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Late-surviving megafauna in Tasmania, Australia, implicate human involvement in their extinction

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Establishing the cause of past extinctions is critical if we are to understand better what might trigger future occurrences and how to prevent them. The mechanisms of continental late Pleistocene megafaunal extinction, however, are still fiercely contested. Potential factors contributing to their demise include climatic change, human impact, or some combination. On the Australian mainland, 90% of the megafauna became extinct by ≈46 thousand years (ka) ago, soon after the first archaeological evidence for human colonization of the continent. Yet, on the neighboring island of Tasmania (which was connected to the mainland when sea levels were lower), megafaunal extinction appears to have taken place before the initial human arrival between 43 and 40 ka, which would seem to exonerate people as a contributing factor in the extirpation of the island megafauna. Age estimates for the last megafauna, however, are poorly constrained. Here, we show, by direct dating of fossil remains and their associated sediments, that some Tasmanian megafauna survived until at least 41 ka (i.e., after their extinction on the Australian mainland) and thus overlapped with humans. Furthermore, a vegetation record for Tasmania spanning the last 130 ka shows that no significant regional climatic or environmental change occurred between 43 and 37 ka, when a land bridge existed between Tasmania and the mainland. Our results are consistent with a model of human-induced extinction for the Tasmanian megafauna, most probably driven by hunting, and they reaffirm the value of islands adjacent to continental landmasses as tests of competing hypotheses for late Quaternary megafaunal extinctions. • Paleoclimate • Pleistocene • sea level change • island colonization • human hunting
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Late-surviving megafauna in Tasmania, Australia,
implicate human involvement in their extinction
Chris S. M. Turney
a,b,c
, Timothy F. Flannery
c,d
, Richard G. Roberts
a,c
, Craig Reid
e
, L. Keith Fifield
f
, Tom F. G. Higham
g
,
Zenobia Jacobs
a
, Noel Kemp
h
, Eric A. Colhoun
i
, Robert M. Kalin
j
, and Neil Ogle
k
aGeoQuEST Research Centre, School of Earth and Environmental Sciences, University of Wollongong, Wollongong NSW 2522, Australia; dDivision of
Environmental and Life Sciences, Macquarie University, North Ryde NSW 2109, Australia; eQueen Victoria Museum and Art Gallery, Launceston, Tasmania
7250, Australia; fResearch School of Physical Sciences and Engineering, Australian National University, Canberra ACT 0200, Australia; gOxford Radiocarbon
Accelerator Unit, Research Laboratory for Archaeology and the History of Art, University of Oxford, Oxford OX1 3QY, United Kingdom; hTasmanian
Museum and Art Gallery, Hobart, Tasmania 7001, Australia; iSchool of Environmental and Life Sciences, University of Newcastle, Newcastle NSW 2308,
Australia; jDavid Livingstone Center for Sustainability, Graham Hills Building, University of Strathclyde, Glasgow G1 1XN, Scotland; and kEnvironmental
Engineering Research Centre, School of Planning, Architecture and Civil Engineering, Queen’s University, Belfast BT9 5AG, United Kingdom
Edited by Jared M. Diamond, University of California, Los Angeles, CA, and approved June 6, 2008 (received for review February 11, 2008)
Establishing the cause of past extinctions is critical if we are to
understand better what might trigger future occurrences and how
to prevent them. The mechanisms of continental late Pleistocene
megafaunal extinction, however, are still fiercely contested. Po-
tential factors contributing to their demise include climatic change,
human impact, or some combination. On the Australian mainland,
90% of the megafauna became extinct by 46 thousand years (ka)
ago, soon after the first archaeological evidence for human colo-
nization of the continent. Yet, on the neighboring island of
Tasmania (which was connected to the mainland when sea levels
were lower), megafaunal extinction appears to have taken place
before the initial human arrival between 43 and 40 ka, which
would seem to exonerate people as a contributing factor in the
extirpation of the island megafauna. Age estimates for the last
megafauna, however, are poorly constrained. Here, we show, by
direct dating of fossil remains and their associated sediments, that
some Tasmanian megafauna survived until at least 41 ka (i.e., after
their extinction on the Australian mainland) and thus overlapped
with humans. Furthermore, a vegetation record for Tasmania
spanning the last 130 ka shows that no significant regional climatic
or environmental change occurred between 43 and 37 ka, when a
land bridge existed between Tasmania and the mainland. Our
results are consistent with a model of human-induced extinction
for the Tasmanian megafauna, most probably driven by hunting,
and they reaffirm the value of islands adjacent to continental
landmasses as tests of competing hypotheses for late Quaternary
megafaunal extinctions.
Paleoclimate Pleistocene sea level change island colonization
human hunting
Since Charles Darwin’s discover y of giant ground sloth re-
mains in South America, debate about the cause of global
late Quaternary extinctions of megafauna (animals 40 kg) has
been intense (1, 2). Potential mechanisms invoked for
megafauna demise include climatic change, human and extra-
terrestrial impacts, or some combination. In Australia, initial
human colonization of the mainland occurred by 50 ka
l
(3–5) and
has been linked to vegetation reorganization (6) and increased
burning (7) in the landscape, driving the megafauna to extinction
on the mainland by 46 ka (6, 8, 9). Some workers have argued
that most megafauna were extinct before human arrival, citing
the apparent disappearance of megafauna in Tasmania before
people reached this island as support for extinction driven by
climatic and/or environmental change (10, 11).
Currently an island of 68,300 km
2
, Tasmania lies 240 km from
the mainland across Bass Strait (Fig. 1) with a climate dominated
by cyclonic activity associated with prevailing westerly airf low.
During the Pleistocene, Tasmania was periodically connected to
mainland Australia (12), allowing faunal migrations. The island
was isolated for much of the interval 135– 43 ka and continuously
from 14 ka to the present day, with the first sustained land bridge
of the last glacial cycle occurring between 43 and 37 ka (12).
Compared with mainland occupation, human colonization was
relatively late, with the earliest radiocarbon (
14
C) ages for arrival
being obtained from rock shelters in southwest Tasmania: these
indicate a human presence before the oldest radiocarbon-dated
horizon of 34,790 510 BP at Warreen Cave (13) (Fig. 1),
equivalent to a calendar age of 40 ka (14); stone artifacts were
present in deeper deposits (13), suggesting that humans arrived
in Tasmania between 43 ka (when the land bridge first emerged)
and 40 ka.
The Tasmanian megafauna consists of seven species (six
marsupials and one monotreme), which also occurred on main-
land Australia. There is some evidence of subspecific endemism:
Tasmanian Simosthenurus occidentalis have different dental
proportions from those of the adjacent mainland (15), and
Tasmanian Thylacoleo also exhibit distinctive dental features.
The island has yielded abundant remains, with at least eight
locations in the northwest and south, producing thousands of
bones (16, 17) (see Table 1). No Tasmanian megafaunal remains
have hitherto been reliably dated. Early attempts at dating
suggested that megafauna may have survived until relatively
recently. For example, charcoal associated with megafaunal
remains in Titans Shelter (17) was radiocarbon dated to 14,310
2,970
/
2,160
BP. Subsequent direct dating of bone from this site
by using amino acid racemization (AAR) and electron spin
resonance (ESR) gave ages of 40–27 ka, suggesting that the
dated charcoal was intrusive (18). No megafaunal remains have
been found in human occupation sites (19), but only 0.6% of the
material examined dates to the first 4 ka of human occupation,
so any temporal overlap of humans and megafauna may have
been missed (20).
Results and Discussion
We undertook dating and paleontological investigations of ar-
chived fossil material from four reported megafauna sites in
Author contributions: C.S.M.T., T.F.F., and R.G.R. designed research; C.S.M.T., T.F.F., R.G.R.,
C.R., L.K.F., T.F.G.H., Z.J., N.K., E.A.C., R.M.K., and N.O. performed research; C.S.M.T., T.F.F.,
R.G.R., C.R., L.K.F., T.F.G.H., Z.J., N.K., E.A.C., R.M.K., and N.O. analyzed data; and C.S.M.T.,
T.F.F., and R.G.R. wrote the paper.
The authors declare no conflict of interest.
This article is a PNAS Direct Submission.
bTo whom correspondence should be sent at the present address:School of Geography,
Archaeology and Earth Resources, Department of Geography, University of Exeter, Exeter,
EX4 4RJ, United Kingdom. E-mail: c.turney@exeter.ac.uk.
cC.S.M.T., T.F.F., and R.G.R. contributed equally to this work.
lIn this paper, calibrated radiocarbon ages and those derived from alternative dating
methods are reported as ka (thousands of calendar years ago). Uncalibrated radiocarbon
ages are reported as BP (before present; relative to 1950 AD).
This article contains supporting information online at www.pnas.org/cgi/content/full/
0801360105/DCSupplemental.
© 2008 by The National Academy of Sciences of the USA
12150–12153
PNAS
August 26, 2008
vol. 105
no. 34 www.pnas.orgcgidoi10.1073pnas.0801360105
Tasmania [Fig. 1 and supporting information (SI) Tables S1–S3]:
Pleisto Scene Cave, Scotchtown, Titans Shelter, and Un-named
Cave. In addition, new fossil finds were investigated from Mount
Cripps (chambers CP118 and CP213). To avoid concerns about
intrusive charcoal and other associated carbon (18), we applied
14
C dating to bone collagen, by using either demineralization
followed by gelatin extraction and step-combustion (C-SC) or
gelatin isolation with ultrafiltration (C-AF) (21). The
14
C con-
tent was measured by accelerator mass spectrometry, and the
ages were calibrated following ref. 14. The fossiliferous cave
sediments were dated by optically stimulated luminescence
(OSL), which indicates the time elapsed since the sediment
grains were last exposed to sunlight (22). In sequences with
articulated megafaunal remains in primary context, OSL dating
gives the time of fossil burial; where no articulation is observed,
minimum estimates of burial age are obtained. Full
14
C and OSL
dating details are given in SI Dating Methods and Results.
The Tasmanian megafauna dated in this work provide a
record encompassing much of the late Pleistocene, from 127
to 41 ka (see Table 1 and Tables S1–S3). The deposits in Pleisto
Scene Cave contained skeletal elements of megafauna in articula-
tion and were dated by OSL to marine isotope stage (MIS) 5e or
earlier (120 and 127 ka, the infinite ages arising from dose
saturation of these samples). The Un-named Cave deposits gave an
OSL age of 103 9 ka, which is indistinguishable from the 97-ka
age obtained on the nonarticulated remains with ESR (18). Evi-
dence of articulation was also not reported for the rich megafaunal
site of Scotchtown Cave, which was interpreted as a carnivore lair
(16). Because articulated remains are not expected in such contexts,
it is not unreasonable to assume that the OSL age of 56 4ka,
obtained for sediment grains in a mixed soil– bone sample from the
original excavation, approximates that of the entombed fauna. The
samples from all of these sites had negligible collagen content and
were unsuitable for
14
C dating.
Younger ages for Tasmanian megafauna were obtained from
Titans Shelter and Mount Cripps. A Protemnodon anak specimen
was obtained from Titans Shelter and dated by
14
C (C-SC) to
39,980 610 BP, equivalent to 44 ka (Table S1). At Mount Cripps
(chamber CP213), faunal remains were discovered lying on the
chamber floor and wedged in rock crevices; their state of preser-
vation was excellent. An entire cranium was recovered and most of
Titans Shelter ,
Un-named &
Beginners Luck
caves
Mowbray,
Scotchtown & Pulbeena
Mt Cripps
Warreen
Cave
Hobart
Melbourne
Lake Selina
Main &
Pleisto Scene
caves
Launceston
Fig. 1. Locations of megafaunal, environmental, and archaeological sites in
Tasmania. Megafaunal sites are marked with solid circles, Lake Selina with a
closed triangle, and Warreen Cave with a solid square.
Table 1. Ages and faunal assemblages of principal Tasmanian megafaunal sites
Event
Age of unit(s),
ka
Megalibgwilia
sp.
Thylacoleo
sp.
Palorchestes
azael
Zygomaturus
trilobus
Protemnodon
anak
Simosthenurus
occidentalis
Metasthenurus
newtonae
Human arrival in
Tasmania
43–40
Mount Cripps,
CP213
42.9–40.9 X
Mount Cripps,
CP118
X
Titans Shelter, Site
G
44 ? X X
Mowbray Swamp 38 X
Main Cave
(MU201)
X
Pulbeena
Limeworks
54 X
Scotchtown Cave 56 4X XX X X X X
Beginner’s Luck
Cave M (JF-79)
80–63 X X
Un-named Cave
(JF-155)
103 9X XX
Pleisto Scene Cave B
(MU203–205; 206)
127 28
120 21
XXX ? X X
See Supporting Information for further details. Note that human arrival in Tasmania is contemporaneous with the most recently dated megafaunal remains
from Mount Cripps, demonstrating that there was some overlap (albeit brief) between humans and megafauna. That the megafauna had survived on Tasmania
for millions of years prior to human arrival suggests that the sudden disappearance of megafauna was caused by humans.
Turney et al. PNAS
August 26, 2008
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GEOLOGY
a second specimen. No skeletons were articulated, but associated
elements were found in close proximity. The only megafaunal
species present in the deposit was P.anak, of which the remains of
three individuals are represented: a large subadult
(QVM:2001:GFV 5, body mass estimate 60 kg) (23), a pouch
young (QVM:2001:GFV 9), and a young at foot (QVM:2000:GFV
10, body mass estimate 30 kg) (see Tables S4 and S5). OSL dating
of sediment wedged in the nasal cavity of the subadult yielded an
age of 36 3ka(Table S3 and Fig. S1), which we view as a
minimum age for the skull because the sediment grains were
emplaced postmortem. Radiocarbon dating of two individuals from
Mount Cripps, with C-SC pretreatment, produced ages of 32,780
370 BP and 30,400 270 BP, but significantly older ages of 36,200
300 BP and 37,920 340 BP were obtained from duplicate samples
by using the C-AF procedure (Table S1); the latter is thought to
yield more accurate ages for ancient bone (21). We attribute the
younger C-SC
14
C ages to the incomplete removal of low-molecular
weight contaminants from the gelatin. The C-AF
14
C ages are
therefore considered more reliable. When these ages are calibrated
and considered in conjunction with the OSL age from Mount
Cripps, they indicate that Tasmanian megafauna survived to at least
42.9–40.9 ka (at 1 SD).
The Scotchtown and Pleisto Scene Cave deposits differ in age
by 70 ka (from 56 to 127 ka) but contain essentially the
same suite of megafauna (Table S4), the only exception being
Metasthenurus newtonae, which is represented by three isolated
molars at Scotchtown (and known also from an undated context
at Mount Cripps, chamber CP118). If our assumption is correct
that the OSL age of the sediments at Scotchtown approximates
that of the faunal remains, then Tasmania experienced no
significant change in its faunal diversity between the last inter-
glacial (MIS 5e) and the succeeding glacial stages. The survival
of all seven species of Tasmanian megafauna until at least 56 ka
argues against proposals for a staggered series of climate-
induced extinctions before human arrival (10), similar to findings
on the Australian mainland (9, 20, 24, 25).
As an independent test of possible climatic and/or environ-
mental influences (including anthropogenic burning) on
megafaunal extinction (6, 10), we investigated the late Quater-
nary vegetation and charcoal records preserved in Lake Selina
(Fig. 1), which provides a crucial southern midlatitude perspec-
tive on paleoecological changes over the past 130 ka (26). The
pollen record indicates that cool temperate rainforest was
present during MIS 5e and the Holocene (MIS 1), with grass-
land, herbs, and heath vegetation dominating throughout the
intervening period (Fig. 2). There is no evidence of a significant
increase in burning at the time of human arrival or any associated
shift in vegetation. The bulk sediments exhibit a relatively
narrow range of stable carbon isotope values (
13
C), reflecting
the local C
3
vegetation, with the small f luctuations probably
representing changes in lake productivity. No major change
occurred at 41 ka.
The overall vegetation trend at Lake Selina mirrors other
regional proxies of environmental and climatic conditions (27),
including winter sea-ice cover in the Southern Ocean, as inferred
from the sea-salt sodium flux in Antarctica (28) (Fig. 2).
Elevated levels of sea-ice persisted from 65 to 17 ka, with no
significant deviation at 41 ka. Furthermore, we note that moa
extinction did not take place ‘‘downwind’’ in New Zealand at this
time (29). We consider it highly unlikely, therefore, that climatic
or environmental change could have played a significant role in
the demise of the megafauna on Tasmania.
Although our dataset is small, the results show that megafauna
persisted in Tasmania until at least 41 ka, which is similar to, or
slightly later than, the time of extinction on the Australian
mainland (48.9–43.6 ka at 1 SD) (9, 30). Importantly, the 41-ka
age postdates the establishment of a land bridge across the Bass
Strait and is statistically concordant (
2
test T3.39; 5% 3.84)
with the minimum age for the earliest evidence of humans in
Alpine/subalpine
Herbs
Other trees/
small trees/shrubs
Rainforest
Pollen %
250
500
750
1000
1250
-32
-30
-28
-26
-24
-22
δ13C, ‰ ssNa flux, µg/m2/yr
100
75
50
25
0 10 20 30 40 50 60 70 80 90 100 110 120 130
0
1 2 3 4 5a 5b 5c 5d 5e
MIS
0 10 20 30 40 50 60 70 80 90 100 110 120 130
Land bridge
Human arrival
Megafaunal ages
800
600
400
200
0
Charcoal particles/cm3
Calibrated age (ka)
Calibrated age (ka)
Fig. 2. Environmental and climatic changes in Tas-
mania and the Southern Ocean. Solid gray boxes de-
note when a land bridge was established between the
Australian mainland and Tasmania (12). For human
arrival, solid (black) arrow indicates minimum age for
earliest known occupation of Tasmania (13); open
(white) arrows delimit 1 SD age range for earliest
occupation of mainland Australia (3–5). Ages associ-
ated with megafaunal remains dated in this work are
shown as 1 SD ranges. Dashed line denotes (minimum)
overlap between most recent megafaunal remains and
earliest human arrival in Tasmania. Summary plots of
vegetation change (26), charcoal concentration (26),
and
13C of bulk sediments (this work) are from Lake
Selina. Sea-salt sodium (ssNa) flux is a measure of win-
ter sea-ice cover in the Southern Ocean, as recorded in
the EPICA ice core (28); note that the ssNa flux scale is
inverted.
12152
www.pnas.orgcgidoi10.1073pnas.0801360105 Turney et al.
Tasmania [Warreen Cave (13)]. This introduces the possibility,
hitherto discounted (10, 11), that humans caused the extinction
of the Tasmanian megafauna. Because we find no evidence for
a major change in vegetation and/or fire dynamics [in contrast to
the mainland (6, 7)] and because the megafauna had relatively
low reproductive rates, we favor the hypothesis that human
hunting led to a rapid population collapse (31). A brief coex-
istence of humans and megafauna is consistent with the absence
of megafaunal remains at human occupation sites (19). To
elucidate the precise mechanism of extinction will require im-
proved age estimates for both the first human arrivals and the
last-surviving megafauna in Tasmania.
Materials and Methods
Samples for 14C dating were obtained from museum specimens held in col-
lections at Launceston and Hobart. Fragments of bone were hand-picked, and
the collagen was extracted in two ways. At the University of Wollongong (C-SC
pretreatment), bone fragments were washed in distilled water to remove
surface contaminants, then they were broken into small pieces and decalcified
with dilute hydrochloric acid. The gelatin was isolated and step-combusted to
remove any labile contaminants. The CO2evolved at 850°C was collected,
purified, and graphitized for accelerator mass spectrometry (AMS) radiocar-
bon measurement at the Australian National University (ANU). At the Univer-
sity of Oxford (C-AF pretreatment), coarsely ground bone powder was given
a series of acid, base, and acid washes, rinsing with ultrapure water between
each reagent. Crude collagen was gelatinized, and the 30-kDa gelatin
fraction was isolated by ultrafiltration for AMS radiocarbon measurement at
Oxford (21). All 14C ages were calibrated following ref. 14. For stable isotope
analysis, samples were combusted in an elemental analyzer interfaced to a
continuous-flow isotope-ratio mass spectrometer at ANU (extracted gelatin)
and Queen’s University Belfast (Lake Selina). Bulk sediments from Lake Selina
were treated before measurement with dilute hydrochloric acid to remove
carbonates, and the CO2evolved was analyzed for isotopic abundance by gas
chromatography.
13C values are reported as per mille (‰) relative to the PDB
scale; analytical precision is 0.15 ‰ at 1 SD. Sediment samples for OSL dating
were obtained from the Launceston and Hobart museum collections, and
analyzed at the University of Wollongong. Quartz grains of 90- to 250-
m
diameter were extracted from the light-safe portion of each sample and
purified by using standard procedures, including etching with hydrofluoric
acid to remove the external
-dosed layer. The burial ages were calculated
from the equivalent dose, estimated by using a single-aliquot regenerative-
dose procedure (22), divided by the total dose rate arising from ionizing
radiation.
ACKNOWLEDGMENTS. We thank members of the Savage River Caving Club,
the Tasmanian Museum and Art Gallery, Sue Wood (Australian National
University) who ran the University of Wollongong bone samples for
13C and
C:N, and Richard Miller (University of Wollongong) who helped prepare Fig.
1. This work was supported by Royal Society Research Grant 24210 and
Australian Research Council (ARC) Grants DP0451152 and F00103154. C.S.M.T.
held an ARC Queen Elizabeth II Fellowship and R.G.R. an ARC Senior Research
Fellowship.
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... Numerically dated vertebrate fossil sites of a similar age remain poorly represented in Australia (see Peters et al., 2019). Only a few have so far yielded diverse faunas (Ayliffe et al., 2008;Price et al., 2011;Prideaux et al., 2010;Turney et al., 2008). By use of a systematic approach and collecting both large-and small-bodied taxa, Kiana Cliff has provided a diverse fauna despite the small scale of investigations so far. ...
... The range of M. newtonae, Si. maddocki, P. browneorum, Si. pales and St. andersoni also extended north along the east coast into northern NSW and southern QLD and both M. newtonae and Si. occidentalis are known from Tasmania (Prideaux, 2004;Turney et al., 2008). Only Si. pales and St. andersoni have records from the more arid inland (Prideaux, 2004). ...
... While the timing of megafaunal extinction has been established in many parts of the world, the causes and impact on the environment remain contested (Brook and Bowman, 2002;Wroe et al., 2013;Barnosky et al., 2016;Villavicencio et al., 2016). Extinction is thought to have been primarily driven by climatic shifts (including a shift in Earth's geomagnetic field) (Brook and Bowman, 2002;Wroe et al., 2013;Cooper et al., 2021;Stewart et al., 2021) or human overhunting/habitat modification (Miller et al., 2005;Turney et al., 2008;Rule et al., 2012;van der Kaars et al., 2017) or a combination of both Bradshaw et al., 2021aBradshaw et al., , 2021bDavid et al., 2021;Nürnberg et al., 2022). However, the environmental consequences which followed megafaunal extinction are still poorly understood in many parts of the world, including in Australia. ...
... However, the environmental consequences which followed megafaunal extinction are still poorly understood in many parts of the world, including in Australia. This is partly due to the paucity of animal-plant interactions in conventional pollen records and human-land transformations around the time of extinction (Miller et al., 2005;Turney et al., 2008;Johnson, 2009;Lopes dos Santos et al., 2013a;De Deckker et al., 2021). These limitations have prompted the use of other plant proxies (e.g., stable carbon isotopes) to examine vegetation response to megafaunal extinctions (Miller et al., 2005;Lopes dos Santos et al., 2013a). ...
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The timing and cause of megafaunal extinctions are an enduring focus of research interest and debate. Despite the developments in the analysis of coprophilous fungal spores (CFS), the proxy for reconstructing past megaherbivore changes, the environmental consequences of this fauna loss remain understudied. This is partly due to the general obscurity of such a signal in pollen records, as well as limitations in disentangling human and extinction ecological impact, and the lack of spatial information of megafauna changes in site-level sedimentary records. In Australia, the debate centres on the possibility that habitat loss through climate change, vegetation-fire change, human intervention, or a combination of these factors led to the extinction of some large animals during the Late Pleistocene. Pollen and plant isotope studies have also demonstrated that vegetation-fire responses following the Late Pleistocene megafaunal extinctions were characterized by increased vegetation density and fire activity due to reduced grazing/browsing pressure. Here, we use a well-dated marine sedimentary core record from the Murray Darling Basin in southern Australia and apply palynological and functional palaeoecological approaches to reconstruct the Late Pleistocene megafaunal abundance changes, the timing and potential cause of extinction across the basin and investigate if extinction was associated with any signal of trait-based vegetation changes. We infer megafaunal abundance changes from the abundance of CFS and compare this with climatic proxies from the same core. We then link modern observations of fruit, seed and fire response traits of plant genera within the basin to the fossil pollen record to reconstruct palaeo vegetation community traits and determine if extinction was associated with any changes in plant community trait composition. Closely-spaced 14C dates obtained from planktonic foraminifera and δ18O tie points place a major decline in CFS, and thus the timing of extinction, within the basin at ∼43.3 ka. While climate-driven environmental changes largely controlled megafaunal presence, human arrival and frequent landscape burning are considered the most likely primary cause of extinction or, at the very least, megafauna decline in the Murray Darling Basin. We also found that the proposed period of megafaunal decline was also accompanied and followed by a decline in the prevalence of plants with larger seeds and fruits that were likely to have been once dispersed by megaherbivores. Our study supports the idea of a human-driven megafaunal extinction in mainland Australia and that the extinction caused changes in vegetation due to reduced plant dispersal and herbivory. However, high fire activity primarily linked to these vegetation changes was not observed, as humans were already practicing landscape burning before the period of megafaunal extinction and likely continued to do so afterward.
... But the majority of phylogeographic studies of Australian taxa suggest that older climate fluctuations explain current genetic structure (Kuch et al., 2005;Oliver et al., 2010Oliver et al., , 2017, especially among marsupials (Macqueen et al., 2010;Potter et al., 2012;Rowe et al., 2008). A rich fossil record of Australian megafauna allows calibration of changes in faunal composition (Hocknull et al., 2020;Miller et al., 2005;Roberts et al., 2001;Saltré et al., 2016;Turney et al., 2008) and it has been suggested that natural climate cycling during the Pleistocene had little impact on mammal assemblages (Prideaux et al., 2007). To determine whether current patterns of genetic structure within a single species date to events that occurred more than 2 million years ago, we examined the phylogeography of the Australian brushtail possum Trichosurus vulpecula. ...
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The causes of the Late Pleistocene extinction of most larger‐bodied animals on the Australian continent have long been controversial. This is due, in no small part, to inadequate knowledge of exactly when these species were lost from different ecosystems. The Nombe rockshelter in the highlands of Papua New Guinea is one of very few sites on Sahul with as‐yet‐unrefuted evidence for the survival of megafaunal species until more recently than 40 thousand years (ka) ago. However, our understanding of the age of this site has been based on radiocarbon dating. Here we present new U–Th ages on large marsupial specimens from the deposit and identify a range of postcranial elements to species that include the diprotodontid Hulitherium tomasettii , kangaroo Protemnodon tumbuna and thylacine Thylacinus cynocephalus . Direct U–Th ages of 27–22 ka ago on faunal remains of Protemnodon tumbuna and another large unidentified macropodid are consistent with the existing radiocarbon chronology, yet are minimum ages due to the potential for post‐depositional uptake of ²³⁸ U and stratigraphic reworking. Pollen analyses indicate perhumid, montane forests dominated by Nothofagus persisted, with minimal human disturbance from at least c.26–20 ka ago up to the terminal Pleistocene. Collagen fingerprinting (ZooMS) demonstrates the potential of protein‐based identification of megafaunal remains at Nombe in the future. This study leaves open the possibility of extended coexistence between some megafaunal species in the montane rainforests of New Guinea and intermittently visiting groups of people, and underscores the need for further investigation of the Nombe deposit. Although preliminary, these findings reinforce the view that debates regarding megafaunal extinctions on Sahul require a greater appreciation of species‐specific temporalities and the degrees of human impact on diverse habitats across the continent.
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Australian and Pacific archaeological research has focused on questions of human origins, behavioral and technological variability, population distribution, the extent of human and climatic impacts on the environment, and the chronology of earliest human occupation of Sahul. These themes have preoccupied Australian archaeologists for over 40 years and while there have been significant advances in dating techniques, understanding of site formation process, and human-environment interaction, many questions remain. This chapter discusses and reviews the evidence for the timing, spread, and settlement by humans of the Australian and Pacific region during the late Pleistocene and early Holocene.
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A critical comment on 'A review of the evidence for a human role in the extinction of Australian megafauna and an alternative explanation' by S. Wroe and J. Field is presented. The authors have highlighted a range of ideas under consideration, and provided a selective interpretation which does not come to terms with biology and ignores or misinterprets current evidence. They rely heavily on the ages reported by Roberts et al. (2001) to argue for a gradual attenuation of the megafauna. They propose a staggered series of extinctions throughout the Middle and Late Pleistocene, with many taxa lost during the Penultimate Glacial Maximum (PGM) 140 130 ka, and relatively few species persisting. They ignore measurement uncertainties associated with the ages, which, when properly considered, means that 20, rather than eight of the species they list have last appearance ages consistent with ́45 ka.
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Overkill by human hunting has been consistently cited as a likely cause of the Pleistocene megafaunal extinctions in Australia, but little archaeological evidence has been found to support the notion of prehistoric Aboriginal people engaging in specialized "big game" hunting more than 40 millennia ago. Here we develop a demographic population model that considers explicitly the possibility of the selective harvest of small, immature (and presumably more vulnerable) individuals of the largest known marsupial, Diprotodon optatum. We show that remarkably low levels of exploitation of juveniles (the equivalent of one or two kills per 10 people per year) would have been sufficient to drive these large species to extinction within centuries, due to their slow life-histories. This conclusion is robust to assumptions regarding the compensatory response of the prey species and declines in the relative efficiency of hunting as the megafaunal populations declined. These findings dispel the idea that evidence of a sophisticated hunting toolkit and massive kill-sites are a necessary adjunct to "blitzkrieg". Ironically, although the extinction event was likely geochronologically instantaneous (given the coarse resolution of dating from that time), on the scale of human (and megafaunal) lifetimes, the unfolding overkill would have been all but imperceptible.
Chapter
Australian and Pacific archaeological research has focused on questions of human origins, behavioral and technological variability, population distribution, the extent of human and climatic impacts on the environment, and the chronology of earliest human occupation of Sahul. These themes have preoccupied Australian archaeologists for over 40 years and while there have been significant advances in dating techniques, understanding of site formation process, and human–environment interaction, many questions remain. This chapter discusses and reviews the evidence for the timing, spread, and settlement by humans of the Australian and Pacific region during the late Pleistocene and early Holocene.
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This work represents an exhaustive review of one of the most important late Cenozoic radiations of Australian marsupials: the short-faced, or sthenurine kangaroos. Sthenurines originated in the Miocene, diversified in the Pliocene, and radiated in the Quaternary to become one of Australia's most conspicuous mammal groups, the only lineage of browsing marsupials comparable in diversity to the browsing artiodactyl guilds of other continents. The culmination of 12 years' research, the monograph details the taxonomy of the sthenurines, redescribing each of the six genera (two new) and 26 species ( ... More This work represents an exhaustive review of one of the most important late Cenozoic radiations of Australian marsupials: the short-faced, or sthenurine kangaroos. Sthenurines originated in the Miocene, diversified in the Pliocene, and radiated in the Quaternary to become one of Australia's most conspicuous mammal groups, the only lineage of browsing marsupials comparable in diversity to the browsing artiodactyl guilds of other continents. The culmination of 12 years' research, the monograph details the taxonomy of the sthenurines, redescribing each of the six genera (two new) and 26 species (four new), and is illustrated with line drawings and more than 100 pages of plates. It presents a cladistic analysis of sthenurines, and by synthesizing systematic, functional morphological, biochronologic, and zoogeographic data, considers the major directions of adaptive change within the group, and the major environmental factors that drove their evolution. The book is a comprehensive study of an extinct marsupial lineage, and is a reference for students of Australian late Cenozoic vertebrates, marsupial evolution, environmental change, and Pleistocene extinctions.
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The Oxford Radiocarbon Accelerator Unit (ORAU) has used an ultrafiltration protocol to further purify gelatin from archaeological bone since 2000. In this paper, the methodology is described, and it is shown that, in many instances, ultrafiltration successfully removes low molecular weight contaminants that less rigorous methods may not. These contami- nants can sometimes be of a different radiocarbon age and, unless removed, may produce erroneous determinations, particu- larly when one is dating bones greater than 2 to 3 half-lives of 14C and the contaminants are of modern age. Results of the redating of bone of Late Middle and Early Upper Paleolithic age from the British Isles and Europe suggest that we may need to look again at the traditional chronology for these periods.