for F–I.
Two fossil associations with several specimens of Ottoia forming a wreath around the carcass of the arthropod Sidneyia ,  indicate that Ottoia had possible scavenging habits (Fig. 13). Decaying carcasses of relatively large epibenthic animals such as Sidneyia (length up to ca 140 mm ) may have represented a substantial food source for Ottoia, easily accessible from its supposed shallow subhorizontal burrows . The tiny pharyngeal teeth of Ottoia (Fig. 2E, F) are interpreted as a possible adaptation for scraping soft material such as decaying tissues.
A, B, USNM 196241, showing at least 5 worms around the decaying carcass of Sidneyia. This specimen was interpreted  as a death assemblage with the worms feeding around the collapsed and decaying carcass of Sidneyia inexpectans. I follow this interpretation here, although the number of worms is more likely to be five than nine . C, D, ROM 61748a, showing an assemblage very similar to USNM 196241; four worms form a wreath-like arrangement around the remains of Sidneyia. E, F, USNM 250218, showing a curved specimen of Ottoia closely associated with Sidneyia. All light photographs (A, courtesy Jean-Bernard Caron, ROM). Scale bar: 1 cm. Abbreviations: an, annulation; dg, digestive glands; gc, gut content; gu, gut; hy, hyolithid conch; ph, posterior hook; px, pharynx; w1–5, worm (Ottoia) 1–5.
The feeding mechanism of Ottoia was remarkably simple, being limited to the transit of food via a tubular gut with no physical breakdown (except the disarticulation of composite exoskeletons) and storage process. Nutrients were probably chemically extracted from food via digestive fluids produced in the midgut lumen as in Recent priapulids . The assumed low nutritional value of some of the food items such as hyolithids, brachiopods that probably contained less protein-rich tissues than arthropods and worms; ) may have been offset by the richer intake of dead tissues from carcasses (Fig. 13). Ottoia lacked visual and complex sensory organs, in contrast with the arthropods from the same horizons that had potential features (e.g. compound eyes, antennae) for visual  and chemo-tactile recognition. Attraction to food was probably triggered by chemical cues released from living and dead tissues (Fig. 14A). Chemoreceptors were possibly located in the well-developed circumoral scalids (Fig. 2G), as is the case in modern priapulids worms ( and Fig. 3E, G).
from the middle Cambrian Burgess Shale. 1, hyolithids (Haplophrentis); 2, brachiopods (Micromitra); 3, polychaete worms (Burgessochaeta); 4, bradoriids (Liangshanella); 5, trilobites (Ehmaniella); 6, agnostids (Ptychagnostus); 7, 8, carcasses of Sidneyia and Wiwaxia. (A–C), feeding behavior of Ottoia: detection of food via possible chemical cues and ingestion. gu, gut; in, introvert with spiny scalids; px(e), everted pharynx; px(i), inverted pharynx; sc, scalid; tr, trunk.
Trophic Complexity of the Cambrian Ecosystem
Ottoia obtained food from diverse animal sources (nine species in GC) and by using different techniques: 1) predation on small invertebrates that lived at or near the water-sediment interface (e.g., hyolithids, brachiopods, and polychaetes); and 2) scavenging on carcasses and detritus. The brachiopods and hyolithids from the Burgess Shale biota were most probably slow moving animals that could have been equally ingested alive or scavenged after death by Ottoia. No fossil evidence indicates that Ottoia favored predation over scavenging or the reverse. In contrast, polychaetes such as Burgessochaeta were probably far more active errant and burrowing animals with capabilities to escape predators such as Ottoia. Again, Ottoia may have fed indiscriminately upon dead and living polychaetes in various proportion depending on its hunting abilities and the rapidity of the prey. The idea that hyolithids were “hunted”  may not reflect the exact reality of feeding relationships. More likely these small invertebrates that often lived in large populations were taken off randomly by Ottoia which may have lived in sub-horizontal burrows just below the water sediment interface . The presence of disarticulated elements in GC, typically trilobites, cannot be interpreted as unambiguous evidence of predation, because it may result from chance ingestion during scavenging. Similarly, fine sediment was inevitably ingested along with consumable food. The high percentage of empty guts indicates that Ottoia was neither a sediment eater sensu stricto nor a continuous feeder. Its straight cylindrical gut is also poorly consistent with continuous deposit feeding exemplified by modern sipunculans . The gut of Recent and Cambrian  sipunculans is typically U-shaped and highly coiled. Although we cannot exclude that Ottoia collected and ingested undifferentiated particles and detritus (as possibly indicated by the organic enrichment of GC), this worm had none of the characteristics of a surface deposit feeder (e.g., introvert with small tentacles). Moreover, the ratio of its body to gut volume (0.8–1.5%)  is much lower than in typical deposit feeders. Ottoia was more likely an intermittent omnivorous feeder with low maintenance requirements. Possible modern analogues are macrobenthic priapulids such as Priapulus and Halicryptus , , in which guts are frequently empty and contain detritus mixed with identifiable animal food items (Table 6; –). Our study undermines the status of Ottoia as an iconic predator and selective hunter  and gives this taxon the more realistic status of being a generalist and possibly facultative feeder  – i.e., an animal with the capacity to vary its diet with local availability. In recent marine ecosystems, facultative feeders play an important role in conferring resilience in the benthic communities to environmental disturbances and habitat changes . Ottoia may have played a comparable and important role at a critical time when the first modern-style ecosystems started to build up.
The recognition of genuinely generalist feeding strategies, as seen here in Ottoia, reveals a high level of trophic complexity and flexibility that has no equivalent in preceding eras (e.g., Ediacaran ecosystem; , ) and foreshadows modern-style ecosystems. Direct documentation of this behavior in the immediate aftermath of the Cambrian explosion indicates that the marine ecosystem had already become too complex to be understood in terms of simple linear dynamics. More likely, the ecosystem already functioned as an interactive web, with multiple interactions between animal species and the exploitation of diverse food sources. This mode of functioning, which probably set up in the Early Cambrian, is likely to have generated important feedback and accelerating effects on diversity, ecosystem stability and macroevolutionary dynamics.
Early Onset of Parallel Trophic Pathways
Predation was undoubtedly one of the driving forces in the early diversification of metazoans and the build-up of complex animal interactions and trophic web , , , , , . Grazing ,  and suspensivory  were also major feeding techniques used by numerous Cambrian animals. The case of Ottoia highlights the role of scavenging as another key-consumption mode. We think that the rise of epibenthic communities  resulting from the Cambrian radiation fuelled the food web with a new pool of detrital material that became a major and abundant food source for numerous scavengers and detritivores thus promoting and boosting the detrital pathway. The input of animal-derived organic matter into the ecosystem probably deeply modified the food supply in terms of quantity, energy, chemical quality and digestibility with probable feedback effects on the evolution of digestive systems  and feeding modes. In common with Ottoia, arthropods may have acquired adaptations to exploiting this detrital food store with relatively low cost of energy expenditure. This requires testing from detailed studies on the digestive systems and appendage functionalities of Cambrian arthropods and their possible modern analogues. Parallel circuits such as the “green pathway” (through primary producers, herbivore/grazers to carnivores) and the detrital pathway that is essential in the energy flow of modern marine ecosystems  may have been already operating in the Cambrian adding to the trophic complexity.
Sponge species that co-occur with Ottoia prolifica in level -120 , ,  of the Walcott Quarry (Burgess Shale Formation, middle Cambrian). A, B, Hazelia nodulifera Walcott, ROM 40317B(1), general view and details. C, D, Hazelia palmata Walcott, ROM 53585, general view in polarized light and details of closely packed spicules. E, F, Falospongia falata Rigby, ROM 40317B(2), general view and details of skeletal tracts. G, H, Pirania muricata Walcott, ROM 53309, general view and details of radiating spicules. I–K, Diagonella hindei Walcott, ROM 61766, general view and details of the spicule network of a small and larger specimen on the same slab. L, Eiffelia globosa Walcott, ROM 53567, details of six-rayed spicules. msp, monaxial spicule; rsp, radial thick spicule; rtr, radial tract; tr, tract composed of numerous spicules. (Scale bar, 2 mm for A, C, E, G, I; 1 mm F, H, J-L; 500 µm for B, D.
Studied material (Ottoia prolifica from the middle Cambrian Burgess Shale, British Columbia, Canada). The specimens are housed in the Royal Ontario Museum (ROM), Toronto, Canada and the Smithsonian National Museum of Natural History (originally US National Museum; USNM), Washington D.C. All the specimens have preserved digestive tracts with or without gut contents.
I thank Jean-Bernard Caron, Peter Fenton, Douglas Erwin and Mark Florence for access to the fossil material deposited in the Royal Ontario Museum (ROM), Toronto and the National Museum of Natural History (USNM), Washington D.C. I am thankful to Fredrik Pleijel, Sylve Robertsson, Stefan Agrenius (Sven Lovén Center for Marine Sciences, Sweden) and Alexander Tzetlin (White Sea Biological Station Kartesh, Russia) for collecting Recent priapulids, Tara Macdonald and Brenda Burd for information on recent marine ecosystems, and Nick Butterfield, Jean-Bernard Caron Mark Williams and Stephen Mojzsis for critical reading of the early versions of the MS. I am thankful to Tom Harvey and two anonymous reviewers for their constructive comments. Lucy Wilson is thanked for images used in Figure 5A–D. This is Royal Ontario Museum Burgess Shale project number 40.
Conceived and designed the experiments: JV. Performed the experiments: JV. Analyzed the data: JV. Contributed reagents/materials/analysis tools: JV. Wrote the paper: JV.
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