Transliterated Name | Language | Name |
---|---|---|
Caesarea | | |
Caesarea Maritima | | |
Keysariya | Hebrew | קֵיסָרְיָה |
Qesarya | Hebrew | קֵיסָרְיָה |
Qisri | Rabbinic Sources | |
Qisrin | Rabbinic Sources | |
Qisarya | Arabic | قيسارية |
Qaysariyah | Early Islamic Arabic | قايساريياه |
Caesarea near Sebastos | Greek and Latin sources | |
Caesarea of Straton | Greek and Latin sources | |
Caesarea of Palestine | Greek and Latin sources | |
Caesarea | Ancient Greek | Καισάρεια |
Straton's Tower | ||
Strato's Tower | | |
Stratonos pyrgos | Ancient Greek | |
Straton's Caesarea | |
King Herod built the town of Caesarea between 22 and 10/9 BCE, naming it for his patron - Roman Emperor Caesar Augustus. The neighboring port was named Sebastos - Greek for Augustus (Stern et al, 1993). Straton's Tower, a Phoenician Port city, existed earlier on the site. When the Romans annexed Judea in 6 CE, Caesarea became the headquarters for the provincial governor and his administration (Stern et al, 1993). During the first Jewish War, Roman General Vespasian wintered at Caesarea and used it as his support base (Stern et al, 1993). After he became Emperor, he refounded the city as a Roman colony. Caesarea is mentioned in the 10th chapter of the New Testament book of Acts as the location where, shortly after the crucifixion, Peter converted Roman centurion Cornelius - the first gentile convert to the faith. In Early Byzantine times, Caesarea was known for its library and as the "home-town" of the Christian Church historian and Bishop Eusebius. After the Muslim conquest of the 7th century, the city began to decline but revived again in the 10th century (Stern et al, 1993). Crusaders ruled the city for most of the years between 1101 and 1265 CE (Stern et al, 1993). After the Crusaders were ousted, the town was eventually leveled in 1291 CE and remained mostly desolate after that (Stern et al, 1993).
Herod the Great named the port city he built on the Mediterranean coast Caesarea, to honor his patron, the emperor Caesar Augustus. He called the neighboring port Sebastos, Greek for" Augustus." The site is located on the Sharon coast, about midway between Haifa and Tel Aviv (map reference 1399.2115). The site's ancient name has survived into modern times in the Arabic Qaisariya. Rabbinic sources reproduced Caesarea as Qisri or Qisrin. Because it was only one of many Caesareas, Greek and Latin sources often specify Caesarea as near (the harbor) Sebastos, Caesarea of Straton, or (more commonly) Caesarea of Palestine. The emperor Vespasian granted Caesarea the rank of Roman colony, making it Colonia Prima Flavia Augusta Caesariensis, and Severus Alexander gave it the title Metropolis of the province Syria Palaestina. The name Caesarea Maritima, widely used today, was apparently unknown in antiquity. Straton's Tower (Στρατωνος Πνργος), a Phoenician port town, existed earlier on the site. The name is Greek for Migdal Shorshon, its equivalent in rabbinic texts. It is a common type of toponym meaning a fortified town, not a bastion or lookout tower, as some have thought. Whatever the meaning of Shorshon, in local legend Straton was a Greek hero, and it was he, not Herod, who founded Caesarea, which has thus also been called Straton's Caesarea.
Modern scholars suggest that the historical Straton was either a general in the Ptolemaic army in the beginning of the third century BCE or one of two Phoenicians named 'Abdashtart who ruled Sidon in the fourth century BCE. Recent ceramic finds do support limited commercial activity at the site this early, but the earliest reference to Straton's Tower is in a papyrus from the Zenon archive (P Cairo 59004) (259 BCE), which also attests an active harbor. The town flourished in the third century BCE (ceramic evidence) and especially in the later second century BCE, when the local tyrant, Zoilos, held it against the expanding Jewish kingdom (Josephus, Antiq. XIII, 324), perhaps fortifying it with the "city wall of Straton's Tower" mentioned in a rabbinic source (Tosefta Shevi'it IV, 11). The rulers of Straton's Tower apparently developed at least two protected harbors, cut into the sandstone bedrock of the coast in characteristic Hellenistic fashion - λιμην κλειστος (close haven).
Caesarea is a large site, comprising about 235 a. within its semicircular perimeter wall. In the eighteenth and nineteenth centuries European travelers, such as R. Pococke and V. Guerin, published more-or-less accurate descriptions of the site. In 1873, C. R. Conder and H. H. Kitchener mapped and described it as part of the Survey of Western Palestine, noting, for example, the aqueducts, the semicircular (outer) perimeter wall, the medieval fortifications, and the theater. Over the next ninety years there were only chance finds. In 1945, J. Ory,forthe Mandatory Department of Antiquities, and M. Avi-Yonah, in 1956 and 1962, for the Israel Department of Antiquities and Museums, explored the meager remains of a synagogue revealed during winter storms along the northern seashore. In 1951, S. Yeivin excavated a marble-paved esplanade east of the Crusader city for the department, where a tractor from Kibbutz Sedot Yam had struck a colossal porphyry statue. In 1955, a large mosaic pavement on a ridge to the northeast of ancient Caesarea was also exposed accidentally.
Large-scale archaeological excavations were carried out at Caesarea from 1992 to 1998 by the Israel Antiquities Authority (IAA); they were directed by Y. Porath. The project included the excavation of a 100–150-m-wide strip along the coast between the theater complex to the south and the excavations of the Combined Caesarea Expeditions (CCE) to the north; the western part of the temple platform and the area between this platform and the eastern quay of the port of Sebastos; both sides of the southern Crusader wall (continuing the salvage excavations carried out in 1989); the bottom of the Crusader moat (cleared in the 1960s by A. Negev), from the southern gateway to the northern gateway; and the area southwest of the theater. In addition, salvage excavations were conducted within the area demarcated by the Byzantine wall; in structures outside the wall; on the necropolis; in agricultural areas to the east, north, and south of the city; and along the aqueducts that carried water to Caesarea from outside the city.
During the 1990s the face of ancient Caesarea underwent dramatic change as excavations on an unprecedented scale exposed much more of the site and resolved earlier puzzles and misconceptions. The Combined Caesarea Expeditions (CCE) organized in 1989 by A. Raban, of the Recanati Institute for Maritime Studies at the University of Haifa, and K. G. Holum, of the University of Maryland, continued work through much of the decade and, on a more limited scale, into the new millennium. In 1993, J. Patrich joined the CCE directorate on behalf of the University of Haifa. Inside the Old City, K. Holum directed excavations on the temple platform (area TP) and in a warehouse quarter north of the inner harbor (area LL). A. Raban led excavations at the presently land-locked inner harbor and its eastern quay (area I), and at two sites along the southern edge of the temple platform (areas Z and TPS). J. Patrich excavated south of the Crusader city in areas CC, NN, and KK. In area KK, he uncovered six warehouse units, while area CC, formerly field C of the Joint Expedition to Caesarea Maritima (JECM), contained a government complex that accommodated the Roman provincial procurator and later the governor of Byzantine Palestine. The CCE team also devoted effort to area CV, the western side of the area CC vaults, and its maritime unit conducted underwater excavations in the harbor.
The CAHEP (Caesarea Ancient Harbour Excavation Project) consortium, led by the Recanati Institute for Maritime Studies at the University of Haifa, in collaboration with the University of Colorado (led by R. L. Hohlfelder), the University of Maryland (led by R. L. Vann), and the University of Victoria, British Columbia (led by J. P. Oleson), was succeeded by the maritime unit of the CCE, a collaborative project of the University of Haifa (led by A. Raban) and McMaster University (led by E. G. Reinhardt). The ongoing project conducts an annual field season with student volunteers from both institutions as well as others from around the world. The focus of the underwater research has shifted lately toward geoarchaeology, in an attempt to comprehend the history of maritime activity at Caesarea and the demise of Sebastos in the context of environmental changes and topographical alternations on the waterfront.
Neither Reinhardt et. al. (2006) nor
Goodman-Tchernov et. al. (2009) nor
Goodman-Tchernov and Austin (2015)
saw evidence of a tsunami in near shore shelf deposits of Caesarea around 304 CE.
Salamon et. al. (2011)
noted that a tsunami was reported in a number of earlier earthquake catalogs (e.g. Shalem, 1956,
Ben-Menahem, 1991,
Amiran et al., 1994) which
several of the cataloguers (Shalem, 1956 and Amiran et al., 1994) viewed as doubtful - according to Salamon et al (2011). The alleged tsunami was likely generated from
Eusebius' report of the sea casting up the body of the martyrdom of Apphian at the gates of Caesarea at the same time as the
[Eusebius Martyr Quake] in Sidon.
Salamon et al (2011) noted that a seismic sea wave is not specifically mentioned in Eusebius' text and it is common along the eastern Mediterranean coast,
even in normal weather conditions, that the sea casts up dead bodies of drowned people at the shore.
Tyuleneva et. al. (2017) identified what appears to be the same tsunamite in a core (Jisr al-Zarka 6) taken offshore of nearby Jisr al-Zakra. This core was located ~1.5-4.5 km. north of the Caesarea cores. The tsunamite deposit from Jisr al-Zarka was more tightly dated to 658-781 CE (1292-1169 Cal BP) – within the time window for the Holy Desert Quake of the Sabbatical Year Earthquake sequence.
which was in use from the Herodian period to the Umayyad period. A storage structure (aka "the warehouse") was identified in the western part of the site which appears to have been constructed in Herodian times and remained in use, as it underwent changes, until the middle of the Umayyad period (~700 CE). After the Islamic conquest of Caesarea (640 CE),
rooms were partitioned, floors were raised, construction was added and some of the openings were sealed.Ceramics indicate that the site was abandoned at the end of the 7th century CE after which it suffered two major destruction events before re-occupation occurred in the mid 8th century CE in what was interpreted as Abbasid Strata V (the Abbasid Caliphate began ruling in 750 CE). During the renewed Abbasid occupation, destruction debris were preserved
as the builders preferred to level the area and build above the destruction layer(s).The destruction events within Stratum VI (Umayyad) appear to be an earthquake and a tsunami; both likely a result of the the Holy Desert Quake of the Sabbatical Year Quake sequence.
several ceilings collapsed inward, and there was evidence of a fire in the eastern warehouse.1 In the collapse in the corridor, the
original order of the courses of the wall or vault could be clearly identified (Fig. 8)adding confidence to a seismic interpretation. During the subsequent tsunami event,
a layer of sand and collapsed building stones had accumulated to a height of more than 2 m in Rooms 8–11 in the western warehouse and to a height of 1.5 m in Rooms 12–14 and the corridor of the eastern warehouse.Everhardt et. al. (2023) further examined the destruction deposits by taking cores and radiocarbon samples as well as examining burn evidence and a baulk inside the collapsed corridor.
from the top 3 cm of sediment in the Umayyad archaeological fill and one untreated sample of various organic material (~20 mg) from the top 5 cm of the same layer in core C1, as close as possible to the contact with the lower anomalous deposit, were collected for radiocarbon dating.Everhardt et. al. (2023:14-15) report that
radiocarbon dates of charcoal and organic material from the upper contact of the Umayyad archaeological deposit (Unit C) range from 605 to 779 CE2 which is in agreement with the phasing of Ad et al (2018) and compatible with destruction layers that were deposited in 749 CE.
Unit | Alias | Description | Interpretation |
---|---|---|---|
A | ‘anomalous’ deposit | clean, loose quartz sand with no sedimentary structures or cultural artifacts. |
tsunami deposit |
B | same sediment as Unit A but with additions of several marine-encrusted potsherds and reddened, partially heat-fused sand clusters. |
earthquake and fire debris mixed with a tsunami deposit | |
C | 'Umayyad archaeological fill' | a dark gray/brown (10YR 6/2), organic-rich layer with many cultural artifacts, including potsherds, glass shards, shells, beach pebbles, charcoal, and bone fragments. |
Post abandonment deposition from the latter half of the Umayyad period - typical of an ancient garbage dump |
D | compact earthen floor |
Umayyad or earlier floor |
reddened, partially heat-fused sand clusterswere
in agreement with the presence of reddened in-situ building blocks along the intact eastern wall of the room (and elsewhere along the walls)which indicated that a fire took place before the tsunami struck. They also noted an
abundance of charcoal found in the upper Umayyad archaeological fill.They viewed the presence of marine-encrusted potsherds as an indicator that
these inclusions were previously submerged in the marine system long enough for the encrustation to take place, suggesting that they were transported from the sea to land at the time of the eventwhich in turn could
indicate that the tsunami water and deposits extinguishedthe fire.
1 Everhardt et. al. (2023:5) reports that fire-reddened walls (see inset of Figure 2C) were found at
the same level as the destruction layer(s).
2 Everhardt et. al. (2023:14-15) described the radiocarbon samples as follows:
A single piece of charcoal from the surface of the Umayyad archaeological fill (Unit C) in core C1 has been radiocarbon dated with 95.4% probability to 649–687 cal CE (73.5%) or 743–773 cal CE (22.0%), consistent with the archaeological finds. A second radiocarbon age was measured on a mix of small organic materials from the same layer as the previous charcoal sample, with a result of 605–665 cal CE (95.4% probability).
Effect | Location | Image(s) | Description |
---|---|---|---|
Liquefaction and Subsidence | outer harbor breakwater
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021)
Fig. 1
Caesarea harbor, overview (adapted from Boyce et al 2009) Dey and Goodman-Tchernov (2010)
Figure 1
View of ancient harbor area showing rubble spill of ancient break-waters, probable configuration of Herod's harbor, fault lines extending through harbor, and excavation areas. JW: Area K is top left Reinhardt and Raban (1998) |
Figure 2
Stratigraphic sections from excavation areas from intermediate and inner harbor (see Fig. 1 for locations). For biofacies characters and 87Sr/86Sr data, see Table 1. Stratigraphic, foraminiferal, and 87Sr/86Sr data from TN1a, I14, and I9 were reported by Reinhardt et al. (1998a), Yule and Barham (1999a, 1999b), and Raban et al. (1999b). 14C samples were measured at Weizmann Institute of Science, Israel (sample numbers RT2585, RT2631, and RT2650-RT2654) and calibrated to calendar ages using method of Stuiver and Reimer (1993). Reinhardt and Raban (1998)
Figure 3
Figure 3. A–D: Possible harbor configurations through time based on stratigraphy from intermediate and inner harbor. C is also based upon earlier archaeological excavations from within inner harbor described by Raban (1996). Reinhardt and Raban (1998) |
Description
|
Tsunami | Offshore Caesarea
Fig. 1
Caesarea harbor, overview (adapted from Boyce et al 2009) Dey and Goodman-Tchernov (2010)
Fig. 3
Location of sediment cores extracted in 2005 and 2007 Dey and Goodman-Tchernov (2010) |
Fig. 4
Dip and strike CHIRP profiles (see Fig. 3), from which sample segments “a” and “b” have been enlarged for comparison with previously identified sediment core and underwater excavation stratigraphic compilations within the surveyed area (Reinhardt et al., 2006; Reinhardt and Raban, 2008; Goodman-Tchernov et al., 2009). Three horizons, representing four tsunami events, are recognizable from the available core evidence within the surveyed area (for core locations, see Fig. 1C). Goodman-Tchernov and Austin (2015)
Fig. 4
Summary of tsunamigenic characteristics identified in cores and excavations from the shore ('NS') and terrestrial area (`T') to greater depths JW: Later publications redated Byzantine 551 A.D. to 749 .A.D. with possible reworked 551 A.D. deposits. If Roman 115 A.D. deposit is tsunamogenic, it was more likely caused by the early 2nd century Incense Road Earthquake rather than the distant 115 A.D. Trajan Quake Dey and Goodman-Tchernov (2010) |
Description
|
Tsunami | Harbor
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021)
Fig. 1
Caesarea harbor, overview (adapted from Boyce et al 2009) Dey and Goodman-Tchernov (2010)
Figure 1
View of ancient harbor area showing rubble spill of ancient break-waters, probable configuration of Herod's harbor, fault lines extending through harbor, and excavation areas. JW: Area K is top left Reinhardt and Raban (1998) |
Figure 2
Stratigraphic sections from excavation areas from intermediate and inner harbor (see Fig. 1 for locations). For biofacies characters and 87Sr/86Sr data, see Table 1. Stratigraphic, foraminiferal, and 87Sr/86Sr data from TN1a, I14, and I9 were reported by Reinhardt et al. (1998a), Yule and Barham (1999a, 1999b), and Raban et al. (1999b). 14C samples were measured at Weizmann Institute of Science, Israel (sample numbers RT2585, RT2631, and RT2650-RT2654) and calibrated to calendar ages using method of Stuiver and Reimer (1993). Reinhardt and Raban (1998)
Fig. 4
Dip and strike CHIRP profiles (see Fig. 3), from which sample segments “a” and “b” have been enlarged for comparison with previously identified sediment core and underwater excavation stratigraphic compilations within the surveyed area (Reinhardt et al., 2006; Reinhardt and Raban, 2008; Goodman-Tchernov et al., 2009). Three horizons, representing four tsunami events, are recognizable from the available core evidence within the surveyed area (for core locations, see Fig. 1C). Goodman-Tchernov and Austin (2015) |
Description
|
Fallen port architecture | harbor
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021)
Fig. 1
Caesarea harbor, overview (adapted from Boyce et al 2009) Dey and Goodman-Tchernov (2010)
Figure 1
View of ancient harbor area showing rubble spill of ancient break-waters, probable configuration of Herod's harbor, fault lines extending through harbor, and excavation areas. JW: Area K is top left Reinhardt and Raban (1998) |
Description
|
Effect | Location | Image(s) | Description | ||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Tsunami | Offshore Caesarea and Jisr al-Zikra
Fig. 1
Topographic map of the study area, depicting the Crocodile River position, aqueducts, dams, and Carmel Ridge in central Israel (adapted from Reinhardt et al., 2003) Location map of sediment cores offshore Caesarea and Jisr al-Zarka: 1–3, 5, 6 (marked as black hexagons) and Area W underwater excavation (marked as a black square), isobaths are in meters. A surface sample from −50 m below sea level was also collected and is indicated by the * within the upper left inset. Tyuleneva et al (2017)
Fig. 3
Location of sediment cores extracted in 2005 and 2007 Dey and Goodman-Tchernov (2010) |
Fig. 8
Stratigraphic correlation of the core 6 offshore Jisr al-Zarka with representative core 2 (see Fig. 1) from Caesarea (adapted from Goodman-Tchernov et al., 2009). Sea level data are according to Sivan et al. (2001, 2004). Tyuleneva et al (2017)
Fig. 4
Dip and strike CHIRP profiles (see Fig. 3), from which sample segments “a” and “b” have been enlarged for comparison with previously identified sediment core and underwater excavation stratigraphic compilations within the surveyed area (Reinhardt et al., 2006; Reinhardt and Raban, 2008; Goodman-Tchernov et al., 2009). Three horizons, representing four tsunami events, are recognizable from the available core evidence within the surveyed area (for core locations, see Fig. 1C). Goodman-Tchernov and Austin (2015)
Fig. 4
Summary of tsunamigenic characteristics identified in cores and excavations from the shore ('NS') and terrestrial area (`T') to greater depths JW: Later publications redated Byzantine 551 A.D. to 749 .A.D. with possible reworked 551 A.D. deposits. If Roman 115 A.D. deposit is tsunamogenic, it was more likely caused by the early 2nd century Incense Road Earthquake rather than the distant 115 A.D. Trajan Quake Dey and Goodman-Tchernov (2010) |
Description
|
||||||||||||||||||||
Tsunami | Harbor
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021)
Fig. 1
Caesarea harbor, overview (adapted from Boyce et al 2009) Dey and Goodman-Tchernov (2010)
Figure 1
View of ancient harbor area showing rubble spill of ancient break-waters, probable configuration of Herod's harbor, fault lines extending through harbor, and excavation areas. JW: Area K is top left Reinhardt and Raban (1998) |
Figure 2
Stratigraphic sections from excavation areas from intermediate and inner harbor (see Fig. 1 for locations). For biofacies characters and 87Sr/86Sr data, see Table 1. Stratigraphic, foraminiferal, and 87Sr/86Sr data from TN1a, I14, and I9 were reported by Reinhardt et al. (1998a), Yule and Barham (1999a, 1999b), and Raban et al. (1999b). 14C samples were measured at Weizmann Institute of Science, Israel (sample numbers RT2585, RT2631, and RT2650-RT2654) and calibrated to calendar ages using method of Stuiver and Reimer (1993). Reinhardt and Raban (1998)
Fig. 4
Dip and strike CHIRP profiles (see Fig. 3), from which sample segments “a” and “b” have been enlarged for comparison with previously identified sediment core and underwater excavation stratigraphic compilations within the surveyed area (Reinhardt et al., 2006; Reinhardt and Raban, 2008; Goodman-Tchernov et al., 2009). Three horizons, representing four tsunami events, are recognizable from the available core evidence within the surveyed area (for core locations, see Fig. 1C). Goodman-Tchernov and Austin (2015) |
Description
|
||||||||||||||||||||
Collapsed Vault or Walls, Tsunami, and a Fire | Area LL
Figure 1D
Aerial view of the archaeological site and southern part of the Upper aqueduct, where reference samples were collected. All colored dots are linked to locations where samples were taken [as references for non tsunamogenic deposits]. Everhardt et. al. (2023)
Figure 1E
Aerial view of Area LL, bordering the northern side of the inner harbor basin.
Everhardt et. al. (2023)
Figure 3
Plan Ad et al (2018) |
Figure 8
Wall Collapse looking west Ad et al (2018)
Figure 3
Cores C1 and C2 (left) and Southern Baulk section (right) Everhardt et. al. (2023)
Figure 2B
Anomalous layer (the top of which touched the Abbasid floor above) Everhardt et. al. (2023)
Figure 2C
Umayyad archaeological fill directly underlying the anomalous deposit. Inset shows fire-burnt stones in the eastern wall of the corridor, at the same level as the top of the Umayyad archaeological fill. Everhardt et. al. (2023) Core LL16 C1 results.
Everhardt et. al. (2023)
Figure 5
'LL Southern Baulk’ Results.
Everhardt et. al. (2023)
Figure 8
Tsunami corridor. Based on the damage to the southern and southwestern walls and orientation of the collapsed building stones, the dominant destruction came from the southern harbor facing side of the corridor. Everhardt et. al. (2023) |
Description
Site LL is located just north of Caesarea's inner harbour. Ad et al (2018) excavated
the site
reddened, partially heat-fused sand clusterswere in agreement with the presence of reddened in-situ building blocks along the intact eastern wall of the room (and elsewhere along the walls)which indicated that a fire took place before the tsunami struck. They also noted an abundance of charcoal found in the upper Umayyad archaeological fill.They viewed the presence of marine-encrusted potsherds as an indicator that these inclusions were previously submerged in the marine system long enough for the encrustation to take place, suggesting that they were transported from the sea to land at the time of the eventwhich in turn could indicate that the tsunami water and deposits extinguishedthe fire. Everhardt et. al. (2023) proposed that the lower southern baulk was also a tsunamogenic deposit related to 'anomalous" deposit Unit A in the cores.
Footnotes
1 Everhardt et. al. (2023:5) reports that fire-reddened walls (see inset of Figure 2C) were found at
the same level as the destruction layer(s). A single piece of charcoal from the surface of the Umayyad archaeological fill (Unit C) in core C1 has been radiocarbon dated with 95.4% probability to 649–687 cal CE (73.5%) or 743–773 cal CE (22.0%), consistent with the archaeological finds. A second radiocarbon age was measured on a mix of small organic materials from the same layer as the previous charcoal sample, with a result of 605–665 cal CE (95.4% probability). |
||||||||||||||||||||
Tsunami deposit ? | Terraced Gardens
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021)
Fig. 1
Late antique/early Islamic Caesarea, with principal sites and excavation areas mentioned in the text. Dey et al(2014) |
Fig. 14
A deposit of broken pottery in the Roman circus (up to 3 m thick):
Galili et al (2021)
Sign from the park at Caesarea explaining the "Archaeological Deposit". Deposits are described as Late Roman and
Early Byzantine deposited in the 3rd and 4th centuries CE. Dating is presumed to be derived from pottery and stratigraphy.
Click on Image to open a higher resolution and slightly magnifiable image in a new tab Photo by Jefferson Williams - 20 April 2023 |
Description
|
Elias, A., et al. (2007). "Active thrusting offshore Mount Lebanon: Source of the tsunamigenic A.D. 551 Beirut-Tripoli earthquake." Geology 35(8): 755-758.
Salamon, A. and P. Di Manna (2019). "Empirical constraints on magnitude-distance relationships for seismically-induced submarine tsunamigenic landslides." Earth-Science Reviews 191: 66-92.
Variable | Input | Units | Notes |
---|---|---|---|
Magnitude | |||
km. | Distance to earthquake producing fault | ||
Variable | Output - Site Effect not considered | Units | Notes |
unitless | Local Intensity | ||
unitless | Conversion from Intensity to PGA using Wald et al (1999) |
Location | Approx. Distance to Caesarea (km.) |
---|---|
en Feshka (N end of Dead Sea) |
105 |
al-Masraa, Jordan (S end of Dead Sea) |
136 |
Safi, Jordan | 173 |
Taybeh Trench | 235 |
Qatar Trench | 290 |
Variable | Input | Units | Notes |
---|---|---|---|
Magnitude | |||
km. | Distance to earthquake producing fault | ||
Variable | Output - Site Effect not considered | Units | Notes |
unitless | Local Intensity | ||
unitless | Conversion from Intensity to PGA using Wald et al (1999) |
Location | Approx. Distance to Caesarea (km.) |
---|---|
al-Harif Aqueduct | 320 |
Apamea | 350 |
Antioch | 430 |
Variable | Input | Units | Notes |
---|---|---|---|
Magnitude | |||
km. | Distance to earthquake producing fault | ||
Variable | Output - Site Effect not considered | Units | Notes |
unitless | Local Intensity | ||
unitless | Conversion from Intensity to PGA using Wald et al (1999) |
Location | Approx. Distance to Caesarea (km.) |
---|---|
Tyre | 88 |
Sidon | 123 |
Beirut | 163 |
Estimated Epicenter of Elias et al (2007) | 175 |
Byblos | 192 |
Variable | Input | Units | Notes |
---|---|---|---|
Magnitude | |||
km. | Distance to earthquake producing fault | ||
Variable | Output - Site Effect not considered | Units | Notes |
unitless | Local Intensity | ||
unitless | Conversion from Intensity to PGA using Wald et al (1999) |
Location | Approx. Distance to Caesarea (km.) |
---|---|
Bet She'an | 56 |
Tiberias | 68 |
‘Ad, U.; Kirzner, D., Shotten-Hallel, Vardit, and Gendelman, P., 2017, the Crusader Market. Preliminary Report; Hadashot Arkheologiyot
‘Ad, U.; Arbel, Y.; Gendelman, P. Caesarea, 2018, Area LL. 2018; Hadashot Arkheologiyot
Dey, H. and B. Goodman-Tchernov (2010). "Tsunamis and the port of Caesarea Maritima over the longue durée: a geoarchaeological perspective." Journal of Roman Archaeology 23: 265-284.
Dey, H., et al. (2014). "Archaeological evidence for the tsunami of January 18, A.D. 749: a chapter in the history of Early Islamic Qâysariyah (Caesarea Maritima)." Journal of Roman Archaeology 27: 357-373.
Everhardt, C. J., et al. (2023). "Earthquake, Fire, and Water: Destruction Sequence Identified in an 8th
Century Early Islamic Harbor Warehouse in Caesarea, Israel." Geosciences 13(4): 108.
Galili, E., et al. (2021). "Archaeological and Natural Indicators of Sea-Level and Coastal Changes: The Case Study of the Caesarea Roman Harbor." Geosciences (Switzerland) 11.
Goodman-Tchernov, B. N., et al. (2009). "Tsunami waves generated by the Santorini eruption reached Eastern Mediterranean shores." Geology 37(10): 943-946.
Goodman-Tchernov, B. N. and J. A. Austin Jr (2015). "Deterioration of Israel's Caesarea Maritima's ancient harbor
linked to repeated tsunami events identified in geophysical mapping of offshore stratigraphy." Journal of Archaeological Science: Reports 3: 444-454.
Irish, J. L., Weiss, R., & Goodman-Tchernov, B. (2020). A MONTE-CARLO MODEL FOR CAISSON OVERTURNING BY TSUNAMIS.
Coastal Engineering Proceedings, (36v), currents.1.
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at least the Hellenistic Period.
Item | Photos | Description |
---|---|---|
The quay of the Hellenistic northern harbor of Straton’s Tower | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 7
Figure 7
Galili et al (2021) |
The quay (Figures 6a and 7a), described by Raban (pp. 82–84, [48]) is built of headers. It is at an elevation that still enables functioning today, suggesting stable sea-level conditions since the 2nd century BCE. |
Harbor wharves in the central basin | 4
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021) 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 7
Figure 7
Galili et al (2021) |
The wharves were built on the kurkar ridge and they retained their original level [41]: On the south-western side of this basin, a Roman quay was built of headers and it is presently at sea level (Figures 4(1) and 7b). Another quay was excavated by Raban on the northeastern side of this basin and was dated to the Herodian period (p. 86 and Figure 22, p. 115 and Figure 6, [48]) (Figures 4(2) and 7c). Both structures are currently at an elevation that enables functioning. |
A surface built of large ashlars | 4
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021) 7
Figure 7
Galili et al (2021) |
The surface was discovered in the western basin at more than 5 m depth (Figures 4(3) and 7d). This structure was interpreted as a submerged pavement, supposedly indicating that the west basin of the harbor underwent tectonic subsidence and could no longer function as a port (p. 96 and Figure 38a,b [48]; [56–59]). This surface, however, could have been originally built underwater (see below). |
Rock-cut Roman-palace pool | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 8
Figure 8
The rock-cut Roman pool in the reef palace, looking south (for location see Figure 6b). Galili et al (2021) |
The rectangular basin in the southern palace (socalled Cleopatra pool) (Figures 6b and 8) (pp. 217–228, [60]), was interpreted as a swimming pool. It was operated by sea-water and its elevation still enables functioning today. |
Roman harbor installations in the eastern basin | 4
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021) |
A Roman mooring stone and staircase leading to it were found on the eastern quay of the eastern basin (p. 208, [46]) (Figure 4). Their elevation enables functioning today |
Byzantine sewer outlet in the northern anchorage | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 9
Figure 9
Byzantine sewer outlet on the coast and partly submerged in the northern anchorage (marked with red arrows, for location see Figure 6c), and a beachrock ridge designating the location of the coastline before the construction of the harbor (marked with blue arrows, for location see Figure 6f), looking north. Galili et al (2021) |
The Byzantine sewer outlet has been ruined by the advancing sea (Figures 6c and 9). The ruins of this stone-built structure are now scattered along the sea bed to a distance of 35 m offshore. Originally, this indicates the location of the Byzantine coastline at the time that the sewer was still operating, some 1500 years ago. Its present location suggests that the coastline has shifted eastwards since the Byzantine period (p. 20, [41]) (Figures 6c and 9). |
Water wells | A study of tens of water wells at Caesarea suggests that the sea level was constant in the last 2 ky, and that there were no tectonic changes in the region during that period [30,61]. |
|
Stone-built pool near Kibbutz Sedot-Yam | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 10
Figure 10
Stone-built pool near Kibbutz Sedot-Yam, looking north-west (for location see Figure 5d) [43] Galili et al (2021) |
The rectangular stone-built pool that can be filled with sea water by gravity is currently at present sea level (Figures 6d and 10). Given its building style and location (close to the southern Byzantine city wall), it can be dated to the Byzantine period. The structure could have served as a swimming pool. |
Crusader mole in the northern part of the central basin | 5
Figure 5
The Caesarea region
Table 1 [41,43] Galili et al (2021) 11
Figure 11
. Crusader mole in the northern part of the central basin of the harbor:
Galili et al (2021) |
The Crusader mole was built of secondary-used pillars, which were placed on the flat, natural rock (probably abrasion platform). Its elevation enables functioning today (Figures 5d and 11). |
Abrasion platforms | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) |
North and south of the harbor, the coastal kurkar ridge was abraded by the sea and the abrasion platforms are at the same elevation as present sea levels (Figure 6e). The abrasion platforms and wave notches in Caesarea and along the entire Carmel coast suggest stable sea-level conditions over the last few thousand years, since sea levels reached their present elevation, ca. 4 ky ago [12,29]. |
Oysters on the quay of the eastern basin of the Roman harbor | 4
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021) |
The mollusks attached to the stones suggest that during the Roman Period, the water level in the eastern basin was similar to that of today (p. 208, [46]) (Figure 4(5)). |
Beachrock north of the northern Crusader wall | 4
Figure 4
The Roman, Herodian harbor of Caesarea left panel—aerial photo right panel—artist reconstruction [43]
Galili et al (2021) 12
Figure 12
Beachrock north of the northern Crusader Wall:
Galili et al (2021) |
(Figures 4(6) and 12)—A 50 m long deposit of beach rock, with Roman marble chank traps in it, is attached to the kurkar rock at present day sea-level elevations, suggesting stable sea-level conditions over the last two thousand years. |
Beach rock ridge in the northern anchorage (Figures 6f and 9) | 6
Figure 6
Aerial photo of the Caesarea coast
Table 1 [41,43] Galili et al (2021) 9
Figure 9
Byzantine sewer outlet on the coast and partly submerged in the northern anchorage (marked with red arrows, for location see Figure 6c), and a beachrock ridge designating the location of the coastline before the construction of the harbor (marked with blue arrows, for location see Figure 6f), looking north. Galili et al (2021) |
A massive strip of in-situ beach rock deposit, about 2.8 m-thick, is at 0.2–3.0 m below the present sea level. The deposit is located parallel to the coast, some 60 m west of the present shore and the remains of the aqueduct foundations (Figures 9 and 6f). This beachrock probably marks the location of the ancient coastline before the construction of the harbor and the aqueduct, and indicates that the shoreline has retreated horizontally some 60 m eastwards since the construction of the Roman aqueduct. This coastline shift must have occurred under stable sea-level conditions (p. 20, [41]). |
References Cited by Galili et al (2021) |
References
[12] Galili, E.; Sharvit, J. Ancient Coastal Installations and the Tectonic Stability of the Israeli Coast in Historical Times. In Coastal
Tectonics; Stewart, I.S., Vita-Finzi, C., Eds.; Geological Society London, Special Publications: Oxford, UK, 1998; Volume 146,
pp. 147–163. |
kmz | Description | Reference |
---|---|---|
Right Click to download | Master Caesarea kmz file | various |
Right Click to download | Location of Stratton's Tower - kmz file | various |