Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, Second Part: Subclass Osculosa; Index: Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIIIHaeckel, Ernst
Science
Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, Second Part: Subclass Osculosa; Index: Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIII
Haeckel, Ernst
Radiolaria
The numerous new genera discovered in the rich collection of the
Challenger, and mainly in the wonderful Radiolarian ooze of the Central
Pacific (Stations 263 to 274) throw a new light upon the complicated
affinities of the whole group, and manifest a far greater richness in
developmental variations and admirable morphological productions than
Bütschli could suppose. The following description, however, must remain
very incomplete, since the exact and thorough study of all individual
forms, in the same manner as {1017}Bütschli had done in the case of a small
number of species, would require several years. I can therefore only give
the basis of further researches.
In the majority of #Spyroidea# the three essential elements of the
Nassellarian skeleton are easily recognisable, viz.:--A, the vertical
sagittal ring of the #Stephoidea#; B, the basal tripod of the #Plectoidea#,
and C, the latticed cephalis of the #Cyrtellaria#. These three elements are
constantly so combined that the primary sagittal ring bisects the cavity of
the lattice-shell and produces an external, longitudinal, more or less
distinct constriction, separating the lateral inflated halves of the
bilocular cephalis; while the three divergent feet of the basal tripod
descend from the cortinar or basal plate of the cephalis. The number of the
feet is often augmented; they are rarely wanting (probably reduced). The
sagittal ring is constantly present, though its relation to the shell-wall
exhibits many modifications. The bilocular form of the fenestrated
cephalis, with its sagittal constriction, is characteristic of all true
#Spyroidea#, and separates them from the #Botryodea# (with multilobate
cephalis) on the one hand, and from the #Cyrtoidea# (with simple cephalis)
on the other. There are, however, some intermediate forms between these
three suborders of #Cyrtellaria#, which show a direct transition to one
another. Almost constantly the length of the three dimensive axes in the
cephalis of the #Spyroidea# is so different that the lateral or frontal
axis is the longest, the sagittal or dorso-ventral axis the shortest, and
the principal or longitudinal axis intermediate between them. As in all
dipleuric or bilaterally symmetrical forms, the two poles of the frontal
axis are equal, whilst the two poles of the sagittal and of the principal
axis are more or less different. In only a few forms of #Spyroidea# these
differences are difficult to make out; usually the dorsal side is
distinctly different from the ventral, and the apical side from the basal.
A perfect knowledge of the dipleuric shell requires therefore accurate
observation from all six sides.
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