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Interwoven Strands for Refining the Chronology of the Neolithic Tell of Vinča-Belo Brdo, Serbia

Published online by Cambridge University Press:  30 August 2016

Nenad Tasić
Affiliation:
Faculty of Philosophy, Belgrade University, Čika Ljubina 18–20, Belgrade, Serbia
Miroslav Marić
Affiliation:
The Institute for Balkan Studies, Serbian Academy of Science and Arts, Knez Mihailova 35, Belgrade, Serbia
Dragana Filipović
Affiliation:
The Institute for Balkan Studies, Serbian Academy of Science and Arts, Knez Mihailova 35, Belgrade, Serbia
Kristina Penezić
Affiliation:
Faculty of Philosophy, Belgrade University, Čika Ljubina 18–20, Belgrade, Serbia
Elaine Dunbar
Affiliation:
SUERC Radiocarbon Dating Laboratory, Scottish Enterprise Technology Park, Rankine Avenue, East Kilbride G75 0QF, UK
Paula Reimer
Affiliation:
14CHRONO Centre, Queen's University Belfast, 42 Fitzwilliam Street, Belfast BT9 6AX, UK
Alistair Barclay
Affiliation:
Wessex Archaeology, Portway House, Old Sarum Park, Salisbury SP4 6EB, UK
Alex Bayliss
Affiliation:
Historic England, 1 Waterhouse Square, 138–42 Holborn, London EC1N 2ST, UK
Bisserka Gaydarska
Affiliation:
Department of Archaeology and Conservation, Cardiff University, John Percival Building. Colum Drive, Cardiff CF10 3EU, UK
Alasdair Whittle*
Affiliation:
Department of Archaeology and Conservation, Cardiff University, John Percival Building. Colum Drive, Cardiff CF10 3EU, UK
*
*Corresponding author. Email: whittle@cardiff.ac.uk.
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Abstract

A formally modeled radiocarbon chronology for a new profile through the great Neolithic tell of Vinča-Belo Brdo, Serbia, is the third interwoven strand in refining the chronology of the tell. This now joins models for the whole sequence based on the archive of early excavations, and for the last two known horizons at the top of the settlement mound, investigated in recent decades. In the new deep sounding, Vinča culture occupation from the 52nd century cal BC is slightly later than in the main sequence, probably reflecting the horizontal extension of the tell as it began to grow. The last dated occupation falls in the late 47th–early 46th century cal BC, slightly earlier than in the main sequence, but the top of the profile is affected by the slippage that caused the new excavations. Formal estimates are given for the succession and varying durations of burnt and unburnt houses, and indicate a period in the first part of the 5th millennium without house burning. Overall, the combined results from the three interwoven strands serve to produce a radically enhanced understanding of the temporality of the tell, which builds on, rather than supplants, previous research. We knew previously that Vinča-Belo Brdo was very long-lived, but now we can time that history with much greater precision. We can assert with much greater confidence that its vertical buildup was steady and largely uninterrupted. We have begun, from the work on the top of the tell and in the new deep sounding, to grasp better the fluctuations in house durations from generation to generation, and can now contrast the relative fortunes of unburnt and burnt houses. We can say much more about the timing and tempo of the ending of the tell, and about the possible circumstances in which that took place.

Information

Type
Research Article
Copyright
© 2016 by the Arizona Board of Regents on behalf of the University of Arizona 
Figure 0

Figure 1 The location of Vinča-Belo Brdo and other important Vinča culture sites, and the approximate extent (shaded dark grey) of the occurrence of Vinča ceramics in southeast Europe.

Figure 1

Figure 2 The section face through the tell at the time of the Vasić excavations.

Figure 2

Table 1 Radiocarbon ages and stable isotopes measurements from the 2004–5 and 2012–14 deep sounding and profile P1/2011 from Vinča-Belo Brdo; the statistical consistency of replicate measurements has been assessed using the method of Ward and Wilson (1978); quoted δ13C values have been measured by IRMS (insufficient carbon remained for this analysis for UBA-22450, UBA-22587, and UBA-22635).

Figure 3

Figure 3 Overall structure of the chronological model for the new deep sounding at Vinča-Belo Brdo. The component sections of this model are shown in detail in Figures 4–8. Each distribution represents the relative probability that an event occurred at a particular time. For each of the dates two distributions have been plotted: one in outline which is the result produced by the scientific evidence alone, and a solid one which is based on the chronological model used. The other distributions correspond to aspects of the model. For example, the distribution start Belo Brdo deep sounding is the estimated date for when the accumulation of Vinča pottery began to accumulate in this trench. Dates followed by a question mark have been calibrated (Stuiver and Reimer 1993), but not included in the chronological model for reasons explained in the text. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 4

Figure 4 Probability distributions of dates from the spine (lower). UBA-22640 (intrusive in H 01-14) is not shown as it dates to the late 5th millennium cal BC. The format is identical to Figure 3. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 5

Figure 5 Probability distributions of dates from the spine (upper). UBA-26548 (intrusive in H 01-12) is not shown as it dates to the 1st millennium cal BC. The format is identical to Figure 3. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 6

Figure 6 Probability distributions of dates from H 02-14 and P 2285. The format is identical to Figure 3. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 7

Figure 7 Probability distributions of dates from P 03-13. The format is identical to Figure 3. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 8

Figure 8 Probability distributions of dates from P 1978, P 1975, O 04-12, H 02-12, and H 01-04. The format is identical to Figure 3. The large square brackets down the left-hand side of Figures 3–8 along with the OxCal keywords define the overall model exactly.

Figure 9

Figure 9 Harris matrix of structures and features from the 2004–2005 and 2012–2014 deep sounding through Vinča-Belo Brdo from which 14C dates have been obtained.

Figure 10

Figure 10 Composite section of the 2004–2005 and 2012–2014 deep sounding through Vinča-Belo Brdo, indicating the positions of deposits incorporated in the spine of the chronological model (Figures 4 and 5). Profile 1 photographed May 2013; Profiles 2 and 3 photographed August 2014. For further detail, see text.

Figure 11

Table 2 Highest posterior density (HPD) intervals for the construction and demolition or destruction of buildings and ovens, and the infilling of dated pits (derived from the model defined in Figures 3–8, and see Figure 13).

Figure 12

Table 3 Highest posterior density (HPD) intervals for the duration and use of buildings and ovens (derived from the model defined in Figures 3–8, and see Figure 14).

Figure 13

Figure 11 Photograph showing cracking around H03/13

Figure 14

Figure 12 Probability distributions for dates and key parameters for Starčevo occupation and the beginning of Vinča occupation at Belo Brdo in different areas of the tell. Posterior density estimates are taken from the model defined in Figures 3–8 (SUERC-59028 and start Belo Brdo deep sounding) and the model illustrated in Tasić et al. (2016: Figure 17; start Starčevo burials, end Starčevo burials, and 9.3m). The 14C measurements from Profile 1/2011 have been calibrated (Stuiver and Reimer 1993).

Figure 15

Figure 13 Posterior density estimates for the construction and demolition/destruction of houses and ovens in the 2004–2005 and 2012–2014 deep sounding at Belo Brdo (derived from the model shown in Figures 3–8).

Figure 16

Figure 14 Posterior density estimates for durations of houses and ovens (derived from the model defined in Figures 3–8); houses destroyed by fire are shown in red.

Figure 17

Figure 15 Miloje Vasić (left) supervising the excavation and recording of a house at 2.91 m in 1911.

Figure 18

Figure 16 Probability distributions for the destruction by fire of dated buildings from Vinča Belo Brdo and Uivar, and for the onset of Vinča C pottery at Belo Brdo (in various typological schemes). Posterior density estimates are taken from the models defined in Figures 3–8, Tasić et al. (2015: Figure 8), and Schier et al. (forthcoming: Figures 6.9 and 6.12–6.22), and that illustrated in Tasić et al. (2016: Figure 17).

Figure 19

Figure 17 Schematic diagram for the chronology of Vinča-Belo Brdo showing the houses excavated in the 2002–2004 and 2012–2014 deep sounding (Figures 3–8) and Sector II (Tasić et al. 2015: Figure 8), the building horizons from the Vasić excavations reconstructed by Stalio (1984), principal episodes of burning recorded in section in the central part of the Vasić excavations (Borić 2015: Figure 4; Tasić et al. 2016: Figure 17), dates for Starčevo features at the base of the tell (Figure 3; Tasić et al. 2016: Figure 17), dates for the earliest Vinča occupation in profile P1/2011 (Figure 12), and date estimates for the main chronological schemes for Vinča ceramics (Tasić et al. 2016: Figure 17).

Figure 20

Table 4 Highest posterior density (HPD) intervals for episodes of burning identified in the central section of the Vasić excavations (derived from the model illustrated in Tasić et al. 2016: Figure 17).

Figure 21

Figure 18 Probability distributions for dates for the end of Vinča occupation at Belo Brdo in different areas of the tell. Posterior density estimates are taken from the model defined in Figures 3–8 (end Belo Brdo deep sounding), and the model illustrated in Tasić et al. (2016: Figure 17; 1.3m), and the model defined in Tasić et al. (2015: Figure 8; Fire 2).