| Literature DB >> 26083101 |
Alan N Williams1, Sean Ulm2, Chris S M Turney3, David Rohde4, Gentry White5.
Abstract
A continental-scale model of Holocene Australian hunter-gatherer demography and mobility is generated using radiocarbon data and geospatial techniques. Results show a delayed expansion and settlement of much of Australia following the termination of the late Pleistocene until after 9,000 years ago (or 9ka). The onset of the Holocene climatic optimum (9-6ka) coincides with rapid expansion, growth and establishment of regional populations across ~75% of Australia, including much of the arid zone. This diffusion from isolated Pleistocene refugia provides a mechanism for the synchronous spread of pan-continental archaeological and linguistic attributes at this time (e.g. Pama-Nyungan language, Panaramitee art style, backed artefacts). We argue longer patch residence times were possible at the end of the optimum, resulting in a shift to more sedentary lifestyles and establishment of low-level food production in some parts of the continent. The onset of El Niño - Southern Oscillation (ENSO; 4.5-2ka) restricted low-level food production, and resulted in population fragmentation, abandonment of marginal areas, and reduction in ranging territory of ~26%. Importantly, climate amelioration brought about by more pervasive La Niña conditions (post-2ka), resulted in an intensification of the mobility strategies and technological innovations that were developed in the early- to mid-Holocene. These changes resulted in population expansion and utilization of the entire continent. We propose that it was under these demographically packed conditions that the complex social and religious societies observed at colonial contact were formed.Entities:
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Year: 2015 PMID: 26083101 PMCID: PMC4471166 DOI: 10.1371/journal.pone.0128661
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Fig 1Map of the archaeological sites within the dataset between 12-0ka.
Data in red indicate sites referenced in the main text: 1) New Guinea II Rockshelter; 2) Kenniff Cave; 3) Native Wells rockshelters; 4) Dabangay shell mounds; 5) Carpenters Gap 1 Rockshelter; 6) Puntutjarpa Rockshelter; 7) Malangangerr Rockshelter; 8) Arkaroo Rock; 9) Serpents’ Glen Rockshelter; 10) Glen Thirsty Well; 11) Puritjarra Rockshelter; 12) Bush Turkey 3 Rockshelter; 13) Devon Downs Rockshelter; 14) Roonka Flat Dune open site; 15) Koongine Cave; 16) Allen’s Cave; 17) Madura Cave; 18) Norina Cave; 19) Marillana A Rockshelter; 20) Loggers Shelter; 21) RTA G1; 22) Sassafras 1 Rockshelter; 23) Yengo 1 Rockshelter; 24) Warragarra Rockshelter; 25) Nimji Rockshelter; 26) Skew Valley midden; 27) Hooka Point midden; 28) Canunda Rocks midden; 29) Clybucca midden; 30) Muyu-ajirrapa midden; 31) Jordan River midden. See S1 Text for references.
A summary of the analysis by time-slice, including the number of data clusters; the size of the MBRs; absolute populations based on work by Williams [8] (and assuming a 50ka colonisation of Australia by 2–3,000 people); and average population density using Williams’ data divided by the continent size of 7.7 million km2.
| Time Slice | Number of Clusters | Minimum Bounding Rectangle (km2) | Population Estimates (000’s) | Population density (1 person / |
|---|---|---|---|---|
| 13-11ka | 6 | 3,370,500 | 27.6 | 122 |
| 12-10ka | 8 | 3,961,066 | 36.2 | 109 |
| 11-9ka | 7 | 3,796,314 | 44.3 | 86 |
| 10-8ka | 8 | 4,729,692 | 54.5 | 87 |
| 9-7ka | 9 | 5,241,223 | 81.8 | 64 |
| 8-6ka | 8 | 5,866,795 | 92.3 | 64 |
| 7-5ka | 9 | 5,551,493 | 92.6 | 60 |
| 6-4ka | 10 | 5,220,601 | 112.0 | 47 |
| 4–3.5ka | 12 | 3,850,687 | 213.6 | 18 |
| 3.5-3ka | 11 | 3,921,567 | 220.1 | 18 |
| 3–2.5ka | 10 | 4,323,604 | 244.8 | 18 |
| 2.5-2ka | 9 | 5,357,885 | 324.0 | 17 |
| 2–1.5ka | 10 | 6,214,773 | 455.2 | 14 |
| 1.5-1ka | 7 | 7,726,433 | 845.1 | 9 |
| 1–0.5ka | 9 | 6,449,991 | 1,108.4 | 6 |
| 0.5-0ka | 9 | 7,307,522 | 1,162.3 | 6 |
Fig 2Demographic change, ranging areas and sites with repeated or ongoing occupation based on archaeological radiocarbon data for Australia between 12-0ka.
A) Average annual growth rates (GRAnn) from Williams [8], showing stepwise population increase through the Holocene. B) Quantitative population estimates using a range of founding populations (n = 50, 500, 1000, 2000, 3,000, 5,000) from Williams [8]. Williams considered founding populations of between 2,000–3,000 most likely, resulting in populations of 0.5–1.5 million through the late Holocene, higher than at any previous time since colonisation. C) Total area of Minimum Bounding Rectangles (MBRs), considered to represent population ranging area or territory using over-lapping (2,000 year) time slices between 12 and 5ka, and firm (500 year) time slices between 5 and 0ka; D) The number of archaeological sites with two or more radiocarbon data within a given time slice (moving firm 500 year time slices), and considered to reflect longer residence time and/or more permanent occupation. Key climatic events are also shown, including Holocene climatic optimum (HCO), El Niño Southern Oscillation (ENSO), Medieval Climatic Anomaly (MCA), and Little Ice Age (LIA).
Fig 3A selection of time-slice maps showing the changing MBR locations and sizes at 9-7ka, 6-4ka, 3.5-3ka, 3–2.5ka, 1.5-1ka and 1–0.5ka.
The size of the MBRs here have been used to create Fig 2C.