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Earth-Science Reviews
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Early Cenozoic evolution of the latitudinal diversity gradient
J. Alistair Crame
British Antarctic Survey, High Cross, Madingley Road, Cambridge CB3 0ET, UK
ARTICLE INFO
Keywords:
Early Cenozoic
Greenhouse world
Latitudinal diversity gradients
Polar generalists
Primary productivity
Evolutionary rates
ABSTRACT
We are beginning to appreciate that the huge radiations of both marine and terrestrial taxa in the aftermath of
the K/Pg mass extinction event were concentrated largely, but not exclusively, in the low-latitude and tropical
regions. This in turn means that significant latitudinal diversity gradients were developed well before the onset
of global cooling at the Eocene/Oligocene boundary. Net rates of evolutionary radiations were significantly
higher through the Early Paleocene – Middle Eocene interval (i.e. ~62–42 Ma) in the tropics than at the poles
but this may be due as much to their retardation in the latter regions as to their acceleration in the former. At
least in the marine realm, polar assemblages are characterised by the phenomenon of high dominance/low
evenness, and it is thought likely that this is due to the extreme seasonality of primary production at the base of
the food chain. Many modern polar marine organisms are de facto trophic generalists and occupy significantly
broader ecological niches than their tropical counterparts. Although we cannot dismiss the roles of both tem-
perature and area in promoting tropical diversity, it could well be that LDGs are just as much the product of a
latitudinal gradient in the seasonality of primary productivity. Such a gradient would have operated in both
greenhouse and icehouse worlds.
1. Introduction
The latitudinal gradient in taxonomic diversity forms one of the
most striking features of life on Earth at the present day. For many
major groups of plants and animals there are simply far more of them in
the low-latitude and tropical regions than there are in the high-latitude
and polar ones; such differences often amount to at least an order of
magnitude at the species level (Hillebrand, 2004;Lomolino et al., 2010;
Tittensor et al., 2010;Valentine and Jablonski, 2015;Worm and
Tittensor, 2018). Understanding how such large disparities in the lati-
tudinal distribution of taxa may have arisen remains a major topic at
the heart of contemporary biodiversity research (Gaston, 2000;
Mittelbach et al., 2007;Erwin, 2009;Krug et al., 2009;Brown, 2014;
Jablonski et al., 2017;Worm and Tittensor, 2018).
One particular area of uncertainty to date has been the precise time
of origin of the modern latitudinal diversity gradient (LDG). One school
of thought has placed it at the Eocene/Oligocene (E/O) boundary (34
Myr ago), a time of rapid global cooling and pronounced shift in the
Earth's climate state from greenhouse to icehouse (Zachos et al., 2001,
2008). At first sight this would seem to be entirely logical as many
warm-temperate and tropical taxa would simply have been unable to
disperse into the newly expanded cold-temperate and polar regions
(Wiens and Donoghue, 2004). A previously diffuse boundary at the
edge of the tropics now became much more clearly defined. Support for
an E/O origin of the modern LDG has come largely, but not exclusively,
from the terrestrial realm, and a combination of molecular phylogenetic
and palaeontological studies on various plants, vertebrates and insects
(Hawkins et al., 2006, 2007;Archibald et al., 2010;Condamine et al.,
2012;Mannion et al., 2014). There is also evidence from the deep sea
fossil record that the origin of the psychrosphere (i.e. the circum-Ant-
arctic cold water current) at this time led to a profound alteration of
global circulation patterns and thermal stratification of the oceans. This
in turn led to a marked reduction in the taxonomic diversity of polar
deep-sea benthic taxa such as foraminifera, as well as certain phyto-
plankton and zooplankton (Thomas and Gooday, 1996;Wilson, 1998;
Culver and Buzas, 2000;Thomas, 2007;Houben et al., 2013;Fenton
et al., 2016). The E/O boundary hypothesis is linked very firmly to the
concept of global climate change and thus, ultimately, to the principle
that temperature directly controls standing levels of biodiversity
(Brown, 2014;Clarke, 2017).
But balanced against an E/O origin for the LDG is the fact that many
modern taxa, in both the terrestrial and marine realms, have their
evolutionary roots in an intense Early Cenozoic radiation in the wake of
the Cretaceous/Paleogene (K/Pg) mass extinction event (i.e. in the in-
terval ~62–42 Ma) (Kafanov, 2001;Briggs, 2006;Jaramillo et al.,
2006;McKenna and Farrell, 2006;Bininda-Emonds et al., 2007;
Stanley, 2007;Ramirez et al., 2007;Schultz and Brady, 2008;
Schuettpelz and Pryer, 2009;Meredith et al., 2011;Near et al., 2013;
https://doi.org/10.1016/j.earscirev.2020.103090
Received 1 November 2019; Received in revised form 14 January 2020; Accepted 15 January 2020
E-mail address: jacr@bas.ac.uk.
Earth-Science Reviews 202 (2020) 103090
Available online 17 January 2020
0012-8252/ © 2020 The Author. Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license
(http://creativecommons.org/licenses/BY-NC-ND/4.0/).
T
Feng et al., 2017). Although this pronounced radiation, which is clearly
indicated in long, time-series datasets (Flessa and Jablonski, 1996;
Stanley, 2007;Alroy, 2010;Sepkoski, 2002;Huang et al., 2014), might
have been spread more or less evenly across the Earth's surface, various
lines of evidence suggest that it was in fact concentrated in the tropics
(Jablonski, 1993, 2005a). If this is indeed the case then we may have to
accept that steep, regional LDGs can form in a greenhouse world. This
in turn suggests that factors other than temperature may be important
in their formation.
2. Evidence for an Early Cenozoic latitudinal diversity gradient
Observational estimates of the extinction intensity at the K/Pg
boundary at various global localities are generally in the range of
60–70% at the species level and 30–40% at the generic one (Stanley,
2007;Krug and Jablonski, 2012;Condamine et al., 2013;Aberhan and
Kiessling, 2015). Even though there is no obvious evidence of a lati-
tudinal bias in extinction intensity from these localities (Raup and
Jablonski, 1993;Zinsmeister et al., 1989;Tobin et al., 2012;Witts et al.,
2016), it is still possible that the LDG may have been significantly re-
duced in scale overall in the immediate aftermath of the extinction
event, and then for several millions of years afterwards (Jablonski,
2005b;Stanley, 2007;Krug et al., 2009). Empirical evidence for such a
reduction is in short supply but in one recent comparison of Early
Cenozoic molluscan faunas between Antarctica (Seymour Island lo-
cality) and two tropical localities (US Gulf Coast and Paris Basin) it was
shown that in the terminal Cretaceous stage (the Maastrichtian) there
was quite a strong diversity contrast between the tropics and the pole
(N.B. the very small number of rudistid bivalves in the Maastrichtian
were excluded from the analyses). Nevertheless, this is reduced sig-
nificantly in the initial Paleogene stage (the Danian), and especially so
in the bivalves (Crame, 2019). This could be taken as a weakening of
the gradient by a stronger reduction of tropical faunas in the extinction
event, but further work is required to verify this pattern on smaller
temporal and taxonomic scales. Work on microbiotas across the K/Pg
boundary suggests that it may have taken as long as 4 Myr for taxo-
nomic diversity levels to be restored to pre-extinction levels, with un-
doubtedly some variation in rates between major clades (D'Hondt,
2005).
The subsequent radiation of both bivalves and gastropods through
the Paleocene and Eocene epochs has been traced between the same
three localities (Beu, 2009;Crame et al., 2014, 2018;Crame, 2019).
When this is done it is apparent that there is a rapid rise through the
later Paleocene stages into the Early Eocene and then Middle Eocene at
all three localities; indeed, this proves to be the Early Cenozoic diversity
maximum in the marine realm (Piccoli et al., 1987;Dockery and
Lozouet, 2003;Crame et al., 2014;Huyghe et al., 2015). This Early
Cenozoic evolutionary radiation is perhaps best documented in the
extensive Neogastropoda clade which is known to have expanded
through the entire Cenozoic era to form one of the largest clades in
shallow seas at the present day (Crame et al., 2018, and references
therein). A latitudinal contrast of Middle Eocene neogastropods gives
totals of approximately 437 species for the US Gulf Coast, 433 for the
Paris Basin, but only 57 for Antarctica (Beu, 2009;Crame, 2019). At
first sight this might be taken as simply reflecting a strong sample bias,
with the Antarctic locality being much less well known than either of
the two tropical ones. Nevertheless, it should be pointed out that that
the Antarctic Middle Eocene gastropod fauna comprises at least 7500
individuals and of these approximately 3500 (47%) are neogastropods
(Crame, 2019). In addition, of the 57 species recorded from the La
Meseta Formation of Seymour Island, only 12 (21%) have individuals in
excess of 50 mm; small (<20 mm) and tiny (<5 mm) taxa are rea-
sonably well represented in this fauna (Crame et al., 2018, Suppl. Inf.).
The very large Imparidentia bivalve clade (formerly Heterodonta),
which includes common, shallow-water taxa such as the Cardiidae,
Tellinidae, Mactridae and Veneridae, also shows a very strong Middle
Eocene diversity contrast: US Gulf Coast – 158 species; Paris Basin –
273; Antarctica – 25 (Beu, 2009;Crame, 2019).
It should be emphasised that in making these large-scale diversity
comparisons it was not possible to use rarefaction or related techniques;
for many of the tropical faunas accurate counts of numbers of in-
dividuals are unavailable. The US Gulf Coast locality is contained es-
sentially within a central eastern Texas – Alabama region, but in the
Middle Eocene there is a significant eastwards extension to include the
upper Santee Limestone of South Carolina. Further details on the
Paleocene, Early Eocene and Middle Eocene Gulf Coast localities, in-
cluding estimates of the stratigraphic thicknesses of the units studied
are contained in the Appendix to Crame et al. (2018) and Crame
(2019). All of the various sites investigated have been comprehensively
sampled, but of course this does not necessarily equate to complete
sample standardisation.
Another prominent feature of the Early Cenozoic evolution of the
Neogastropoda is the rapid increase in the proportion of taxa that can
be assigned to modern genera. Whereas only 7% of the Maastrichtian
species on the US Gulf Coast fall into this category, 44% of the Middle
Eocene ones do; in Antarctica there are no modern Maastrichtian
genera but the figure rises to 37% in the Middle Eocene (Crame et al.,
2018). In both the tropics and the pole the pronounced evolutionary
radiation is accompanied by a rapid rise of the modern neogastropod
fauna.
As well as these direct latitudinal contrasts it is important to em-
phasise just how diverse the tropical Middle Eocene fauna of the Paris
Basin as a whole is. From the Lutetian (i.e. early Middle Eocene)
Calcaire Grossier Formation alone some 1550 species of gastropods and
540 species of bivalves have been recorded, and at one single outcrop at
Falunière (Grignon, Yvalines) >800 species of molluscs have been
collected from just one 13 m section (Cossmann and Pissarro, 1904–13;
Pacaud and Le Renard, 1995;Gély, 2008;Merle, 2008;Huyghe et al.,
2012). There is no obvious preservational bias between the Early,
Middle and Late Eocene, and the diversity hotspot actually coincides
with an interval of slight global cooling between Early and Middle
Eocene climatic optima (Huyghe et al., 2012, 2015). This huge phase of
Early Cenozoic diversification, which is also recorded in other Paris
Basin taxa such as corals, brachiopods, decapod crustaceans and
benthic foraminifera, took place on a series of very shallow-water
carbonate platforms and banks, and laid the foundations for the modern
hyper-diverse tropical molluscan fauna (Vermeij, 2001;Kafanov, 2001;
Briggs, 2006;Harzhauser et al., 2002, 2008).
Similarly, the Bolca Lagerstätten (BL) of northern Italy has yielded a
spectacular ichthyofauna of some 250+ species contained within ap-
proximately 90 families and 17 orders (Bellwood, 1996;Bellwood and
Wainwright, 2006;Carnevale and Pietsch, 2009;Carnevale et al., 2014;
Friedman and Carnevale, 2018;Marramà et al., 2018). Dated by cal-
careous nannoplankton as between 50.5 and 48.96 Ma in age, i.e. late
Early Eocene (Ypresian) (Friedman and Carnevale, 2018), it reveals a
major radiation of acanthomorph (i.e. spiny-rayed) teleosts in general,
and various percomorph families in particular. The latter comprises a
suite of grazers and herbivores, many of which bear a striking resem-
blance to modern coral reef taxa (Bellwood and Wainwright, 2006;
Friedman and Carnevale, 2018). The taxonomic richness shown by the
BL is higher than that of other Ypresian Lagerstätten (Friedman et al.,
2016), and can also be linked to the initial development of modern
coral reef assemblages (Bellwood, 1996;Friedman and Carnevale,
2018). The BL accumulated in a coastal area periodically affected by
anoxia, probably a protected lagoonal system in close proximity to both
coral reefs and seagrass beds (Carnevale and Pietsch, 2009;Carnevale
et al., 2014).
Like the Calcaire Grossier Formation of the Paris Basin, the BL is
also thought to have been associated with an extensive archipelago in
the western Tethyan circum-tropical ocean. Although it is slightly older
than the prolific faunas of the Calcaire Grossier Formation (late Early
Eocene as opposed to early Middle Eocene), both would seem to have
J.A. Crame Earth-Science Reviews 202 (2020) 103090
2
been part of a distinct biodiversity hotspot that may have been com-
parable in scale to the modern Atlantic – Caribbean – East Pacific
(ACEP) and Indo-West Pacific (IWP) ones (Merle, 2008;Huyghe et al.,
2012;Renema et al., 2008;Friedman and Carnevale, 2018). However, it
has to be stressed that the boundaries of this western Tethyan hotspot
remain poorly defined. What we do know is that the Paleocene – Middle
Eocene tropical belt, in both the marine and terrestrial realms, was
some 40–50% larger than the present day, extending, at least inter-
mittently, to palaeolatitudes of 55°- 65° N and S, and occasionally even
higher (Wolfe, 1985;Adams et al., 1990;Greenwood and Wing, 1995;
Collinson, 2000;Morley, 2007;Pross et al., 2012).
The strong high – low latitude diversity contrast seen in Early
Cenozoic molluscan faunas is very probably also present in the ich-
thyofaunas. In this particular instance the comparisons are not between
precisely contemporaneous units as the BL fauna is late Ypresian in age
and the most prolific Antarctic one is slightly younger at un-
differentiated Middle Eocene age (Crame et al., 2014;Douglas et al.,
2014;Amenábar et al., 2019). The latter comes from the lithostrati-
graphic unit Telm 4 of the La Meseta Formation, Seymour Island which
is essentially a condensed shell bed from which some 10,000 specimens
of fish teeth, vertebrae, bone fragments, spines and otoliths have been
recovered by a combination of surface collecting and dry-sieving
(Reguero, 2019;Regeuro et al., 2002;Reguero et al., 2012). Such an
abundant assemblage is of surprisingly low taxonomic diversity, with
only approximately 35 species from 23 families being recorded. And of
these some 71% are chondrichthyans, with sharks in particular being
very well represented (Reguero et al., 2012). At least 21 species of shark
have been identified and it is clear that taxa from many different types
of habitat converged on this one locality (Long, 1992;Kriwet, 2005). In
marked contrast, the BL chondrichthyans comprise only 7% of the total
ichthyofauna (Marramà et al., 2018). The full ecological and evolu-
tionary significance of the pronounced shift in the ratio of teleosts to
chondrichthyans with latitude in the Early – Middle Eocene has yet to
be assessed.
The precise status of LDGs in the Early Cenozoic terrestrial realm is
currently uncertain. The presence of large-scale LDGs in the Eocene
floras of North America (Harrington, 2004) has been challenged by the
subsequent demonstration of mid-latitude diversity peaks in both plants
and insects (Archibald et al., 2010), and a flat-lying LDG in Early Pa-
leocene mammals (Rose et al., 2011;Mannion et al., 2014). Never-
theless, it is apparent from extensive sporomorph (i.e. spores and
pollen) assemblages from central Colombia and western Venezuela that
there was a very marked increase in equatorial diversity values between
the Early Paleocene and Middle Eocene (Jaramillo and Dilcher, 2000;
Jaramillo et al., 2006;Jardine et al., 2018). Indeed, this was such as to
generate peak Middle Eocene values in excess of those in the present-
day paratropical rainforest (Jaramillo et al., 2006). The rate of Paleo-
cene – Eocene diversification of this equatorial rainforest exceeds that
of floras on the US Gulf Coast (30°N), as well as mid-latitude floras in
both hemispheres (Jardine et al., 2018;Jaramillo and Cárdenas, 2013).
A comparison of Early – Middle Eocene sites between equatorial Co-
lombia/Venezuela and temperate southern Argentina, using both pa-
lynological and megafloral records, established 572 species from the
former but only 93 from the latter (Jaramillo and Cárdenas, 2013).
Although comprehensive LDGs are still at a premium, there is now a
distinct impression that the Early Cenozoic global radiation of both
marine and terrestrial taxa proceeded at a much higher net rate in the
tropics than at the poles. This is particularly so in three major benthic
marine groups that show very strong LDGs at the present day:
Neogastropoda, Imparidentia bivalves, and teleost fishes (Jablonski
et al., 2013;Crame et al., 2018;Rabosky et al., 2018). Each of these
taxa radiated globally in the Paleocene – Middle Eocene, but a series of
tropics – Antarctica comparisons indicate that they did so at a much
higher net rate in the former region than the latter. A very strong la-
titudinal diversity contrast had developed by the Middle Eocene
(~45 Ma), and this has continued through to the present day.
The precise stratigraphic, taxonomic and biogeographic status of a
prolific Early Paleocene molluscan fauna from the Agatdal Formation,
Nuussuaq Group, West Greenalnd (~63°N palaeolatitude) is uncertain
(Kollmann and Peel, 1983;Petersen and Vedelsby, 2000;Dam et al.,
2009;Grimsson et al., 2016). There are some indications that it is
linked to a series of Early Paleocene (i.e. Danian – Selandian) faunas of
moderately high taxonomic diversity from northern and central Europe
that comprise a genuine admixture of warm- and cool-temperate ele-
ments (Schnetler, 2001;Lauridsen and Schnetler, 2014). But what is
certain is that polewards of these Greenland – European faunas there
was a distinct Early Paleocene (Danian) Arctic/boreal fauna in the
highest northern latitudes. This can be traced from Alaska through El-
lesmere Island to Svalbard and is characterised by a sparse molluscan
fauna of temperate aspect (Crame, 2013, and references therein).
3. Structure of Early Cenozoic latitudinal diversity gradients
The Early Cenozoic interval of high – low latitude biotic differ-
entiation is constrained to an approximately 20 Myr interval between
62 and 42 Ma (i.e. late Early Paleocene to late Middle Eocene). As this
was almost exactly coincident with a period of global greenhouse
warmth (Zachos et al., 2008), the question has to be asked whether this
differentiation can be attributed to the effects of temperature alone?
Early Eocene latitudinal temperature gradients were very much shal-
lower than those of the present day, with one estimate being that there
was almost no latitudinal sea surface temperature (SST) gradient at this
time between subequatorial and subpolar regions (Bijl et al., 2009).
Even when global cooling began in the late Middle Eocene it is still
likely that latitudinal temperature gradients were less than half their
present day value, and quite possibly substantially so (Pross et al.,
2012;Douglas et al., 2014;Crame et al., 2018). Some clues as to what
else might be contributing to the latitudinal differentiation of biotas
through the Early Cenozoic have recently come to light from a detailed
comparison of the structure of high- and low-latitude marine faunas.
When we look at the latitudinal diversity contrast of the very large
Neogastropoda clade at the present day two things are immediately
apparent: firstly, there are far fewer species at the poles than in the
tropics, and secondly, those species that are present tend to be con-
centrated in just a few families (Fig. 1). In the Arctic, Buccinidae s.l.
plus Conoidea (minus Conidae and Terebridae) comprises 89% of the
fauna, and in the Antarctic the equivalent figure is 74%; however, in
comparison, the tropical fauna comprises only 32% of these families/
family groups (Crame, 2013) (Fig. 1). The two polar faunas show pat-
terns of higher dominance/lower evenness than the tropical one and
can perhaps be taken to be end-members of latitudinal gradients in
species evenness in both hemispheres. This pattern is very similar to
that established in the northern hemisphere for predatory gastropods as
a whole (i.e. Neogastropoda + littorinimorph superfamilies Naticoidea
and Tonnoidea) (Taylor and Taylor, 1977).
When relative abundance distributions (RADs) are fitted statistically
to the three faunas shown in Fig. 1, using the R ‘vegan’ package
(Oksanen et al., 2016), and the number of species occurring in each
family, they show two sharply contrasting patterns: whereas the tro-
pical fauna was best fit by the broken stick model, both the Arctic and
Antarctic were closest to a Zipf distribution (Fig. 2) (Crame et al.,
2018). The former of these distributions represents the comparatively
even apportionment of some major environmental resource, and may
perhaps be expected for a large group of species from essentially the
same trophic guild (May, 1975). But the latter has a very different
shape and reflects the much higher level of dominance in the polar
faunas (Matthews and Whittaker, 2014) (Fig. 2).
Comparisons of polar – tropical RADs were also used by Harnik
et al. (2010) in their investigation of the taxonomic structure of global
marine bivalve faunas. In this they used numbers of species within the
component genera of each fauna and found that the best fit for four out
of five climatic zones and 26 out of 27 provinces was to the Zipf and
J.A. Crame Earth-Science Reviews 202 (2020) 103090
3
Zipf-Mandelbrot (Z-M) family of distributions. The Z-M is influenced by
two component parameter estimates: gamma, which measures the
evenness of species within genera, and beta, which measures evenness
within the most diverse genera; the Zipf uses only gamma, and is
equivalent to a Z-M where beta = zero. Both polar provinces were
found to have higher gamma values than their temperate and tropical
counterparts, and thus a significantly more uneven taxonomic structure
(Harnik et al., 2010).
RADs (again using the number of species per family) have also been
used to compare the structure of the Antarctic Middle Eocene neogas-
tropod fauna with those of the two Middle Eocene tropical localities, US
Gulf Coast and Paris Basin (Crame et al., 2018). The result obtained is
almost exactly the same as that found for modern neogastropod faunas,
as the two tropical localities are best fit by a broken stick, and the
Antarctic by a Zipf (Crame et al., 2018) (Fig. 2). An Early Cenozoic
latitudinal gradient in species richness was also matched by a gradient
in species evenness; the level of high – low latitude differentiation seen
at the present day in neogastropod faunas was already established by
the Middle Eocene (i.e. ~45 Myr ago) (Fig. 2).
Even though we lack further examples of RADs being fitted to re-
gional faunas, there are strong indications that other modern polar
marine faunas are also characterised by the phenomenon of strong
dominance/low evenness; this is particularly so in the Southern Ocean.
4. The phenomenon of higher dominance/lower evenness in
modern polar biotas
An important example of high polar dominance is provided by
benthic (including bentho-pelagic) fish on the Antarctic continental
shelf and slope (Eastman, 2000). In total, some 213 species are known
from 18 different families, but, within these, three groups are particu-
larly prominent: Liparidae (snail fishes; 67 species), Zoarcidae (eelp-
outs; 23 species), and Notothenioidei (five component families; 96
species). Together, these three groups comprise 88% of the total benthic
fish fauna of Antarctica, and this figure rises to 92% in the most
southerly shelf seas (Eastman, 2000). Nevertheless, species richness on
its own fails to reflect the overwhelming dominance of notothenioids in
the Antarctic fish fauna in terms of abundance and biomass. This is
estimated to be as high as 90–95%, and it is apparent that no other
oceanic ecosystem is so dominated by a single taxonomic group of
benthic fish (Eastman, 2000;Clarke and Johnston, 1996;Briggs, 2003).
Unfortunately, the fossil record of notothenioids is extremely poor.
A partial dorsal cranium from the La Meseta Formation of Seymour
Island has been assigned to the modern non-Antarctic notothenioid
family Eleginopidae, and if this determination is correct then the stem
group of the modern Antarctic clade could be as old as 45 Ma (i.e.
Middle Eocene judging from the position of the locality on the revised
geological map of Seymour Island) (Eastman and Grande, 1991;Near,
Fig. 1. Regional comparison of present day neogastropod faunas between the
Arctic, Tropics and Antarctic. The histograms represent the number of species
within 18 common neogastropod families. The Arctic fauna is a compilation of
all shelf-depth taxa occurring north of 60°N, and the Antarctic of all shelf and
bathyal taxa south of the Polar Front. The Tropics fauna is an average of six
faunas: two from the Americas and four from the Indo-West Pacific province.
Reproduced with slight modifications from Crame, 2013, (Fig. 1), where further
details on the construction of the three faunas are given. Neogastropod family
classification based on Bouchet and Rocroi (2005) and Bouchet et al. (2011).
Fig. 2. Relative abundance distributions to show the contrast between present-
day polar and tropical neogastropod faunas. Relative abundance distributions
(RADs) are used to examine the structure of biotic assemblages by plotting %
relative abundance for each taxon (log scale, y axis) against its rank within the
assemblage (x axis). They can be constructed using either the number of in-
dividuals per species, or, as in this particular instance, the number of species
within a higher taxon such as a family. They are based on the principle that the
abundance of a particular taxon reflects the size of its realised niche, which in
turn is shaped by ecological interactions within a community or assemblage
(Magurran, 2004). Sometimes referred to as dominance – diversity plots, they
range in form from sub-vertical curves at one extreme (strong dominance) to
sub-horizontal, sigmoidal curves at the other (strong evenness). The polar fauna
(from Antarctica) fits closest to the former category and a Zipf distribution, but
the tropical one is closer to the latter and a broken stick model. Redrawn from
Crame et al., 2018, (Fig. 3) where further information on the composition of the
respective faunas and the methods of model fitting are contained. As the two
polar faunas show very similar Zipf distributions they have been amalgamated
here into just one curve. It should be noted that the polar – tropical contrast
seen at the present day is almost exactly repeated by a similar comparison of
Middle Eocene faunas of approximately 45 Ma age.
J.A. Crame Earth-Science Reviews 202 (2020) 103090
4
2004;Eastman, 2005). There is even some phylogenetic evidence to
suggest that it could be considerably older than this (Near, 2004).
Within the marine invertebrates the dominant group on the
Antarctic shelf is the peracarid crustaceans, comprising some 1350
species that are very largely assigned to either the Amphipoda or
Isopoda (Arntz et al., 1997;Clarke and Johnston, 2003;Dayton, 1990;
De Broyer et al., 2003;Brandt et al., 2007a). Two families, Iphime-
diidae and Epimeriidae, predominate within the approximately 470
amphipod shelf species (Lörz and Held, 2004), and consist of a series of
predators, scavengers and necrophagous taxa on largely sedentary
sponges, cnidarians, bryozoans and holothurians (De Broyer et al.,
2003;De Broyer and Jazdzewski, 1996). Continental shelf isopods in
turn constitute approximately 371 species, with 52% of them being
assigned to just four families: Munnopsididae, Paramunnidae, Serolidae
and Arcturidae (Dayton, 1990;Brandt et al., 2007a). As with the pro-
minent amphipods, our knowledge of the ecology of these families is
limited, but whereas the Arcturidae are thought to be mainly passive
filter feeders, the Serolidae are known to be both active predators and
scavengers (Brandt et al., 2007a, 2007b).
Although there is no Antarctic fossil record for the peracarid
Crustacea, a preliminary phylogenetic analysis links the South
American shelf-depth genera Cristaserolis and Leptoserolis with the
Australian genus Serolina (Brandt, 1991, 1992). It is suggested that
these taxa were only separated at the time of opening of the Tasman
Gateway some 30 Myr ago (Scher et al., 2015), and before this there
was a distinctive Eocene serolid isopod fauna around the shallow-water
southern Gondwana margins (Brandt, 1991, 1992).
5. Significance of high dominance/low evenness in polar biotas
There is a general impression that, as high-latitude and polar or-
ganisms have to contend with more extreme and widely fluctuating
environmental conditions, their constituent species have broader tol-
erances and less specific microhabitat requirements; selection for gen-
eralism and vagility would form an effective barrier to extinction
(Chown and Gaston, 2000;Dynesius and Jansson, 2000). When di-
versity-dependent resources (i.e. those that can potentially be used up)
are considered in the marine realm it is apparent that attenuation of
trophic resources may be paramount, and in particular that caused by
the extreme seasonality of primary production at the base of the food
chain (Valentine, 1973, 1983;Clarke, 1988, 1990;Arntz et al., 1994;
Valentine et al., 2008). It has been estimated that there is over an order
of magnitude variability in primary production between the relatively
stable tropics and fluctuating polar regions (Valentine and Jablonski,
2015;Krug et al., 2009), and within the latter there will be selection for
organisms that can either sustain long periods of starvation, or live on
material other than primary production (Valentine, 1983).
Many of the dominant benthic marine taxa in both polar regions are
clearly trophic generalists (Dayton, 1990;Valentine, 1983;Valentine
et al., 2008;Pearse, 1965;Arnaud, 1977). This is particularly so in the
Antarctic where examples of taxa known to have very broad-based diets
include the common buccinid gastropod, Neobuccinum eatoni, the star-
fish Diplasterias brucei, various lysaniassid amphipods, Parbolasia cor-
rugatus (common nemertean), at least four species of holothurians, and
three ophiuroids (Arntz et al., 1994;Pearse, 1965;Arnaud, 1970, 1977;
White, 1984;McClintock, 1994). Studies in both Adélie Land and
McMurdo Sound have shown that certain asteroids, echinoids, pycno-
gonids, isopods and amphipods are only necrophagous during the
austral winter when food supplies are particularly low (Arnaud, 1977).
Some benthic and bentho-pelagic notothenioid fish have been recorded
as feeding on up to 16 different types of prey (Eastman, 2000;Brandt,
2000). In marked contrast, many tropical marine invertebrate species
have become specialised on a much narrower range of diversity-de-
pendent resources without the risk of extinction, and thus far more of
them can be packed into any given area (Taylor et al., 1980;Kohn,
1997;Krug et al., 2009).
Latitudinal gradients in the species richness of predatory gastropods
have already been linked to the stability of the production cycle in the
eastern and western Atlantic, and eastern Pacific (Taylor and Taylor,
1977;Taylor et al., 1980;Taylor, 1981;Valentine et al., 2002). Broader
feeding types, and in particular members of the Buccinidae, char-
acterise the highest latitudes, and in the tropics neogastropod families
such as the Muricidae, Mitridae, Conidae and Terebridae have much
more restricted diets and frequently specialise on single prey items. The
prominence of certain conoidean families, such as the Mangeliidae, in
Arctic/sub-Arctic regions is linked to a preference for predation on
polychaetes. These are thought to be predominantly deposit feeders and
thus a predictable food resource not greatly influenced by seasonal
fluctuations in the way that many suspension feeders would be (Taylor
and Taylor, 1977;Taylor, 1981).
6. The link between dominance, seasonality, and the diversity of
polar marine faunas
Production of diatoms and other phytoplankton at the base of the
polar marine food chain is concentrated within a dense but brief
summer bloom that is matched by an approximately six-fold increase in
herbivorous, carnivorous and omnivorous zooplankton species (Clarke,
1988). As well as its effect on the dietary breadth of predatory taxa, a
short summer season of primary production is also very probably the
reason why many globally common families of suspension-feeding bi-
valves are either poorly represented, or completely absent, from both
polar regions (Nicol, 1967;Dell, 1972;Valentine et al., 2008). Unless
such bivalves have evolved the capacity to lie dormant for long periods,
or utilise an alternative food resource, they would simply not be able to
survive in the polar regions (Arntz et al., 1994, 1997).
When traced from south to north in the North Atlantic Ocean, both
benthic and pelagic groups show a significant fall in diversity at ap-
proximately 40°N (Taylor and Taylor, 1977;Taylor et al., 1980;Angel,
1997). Whereas at latitudes <40°N warm surface waters contain low
concentrations of nutrients and the phytoplankton production cycle is
only weakly seasonal, at latitudes >40°N winter cooling of surface
waters results in convective overturning, mixing, and resupply of nu-
trients back into surface waters (Angel, 1997). At 40° - 60°N there is a
bimodal phytoplankton bloom (i.e. spring and autumn), and at >60°N
there is a single summertime bloom. These latitudinal changes in the
production cycle are thought to have a profound influence on both
pelagic and benthic diversity values (Angel, 1997), and as the 40° dip in
diversity is clearly marked at the family level (Taylor and Taylor,
1977), they may have done so over a considerable period of time.
The concentration of generalist and opportunist taxa in the polar
regions leads us to consider whether polar – tropical diversity contrasts
could be attributable, at least in part, to a latitudinal gradient in niche
width or overlap? This is especially so in terms of the trophic niche
where there is strong circumstantial evidence to indicate that, for es-
sentially predatory groups such as the Neogastropoda, diets are much
broader in the polar regions than the tropics. Such a concept is indeed
appealing but it has to be emphasised that it has not yet been subjected
to any rigorous form of testing. A rare attempt to do this was based very
largely in the terrestrial realm, but could not find a positive relation
between latitude and either niche breadth or the number/proportion of
specialist taxa (Vázquez and Stevens, 2004). In the past, niche theory
has focused primarily on the individual niche and the phenomenon of
resource partitioning between potentially overlapping species. Never-
theless, this is only part of the story and we also need to consider the
concept of the population niche, which centres on how populations of
species are distributed within specific regions (Ricklefs, 2010). The
population niche is influenced by a series of regional gradients, such as
temperature, that cannot be partitioned directly by different species
within a habitat. A mosaic of shifting patterns in the population niche
may allow species within a clade to coexist within otherwise similar
niche space (Ricklefs, 2010). Our concept of niche width is clearly
J.A. Crame Earth-Science Reviews 202 (2020) 103090
5
changing, and there would seem to be considerable scope to reassess its
applicability in the marine realm using taxa such as the Neogastropoda.
It remains as a potentially key, but largely unproven, mechanism for
generating polar – tropical diversity contrasts.
7. Synthesis: evolution of Early Cenozoic LDGs
A synopsis of how very strong latitudinal contrasts in marine
benthic diversity may have evolved through the Cenozoic is presented
in Fig. 3. In stage 1, 66 - ~62 Ma, there is very little direct evidence as
to how steep LDGs may have been, but it is suggested that the recovery
took place from a relatively flat, low diversity feature with weaker la-
titudinal contrasts. It is stage 2, ~62–42 Ma, where significant diversity
differences between the tropics and the poles were re-established and
steep LDGs produced (Fig. 3). This is where, at least in Antarctica, the
modern polar fauna first becomes recognisable, but there is evidence to
suggest that some of the key component clades radiated at a much
slower rate than tropical counterparts; this is particularly so of very
large cosmopolitan clades such as the Neogastropoda, Imparidentia
bivalves and teleost fishes. On reflection, it may well be that the evo-
lution of the modern LDG through the Early Cenozoic was due not so
much to an acceleration of net evolutionary rates in the tropics as to
their retardation in the high-latitude and polar regions. This in turn is
linked to the marked seasonality of primary production which is es-
sentially a time-invariant feature of both greenhouse and icehouse
worlds. Seasonality leads to a preponderance of generalist taxa in the
high-latitude and polar regions, and simply far fewer of these can be
accommodated than in the low-latitude and tropical regions.
Although steep LDGs evolved in the interval ~62–42 Ma, their
overall form was somewhat different from that of today (Fig. 3). This
was the acme of the greenhouse world and we know that the tropics
reached into latitudes of 50°+, and occasionally even higher. There-
fore, the overall profile of the LDG in both hemispheres is more likely to
have been that of a broad dome rather than the bell-shaped curve with
narrow peak of the present day (Fig. 3). The latter feature (stage 3) is
seen as at least a partial retraction feature in response to the onset of
global cooling at 34 Ma, but diversity is still expanding at a significantly
higher rate in the tropics than in the high-latitude and polar regions.
All the indications are that in the critical greenhouse interval,
~62–42 Ma, evolutionary radiations were at a significantly higher net
rate in the tropics than in the high-latitude and polar regions, and this is
the fundamental process driving the evolution of the LDG through the
Early Cenozoic (Jablonski et al., 2006;Mittelbach et al., 2007;Krug
et al., 2009;Gillman and Wright, 2014). However, it should be em-
phasised that such a process is not necessarily detrimental to the long-
term stability of polar biotas. There is in fact strong theoretical evidence
to suggest that broad-niched polar species will have saturated all the
available ecological space and are thus inherently resistant to invasion.
There is very probably a high proportion of stable, incumbent taxa in
the polar marine realm (Turner et al., 1996;Valentine et al., 2008).
The importance of temperature in playing at least a partial role in
the Early Cenozoic evolution of LDGs should not be overlooked.
Temperature can clearly influence the rate at which energy is trans-
ferred through the ecosystem, and some form of Metabloic Theory of
Biodiveresity, where an increase in temperature speeds up biochemical
kinetics and rates of molecular evolution, may yet be shown to have
widespread applicability (Brown, 2014;Clarke, 2017). In addition, it is
readily apparent that latitudinal range shifts driven by climate change
are a persistent feature through time and some of these clearly have the
ability to mould large-scale patterns (Jablonski et al., 2006;Condamine
et al., 2012;Huang et al., 2014). The concept of tropical niche con-
servatism, where modern taxonomic groups originated in the extensive
Early Cenozoic tropics but subsequently had little or no success in co-
lonising the high-latitude and polar regions, may have significantly
enhanced existing LDGs over the last 34 Myr (Hawkins et al., 2006,
2007;Buckley et al., 2010;Jansson et al., 2013). Furthermore, in the
Fig. 3. Evolution of latitudinal diversity contrasts through the
Cenozoic era. Stage 1 represents the immediate aftermath of
the K/Pg mass extinction event when global faunas were still
in a recovery phase. In all probability the LDG was greatly
reduced at this time. Stage 2 represents the Early Cenozoic
greenhouse world when latitudinal temperature gradients
were much shallower than at the present day. However, la-
titudinal diversity gradients were present in the mid- to high-
latitudes and the overall form of the high – low latitude di-
versity contrast was that of a broad, low dome. Stage 3 is set
in the Late Cenozoic after the onset of global cooling at the
Eocene/Oligocene boundary. The high – low diversity con-
trast now has the more familiar modern profile of a bell-
shaped curve with a much narrower peak. It is envisaged that
this is achieved by both the intensification of seasonality in
the high-latitude and polar regions, and range retraction into
lower latitudes. Net rate of species increase (i.e. speciation
minus extinction) is significantly higher in the tropics than at
the poles throughout the Cenozoic era.
Key: N – northern polar regions; S – southern polar regions; Eq
– Equator.
J.A. Crame Earth-Science Reviews 202 (2020) 103090
6
very highest levels of the Seymour Island sedimentary section (informal
mapping units Telm 6 & 7, also known as the Submeseta Formation) a
very marked reduction in taxonomic diversity has been linked to the
onset of major global cooling close to the E/O boundary (Ivany et al.,
2008). Durophagous (i.e. shell-breaking) predators such as crabs,
sharks and most teleost fish are almost completely absent from this
interval and it is thought that this in turn led to the proliferation of
dense, epifaunal, suspension feeding echinoderm communities domi-
nated by ophiuroids and crinoids (Aronson and Blake, 2001;Aronson
et al., 2007).
Nevertheless, the correspondence between temperature and taxo-
nomic diversity change through the studied Early Cenozoic sections is
not exact. At least in the marine realm, it is apparent that the really
steep diversity increase occurs between the Early and Middle Eocene,
just when global temperatures begin to level off and then gradually
decline (Zachos et al., 2008). This may represent some sort of time-lag
effect in the diversification process, or perhaps the intensity of the
Middle Eocene Climatic Optimum at ~40 Ma has been underestimated
(Crame et al., 2018)? And on a grander timescale it is very unlikely that
the long-term decline of global temperatures from the late Middle Eo-
cene onwards (Zachos et al., 2008) is matched by a parallel decline in
global biodiversity. In the marine realm, there is compelling evidence of
major later Cenozoic evolutionary radiations, including those in the
very large groups such as the Neogastropoda, Imparidentia bivalves and
teleost fishes (Briggs, 2003;Stanley, 2007;Norris et al., 2013;Bush and
Bambach, 2015). Even in the Late Cenozoic, which has been regarded
traditionally as a period of low temperatures, ice sheet extension, and
extinction, it is clear that there was a pronounced phase of polar ra-
diations linked to a major expansion of diatom-based ecosystems (at ~
14 Ma) (Crampton et al., 2016;Crame, 2018). The full effect of these
radiations in the benthic realm has yet to be established, but in the
pelagic realm it has clearly led to the development of low diversity –
high abundance assemblages showing strong dominance at each trophic
level (Ducklow et al., 2007;Murphy et al., 2016). In all probability this
is another area where marine taxonomic diversity levels are dictated
more by food supply than temperature. The widespread assumption
that temperature has been the primary driver of the LDG through deep
time (Brown, 2014;Mannion et al., 2014;Worm and Tittensor, 2018)
now needs to be critically re-examined.
We should also consider the effects of area on the evolution of LDGs,
as the large extent of the Early Cenozoic tropics could have promoted
both speciation and reduced extinction relative to smaller biomes
(Rosenzweig, 1995). In a large-scale study of tree species diversity, Fine
and Ree (2006) could find no correlation between the estimated area of
the modern tropical forest biome and tree species richness. However,
there was a good correlation with the expanded area of the Eocene
tropics and this has led to the development of a time-integrated, species
– area concept to explain high tropical diversity (Fine and Ree, 2006;
Fine, 2015). Within the marine realm the later increase in Cenozoic
diversity levels was undoubtedly influenced by the proliferation of coral
reefs (Bellwood and Wainwright, 2006;Harzhauser et al., 2008;
Kiessling et al., 2010;Norris et al., 2013), but this may be due as much
to an increase in three-dimensional habitat complexity as to two-di-
mensional surface area.
8. Conclusions
•A huge global pulse of biological diversification in the wake of the
K/Pg mass extinction event was concentrated in the low-latitude
and tropical regions. This in turn led to the development of steep
LDGs well before the onset of global cooling at 34 Ma.
•We are beginning to appreciate that, at least in the marine realm,
high-latitude and polar regions are characterised not only by low
taxonomic diversity but also by high dominance/low evenness. The
taxonomic structure of polar communities is fundamentally different
to that of tropical ones.
•The phenomenon of high dominance in polar communities is linked
to the marked seasonality of primary productivity at the base of the
food chain. This leads to available ecospace being dominated by
comparatively few broad-niched generalists.
•The form of the Early Cenozoic LDG was very different to that of
today. The tropical zone was much broader and the steep drop-off in
species numbers occurred at a higher latitude.
•Both elevated temperatures and extended area could have promoted
diversification in the Early Cenozoic tropics. But it is likely that the
evolution of steep LDGs was also significantly enhanced by the re-
tardation of net evolutionary rates in the high-latitude and polar
regions. The seasonality of primary productivity is a time-invariant
feature that would have affected both greenhouse and icehouse
worlds.
Declaration of Competing Interest
The author declares that he has no known competing financial in-
terests or personal relationships that could have appeared to influence
the work reported in this paper.
Acknowledgements
The pioneering studies of both J.D. Taylor and J.W. Valentine into
the possible links between primary productivity and LDGs have greatly
influenced my thinking, as did the fundamental insights into the sea-
sonality of primary productivity by my BAS colleague, A. Clarke. I am
grateful to all of them for showing me a potential way forward with
their thought-provoking studies. Many BAS, UK, and international
collaborators have contributed to the establishment of the Early
Cenozoic biostratigraphy and palaeontology of Seymour Island; the
work of W.J. Zinsmeister and his associates has been particularly im-
portant in this respect. Financial support from the British Antarctic
Survey, Natural Environment Research Council, and NE/I005803/1 is
gratefully acknowledged. I would also like to thank two reviewers and
A. Negri for their helpful comments on the manuscript.
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