Aspendos, Kelenderis and Tarsos

Summary Analysis

Coin catalogue sections: Kelenderis
Coin corpus datasets: Kelenderis, staters, Group 1, Kelenderis, staters, Group 2, Kelenderis, staters, Group 3, Aspendos, staters, Tarsos, staters after c. 388 BC

Summary

The subject of this analysis is a comparison of the weights of the Kelenderis staters with the weights of the Aspendos staters minted between approximately 465 and 250 BC and satrapal staters minted in Tarsos from about 388 to 323 BC. A comparison of the Kelenderis coin production with that of the Aspendos mint suggests that two weight standards were used simultaneously in Pamphylia and Cilicia Trachea. Additionally, the late Kelenderis issues appear to have been minted in a lighter weight standard than all the issues of the Aspendos mint and Taros mint. This suggests that the Kelenderis mint was either using a different weight standard, or that these late issues fall into a much later period than is usually assumed. However, these observations are still very preliminary and for reliable conclusions it is necessary to analyze also the production of Tarsos before 388 BC and to expand the analyzed data sets to ensure their representativeness and reduce statistical errors.

Analysis

The production of the Kelenderis mint is compared with the pre-Hellenistic and early Hellenistic production of the Aspendos mint, and with the pre-Hellenistic production of the Tarsos mint during the reign of the satraps Tiribazos to Balakros. The Kelenderis staters are divided into Groups 1, 2 and 3 (see page Coin Catalogue / Kelenderis / Overview), with Group 3 being further divided into three subgroups 3A, 3B and 3C (see page Weight Analyses / Kelenderis, staters). The Aspendos staters are divided into early issues with a warrior on the obverse and a triskeles on the reverse, and later issues with two wrestlers on the obverse and a slinger on the reverse, with these later issues further divided into five series according to Tekin 1997. The Tarsos satrapal staters are divided by individual Cilician satraps, and these groups are further divided by major coin types (not all types are considered, but only the types with sufficient representation). An overview of the analysed groups of coins is given in Table 1. The usual dating of these groups is given in Table 2.

Mint Group Description
Aspendos Warrior / Triskeles Obv.: Warrior advancing right,.
Rev.: Triskeles.
Wrestlers / Slinger Tekin 1997, Series 1
Tekin 1997, Series 2
Tekin 1997, Series 3
Tekin 1997, Series 4
Tekin 1997, Series 5
Kelenderis Group 1 Types 1.1–3
Group 2 Types 2.1–12
Group 3A Types 3.1–3 and 3.7–12
Group 3B Types 3.13–14
Group 3C Types 3.4–6 and 3.15–17
Tarsos Tiribazos 1 Obv.: Baaltars standing half-left, holding eagle and lotus-tipped scepter.
Rev.: Ahura-Mazda facing, head right, body terminating in solar disk with wings and tail feathers, holding up wreath and lotus blossom.
2 Obv.: Satrap seated right on throne, wearing Persian headdress, raising his right hand and left hand placed on bow set on ground.
Rev.: Bearded head right, wearing satrapal headdress.
3 Obv.: Athena seated left, holding spear in her right hand and leaning left elbow on shield; behind, olive tree.
Rev.: Female kneeling left, casting astragaloi; behind, lotus plant.
4 Obv.: Head of Hera (?) left, wearing decorated tiara.
Rev.: Herakles strangling the Nemean lion.
Pharnabazos 1 Obv.: Head of Herakles facing slightly right, wearing lion’s skin.
Rev.: Bearded male head (Ares?) left, wearing crested Attic helmet.
2 Obv.: Baaltars seated left on throne.
Rev.: Bearded male head (Ares?) left, wearing crested helmet.
3 Obv.: Head of Arethusa facing slightly left.
Rev.: Bearded male head (Ares?) left or right, wearing crested Attic helmet.
Datames
(Tarkumuwa)
1 Obv.: Head of Arethusa facing slightly left.
Rev.: Bearded male head (Ares?) left or right, wearing crested Attic helmet.
2 Obv.: Baaltars seated right, torso facing; all within crenellated wall.
Rev.: Satrap seated right, wearing Persian dress, inspecting arrow.
3 Obv.: Baaltars seated right, torso facing; all within crenellated wall.
Rev.: Ana, standing right, extending hand and pointing at the head of Tarkumuwa, standing left, right hand raised; between them, thymiaterion; all within square dotted border in linear border.
Mazaios 1 Obv.: Baaltars seated left on throne.
Rev.: Lion left attacking stag left.
2 Obv.: Baaltars seated left on throne, head facing.
Rev.: Lion left attacking bull left.
3 Obv.: Baaltars seated left on throne.
Rev.: Lion left attacking bull left; below, pair of crenellated walls, each with four towers.
Balakros 1 Obv.: Baaltars seated left on throne.
Rev.: Lion left attacking bull left; below, pair of crenellated walls, each with four towers.
2 Obv.: Facing bust of Athena, draped, wearing triple-crested helmet and necklace.
Rev.: Baaltars seated left on throne.

Table 1: Analyzed groups of coins of Aspendos, Kelenderis and Tarsos.

Mint Group Approximate dating
Aspendos Warrior / Triskeles 465 – 430 BC
Tekin 1 420 – 410 BC
Tekin 2 415 – 400 BC
Tekin 3 400 – 380 BC
Tekin 4 380/75 – 330/25 BC
Tekin 5 330/25 – 310/250 BC
Kelenderis Group 1 around 450 BC or possibly 440 – 430 BC
Group 2 450 – 405 BC or possibly 430 – 405 BC
Group 3 405 – 375 BC
Tarsos Tiribazos 388 – 380 BC
Pharnabazos 380 – 374/3 BC
Datames 384 – 361/0
Mazaios 361/0 – 334
Balakros 333 – 323 BC

Table 2: Approximate dating of analyzed groups of coins

An analysis of the Kalenderis staters is presented on page Weight Analyses / Kelenderis, staters and is therefore not included here. Box plots1 of the Aspendos staters are shown in Figure 1. This chart and Table 3 below show that the warrior/triskeles type coins and the wrestlers/slinger type coins belonging to Tekin’s Series 1–3 were minted in the same weight standard. For Series 4, there is a slight decrease in the weight standard, and Series 5 is already minted at a significantly lower weight standard. In addition, the greater weight volatility and unclear minting time range of Series 5 suggests that it may not have been a homogeneous series, but that there may have been a further lowering of the weight standard.

Figure 1: Box plots of individual stater groups

Figure 1: Aspendos, box plots

Box plots of the Tarsos staters divided by the coin types (see Table 1) and aggregated by individual satraps are shown in Figures 2a and 2b, respectively. These charts and Table 3 below indicate that the lowest weight standard was used during the reign of Tiribarzos, then increased during the reigns of Pharnabazos and Datames, and then increased further during the reigns of Mazaios and Balakros.

Figure 2a: Cumulative distributions of individual stater groups

Figure 2a: Tarsos, box plots of individual types

Figure 2b: Cumulative distributions of individual stater groups

Figure 2b: Tarsos, box plots of aggregated data by individual satraps

Figure 3a shows the box plots of all three mints together. On the left is Aspendos, the light green shaded area in the middle shows Kelenderis and on the right is Tarsos. Figure 3b shows the same, but outliers are omitted for clarity. The basic statistic characteristics of all these coin groups are presented in Table 3 (Std. Dev. denotes the standard deviation and IQR the interquartile range).

These results suggest that Kelenderis issues falling into Groups 1, 2 and 3A were minted at a slightly lower weight standard than the Aspendos issues from the warrior/triskeles type to Tekin’s Series 4. The median of Kelenderis Group 3B roughly corresponds to Tekin’s Series 5, while Kelenderis Group 3C lies well below Tekin’s Series 5. Since a significant part of the coinage of the Aspendos mint overlaps in time with a significant part of the coinage of the Kelenderis Mint (see Table 2), this raises the question of whether the two mints used the same Persian weight standard, or whether multiple weight standards were used simultaneously in Pamphylia and Cilicia Trachea.

As for Tarsos, Kelenderis Group 3B can be roughly compared with the coins of Pharnabazos and Datames, while Group 3C has no comparison with any part of the coinage of Tarsos in the period c. 388–323 BC. Group 3C is thus beyond comparison with the analyzed production of both mints. This suggests that the Kelenderis mint was either using a different weight standard, or that these late issues fall into a much later period than is usually assumed.

However, it must be emphasized that all these observations are preliminary and for reliable conclusions it is necessary to analyze also the production of Tarsos before 388 BC and to enlarge the analyzed data sets to ensure their representativeness and reduce statistical errors.

Figure 3a: Cumulative distributions of individual stater groups

Figure 3a: Cumulative distributions of individual groups of staters

Figure 3b: Cumulative distributions of individual stater groups

Figure 3b: Cumulative distributions of individual groups of staters

Mint Group Count Mean Median Std. Dev. IQR
Aspendos Warrior 50 10.88 10.89 0.13 0.15
Tekin 1 18 10.82 10.86 0.14 0.19
Tekin 2 55 10.85 10.89 0.13 0.11
Tekin 3 55 10.81 10.87 0.22 0.13
Tekin 4 55 10.75 10.79 0.20 0.24
Tekin 5 55 10.27 10.40 0.59 0.45
Kelenderis Group 1 13 10.73 10.78 0.23 0.21
Group 2 229 10.73 10.74 0.10 0.13
Group 3A 180 10.64 10.68 0.23 0.18
Group 3B 14 10.45 10.43 0.20 0.36
Group 3C 29 9.90 9.98 0.34 0.19
Tarsos Tiribazos 35 10.15 10.22 0.41 0.55
Pharnabazos 87 10.52 10.64 0.38 0.29
Datames 104 10.43 10.50 0.33 0.45
Mazaios 102 10.68 10.75 0.34 0.32
Balakros 62 10.73 10.82 0.31 0.25

Table 3: Basic descriptive statistics

 

1The bottom and top of each box are the 25th and 75th percentiles of the dataset, respectively (the lower and upper quartiles). Thus, the height of the box corresponds to the interquartile range (IQR). The red line inside the box indicates the median. Whiskers (the dashed lines extending above and below the box) indicate variability outside the upper and lower quartiles. From above the upper quartile, a distance of 1.5 times the IQR is measured out and a whisker is drawn up to the largest observed data point from the dataset that falls within this distance. Similarly, a distance of 1.5 times the IQR is measured out below the lower quartile and a whisker is drawn down to the lowest observed data point from the dataset that falls within this distance. Observations beyond the whisker length are marked as outliers and are represented by small red circles.

 

5 May 2024