Abstract
The heart of the book is found in this Chapter, the geology of Nisyros Volcano. The compilation of the new “Geological Map of the Island of Nisyros (Dodecanese Archipelago)” with cross sections serves as the basis for the interpretation of the eruptive history of Nisyros volcano. The volcano-tectonic structures of the 698 m high stratovolcano are marked by the central, almost circular caldera with a diameter of 3.6 km and a drop of 300–400m of its steep walls. This dominant structural feature is crosscut by two conjugate major and three minor fault systems. Since accurate geochronological data are still missing due to the rarity of potassium bearing minerals, such as sanidine and biotite as well as to other petrologic and chemical reasons, the eruptive history can only be based on relative ages of a detailed lithostratigraphy of thirty-two mappable eruptive units. A major division into five volcanic cycles has been devised using eruptive successions, contact relationships, epiclastic deposits and intercalated paleosols. Volcanic activity started with shallow submarine basaltic-andesitic lavas during the “Early Shield Volcano Cycles” evolving into a subaerial environment with local lacustrine lakes. Progressively, a composite stratovolcano built up the circular shape of Nisyros Island, with eruptions on the northern and southern part of the island, the latter with effusion of rhyolitic lava. Along the east coast, mainly explosive eruptions produced two larger tuff cones of andesitic and dacitic compositions. During an evolved stratovolcanic stage, basaltic-andesites and andesites were emitted as lavas and pyroclastics from several smaller cinder, spatter and scoria cones covering the southern, western and northern slopes of the island. The “Composite Stratovolcanic Cycles” ended with the effusion of a large dacitic dome in the northern part of the island, which generated a major dome collapse of the northern slopes into the sea. With an unknown time gap, voluminous eruptions of rhyolitic pyroclastics started from the northern and southern eruptive centers, “Caldera Eruptive Cycles”, followed by a first caldera collapse and successive voluminous rhyolitic lava flows, which extruded towards southeast. The youngest major explosive rhyolitic eruption occurred after an unknown time interval from a northern centre, covering the northern and eastern slopes with major pumice deposits and inducing a second-stage of the caldera collapse. Afterwards, during the “Post Caldera Eruptive Cycle”, voluminous effusions of rhyodacitic magma filled the western part of the caldera with large domes and flows that extend towards the sea, in the southwest. Since then, Nisyros Volcano remains in a dormant stage. Magmatic counterparts, such as gabbroic and dioritic intrusives, as well as mafic cumulates have generated a large hydrothermal system at depth, which is still highly active today.
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3.1 The Geological Map of the Island of Nisyros (Dodecanese Archipelago) (1:15,000 with Geological Cross Sections)
The first geographic and geological studies on Nisyros Island were undertaken by the Italian geologists Martelli (1917), Chap. 5.2, Fig. 5.4 and Desio (1931). Detailed geological investigations started in the late sixtieth (Davis 1967), followed by Di Paola (1974), and Papanikolaou et al. (1991) with geological sketch maps at various scales. Vougioukalakis (1993) presented the first geological map of Nisyros Island on a topographic base in the scale of 1:12,500, which was updated in the Sheet Nisyros, Geological Map of Greece, 1:25,000 (2003) by IGME (Institute of Geology and Mineral Exploration, Athens, Greece).
During the GEOWARN—IST 12310 project (2003) a Topographic and a Geological Map of Nisyros in the scale 1:10,000 with equidistance 10 m contour lines resulted using a completely new digital technology. As basis served an orthorectified 3D IKONOS-2 satellite image from Nisyros volcanic island (2000) with a 1 m resolution on ground, cartographic field mapping and extraction from the topographical map 1:50,000 (Hellenic Military Geographical Service 1972). This work was done by the Institute of Cartography and Geoinformation, Department of Civil, Environmental and Geomatic Engineering, Swiss Federal Institute of Technology, Zurich, Switzerland. The detailed Geological Map of Nisyros Volcano 1:12,500 by Volentik et al. (2005) was the first result of the accurate topography.
The current updated digital and fully vectorised version of the “Geological Map of the Island of Nisyros (Dodecanese Archipelago) 1:15,000 with Geological Cross Sections” represents a compilation of all available former geological data, as well as unpublished results of field mapping during the periods 2000–2003, 2010–2015. The online version of the “Geological Map of the Island of Nisyros (Dodecanese Archipelago)” 1:15,000 with “Geological Cross Sections” as well as detailed descriptions of the lithostratigrapjic units to Chap. 3 are available to authorized users.
Lithostratigraphic units (LSU) with numbers from 1 (lower most outcropping rocks on the island) to 33 (upper most or bounded with unconformity rocks) were used to designate mappable lavas and pyroclastic sequences. The numbering system of the units bears the advantage to the reader to recognize immediately their stratigraphic position. Local names and abbreviations were restricted to a minimum to avoid confusion. On Nisyros Island the same or similar names occur for different localities and have changed throughout time. The grouping and division of units into cycles is based on unconformities, erosional surfaces, interbedded soils and epiclastic deposits.
The map is compatible with the Hellenic Geodetic Reference System GGRS 87 , Datum WGS 84 and the Projection UTM Zone 35N (24E–30E). All geographic features are updated to 2015.
3.2 Volcanic and Volcano-Tectonic Structures
The present-day structural map of Nisyros volcano (Fig. 3.1) comprises volcanic eruption vents, such as necks, inferred dome vents, scoria cones (spatter and cinder cones included), tuff cones and sub-volcanic dikes, as well as hydrothermal explosion craters and emission spots: fumaroles, hot steam, and hot springs.
3.2.1 The Caldera
The most characteristic and dominant structural feature of Nisyros volcano is the caldera with an approximate diameter of 3.6 km (Fig. 3.2). The assumption of its post eruptive collapse origin led no doubts to all precious workers (see introduction) due to its almost circular structure and steep walls with a drop of 300–400 m between the northern and eastern rim down to the Lakki plain of 110 m a.s.l and to the filling of the western part with voluminous rhyodacitic domes up to 698 m. After the recognition of the two major young plinian eruptive cycles, which produced the lower and upper pumice, as well as the large rhyolitic lava flows in the southeast of the island, the discussion focused on caldera formation during one or two collapse episodes (Papanikolaou et al. 1991; Limburg and Varekamp 1991; Vougioukalakis 1998). However, it is possible that the general shape and structure of the present-day caldera resulted from earlier depression, which is indicated by two large stratovolcano flank collapses, prior or simultaneously to the plinian eruptions. Volentik et al. (2005) could establish three older phreato-magmatic to sub-plinian eruptive phases during the early shield volcano cycles, which also emitted large volumes (lithostratigraphic units Nos. 4, 6, 11, Electronic Supplementary Material Appendix 3.3) of pumice fallout, pyroclastic flows, and surges. The existence of two lacustrine cycles could be interpreted as an early internal lake-stage with limited dimensions of probably few hundred meters only (Volentik et al. 2002) as an expression of a depression in north–eastern center of the island.
Despite alteration effects, no large hydrothermal deposits or strong hydrothermal alteration have been recognized as possible earlier indications of high-crustal level magma reservoirs accompanied with a post-eruptive caldera forming collapse.
3.2.2 The Fault Systems
Two major and three minor fault systems can be distinguished within the volcanic edifice of Nisyros Island (Figs. 3.1 and 3.3). The directions are in accordance with previous structural and geological investigations (Papanikolaou et al. 1991; Vougioukalakis 1993; Nomikou and Papanikolaou 2000, 2011):
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(F1, 2) N30E 1st order faults with local changes to NE directions
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(F3, 4) N30W 1st order faults with changes between N0° and N40°W
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(F5) E–W 2nd order faults
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(F6) N–S 2nd order faults
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(F7) WNW–ESE 2nd order faults (approx. 120°)
The NE–SW (F1, 2) 1st order fault system
F1 Fault Zone. It is located along the central part of the caldera comprising two or three parallel fault surfaces with a N30°E strike and a 70–80° dip to the SE. Its throw is more than 100 m and it separates the Profitis Ilias lavas and domes to the northwest from the caldera deposits to the southeast (Figs. 3.1 and 3.7a, b). Its morphological impact is very strong within the caldera and less outside of it. Towards the northeast it is not very prominent and there is no abrupt break of the caldera rim in the area of Emborios village.
F2 Fault Zone. This fault zone is parallel to F1 and runs along the southern caldera wall roughly 1.5 km southeast of F1 (Figs. 3.1 and 3.4). It strikes N30°E and dips 70–80° to the WNW forming a tectonic graben with the opposite facing F1 (Figs. 3.7a, b and 3.8). This graben structure comprises the remnant of the 160,000 years Kos caldera plain with lacustrine and alluvial deposits, known as Lakki plain. Its throw may be estimated to be about 100–120 m, on the basis of the offset of the lavas and pyroclastics of the lithostratigraphic units 17, 21, and 22 (Figs. 3.6, 3.7 and 3.8).
Horizontal displacements of the F1 fault system with dextral strike-slip motion and extension SE–NW have been interpreted from focal mechanisms of major earthquakes (M > 5) at shallow and intermediate crustal depths (Drakopoulos and Delibasis 1982).
The F1 system seems also to have played a major role during the emplacement of the post-caldera dacites (Fig. 3.7a, b). Their eruptive centers are aligned along an N30°–40°E striking fault plane. Since these magmas were derived from reservoirs at deep crustal levels, the F1 fault system must document a zone of weakness reaching the deepest crustal parts. Further evidence of such an interpretation can be taken from the spatial distribution of earthquake epi- and hypocenters.
The NW–SE (F3, 4) 1st order fault system
The major N30 W fault system have steep inclinations of 70°–80° at the surface changing the direction of dips depending on the geotechnical rock properties between NE and NW. These faults run perpendicular to the large Kos horst-graben system (Figs. 3.1, 3.9, 3.10 and 3.11). Characteristics of this fault system are extensional features and downfaulting up to 70 m. They extend from the northwestern parts of Tilos Island into Nisyros Island in the area of Avlaki , crosscut the entire island, run along the western part of Yali and merge into Kos Island at the “Paradise bubble beach ”.
The F3 fault zone is located in the northwestern part of Nisyros Island with a general trend to N30°W and dip 70–80° to the NE (Figs. 3.9 and 3.10). It juxtaposes different stratigraphic formations both within and outside the caldera. Inside the caldera it separates the main outcrops of the Profitis Ilias lava domes from the smaller domes to the northeast whereas outside the caldera it separates the outcrops of white pumice to the down faulted block in the northeast from the uplifted block in the southwest (where the pillow lavas No. 1 occur just above sea level). Its throw is more than 100 m.
The Mandraki fault runs parallel to the F3 fault zone at a distance of about 1 km to the southwest. The kinematic characteristics of the two faults are similar, with a general strike in the NNW–SSE direction and dip towards the ENE. The Mandraki fault is normal with a throw of about 100 m a.s.l indicated by the offset of the characteristic stratigraphic formations (Fig. 3.11a, b). The western block is topographically higher by 100 m and hosts the two important monuments of the island, which are the ancient castle of 4th century B.C. and the Panaghia Spiliani Monastery within the Byzantine/Venetian castle. The eastern block comprises the town of Mandraki with its westernmost buildings reaching the valley running along the Mandraki fault known as “Langhadi ”.
In continuation, a series of NW–SE parallel faults cut the Nisyros Island in the area of Avlaki and Aghia Irini (Figs. 3.1 and 3.6). Best evidence for downfaulting of the Aghia Irini block can be taken from the offset of the southern caldera rim. The fault system runs through the Stefanos Crater extending into the hydrothermal craters of Mikros Polyvotis and Megalos Polyvotis. One branch cuts through the domes of Profitis Ilias and Nifios into the northwestern crater rim and splits into several minor faults west and east of the Monastery Evangelistra . There, the system forms a series of step-like downfaulted blocks between the Monastery Spiliani, the town of Mandraki and Loutra.
The F4 fault zone on Nisyros defines a tectonic graben, striking N20W, consisting of two conjugate faults with opposing dips. This fault zone is younger than the Nikia rhyolites (No. 30) and its throw is about 40–50 m. These fault zones of Nisyros Island produce a number of neotectonic blocks, each characterized by its relative uplift or subsidence (Fig. 3.3). The maximum uplift is observed in the western block/horst bounded by the F1 and F3 fault zones, which incorporates the maximum elevations of Profitis Ilias and surrounding summits. The maximum subsidence is observed in the southern block/graben of Aghia Irini, bounded by the F1 and F2 parallel fault zones.
All hydrothermal explosion craters are located in the intersections between the conjugate fault system F1, F2 and F4. At the northern and southern extensions of the F1 system, hot springs occur at sea level (Cape Katsuni and Thermiani in the north and Lefkos in the south). It is obvious from the bathymetric digital elevation model (BDEM) that these faults extend northeastward into the eastern Kos basin bordering the down-faulted slopes of Kos and the peninsula of Datça .
The rest of Nisyros Island constitutes the large neotectonic block of Emborio/Nikia, east of the F3 and F4 fault zones, with intermediate kinematic character since it has subsided with respect to the western block but has been uplifted with respect to the southern block. The Emborio area of the block is made of the stratovolcano stratigraphic formations, whereas the Nikia area is made of the Nikia rhyolite flows. A minor neotectonic block bounded by the F2 and F4 fault zones is observed in the southern part of Nisyros at the area of Avlaki with transitional character between the Aghia Irini and the Emborio/Nikia blocks.
The E–W (F5) 2nd order faults
The E–W oriented fault system seems to occur at present only at a local scale (Figs. 3.1 and 3.32a) and might represent a result of the deep reaching conjugate fault system F1 and F3. Surface expressions are visible along the north coast of Nisyros at the town of Mandraki, between the harbors Mandraki and Loutra, between Pali and Faros , along the western Karaviotis lava flows bordering the Kateros cove and in the valley between the Monastery Panagia Kyra and the southern border of Pachia Ammos beach . The hot spring of Afionas at sea level might also be a result of this fault system.
The N–S (F6) 2nd order faults
A subordinate N–S fault system can be locally established in the volcanic edifice of Nisyros Island (Fig. 3.12): Along the northwest coast, between the rhyodacitic domes of Karaviotis and Trapezina and at Cape Akrotiri . According to the bathymetric map (BDEM) the latter fault seems to extend into a small N–S graben between Yali and Strongyli (Fig. 2.6, Chap. 2). An equivalent system appears to also be present in the peninsula of Kefalos on Kos. Similar to the F4 system, the N–S might also be a result of the dominant conjugate F1 and F3 systems.
3.2.3 The Lakki Rupture 2001, 2002, and 2011
3.2.3.1 Annual Episodes of Rupturing
A large N–S trending fracture (“Lakki rupture ”) opened in the Lakki plain of the Caldera in early December 2001 (Figs. 3.13 and 3.14). Although this large rupture extended over a distance of 350 m and up to 5 m wide and up to 10 m (in few cases 20 m) deep, neither gas and thermal waters were recognized nor seismic signals were recorded. In December 2002, the fracture continued to extend southward for another 500 m showing smaller perpendicular offsets (Fig. 3.15). During a heavy rainstorm during November 12/13, 2011 another large rupture was formed (Figs. 3.16 and 3.17) intersecting the 2001/2002 rupture in the central part of the Lakki plain. The direction of the new rupture was NNW–SSE with approximately 320o, starting in the south as reactivation of the 2001 rupture and continuing for approximately 450 m towards NNW crossing the road. The northern and the southern parts of the old rupture were not affected.
3.2.3.2 Interpretation and Origin of Ruptures
The rupture is interpreted as surface stress release in the consolidated and cemented epiclastic and hydrothermal sediments of the caldera floor, due to progressive uplift and East–West extension of the central parts of the island since the seismic crisis 1996/1997 and a possible magma input at greater crustal depth (GEOWARN project 2003). No significant earthquake activity has been recorded during the formation of all ruptures.
In addition, subrosion by meteoric waters and their drainage from large cavities and tunnels several tens of meters beneath the Lakki plain may have enhanced the stress release, leading to breakdown of ruptures and “doline type” holes (Fig. 3.13, location D). This interpretation is favored by the timing of the rupture formation after a long dry summer and fall during and shortly after the first large rainstorm in the beginning of wintertime (e.g. ruptures: 12/2001, 12/2002 and 11/2011).
The direction of the 11/2011 ruptures coincides with well-known NW–NNW trending fractures and faults cross cutting the island. Therefore, deeper zones of weakness in the island, expressed in form of fractures and faults enhance the weakening of the Lakki plain. However, the new rupture must be regarded as a simple surface phenomenon, since no heat, gases and hot waters have been recognized.
According to all observations, the Lakki rupture does not indicate any volcanic phenomena or reactivation of magmatic activity at depth.
3.3 Detailed Lithostratigraphy of Nisyros Volcano
Volcanoes in oceanic and continental arc environments are built up mainly by eruptions of water-bearing ranging from basalts to rhyolites and eruptions of typically volatile-rich magmas. The life-time of a single volcanic edifice can vary from thousands to several millions of years depending on the geotectonic and geodynamic environment, thickness and constitution of the crust, and consequently on the emplacement and differentiation mechanism of the magmas through the crust to the surface (Hildreth 2007). The construction of these volcanoes occurs during eruptive episodes, that typically follow a cyclic pattern: An eruption generally starts with hydro-magmatic explosions, is followed by phreato-magmatic eruptions producing mostly fallout deposits and surges, then grades into magmatic explosive activity, feeding surges and pyroclastic flows, before, final emplacement of degassed lavas forming, domes and necks. These eruptive cycles are then followed by periods of dormancy, during which magma reservoirs get refilled. Hydrothermal activity can be important while the volcano is dormant, and the edifice typically undergoes intense erosion, sometimes catastrophically by flank collapse.
As the Nisyros volcanic history is based on the litho- and tephrostratigraphy of the edifice (mostly defined by the mapped lavas and pyroclastic rocks), it is best to describe it using these cycles of eruptive activity, separated by epiclastic deposits and the paleosols, which mark the periods of dormancy (Table 3.1). Depending on the state of development of these volcanoes, one can find initial, embryonal stages with short cycles of years to hundreds of years, and more evolved stages, composed of numerous equivalent short eruptive cycles merging into a major cycle with long temporal intervals.
The detailed lithostratigraphy of the Geological Map of the Island of Nisyros is given in the Electronic Supplementary Material Appendix of this chapter.
3.4 The Eruptive History of Nisyros Volcano
3.4.1 Introduction
The island of Nisyros is a Quaternary composite stratovolcano located at the easternmost end of the Aegean volcanic arc, in the Dodecanese archipelago, south of Kos. The island is almost circular, with an average diameter of 8 km, covering an area of about 42 km2. It lies above a basement of Mesozoic limestone (Geotermica Italiana 1983, 1984) and a thinned crust, with the Moho located at a depth of about 27 km (Makris and Stobbe 1984). The references of previous studies in volcanology, petrology, geochemistry of volcanic rocks, fumarolic gases and hydrothermal waters has been listed chronologically at the end of this chapter; geological maps have been published by Di Paola (1974), Papanikolaou et al. (1991), Vougioukalakis (1993, 1998, 2003), GEOWARN (2003), Volentik et al. (2005).
The volcanic edifice of Nisyros with a summit caldera of a 4 km average diameter is the result a large variety of explosive and effusive eruptions producing calc-alkaline pyroclastic deposits and lavas from basaltic andesitic, dacitic, rhyodacitic, and rhyolitic composition. According to previous studies, the volcanic history has been generally assigned to four major episodes: starting with shallow marine to subaerial basaltic to andesitic volcanism followed by moderate andesitic explosive and effusive activity, building up a first major strato-cone surrounded by several satellite eruption centers (scoria and tuff cones). The present morphology of the island is finally due to two major rhyolitic plinian explosive phases each accompanied with consecutive effusive voluminous lava flows and domes, which may have followed the caldera collapses.
3.4.2 Early Shield Volcano Cycles of Nisyros
3.4.2.1 Submarine Volcanic Base
Nisyros is entirely volcanic: metamorphic or sedimentary rocks have been mapped anywhere on the island. Geothermal drilling from the lowest part of the caldera in the Lakki plain (Well NIS 1 in the southeastern side at 110 m altitude asl and NIS 2 at the eastern foot of the young rhyodacitic Lofos dome at the western side at 145 m a.s.l) reached Mesozoic limestones at a depth of approximate 650 m depth bsl. The 750 m caldera filling consist of unconsolidated talus and alluvial deposits in the upper 150 m and poorly-documented tuffs, pyroclastic flows intercalated with basaltic to andesitic flows and epiclastic breccias in the last 600 m (Geotermica Italiana 1983, 1984). The evolution of the volcanic history of Nisyros Island described in this paper is solely based on the outcropping litho- and tephrostratigraphic successions.
The oldest occurrence of volcanic activity is represented by a shallow submarine to subaerial formation of hyaloclastites (LSU No. 1), pillow breccia, and pillow lava of up to 50 m thickness in the north–western corner of the island in the cliffs of Monastery Panagia Spiliani at Mandraki and in the western coastal part between Hochlaki beach (Fig. 3.18) and Cape Kanoni (Fig. 3.20). The hyaloclastics and loosely packed pillows and pillow breccia appear to be the front of subaerial basaltic andesite lava flows, which covers the brecciated units. A few dikes cut the whole formation; internal tilting and faulting is present. Extrusions from submarine fissures seem to be unlikely, since no typical close-packed pillow lava is present. To produce such high amounts of pillow breccia and hyaloclastic, palagonized material, an explosive origin from shallow submarine a subaerial vents, similar to processes forming peperites (Skilling et al. 2002; de Goer de Herve 2008) are envisaged. Such a process might be supported by intercalated lava lenses of variable thickness (up to 10 m) within the pillow-hyaloclastic sequence, partly mixed with intensively hydrothermally altered tuffs and tuffites (LSU No. 2, Fig. 3.20). The outcrops occur at Cape Kanoni and along its southern coastal strip. Since they are aligned to NE–SW (approx. 30°) tending faults, they could also be interpreted as channel fills.
Similar volcanic and volcanoclastic sequences have not been clearly linked to specific units in the geothermal wells. However, between −480 and −540 m b.s.l depth, breccias and a fine tuff/tuffite occurs on top a several ten meter thick “blocky tuff in a palagonitic matrix” (−540 to −585 m b.s.l). These units are suspiciously similar in two ways, and either they represent equivalents of the KIU-formation, the “Kos acoustically incoherent unit within the sedimentary cover in the west- and east Kos basins (Fig. 2.10) as part of the 161 ka Kos-Plateau-Tuff (KPT ) eruption cycle (Stadlbauer 1988; Smith et al. 1996; Allen 2001; Bachmann 2010), or local eruptive equivalents of the early volcanic cycles of Nisyros Island.
A paleogeographic reconstruction of the volcanic environment is difficult to achieve because of the lack precise data from the geothermal drill holes in the caldera. However, the thickness and extension of the “hyaloclastite formation” units Nos. 1 and 2 allows to establish a volcanic edifice similar to a subaerial shield volcanic structure, most probably with vents aligned a NE–SE trending fracture zone from were the lavas were emitted. In addition, a tilting towards NW is obvious due to unconformities in the hyaloclastite formation, e.g. within the uplifted cliffs of the M. Panaghia Spiliani.
The autobrecciation of the atypical pillow lava and pillow breccias without typical glassy rims und textural changes between outer and inner parts of the pseudo-pillow fragments leads to an interpretation either of water intrusion into the vents at very shallow aquatic levels or lava into muddy tuffaceous sediments, and thus instant brecciation. Similar brecciation processes have been described for the formation of peperites within small volcanic maar-lakes (for review see Skilling et al. 2002).
Up to now, no marine fossils have been found within the yellowish palagonitic matrix.
3.4.2.2 Early Nisyros Shield Volcano Cycles
The following volcanic activity comprises three major cycles, producing pyroclastics and lavas with basaltic andesite composition, but slightly different in their eruption characteristics. The exposures of these cycles are limited to the eastern parts of the inner caldera cliffs between Kato Lakki and Chonia and represent mainly proximal facies deposits (Figs. 3.21 and 3.22). Time intervals between these cycles must have been short, as erosional contacts or signs of paleosol are missing.
At the north–eastern lower part of the inner caldera above the Lakki plain, a subaerial lava flow up to 35 m thick and covering a distance of 1.2 km, records a first major subaerial eruption (unit No. 3). The lower part appears in several places strongly tectonised, which likely indicate recent faulting, such as break down and collapse of the caldera. It is possible that this cycle started with a major strombolian eruption, producing surges and pyroclastic flows, although such deposits are not preserved due to the coverage with talus and alluvial filling of the caldera. Papanikolaou et al. (1991) have correlated this lava flow with the stratigraphically lowermost basaltic andesite pillow and hyaloclastite sequence at the north–western corner of the island.
A second eruptive cycle (Fig. 3.23), producing ca. 35 m of pyroclastic deposits during a violent explosive phase (unit No. 4) seems to have started within a short time interval after the effusion of the underlying lava. The eruption started with a typical sub-plinian phase followed by a sequence of fine-grained pyroclastic flows and surges and terminated again with sub-plinian eruptions. The subsequent effusion produced an up to 40 m thick lava flow with a basaltic andesite composition (unit No. 5).
The explosive phase of the third cycle (unit No. 6) started with the deposition of coarse-grained planar-bedded surges indicating a high water/magma interaction ratio. After a short period of fallout, two thick pyroclastic flows, disrupted by two coarse-grained surges, planar bedded and with sandy-waves, were deposited.
The geometrical distribution and chemical similarity of the volcanic edifice produced during these three eruptive cycles during one consecutive period of time leads to the assumption of the generation of a subaerial shield volcano with a maximum diameter of several kilometers and a height of a few hundred meters. The large volume of erupted material during the third cycle, producing up to 60 m of pyroclastic deposits, the high lithic content of large fragments with an average size of 25 cm in the upper pyroclastic flow and the dip of the underlying lavas with respect to the present day caldera depression, support a collapse of the early shield volcano, leaving a small caldera behind (Volentik et al. 2002).
The geometric distribution and thickness of the lava and pyroclastics allow to a certain extent a reconstruction of the early volcanic edifice. A subaerial volcanic shield with a center more or less in respect to the present day caldera seems to be the most feasible interpretation. The lavas show slight inclinations and reduction of thickness outward. Indication of the position of the original vents can only be taken from the direction of a few dikes in the north–eastern caldera wall, which trend N 70°E. We assume that at this early volcanic stage the general structural trends and tectonics of the regional volcanic field controlled the emplacement of magmas from the upper mantle through the crust to the surface. The conjugate faults, N30°E and N20°W seem to have played the most important role.
3.4.2.3 Internal Lake-Stage and Associated Volcanic Cycles
In the north–eastern part of the internal caldera cliffs between Kato Lakkì— Ghonia and on top of the three pyroclastic and lava cycles described above, two volcanoclastic, lacustrine sedimentary successions (LSU Nos. 7, 9) are found (Figs. 3.24 and 3.25). They are continuous over a distance of five hundred meters, divided by a few meters thick subaerial basaltic andesite lava (unit No. 8), indicating the presence of an “internal lake” within a period of minor volcanic activity. The fact that the lower contact of the intermediate lava flow is very sharp and without any sign of scoria or development of pillowed breccia shows that the early lake must have been shallow.
The varved beds of the two intra-caldera lakes and associated volcanic cycles indicate sedimentation of volcanic ashes and fine-grained lapilli mixed with sandy layers within an aqueous system (details in Electronic Supplementary Material Appendix 3.3; Volentik et al. 2002). Characteristic maar-type phreatomagmatic sedimentary structures have not been observed. These sediments seem to be limited in their lateral extension to the north–eastern segment of the caldera, since they are absent in other similar stratigraphic positions inside the caldera wall. Surge deposits are few in the lowest part of the section, but become abundant at the upper part. The lifetime of the two lacustrine cycles could not have exceeded several hundred to a thousand years due to the restricted thickness of the varved successions.
The lake stadium was terminated by an effusive cycle (unit No. 10), which produced several basalt-andesitic flows with scoriaceous base and top, building up 70 m of the northern and north–eastern caldera walls (Fig. 3.26), forming the cliffs below the village of Emborio, and cover the eastern slopes towards Kremastos . Since these units are also exposed in the southern inner caldera cliffs, although with reduced thickness, they likely represent the filling of the early caldera with a diameter similar but smaller than the present day one. The neck west of the Kato Lakki plain can be seen as one of the eruptive centers.
Soon after the end of this effusive episode, a major explosive cycle started from a vent most probably located within the northern part of the caldera, covering the northern and eastern slopes of the island with 35 m of pyroclastic deposits (unit No. 11). This cycle started with a high explosive sub-plinian activity erupting a characteristic red pumice fall-out and intermittent fine-grained surges followed by strong pyroclastic flows including large blocs of lithics and pumice at their base.
The cycle terminated with a minor surge and fallout. The growth of a stratovolcano on top of the relicts of the early caldera may have been the result of the last strong explosive cycle. Minor epiclastic deposits (unit No. 12), which contain reworked material of the underlying pyroclastic succession, indicate both a time gap of volcanic activity permitting erosion and tectonic movements, e.g. local uplift between the NE corner and central part of the island and could be interpreted as bulging effect of a magma emplacement in the upper crust.
3.4.3 Composite Stratovolcano Cycles
3.4.3.1 Transition from Shield Volcano to Stratovolcano (Northern and Eastern Eruptive Centers)
After an unknown time gap, several short volcanic cycles contributed to the growth of a stratovolcano, erupting more evolved magmas from a central vent and from peripheral volcanic vents more or less aligned along the major regional fault systems (N30–50°E & N30°W; dike N20°W). This volcanic period can be limited between the early epiclastic deposits (unit No. 12) and the wide spread epiclastites and conglomerates of Paleokastro (unit No. 23) and with a sequence of three dominant lava flows (LSU Nos. 13–15) derived from northern and eastern central eruptive centers (Fig. 3.27). These flows form the upper parts of the caldera walls in the northern, northeastern and eastern segments and cover the north–western slopes down from Monastery Evangelistra and the eastern slopes between the areas of Linevrochia and Kremasto .
During this new cycle, more differentiated (andesite and dacite) magmas reached the surface. The first, 40 m thick andesitic lava flow (unit No. 13, Fig. 3.28) was emitted from a main central vent, since it appeared all around the upper caldera walls with the exception in the southwest, where the young Profitis Ilias rhyodacitic lava flows probably cover it. An andesitic neck and a small scoria cone in the upper eastern slopes close to the present day caldera rim represent two additional satellite eruptive centers.
A 25 m thick dacitic lava flow (unit No. 14), which covered the andesitic lava without any observable time break, erupted most probably from the same central vent. It is present from the village of Emborio throughout the northern and eastern segments of the upper caldera cliffs and extends towards south in the cliffs below the village of Nikia. This unit contains up to 30% of andesitic inclusions with both reddish and grey colors. The grey enclaves appear quenched, and likely indicate the reinjection of andesitic magma into a dacitic reservoir. The red oxidized andesitic inclusion, in contrast, are interpreted as older lithic material incorporated into the dacitic magma during the emplacement.
The final, 40 m thick andesitic lava flow (unit No. 15) forms the top of the “lava trilogy cycle” with a thick base of red scoria. It covers mainly the upper northern segment of the caldera and parts of the northeastern slopes of the island.
3.4.3.2 Southern Eruptive Centers (Monastery Stavros —Avlaki)
The following volcanic sequences can mainly be assigned to remnant eruption centers, which are exposed in the southern segment of the caldera walls below the Monastery of Stavros and cover the southern slopes (between the coves of Lefkos in the southwest and Aghios Nikolakis , Avlaki) with pyroclastic flows and lava (Figs. 3.27 and 3.29). They are assigned to one eruptive cycle slightly younger than the previous “trilogy cycle”. The beginning of this cycle starts with a 30 m thick basaltic andesite pyroclastic succession of several small base surges of grey lapilli followed by pyroclastic flows, rich in andesitic lithics (unit No. 16). The strong hydrothermal alteration, within this unit (including the lithics) requires the existence of a larger magma reservoir at higher crustal depth and heat supply to a hydrothermal system.
The cycle ends with the effusion of voluminous, up to 40 m black, massive, partly glassy, and perlitic rhyolitic lava flows (unit No. 17, Fig. 3.30). The Tsimi neck west of the Village of Nikia at the southern caldera rim marks one eruptive center of the blocky lava. Other vents are probably covered by the young rhyodacitic domes and lavas in the southwestern segment of the caldera.
The different trends of the dikes N20°, 50°, 70°E; N10, 20°W, as well as the measurable faults N30°, 70°E and N60°W indicate a complex extensional system along which the magmas were emplaced.
3.4.3.3 Eastern Eruptive Centers (Tuffs Cones of Kyra—Afionas; Kremastos —Lies —Evria )
The eastern flanks of the island comprise several similar eruptive cycles represented by successions of surges, pyroclasic flows and fallout which may have been derived from at least two major eruptive centers, the hills of Afionas and Lies, both remnants of large tuff cones (Fig. 3.27). Most of the unconsolidated tuffs have been eroded and washed down into the sea during rainstorms and mudflows, causing small frontal deltas and submarine channels close to the shore. In addition, the entire area of the eastern slopes resembles a large down-faulted block between major regional fault systems (Fig. 3.29 and structural Sect. 3.2). The two cones tuff cones seem to have been aligned along N20°W faults intersecting N50°E faults. A dike strikes N80°E.
Their ages cannot be precisely determined by lithostratigraphy. On the eastern slopes, these successions overlay older andesitic and dacitic lavas derived from the eastern caldera walls (the “trilogy cycle”, units Nos. 13–15), while, to the South, everything is covered by the thick younger rhyolitic lavas flowing down from the south–eastern caldera rim. Only one light grey dacitic flow (unit No. 18), occurring at sea level along the shore at the base of Afionas tuff cone over a distance of 300 m between the beaches of Lies and Pachia Ammos , could be correlated with the first dacitic flow of the island (unit No. 14). However, this flow has slightly different petrographic characteristics (e.g. the lack of abundant andesitic inclusions). Over a distance of 150 m, the surface of this grey dacite contains up to 1.6 m deep pockets filled with a strange brecciated fine-grained whitish rhyolitic flow with irregular enclaves of “andesitic schlieren” and mafic cumulates. In places, the yellowish color indicates the formation of a paleosol.
The andesitic to dacitic pyroclastic successions of the Afionas tuff cone (No. 19, Figs. 3.31 and 3.32), with a maximum thickness of 80 m, comprises at least three major explosive cycles from the same vent, separated by erosional contacts and thin paleosols. The deposits consist of light gray surges, proximal strombolian fallout and minor pyroclastic flows. The fallout contains lithics of andesite lava fragments and cumulates, in addition to limestones and contact metamorphic marbles and calc-silicate skarns. The fresh lithic andesitic fragments suggest that a recharge of andesitic magma into a dominantly dacitic reservoir occurred shortly prior to the eruption. A detailed stratigraphic description is given in the Electronic Supplementary Material Appendix 3.3.
3.4.3.4 The Composite Stratovolcano (Mandraki—Pali—Kremares)
Lavas and pyroclastic deposits from the growing composite Stratovolcano occur throughout the island, typically in lateral cones, and are associated only in parts with the underlying sequences. They include remnants of cinder, spatter and scoria cones. This random distribution indicates that smaller eruption centers as lateral vents from radial feeder dikes could were formed around a central growing stratovolcano within the limits of the early caldera. The deposits from the peripheral vents contributed to the growth of the entire island.
The locations of the vents seem to be controlled at the by main fault pattern, N30°E, N70°E, as well as N30°W, N60°W, and E–W (Fig. 3.33).
The duration of this volcanic activity period can only be estimated by relative litho-stratigraphy and by the appearance of erosional features and paleosols. Since the latter time markers are missing, a rather short time period of several hundred to a few thousand years is envisaged. This assumption is compatible with the occurrence of the basal debris flows on the eastern flanks and in channels (unit No. 20), which require uplift, leading to massive (up to 20 m thick) debris flow deposits of reworked underlying pyroclastics (unit No. 19), channeled within deep valleys in the eastern flanks.
In addition, remnants of basaltic andesite cinder/scoria cones of strombolian activity have been recognized all over the island (unit No. 21, e.g., East of Ag. Marina and east of Koftaka (western flanks), south and north of M. Evangelistra, west of Akimaronas at the caldera rim, at Linevrochia and Kremastos on the eastern flanks (Fig. 3.34), at M. Stavros and at Tsimi on the southern caldera rim, and north of Avlaki in the southern flank (Fig. 3.35).
These small individual eruptive cycles have been combined into one up to 20 m thick pyroclastic unit of black lapilli, red and black scoria fallout deposits, spatter cone facies with agglutinated fragments of fresh lava and of planar-bedded surges (Fig. 3.36). In few cases, proximal thick and unsorted basal fallout deposits indicate violent strombolian eruptions as early phases. Often the scoria cone deposits contain abundant lithic components, such as fresh andesitic lava, anorthositic and amphibole-pyroxene-rich cumulates, limestones, contact metamorphic marbles and skarns. Several small basaltic andesite lava flows (unit No. 22) with individual thickness up to 10 m are closely associated with pyroclastic deposits described above and have originated as effusive part from the same spatter and scoria cones.
The stratovolcano period probably ended with a major summit collapse since up to 20 m thick debris flows with hyper-concentrated flow deposits occur on western and northern slopes. The latter process also required strong central uplift and tilting towards W, NW and N, which also favored the formation of beach conglomerates (unit No. 23) at the north–western corner of the island.
3.4.4 Terminal Cycle and Dome Collapse
The following volcanic cycle, subsequent to the stratovolcano cycles and after a significant period of dormant activity, can be bracketed by the appearance of epiclastic debris flows at its base and by the large « Loutra » debris avalanche as a result of a collapse of the northern caldera rim, probable at the end. These cycles differ from all previous volcanic cycles because of the dominance of their effusive eruption styles. Large volumes of differentiated lavas contributed to the filling of the northern sectors of the caldera and coverage of the northwestern and northern slopes of the island (Fig. 3.37). The cause of the dramatic change of the eruptive mode from all previous strombolian to sub-plinian explosive cycles to mainly effusive cycle is not clear, but it might be related to a sudden change in the geotectonic environment or to a major change in the magma reservoir.
Evidently, all lavas cover large portions of the upper slopes of the northern half of the island and may have derived from fissures and eruptive centers along a northern early caldera rim controlled by faults N30°E and N30–50°W generating intersections, thus extensional ways for magma emplacement. In addition, strong uplift of the central and south–eastern parts of the island is required to facilitate the east- and northward flow directions of all lavas. An associated process was the doming of dacitic magmas in the resurging caldera after the stratovolcano collapse.
During the first effusive cycle, a series of thin basaltic andesite-to-andesite lava flows with a total thickness of ca. 25 m (unit No. 24) was emitted from vents aligned along the early western caldera rim and covered the western slopes down to the sea. The second effusive cycle produced large volumes of dacitic lava flows with a thickness up 150 m, the “Emborio” lava dome and a neck (unit No. 25).
The time gap between the terminal caldera cycle and the collapse of the northern caldera rim is difficult to establish. The most plausible hypothesis favors a collapse after the emplacement of the voluminous dacitic lava flows. At the base of the chaotic collapse breccias, a 0.3–1 m horizon of dacitic ejecta with normal gradiation and fragments of dacitic lava have been observed in certain places. This deposit is interpreted as an indication of the start of a new cycle, emplacement of new magma from depth and bulging of high crustal levels.
The giant debris avalanche deposit (unit No. 26), named after the most diagnostic type locality “Loutra”, reached variable thickness depending on the pre-existing morphology of the northern slopes between Mandraki and Pali (Figs. 3.37, 3.38, 3.39 and 3.40). The most characteristic megascopic feature of this large epiclastic unit is the hammocky topography, forming small hills of 20–30 m heights in the lower slopes along the shore. In fresh road cuts and in the cliffs along the shore, the chaotic internal structure of these unconsolidated deposits is evident. Fragments are mostly of dacitic composition, but rare pieces of andesites and red scoria from earlier strombolian eruptive cycles are also found.
An isolated andesitic lava flow, ~7–10 m in thickness (unit No. 27), appeared after the emplacement of the “Loutra” avalanche in the slopes of Loubounia (south of Loutra). It seems that the flow poured out of a fissure inside a scarp, produced by the Loutra avalanche. Apparently this flow marks the last andesitic eruption in the volcanic history of the island.
3.4.5 Caldera Eruptive Cycles and Caldera Collapse
A paleosol covers in many places the debris flows (unit No. 23), the dacitic lavas of Emborio (unit No. 25) and parts of the “Loutra” debris avalanche (unit No. 26). This is the indication that a large time interval and repose period occurred between the last dacitic and andesitic magmatic activity and the beginning of a major cycle of high explosive activity from highly differentiated rhyolitic magmas. During the “Caldera Eruptive Cycles”, two vast successions of rhyolitic pumice derived from plinian eruptive cycles, designated as “lower and upper pumice”, were deposited and divided by epiclastic deposits, the effusion of voluminous rhyolitic lava flows and the breakdown of a large caldera to the present day dimensions (Fig. 3.41). The lifetime of volcanic activity of each individual cycle, as well as of the total time-span is still not known, despite the occurrence of two widespread paleosols separating these two cycles, well exposed at Cape Katsouni (Fig. 3.42).
3.4.5.1 First Eruptive Cycle
The first voluminous (up 20–30 m thick) rhyolitic pyroclastic sequence, the “First Eruptive Cycle”, designated as “lower pumice” (unit No. 28) resulted from a major plinian eruption and were deposited all over the island. Major occurrences are still present on the southern slopes, because of lack of coverage with younger pumice deposits (Fig. 3.41). However, no stratigraphic contacts occur to the northern and eastern equivalent of the “lower pumice units”. Both are overlain by a paleosol and the large eastern rhyolitic lava flows (unit No. 30) of the second eruptive cycle.
Explosive phase
The explosive phase of the “lower pumice” LP can be divided into (1) in the lower part, plinian fall deposits, which contain lag breccias and up to 50% of lithics (some up to meter size) (unit No. 28a and b) and (2) in the upper part, poorly bedded fall layer with surges and pyroclastic flows (unit No. 28c). Both parts were probably deposited during one eruptive event since no major unconformity has been recognized within the deposits. The lithics include metamorphic limestones, skarns, hydrothermally altered rocks, unaltered volcanics and mafic cumulates, thus witnesses of a larger magma reservoir and an existing hydrothermal system. Yellowish weathering is a widespread feature within the “lower pumice”. A chaotic debris-avalanche deposit has been recognized in the south–eastern coastal cliffs and along the beach at Ghrana bay over a distance of at least 500 m overlaying the basal pumice fallout flows indicating a southern slope failure during the initial phase of the first plinian fallout (Fig. 3.43).
Two eruption vents may have occurred in areas between the present southern and northeastern caldera rim aligned to a N30°E trending fissure and intersecting a N60°W faults (Fig. 3.41). The wide distribution of large fallout pumice blocks and lithic fragments, the presence of lag-breccias, poor bedding and sorting, as well as the greatest amount of fine-grained ash indicates proximal deposition in the southern part (Fig. 3.44a, b). In contrast, the plinian fallout of the northern part along the north and east cost exhibit more distal features (large lag breccia but thinner deposits, smaller diameters of pumice blocs and lapilli, sorting, reverse grading, and much lower lithic contents; Fig. 3.45). In addition, small ash- and mudflows occur.
The uneven areal distribution in grain size of the lower pumice pyroclastics on the island and the scarcity of the lower pumice deposits at the western half of the islands suggest an uplift of the western area during or shortly after the eruptive “lower pumice” cycle. Additional evidence of the uplift exists in the appearance of debris flows, mainly on the northern half of the island (unit No. 29), with components of lavas, pyroclastics and pumice (No. 25–28). All deposits are covered by a paleosol.
First Caldera Collapse
The “First Caldera Collapse” can only be estimated in space and time. We tend to place the collapse after the vast explosive phase. The highly differentiated rhyolitic magma may have been derived from rather shallow reservoirs in the upper crust (see later chapter of petrology and magma dynamics). As consequence of eruption the large volume deficiency could have generated a surficial depression and thus, initiated a first collapse that caused a first caldera. In addition, a major break in the steep morphology into two steps of the south–eastern caldera walls indicates a breakdown along slightly concentric normal N30°E striking fault before the extrusion of the rhyolitic flows (Fig. 3.41). The subsequent emplacement and doming of rhyolitic magma in the south–eastern part of the first caldera may have triggered a large flank collapse, (“Nikia Flank Collapse”) and causing a major debris avalanche similar as the one on the northern half of the island (“Loutra” debris avalanche”). The voluminous rhyolitic lava flows do not flow into the caldera but into a major pre-existing southeast direction towards the sea.
The SE Nikia Flank Collapse
A major lateral collapse at the SE flank of Nisyros volcano (Fig. 3.46) has been recognized based on sea floor topography covered with hammocks at a water depth of 250 and 380 m offshore the southeastern Nisyros flank. The large debris avalanche deposit covers an area of about 18 km2 with a volume of about 1 km3 and an average thickness of 40–50 m. The elongated hummocks show a fan-shaped distribution of their major axes with the apex pointing to the southeastern flank of Nisyros Island (Tibaldi et al. 2008; Nomikou et al. 2009). The evidence is based on multibeam data and lithoseismic profiles from the oceanographic research vessel ‘‘AEGAEO’’ of the H.C.M.R. The large debris avalanche deposit covers an area of about 18 km2 with a volume of about 1 km3 and an average thickness of 40–50 m.
Effusive phase
At least three major rhyolitic lava flows with a thickness up to 150 m and a total volume >1 km3 (unit No. 30) represent a cycle during an extensive period of effusion (Fig. 3.41). A large morphological depression must have existed during that time in the southeastern part of the island since it facilitated the major flow directions towards southeast. The glass-rich, partly perlitic flows plunge down from the area in the present day eastern caldera walls between the Monastery Panaghia Kyra and the village of Nikia and enter the sea between the beach of Pachia Ammos and Avlaki (Fig. 3.47). Domes and a neck at Parletia piled up forming the eastern rim of the caldera. In several cases, the blocky surface of the flows is covered by a paleosol. The rhyolitic lava flows are younger than the plinian “lower pumice” deposits and older than the beginning of the second plinian eruptions of the “upper pumice”. However, the time gap between these cycles remain unresolved up to now.
3.4.5.2 Second Eruptive Cycle
The palaeosol on top of the lower pumice forms a characteristic “marker horizon” between “lower and upper pumice” on the northern slopes of the volcano. However, the duration of this time gap is still not known. A debris flow (unit No. 29), containing components of lavas, pyroclastics and pumice of older units (units No. 23–26), with a maximum thickness between 5 and 20 m occurs along the northern coast close to the little harbour of Loutrà.
The first volcanic phase of the “Second Eruptive Cycle” (Fig. 3.48) is not well documented. Only one outcrop (at the base of the Nikia lava), a 1 m thick fallout horizon occurs above the “lower pumice”, which consists of lapilli and blocks of slightly vesicular perlitic obsidian, indicating an explosive beginning before the effusion and emplacement of the major rhyolitic lava flow on top.
Explosive phase
The climactic explosive cycle produced an up to 60 m thick rhyolitic pyroclastic sequence, the “upper pumice” UP (unit No. 31) with a fall-surge-flow-surge sequence, which has been deposited all over the island (Fig. 3.48). Major occurrences lie between Loutrà, Pali and Cape Katsouni in the northern and northeastern slopes of the island (Figs. 3.49 and 3.50). Smaller occurrences exist on the SE slopes, on the Nikia rhyolite. Deposits have not been found in the western and southern part of the island.
The proximal-to-distal transition in these bedforms may result from cooling of hot, dry steam propelled surges with condensation of water in the more distal zones (Limburg and Varekamp 1991). Water condensation caused the formation of accretionary lapilli and accelerated rates of deposition of fines, leading to thicker deposits and climbing ripple sets (Fig. 3.50). The upper units were deposited as non-turbulent pyroclastic flows with massive bedding, but absence of grading and stratification. They also contain lithic-rich layers and in the northeast coastal deposits several wavy surge layers. The upper part of the eruptive cycle represents a sequence massive surge deposits with extreme fragmentation, may be the result of water-magma interaction (Fig. 3.51).
The eruption centre of the “second eruptive cycle” may have occurred in the north–western segment of the caldera, controlled by intersecting fault zones N30°E and N30°W (Fig. 3.48), since the distribution of the maximum thickness of the fallout as well the pumice bomb and lithic last size clast sizes point towards the north–western and northern half of the island.
Limburg and Varekamp (1991) recognized a progress in the degree of hydrothermal alteration in the lithics from the lower part to the upper part of the entire succession. The temperatures of hydrothermal alteration, according to the mineral assemblages in the lithics start from 70–150 °C (argillite chunks) to >350 °C in epidote and diopside bearing skarns. This is in accordance with temperatures encountered in the geothermal drill holes NIS 1 and 2 below the caldera floor between 1000 and 1880 m depth (Barberi et al. 1988).
Erupted volume and plume shape
A first attempt to estimate the erupted volumes during the “Caldera Eruptive Cycles” was given by Limburg and Varekamp (1991). Isopach and isopleth patterns were derived from of the thickness distribution of the plinian eruptive sequences of both, the first and the second eruptive cycles. For the second plinian eruptive cycle, an 8 m average thickness at the source and a 7 cm thickness at 120 km distance (Vinci 1983) was assumed. Using a model with circular isopachs and exponential thickness decay, the calculation showed an upper volume of 32 km3, which is equivalent to a DRE (“Dry Rock Equivalent”) of 10 km3. The more realistic approach, using an elliptical distribution of isopachs reduced roughly the volume by the factor 4, which means a volume of 2–3 km3. A crude volume calculation of the caldera before infill of ca. 100 m of talus and alluvial deposits yielded a maximum of extracted volume of 5 km3. The approximate half-width of 1.9 km and a height of 15 km for the column during the plinian phase at minimum cross-wind was calculated using the 7 cm lithic isopleth distribution. A maximum column height of 20 km was estimated from the shape of the isopleth and isopach pattern. Longchamp et al. (2011) derived an “erupted volume for the south vent (considered as the best vent location) ranges between 2 and 27 x108 m3 for the LP and between 1 and 5 x108 m3 for the UP based on the application of four different methods (integration of exponential fit based on one isopach line, integration of exponential and power-law fit based on two isopach lines, and an inversion technique combined with an advection-diffusion model )”.
The second Caldera collapse
During both eruptive cycles, large volumes of similar magnitudes of highly differentiated magmas were discharged. According to the lithics (composition, metamorphic state (Limburg and Varekamp 1991), they originated from magma reservoirs at high crustal levels. The mass deficiency after each eruptive cycle must necessarily have caused an internal collapse of the central part of the island and formation of the caldera structure. The first eruptive cycle was possibly followed by a first caldera collapse. The second caldera collapse must have happened in a very similar way. The possible evidence for such a situation is found in the hydrothermally altered clay chunks as part of the first caldera alluvial beds in the lower fall-flow sequence of the second eruptive cycle. However, the first caldera must have had a smaller diameter than the present day one, which formats the present day state.
3.4.6 Post-caldera Eruptive Cycle
The post-caldera rhyodacitic lava domes comprise six groups of endogenous domes and with light gray perlitic lava flows originating from them (unit No. 32). They fill up the western half of the caldera with a max. thickness of 600 m and seem to be aligned along three parallel 30°NE trending fissure zones intersecting several N30°W fault zones (Figs. 3.48 and 3.52). They were emitted during the last eruptive cycle of Nisyros volcano during purely effusive phases and lack any sign of explosive precursors. The domes are: Mt. Profitis Ilias (698 m), Boriatiko Vouno (437 m), Nymfios , Visternia , Dhiavatis, Trapezina , and Karaviotis (539 m). In addition, a small dome (Lofos, 214 m) is found in the southeastern edge, which has been devastated by recent hydrothermal explosions and fumarolic activity. All domes can be subdivided into four older central groups, Dhiavatis —Profitis Ilias, Nymfios , Visternia , Trapezina , and Lofos and two much younger domes, Boriatiko Vouno in the Northeast and Karaviotis with the silicic flow lobes of Kateros , Kilia , and Drakospilia in the Southwest. They exhibit steep spines and scoria at the surface, as well as they lack soil deposits and minor proximal scree deposits.
3.5 Geochronology
Geochronological data of volcanic rocks and soils from Nisyros Island and the Kos-Yali-Nisyros Volcanic Field are relatively few. During the past 40 years numerous attempts have been undertaken, however without consistent and conclusive results in most cases. Earlier data are controversial and accompanied with large errors (Table 3.2). The following methods have been applied:
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14C fission track analysis on obsidian glass,
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K–Ar on whole rock and volcanic glass,
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40Ar/39Ar on feldspars, and
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U–Th disequilibrium measurements on paleosols sandwiched between volcanic and pyroclastics, the latter discussed in Büttner et al. (2005),
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Th/U measurements on whole rocks and zircon and Pb–U dating on zircon using laser ablation inductively coupled plasma mass spectrometry (LA–ICP–MS , Guillong et al. 2014).
Reliable age determinations with the 40Ar/39Ar method have been obtained from the Kos Plateau Tuff (KPT ) with 161 ± 1 and 166 ± 2 ka (Smith et al. 1996; Bachmann et al. 2010). The new Pb–U ages of the youngest zircons (Guillong et al. 2014) measured from the Nisyros silicic volcanics provide the first geochronological estimates, which are in accordance with the established lithostratigraphy and interpreted as maximum ages of their eruption: The Lower Pumice with 124 ± 35 ka (unit No. 28), the Nikia rhyolite flows with 111 ± 42 ka (unit No. 30), and the upper Pumice with 70 ± 35 ka (unit No. 31). The K–Ar data of 66 ± 2 and 24 ka on fission track (Table 3.1) are of restricted geological meaning.
Some of the major reasons for the lack of accurate geochronological data are as follows:
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The rarity of sanidine and biotite in the evolved rocks of Nisyros volcano do not permit high-precision Ar/Ar analyses. Low-K Amphibole and plagioclase crystals do not provide reliable ages for such young systems, and glass (where most of the potassium is) is typically unreliable (hydration, alteration).
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14C analysis in soils, charcoal and paleosols on Nisyros Island may be contaminated by the strong CO2 degassing all over the volcano (in the order over 1000 tons/day, see Chap. 5).
Future age determination studies using LA-ICP-MS U/Pb dating on single zircon crystals may help resolving some of these issues.
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Dietrich, V.J. (2018). Geology of Nisyros Volcano. In: Dietrich, V., Lagios, E. (eds) Nisyros Volcano. Active Volcanoes of the World. Springer, Cham. https://doi.org/10.1007/978-3-319-55460-0_3
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