Field of Science

Showing posts with label Trilobitomorpha. Show all posts
Showing posts with label Trilobitomorpha. Show all posts

Hadromeros: A Trilobite Survivor

Reconstruction of Hadromeros subulatus, from Kielan-Jaworowska et al. (1991).


Trilobites of the genus Hadromeros were widespread in the Late Ordovician and Early Silurian of Eurasia and North America. They are classified in the Cheiruridae, the same family that includes another trilobite genus that has been featured on this site, Sphaerexochus. However, Hadromeros differs from Sphaerexochus in that its glabella (its 'nose') is not as large. Whereas in my earlier post I suggested that Sphaerexochus may have been a predator, Hadromeros was probably a less aggressive feeder. It was possibly a detritivore, picking bits of nutritious material out of the sand and mud. This interpretation is supported by the known leg morphology of a closely related genus, Ceraurus, in which the legs are fairly generalised and show little adaptation for food processing (Bergström 1973).

Hadromeros and Ceraurus are placed in the Cheirurinae, a distinct subfamily from the Sphaerexochinae that includes Sphaerexochus. One characteristic feature of many members of the Cheirurinae is that the bases of the pleura, the plates that run down each side of the thorax, are swollen in dorsal view. The purpose of these swellings remains unknown. You might expect that, trilobites being as abundant in the fossil record as they are, we would know a great deal about them, and in many respects that is quite true. However, in other respects our knowledge is also frustratingly incomplete. Trilobites have an extensive fossil record because their dorsal exoskeleton was mineralised, and it is this that is usually preserved. The ventral section of the body, on the other hand, was not mineralised, and is only preserved under exceptional circumstances. This includes such significant features as the legs and mouthparts (as indicated above, we have some knowledge of the leg morphology of Cerarurus, but no direct evidence for Hadromeros). It is possible that the cavities underneath the cheirurine pleural bases housed some modification of the gills, if the gills in trilobites were comparable to those of living crustaceans. But how or to what purpose the gills were modified can only be speculated upon.

Morphologically, Hadromeros was a fairly unremarkable trilobite, but it stands out from the other genera of the Cheirurinae in one important respect (that has, indeed, already been alluded to in this post). The end of the Ordovician saw a mass extinction in marine life, by some measures the second largest to have ever occurred. Few groups of animals made it through unscathed, and the cheirurids were no exception. Of the eight subfamilies of Cheiruridae recognised by Přibyl et al. (1985), only three made it through to the Silurian: the Cheirurinae, Sphaerexochinae and Deiphoninae. Within the Cheirurinae, Hadromeros is the only genus currently known from both sides of the Ordovician-Silurian boundary, and may have been ancestral to all other post-Ordovician cheirurines. While other genera were whisked away, Hadromeros became the Trilobite that Lived.

REFERENCES

Bergström, J. 1983. Palaeoecologic aspects of an Ordovician Tretaspis fauna. Acta Geologica Polonica 23 (2): 179-206.

Kielan-Jaworowska, Z., J. Bergström & P. Ahlberg. 1991. Cheirurina (Trilobita) from the Upper Ordovician of Västergötland and other regions of Sweden. Geologiska Föreningen i Stockholm Förhandlingar 113 (2-3): 219-244.

Přibyl, A., J. Vaněk & I. Pek. 1985. Phylogeny and taxonomy of family Cheiruridae (Trilobita). Acta Universitatis Palackianae Olomucensis Facultas Rerum Naturalium Geographica-Geologica XXIV 83: 107-193.

Horny-Arsed Trilobites

Reconstruction of Ceratopyge, from here.


Just a short post for today. The Ceratopygidae are a family of trilobites known from the Late Cambrian and Early Ordovician. The name of the type genus, Ceratopyge, means 'horned rump', and one of the features that has classically defined the family is the presence of one or two pairs of spines on either side of the pygidium, the plate the makes up that hind end of a trilobite. These spines appear to be derived from lateral extensions of one of the anterior segments incorporated into the pygidium. However, there are also some genera without pygidial spines that share other features with the family (such as a narrow rim to the cheeks) and so have also been recognised as ceratopygids. Ceratopygids also possessed narrow spines extending back from the posterior corners of the head. The number of segments between head and pygidium varied between genera: early genera have nine segments, but some later genera have only six (Fortey & Chatterton 1988) (offhand, the drawing above looks to have one too many segments).

Proceratopyge gamaesilensis, from here.


Otherwise, ceratopygids seem to have been fairly generalised trilobites. The eyes were present but not large, and there don't appear to be any features suggesting they were swimmers. The features of the underside of the head are poorly known in ceratopygids overally, but where known, the hypostome (the plate on the underside of the head that would have sat in front of the mouth) is firmly attached to the anterior margin of the head. Trilobites with this arrangement are believed to have been scavengers or predators on small invertebrates (Fortey & Owens 1999). In some later genera, such as Ceratopyge, the glabella in the midline of the cephalon expanded forward, with a corresponding reduction in the width of the anterior margin. As the glabella would have contained the trilobite's stomach, its enlargement may indicate that these later ceratopygids were taking larger prey.

REFERENCES

Fortey, R. A., & B. D. E. Chatterton. 1988. Classification of the trilobite suborder Asaphina. Palaeontology 31 (1): 165-222.

Fortey, R. A., & R. M. Owens. 1999. Feeding habits in trilobites. Palaeontology 42 (3): 429-465.
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