The phenomenon of bipolarity, one of the major disjunct distribution p
atterns on the face of the earth, has been investigated repeatedly sin
ce the mid-nineteenth century. Running through the many hypotheses tha
t have been put forward to account for its occurrence, it is possible
to detect two persistent themes: it is usually interpreted within a di
spersal framework, and it is generally believed to be of comparatively
recent origin. To many authors, the phenomenon is intimately linked t
o the Plio-Pleistocene glaciations. Recent palaeontological investigat
ions have established that bipolarity can now be traced back to at lea
st the Early Jurassic period (i.e. 200 m.y.a.). Here it is well marked
in the Pliensbachian stage by a variety of pectinacean bivalve taxa.
Further bivalves indicate probable Middle Jurassic examples, but the p
henomenon is more clearly seen in the Late Jurassic, especially in the
Tithonian stage. At this time, inoceramid, buchiid and oxytomid bival
ve occurrences at northern hemisphere localities such as arctic Canada
, N.W. Europe, Siberia, N.E. USSR and Japan can be matched with those
in southern South America, Antarctica and Australasia. A striking Earl
y Cretaceous (Aptian-Albian) bipolar pattern for the oxytomid Aucellin
a may be complemented by several infaunal bivalves, brachiopods and at
least one gastropod. There is strong circumstantial evidence to sugge
st that bipolar molluscs continued to develop through the Cenozoic era
. Such is the level of generic and subfamilial differentiation within
certain living forms as to suggest that they must be the product of a
considerable evolutionary history. It is likely that present-day distr
ibution patterns of prosobranch gastropod groups such as the whelks (B
uccinidae), together with certain fissurellids, littorinids, naticids
and turrids, can be related to a late Paleogene-early Neogene phase of
bipolarity. Many amphitropical taxa, in both the marine and terrestri
al realms, have probable late Neogene-Pleistocene origins. It is possi
ble to set the Jurassic and Cretaceous examples of bipolarity within a
largely vicariant framework based upon the disintegration of the Pang
ean supercontinent. In this way the widespread ranges of putative Tria
ssic ancestors were disrupted by tectonic processes in low latitude re
gions, although it should be emphasized that major climatic and oceano
graphic changes were almost certainly involved too. Similarly, it is p
ossible to view late Paleogene-early Neogene bipolarity as a vicariant
event, but this time with climatic change identified as the single mo
st important agent. Widespread or cosmopolitan distributions are held
to have formed during global cool phases (such as the late Eocene-earl
y Miocene) only to be disrupted by global warming (such as in the late
early Miocene). It is even possible to view Plio-Pleistocene patterns
as, at least in part, the products of vicariant events caused by rapi
d temperature and sea level shifts. Clearly, there is an urgent need h
ere for more critical taxonomic data to test these various hypotheses.
Phylogenetic studies of groups such as the Mesozoic bivalve superfami
ly Monotoidea and the Cenozoic Buccinidae, in particular, should const
itute future rigorous tests. In so doing, they should also provide muc
h useful information on the relative roles of dispersal and vicariance
in promoting global disjunction in marine faunas. Repeated formation
of bipolar patterns through geological time may have had important imp
lications for modes of speciation and phenomena such as the origin of
taxonomic diversity gradients.