Reexamination of the immature hominid maxilla from Tangier, Morocco

Allometric scaling of infraorbital surface topography in Homo

Infraorbital morphology is often included in phylogenetic and functional analyses of Homo. The inclusion of distinct infraorbital configurations, such as the "canine fossa" in Homo sapiens or the "inflated" maxilla in Neandertals, is generally based on either descriptive or qualitative assessments of this morphology, or simple linear chord and subtense measurements. However, the complex curvilinear surface of the infraorbital region has proven difficult to quantify through these traditional methods. In this study, we assess infraorbital shape and its potential allometric scaling in fossil Homo (n=18) and recent humans (n=110) with a geometric morphometric method well-suited for quantifying complex surface topographies. Our results indicate that important aspects of infraorbital shape are correlated with overall infraorbital size across Homo. Specifically, individuals with larger infraorbital areas tend to exhibit relatively flatter infraorbital surface topographies, taller and narrower infraorbital areas, sloped inferior orbital rims, anteroinferiorly oriented maxillary body facies, posteroinferiorly oriented maxillary processes of the zygomatic, and non-everted lateral nasal margins. In contrast, individuals with smaller infraorbital regions generally exhibit relatively depressed surface topographies, shorter and wider infraorbital areas, projecting inferior orbital rims, posteroinferiorly oriented maxillary body facies, anteroinferiorly oriented maxillary processes, and everted lateral nasal margins. These contrasts form a continuum and only appear dichotomized at the ends of the infraorbital size spectrum. In light of these results, we question the utility of incorporating traditionally polarized infraorbital morphologies in phylogenetic and functional analyses without due consideration of continuous infraorbital and facial size variation in Homo. We conclude that the essentially flat infraorbital surface topography of Neandertals is not unique and can be explained, in part, as a function of possessing large infraorbital regions, the ancestral condition for Homo. Furthermore, it appears likely that the diminutive infraorbital region of anatomically modern Homo sapiens is a primary derived trait, with related features such as depressed infraorbital surface topography expressed as correlated secondary characters.

Krapina 1: a juvenile Neandertal from the early late Pleistocene of Croatia

The juvenile A Skull from Krapina, Croatia (Krapina 1) has been the subject of considerable debate since B. Skerlj first suggested that it might not be a Neandertal. Although widely known by its original designation, the Krapina A Skull was recatalogued, along with all of the Krapina hominids, in the 1980's (Radovcic, et al., [1988]. The Krapina Hominids: An Illustrated Catalog of Skeletal Collection. Zagreb; Mladost). It is now catalogued as Krapina 1 in the archives of the Hrvatski Prirodoslovni Muzej, Zagreb, Croatia. We present a detailed, morphometric analysis of this specimen, comparing it to other Krapina specimens, juvenile late Pleistocene hominids (including Neandertals), and subadult recent humans. This analysis demonstrates that Krapina 1 possesses morphological features that are primitive retentions; others that represent derived Neandertal specializations; and still others that are typical for all European late Pleistocene humans. Morphological features associated with the browridges are intermediate between Neandertal and early modern European form. Nevertheless, a thorough analysis of the morphology of this specimen, in ontogenetic and regional contexts, leads to the conclusion that it cannot be excluded from the Neandertal range of variation. We conclude that the most parsimonious explanation for this 130 ka specimen is that it should be regarded as a Neandertal.