Dj. Furbish et Aj. Arnold, HYDRODYNAMIC STRATEGIES IN THE MORPHOLOGICAL EVOLUTION OF SPINOSE PLANKTONIC-FORAMINIFERA, Geological Society of America bulletin, 109(8), 1997, pp. 1055-1072
To counter gravitational settling, planktonic foraminifera adjust thei
r buoyancies, in part by manufacturing low-density lipids or gases. Th
e biochemical energy that a foraminifer expends in this way is a funct
ion of the speed at which it would otherwise settle if it did not expe
nd this energy. In turn, the settling speed varies with foraminifer sh
ape. We consider here foraminifera that have acicular spines, for exam
ple Orbulina universa and Globigerinoides sacculifer. Growing spines p
roduces two counteractive effects: spines increase the weight of a for
aminifer, and therefore tend to increase its settling speed; they also
increase the fluid drag on the foraminifer, and therefore tend to dec
rease its settling speed. If growing spines is part of an evolutionary
strategy to impede settling, then it is reasonable to expect that the
advantage of increasing drag by growing spines outweighs the disadvan
tage of increasing weight.The complexity of foraminiferal shapes precl
udes directly solving the equations of fluid motion for drag and settl
ing speed. We therefore appeal to the efficacy of dimensional analysis
to define a coefficient of drag C-D and a Reynolds number Re for spin
ose foraminifera. Experiments that involve settling scaled models of f
oraminifera (constructed from beeswax and pins) in viscous liquids are
then used to confirm the forms of generalized dimensional formulae re
lating the settling speed W to test radius R, spine number n, spine le
ngth l, and spine radius r. Geometrically similar foraminifera whose s
pine arrangements possess quasispherical symmetry settle according to
an inverse relation between C-D and Re, homologous to Stokes's law for
spheres. Fluid drag systematically increases with both n and l. For g
iven R, l, and r, a minimum settling speed occurs at an intermediate s
pine number no. Similarly, for given R, n, and r, a maximum settling s
peed W-0 occurs at an intermediate spine length l(0). Results suggest
that insofar as there is disadvantage in settling rapidly, there is ad
vantage in remaining small; or, if growth of tests occurs, there is ad
vantage in manufacturing many long thin spines. Investments of mass an
d energy associated with this strategy must be weighed against those i
nvolved in achieving neutral (or positive) buoyancy by other mechanism
s, and limitations on lengths of spines imposed by their finite streng
th. A comparison of the theory with modern foraminifera suggests that
the geometries of adult Orbulina universa and Globigelinoides sacculif
er, in the absence of external protoplasm, are well suited to impede s
ettling. With external protoplasm, however, l is effectively decreased
and the drag associated with spines is not sufficient to provide visc
ous settling unless the protoplasm possesses positive buoyancy. For an
individual at or near a state of neutral buoyancy, drag associated wi
th spines decreases the sensitivity with which its settling speed resp
onds to unavoidable changes in the buoyancy of its protoplasm related
to metabolic activity, and to changes in the density and viscosity of
sea water related to external factors. The effect is to hydrodynamical
ly dampen vertical motions that would otherwise occur if the individua
l did not possess spines. In contrast, the small drag associated with
few short spines is advantageous to juveniles that must ascend from de
ep to shallow waters during their ontogenies. A partitioning of finite
spine mass into many moderate to short spines is less effective in pr
oducing drag than one involving fewer long spines. Long spines, howeve
r, are more susceptible to mechanical breakage due to the torque that
viscous forces apply to them. Foraminifera with approximately 10 (or f
ewer) spines that possess mechanical properties equivalent to those of
spines of adult Orbulina universa and Globigerinoides sacculifer can
withstand motions at speeds of only a few tenths of a centimeter per s
econd (or more, depending on spine strength) without breakage. With in
creasing numbers of spines, the resulting hydrodynamic interaction amo
ng them has the effect of significantly reducing the chance of spine b
reakage related to momentarily rapid motions; this is attributable to
a decrease in the proportion of the spine length l exposed to signific
ant viscous forces, whereby the torque on individual spines is decreas
ed. External protoplasm also reduces the chance of breakage by decreas
ing the length of spines exposed to surrounding fluid.