Birds of paradise, biogeography and ecology in New Guinea: a review
Birds of paradise, biogeography and ecology in New Guinea: a review
Birds of paradise, biogeography and ecology in New Guinea: a review
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894 M. Heads<br />
Aga<strong>in</strong>, this `discrepancy' or `paradox' has been expla<strong>in</strong>ed<br />
as result<strong>in</strong>g from the different means <strong>of</strong> dispersal (Mayr,<br />
1953), but it seems more likely to be simply because <strong>of</strong><br />
different groups hav<strong>in</strong>g different evolutionary centres;<br />
angiosperms <strong>and</strong> <strong>in</strong>sects both have major centres <strong>in</strong> the<br />
Indian Ocean <strong>and</strong> Paci®c Ocean regions, whereas passer<strong>in</strong>es<br />
<strong>and</strong> mammals have major centres around the Indian <strong>and</strong><br />
Atlantic Oceans.<br />
Figure 1 Distribution <strong>of</strong> Paradisaeidae, show<strong>in</strong>g areas with ³ 10<br />
species (stippled) <strong>and</strong> ³ 20 species (black) per 1° ´1° grid cell.<br />
<strong>ecology</strong> <strong>in</strong> <strong>New</strong> Gu<strong>in</strong>ea. Some ma<strong>in</strong> aspects <strong>of</strong> distribution <strong>in</strong><br />
the birds <strong>of</strong> <strong>paradise</strong> are discussed ®rst.<br />
BIOGEOGRAPHY<br />
The major species concentrations <strong>in</strong> <strong>New</strong> Gu<strong>in</strong>ea <strong>of</strong> such<br />
dist<strong>in</strong>ctive bird families as birds <strong>of</strong> <strong>paradise</strong>, bowerbirds<br />
(Ptilonorhynchidae) <strong>and</strong> cassowaries (Casuariidae) renders<br />
the absence there <strong>of</strong> major, widespread groups such as<br />
trogons (Trogoniformes) <strong>and</strong> woodpeckers (Piciformes)<br />
`almost mysterious' (Gilliard, 1969) <strong>and</strong> certa<strong>in</strong>ly worth<br />
<strong>in</strong>vestigat<strong>in</strong>g. This presence <strong>and</strong> absence are sometimes<br />
attributed to dispersal <strong>in</strong>to <strong>New</strong> Gu<strong>in</strong>ea, or lack <strong>of</strong> it,<br />
because <strong>of</strong> different means <strong>of</strong> dispersal <strong>in</strong> the respective taxa.<br />
However, employ<strong>in</strong>g the usual concept <strong>of</strong> dispersal does<br />
leave the patterns rather enigmatic. Instead, it is suggested<br />
that these patterns <strong>of</strong> replacement are not caused by<br />
`dispersal' as physical movement, but are the result <strong>of</strong><br />
vicariant evolution mediated by tectonic processes on prior<br />
l<strong>and</strong>scapes.<br />
Different groups <strong>in</strong> <strong>New</strong> Gu<strong>in</strong>ea show af®nities with<br />
different parts <strong>of</strong> the world. For example, plants <strong>and</strong> <strong>in</strong>sects<br />
there show many connections with Indo-Malaysia <strong>and</strong> there<br />
are also many trans-tropical-Paci®c groups, whereas the<br />
passer<strong>in</strong>es <strong>and</strong> mammals show strong Australian connections.<br />
(There are few trans-Paci®c ties <strong>in</strong> these groups ± the<br />
<strong>New</strong> Zeal<strong>and</strong> bat family Mystac<strong>in</strong>idae <strong>and</strong> South American<br />
taxa, possible af®nities <strong>in</strong> marsupials, <strong>and</strong> possible af®nities<br />
between the passer<strong>in</strong>es Acanthisittidae <strong>of</strong> <strong>New</strong> Zeal<strong>and</strong> <strong>and</strong><br />
subosc<strong>in</strong>es <strong>in</strong> South America ± <strong>and</strong> these are <strong>in</strong> the far<br />
south).<br />
The <strong>New</strong> Gu<strong>in</strong>ea orogen<br />
The birds <strong>of</strong> <strong>paradise</strong> are distributed rather evenly throughout<br />
the folded <strong>and</strong> faulted mounta<strong>in</strong> ranges <strong>of</strong> the sp<strong>in</strong>e <strong>of</strong><br />
<strong>New</strong> Gu<strong>in</strong>ea ± the <strong>New</strong> Gu<strong>in</strong>ea orogen (Figs 2, 4 & 29).<br />
This mounta<strong>in</strong>ous belt was formerly regarded as the result <strong>of</strong><br />
a simple cont<strong>in</strong>ent±isl<strong>and</strong> arc collision, but Pigram & Davies<br />
(1987) gave a radical re-<strong>in</strong>terpretation. They described the<br />
orogen as consist<strong>in</strong>g <strong>of</strong> a southern part (the Australian<br />
craton), <strong>and</strong> a northern part made up <strong>of</strong> at least thirty-two<br />
tectonostratigraphic terranes ± fault-bounded geological<br />
prov<strong>in</strong>ces with <strong>in</strong>dependent histories from other terranes.<br />
The <strong>New</strong> Gu<strong>in</strong>ea terranes, <strong>in</strong>clud<strong>in</strong>g <strong>in</strong>trusive <strong>and</strong> metamorphic<br />
rocks, formed <strong>and</strong> sometimes amalgamated with<br />
others some distance from their present position <strong>and</strong><br />
subsequently accreted to the craton marg<strong>in</strong>. In the Vogelkop<br />
accretion history <strong>in</strong>volves ma<strong>in</strong>ly cont<strong>in</strong>ental terranes. The<br />
central Kemum terrane was detached from Gondwana by<br />
the early Cretaceous <strong>and</strong> then had a history <strong>of</strong> movement<br />
<strong>in</strong>dependent <strong>of</strong> the Australian craton until the Miocene. In<br />
central <strong>New</strong> Gu<strong>in</strong>ea, the Sepik <strong>and</strong> Rouffaer terranes had<br />
docked with the craton by the Late Oligocene, when the<br />
<strong>New</strong> Gu<strong>in</strong>ea orogeny was <strong>in</strong>itiated. In eastern Papua <strong>New</strong><br />
Gu<strong>in</strong>ea (PNG) several terranes <strong>of</strong> diverse orig<strong>in</strong> amalgamated<br />
<strong>in</strong> the Palaeogene (Early Eocene if this caused the<br />
metamorphism <strong>of</strong> the proto-Owen Stanley terrane), <strong>and</strong> this<br />
composite terrane then docked with the Australian craton <strong>in</strong><br />
the Miocene. F<strong>in</strong>ally the F<strong>in</strong>isterre terrane was accreted to<br />
the ma<strong>in</strong>l<strong>and</strong> at 3.0±3.7 Ma (Abbott et al., 1994), <strong>and</strong> rapid<br />
uplift cont<strong>in</strong>ues there. Probably <strong>New</strong> Brita<strong>in</strong> will dock next.<br />
Pigram & Davies (1987) discussed transcurrent movement<br />
Figure 2 Geological map show<strong>in</strong>g the Australian craton (grey), the<br />
<strong>New</strong> Gu<strong>in</strong>ea orogen (between the heavy broken l<strong>in</strong>es), <strong>and</strong> the<br />
accreted <strong>New</strong> Gu<strong>in</strong>ea terranes (black). Blank areas on the map are<br />
successor bas<strong>in</strong>s (simpli®ed from Pigram & Davies, 1987).<br />
Ó Blackwell Science Ltd 2001, Journal <strong>of</strong> Biogeography, 28, 893±925