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The Roman amphitheatre in Mérida, Spain ˗Augustan or Flavian? Radiocarbon dating results on mortar carbonate


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Fig 1

Sample positions 1-4 in the amphitheatre. Sampling: Upper left, Mérida 001; Upper right, Mérida 002; Lower left, Mérida 003; Lower right, Mérida 004. See details in the text.
Sample positions 1-4 in the amphitheatre. Sampling: Upper left, Mérida 001; Upper right, Mérida 002; Lower left, Mérida 003; Lower right, Mérida 004. See details in the text.

Fig 2

Thin section images. Upper left: 100μm section of sample Mérida 001 in transmitted light. Transparent minerals are mostly quartz. CL images: Upper right, cut and polished surface of a piece from sample Mérida 003 showing distribution between calcite (red) and other binder minerals (black). Mid left, the dated 46-75μm grainsize fraction of sample Mérida 001; Mid right, Mérida 003 ditto. Lower left, Mérida 004 ditto. Images from sample Mérida 002 are omitted because it turned out to be younger and less relevant. Red minerals are calcite and dark red ones have a dolomitic component while more orange ones are purer. Blue and turquoise are quartz and dull green are feldspar. The green dust-like powder in the slice is secondary aragonite from grinding. There is also a void filled with an extremely luminescent mineral in lilac, which we have not tried to identify.
Thin section images. Upper left: 100μm section of sample Mérida 001 in transmitted light. Transparent minerals are mostly quartz. CL images: Upper right, cut and polished surface of a piece from sample Mérida 003 showing distribution between calcite (red) and other binder minerals (black). Mid left, the dated 46-75μm grainsize fraction of sample Mérida 001; Mid right, Mérida 003 ditto. Lower left, Mérida 004 ditto. Images from sample Mérida 002 are omitted because it turned out to be younger and less relevant. Red minerals are calcite and dark red ones have a dolomitic component while more orange ones are purer. Blue and turquoise are quartz and dull green are feldspar. The green dust-like powder in the slice is secondary aragonite from grinding. There is also a void filled with an extremely luminescent mineral in lilac, which we have not tried to identify.

Fig 3

TGA profiles of the four samples from Mérida. The profiles are similar, but the most hydraulic samples Mérida 003 and 004 have lower CO2 yields and consequently more residue.
TGA profiles of the four samples from Mérida. The profiles are similar, but the most hydraulic samples Mérida 003 and 004 have lower CO2 yields and consequently more residue.

Fig 4

14C profiles from three different sample preparations of sample Mérida 001: Open circles are from the first dating attempt in 2001. Open boxes are from supplementary measurements later the same year and black diamonds from re-dating 2018. The grey bars along the abscissa denote the size of each CO2 fraction relative to the total CO2 yield. In all the following 14C profile plots the size of the CO2 fractions will be presented the same way without specific mention.
14C profiles from three different sample preparations of sample Mérida 001: Open circles are from the first dating attempt in 2001. Open boxes are from supplementary measurements later the same year and black diamonds from re-dating 2018. The grey bars along the abscissa denote the size of each CO2 fraction relative to the total CO2 yield. In all the following 14C profile plots the size of the CO2 fractions will be presented the same way without specific mention.

Fig 5

14C profiles of sample Mérida 002. Open circles present dating in 2001 and black boxes dating in 2018.
14C profiles of sample Mérida 002. Open circles present dating in 2001 and black boxes dating in 2018.

Fig 6

14C profiles of sample Mérida 003. Open circles denote dating in 2001 and open boxes a profile in six CO2 fractions dated later the same year. Black diamonds represent re-dating in 2018. For this sample we used the same powder that had been in a non-airtight container for 17 years. The data point with low F value representing initially effervesced CO2 was measured to ensure that the sample powder had not captured modern CO2 and grown new calcite on the grains.
14C profiles of sample Mérida 003. Open circles denote dating in 2001 and open boxes a profile in six CO2 fractions dated later the same year. Black diamonds represent re-dating in 2018. For this sample we used the same powder that had been in a non-airtight container for 17 years. The data point with low F value representing initially effervesced CO2 was measured to ensure that the sample powder had not captured modern CO2 and grown new calcite on the grains.

Fig 7

14C profile from sample Mérida 003 after heating the sample to 620˚C. Some of the young carbonates have been lost and the profile now increases more rapidly in the beginning compared with the profile from the non-heated original sample powder (Fig. 6).
14C profile from sample Mérida 003 after heating the sample to 620˚C. Some of the young carbonates have been lost and the profile now increases more rapidly in the beginning compared with the profile from the non-heated original sample powder (Fig. 6).

Fig 8

14C profiles from sample Mérida 004. Open circles, dating 2001. Black boxes, dating 2018.
14C profiles from sample Mérida 004. Open circles, dating 2001. Black boxes, dating 2018.

Fig 9

14C data from 2018. Data points for each sample are connected with lines for clarity. Samples Mérida 001, 003 and 004 yield similar 14C ages after about 20% dissolution (F>0.2) whereas sample Mérida 002 appears younger in all fractions.
14C data from 2018. Data points for each sample are connected with lines for clarity. Samples Mérida 001, 003 and 004 yield similar 14C ages after about 20% dissolution (F>0.2) whereas sample Mérida 002 appears younger in all fractions.

Fig 10

Combined calibration of 5 CO2 fractions with similar ages. The calibration includes the 3 last fractions from sample Mérida 001 and the two last ones from Merida 004 in Fig 9.
Combined calibration of 5 CO2 fractions with similar ages. The calibration includes the 3 last fractions from sample Mérida 001 and the two last ones from Merida 004 in Fig 9.

ICP-OES analyses of the soluble phase of the samples when dissolved for 1h in 1M HCl at room T. For comparison, 3 samples from the Medieval Bishop Masonas Hospital (Mérida 005, 006 and 007) and 3 samples from the Colosseum are included. Major elements are converted to oxides.

Sample IDAl2O3BaCaOFeOK2OMgOMnNa2OSiO2SrHydraulic
%mg/kg%%%%mg/kg%%mg/kgindex
Mérida 0010.0870.830.20.21<0.053.122530.090.515780,02
Mérida 0020.0861.927.30.21<0.054.222950.580.685520,03
Mérida 0030.1160.717.90.13<0.052.591330.040.343760,03
Merida 0050.1456.919.00.190.021.182250.050.253780,03
Mérida 0061.6916915.30.250.090.7173.30.020.36510,17
Mérida 0071.5418415.60.210.120.8261.20.011.79850.13
Colosseum0015.6151915.80.542.040.283121.492.654900,55
Colosseum0025.2962120.70.551.850.351651.263.175880,43
Colosseum0038.0116606.660.761.870.933551.283.836901,66

Numerical TGA data and the CO2 yield in H3PO4 hydrolysis for aliquots of the same sample material. For TGA about 10mg of the 46-75μm was heated and in the hydrolysis about 50mg was reacted with 85% H3PO4. The acid was taken from an ice bath but it reached room T before the reaction ceased after about 1h.

SampleLOI 550LOI 850CO2 yieldResidueLOI(850˚/550˚)
ID(%)(%)H3PO4 (%)(%)ratio
Mérida 0013.62626697.2 hydraulic
Mérida 0024.32716666.3 hydraulic
Mérida 0034.01916744.8 hydraulic
Mérida 0044.82225714.6 hydraulic
Colosseum 0032.77.63.7812.8 hydraulic

j.geochr-2020-0028.tab.003.w2aab3b7d106b1b6b1ab2b2ab1Aa

SiteSample nrReactionCarbonFraction14C±δ13CLaboratory
locationrun nrtimeyieldsizeAge
CO2 fraction nr(s) from t0(tot %)(relative 1)(BP)VPDBnr
Merida amphiteaterMerida 001.1.1677.40-0.198152035-13.0AAR-6721.1
Main entanceMerida 001.1.27270.198-0.408160040-8.96AAR-6721.2
Merida 001.2.16006.90-0.325158035-10.1AAR-6721.2.1
Merida 001.2.228200.325-0.646178030-8.40AAR-6721.2.2
Merida 001.3.320-1157.20.174-0.337186521-8.3ETH-87848
Merida 001.3.45400.337-0.604187622-10.2ETH-87849
Merida 001.3.513800.604-0.820188122-10.9ETH-87850
Merida 001.3.619800.820-0.919189924-9.3ETH-89323
Main entranceMerida 002.1.1438.00-0.187162645-13.7AAR-6722.1
Merida 002.1.25230.187-0.386179040-7.10AAR-6722.2
Merida 002.2.230-1204.40.273-0.470171122-7.0ETH-87851
Merida 002.2.36000.470-0.798178121-7.5ETH-87852
Merida 002.2.411800.798-0.937182525-5.3ETH-87863
Passage towards NEMerida 003.1.11045.60-0.191153040-12.5AAR-6723.1
Merida 003.1.28840.191-0.394181540-9.9AAR-6723.2
Merida 003.2.1303.20-0.068133540-18.4AAR-6723.2.1
Merida 003.2.25100.068-0.365171535-9.82AAR-6723.2.2
Merida 003.2.324900.365-0.631189535-9.66AAR-6723.2.3
Merida 003.2.487900.631-0.850198035-10.4AAR-6723.2.4
Merida 003.2.5159900.850-0.943196040-11.8AAR-6723.2.5
Merida 003.2.6630000.943-1.00214045-10.2AAR-6723.2.6
Merida 003.3.1304.40-0.093138325-15.7ETH-87864
Merida 003.2.8530-19500.487-0.777185221-12.2ETH-87853
“Roasting”Merida 003 Roa1.182.40-0.0174
hydrolysis afterMerida 003 Roa1.2250.0174-0.109153934-13AAR-30431
heating to 620˚CMerida 003 Roa1.31000.109-0.294182129-6
Merida 003 Roa1.45800.294-0.582185930-8
Merida 003 Roa1.513200.582-0.800187333-10
Passage towards NEMerida 004.1.1146.30-0.18513205017.7AAR-6724.1
Merida 004.1.21940.185-0.393179540-7.10AAR-6724.2
Merida 004.2.26-196.80.068-0.128163125-14.1ETH-87854
Merida 004.2.31050.128-0.343182723-7.8ETH-87855
Merida 004.2.45800.343-0.658192322-11.6ETH-87856
Merida 004.2.514400.658-0.870190825-10.6ETH-89324
eISSN:
1897-1695
Język:
Angielski
Częstotliwość wydawania:
Volume Open
Dziedziny czasopisma:
Geosciences, other