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Réflexion sur le processus coracoïde des hominoïdes et des atèles ; application à quelques hominidés fossiles
Jean-Luc VoisinTo cite this version:
Abridged versionA lot of studies have been done about primates' scapulae [1,3,6,13,16,18,21,25,27]. However, apart from Martin and O'Brien's work [10], there are no studies about the coracoid process yet.This work is a study of the orientation and morphology of the coracoid process in hominoids, spider monkeys, colobus monkeys, two neandertal and Homo ergaster remains (table I). Among fossil hominids, there are only four remains that still possess a coracoid process. Five points are used (figure 1). Three of them (E, F, Q) define two perpendicular planes P and P , and the two others (U, R) define the great axis of the process. The projection of these five points in P and P planes allows to know the coracoid process orientation in comparison with the glenoid cavity (gleno-coracoid-p and gleno-coracoid-p * Correspondance et tirés à part.Adresse e-mail : jeanlucv@mnhn.fr (J.-L. Voisin).angles). The coracoid process morphology is described by three indexes. The coracoid indices illustrate the length of the coracoid process and the two others (maximum and minimum robustness index) its breadth. The gleno-coracoid-p and the gleno-coracoid-p angles show two groups. The first one, with the greatest value, contains only man. The second one includes all the other primates' studies here ( figures 2 and 3, table II). The coracoid index has the greatest value in gibbons and spider monkeys ( figure 4, table III), the most brachiating primates. The two coracoid robustness indices define also two groups, the spider monkey with the breadless coracoid process and the hominoids and the colobus monkey with a more robust coracoid process (figures 5 and 6, table III).When the coracoid process orientation put in relation to the glenoid cavity, there is a great difference between man and the other hominoids and spider monkeys. On 299 J.-L. Voisin / C. R. Acad. Sci. Paris, Sciences de la Terre et des planètes / Earth and Planetary Sciences 332 (2001) 299-306