Introduction

The Alpine Mediterranean mountain system results from subduction and partial obduction of former Mesozoic ocean basins during the collision of Africa, Europe and a number of smaller intervening microplates (Dewey et al. 1973; Boccaletti et al. 1974; Stampfli et al. 1991; Ricou 1994). One of the major remaining questions on this mountain system concerns the Balkan region where north- to east- (eastern Alps, Carpathians) and south- to west-vergent (Dinarides, Hellenides) belts merge and diverge around continental fragments (Burchfiel 1980) previously considered to be ancient microcontinents (Kober 1928) trapped within the Alpine orogenic belt (Fig. 1). Of these fragments, the Rhodope “massif” of southern Bulgaria and northern Greece is now portrayed as a complicated collage of reworked continental and locally oceanic crust and sediments actively involved in several phases of Alpine deformation and metamorphism (Ivanov 1988; Burg et al. 1990; Burg et al. 1996; Liati and Gebauer 1999). The Rhodope also appears to include rock units of the Serbo-Macedonian high-grade metamorphic series (Ricou et al. 1998), so that the tectonic significance of the Serbo-Macedonian crystalline basement requires reassessment in order to understand the orogenic history of this seismically still very active region.

Fig. 1
figure 1

Location of the study area (black square with K for Kraishte) within its Alpine tectonic framework.

Ongoing research has demonstrated that, perhaps more than collisional deformation, extension-related exhumation of deep continental crust has shaped the Balkan orogenic segments (Bonev et al. 1995; Burg et al. 1996; Kilias et al. 1997; Ricou et al. 1998; Schmid et al. 1998; Krohe and Mposkos 2002). It becomes crucial to determine whether exhumation was a syn- to post-orogenic event or if it is a far-field expression of the supra-subduction extension known farther south, in the Aegean realm (Lister et al. 1984; Gautier and Brun 1994; Jolivet et al. 1999). The answer requires time constraints and recognition of the exhumation processes involved.

The relationships between the European and the Rhodope-Macedonian units can be studied in the Kraishte area, in western Bulgaria (Fig. 1). In order to determine the Alpine geological history of this part of the Serbo-Macedonian massif and to clarify its original tectonic position with respect to the surrounding rocks, we applied fission-track analysis on the Vendian-early Cambrian basement and the Oligocene Osogovo intrusions, and to volcanic zircons and apatites of the rhyolites and tuffites interlayered with sediments of the middle Eocene–Oligocene basins. Some Paleozoic, Mesozoic and Paleogene sediments were also analysed in order to complete the regional picture. These new results reveal the particular importance of the Tertiary exhumation history of the Osogovo–Lisets Complex. They constrain the rates of exhumation of the crystalline rocks and provide correlations between basement exhumation, formation of sedimentary basins and volcanic activity. They also document a new example of heat transfer across low-angle extensional normal faults from a relatively warm footwall to the adjacent colder hanging wall.

Geological setting

The Kraishte zone of western Bulgaria is the tectonic area located between the Serbo-Macedonian high-grade metamorphic unit, to the SW, the Rhodope massif to the S and the European margin (late Cretaceous Sredna Gora volcanic arc) to the NE (Fig. 1).

Four major tectono-stratigraphic units are distinguished (Fig. 2):

  • The Morava thrust nappe, which has a continental basement and an Ordovician to Devonian sedimentary cover (Spassov 1973; Zagorchev 1984; Zagorchev 1996). It was thrust over the Struma unit during the early Cretaceous (Dimitrov 1931; Bonchev 1936; Zagorchev and Ruseva 1982).

  • The Struma unit, which consists of variably deformed continent- and ocean-derived rocks of Vendian—early Cambrian protolith age (Stephanov and Dimitrov 1936; Zagorchev and Ruseva 1982; Haydoutov et al. 1994; Graf 2001; Kounov 2003), unconformably overlain by a Permian to lower Cretaceous sedimentary cover (Zagorchev 1980).

  • The Osogovo–Lisets Complex, on which we will concentrate, includes a suite of calc-alkaline plutonic rocks of Vendian—early Cambrian age (Graf 2001; Kounov 2003) and an intrusion of undeformed granite, the Osogovo Granite, dated at 31±2 Ma (Graf 2001).

  • The Paleogene basins in which sedimentation was first continental with alluvial deposits (middle Eocene). Late Eocene—early Oligocene turbidites (with intercalated layers of tephra) indicate a change to a deep-water environment of deposition (Moskovski and Shopov 1965; Moskovski 1968, 1969, 1971; Zagorchev et al. 1989). Sedimentation ceased sometime towards the end of the Oligocene. The amount of sediment that was deposited is unknown because some of it has been removed by erosion.

Fig. 2
figure 2

Geological map of the Kraishte area (SW Bulgaria) modified from Moskovski (1969), Zagorchev and Ruseva (1993) and Zagorchev (1993). Inset: geographical location of the map (black area).

The Osogovo and Lisets Mountains (Fig. 2) form a prominent NW–SE elongated topographic high cored by lower amphibolite-facies (hornblende-garnet-andalusite) metamorphic rocks (Dimitrova 1964). The dome structure was initially interpreted as an old Cadomian (Cambrian) anticline covered by Permian and Triassic sediments (Zagorchev and Ruseva 1982; Zagorchev 1984; Vardev 1987). According to these authors, the supposedly Precambrian or Cambrian amphibolite-facies metamorphic rocks were intruded by Cambrian granitoids and Cambrian or older diorites and granites. The exposure of this basement was attributed to late Alpine extension and the formation of two horsts bounded by steep normal faults in the Lisets and Osogovo Mountains. An alternative interpretation linked the Osogovo–Lisets dome to late Alpine extension accommodated by low-angle detachment faulting and accompanied by retrogression to greenschist facies (Graf 2001).

The Osogovo–Lisets dome is bounded by the Eleshnitsa detachment along its southwestern slope and the Dragovishtitsa detachment on its northeastern side (Fig. 2; Graf 2001). Structural, petrological and geochemical data suggest that the Osogovo–Lisets gneisses are parts of the Struma basement from which they were separated by the Cenozoic extensional fault system (Graf 2001; Petrov 2001). The Osogovo granite belongs to the W–NW trending Oligocene magmatic belt traced from Turkey through the Balkan Peninsula (Burchfiel et al. 2000).

Cenozoic extension created the sedimentary basins in the hanging wall of the detachments along which structural data indicate generally top-to-the-SW normal faulting. The basin-bounding faults are steep at the surface and cut down into basement; their shape at depth is unknown but they may merge into a low-angle detachment system (Graf 2001). Eocene—Lower Oligocene sediments and their basement are intruded by rhyolitic to dacitic subvolcanic bodies and dykes; the K/Ar radiometric ages on feldspar phenocrysts and whole rock samples scatter from 30±1 to 32±1 Ma (Harkovska and Pecskay 1997).

Analytical methods and results

The fission-track (FT) analytical procedure is described in the Appendix. Zircon and apatite mineral grains contain the signatures of their cooling histories. Approximate closure temperatures vary according to such factors as chemical composition and rates of cooling. When dealing just with the apparent ages, we use 260±50°C for zircon and 110±10°C for apatite (Green and Duddy 1989; Corrigan 1993; Yamada et al. 1995). Because no chemical compositions were determined for the apatites, the modelled thermal histories were based on the composition of Durango using the Laslett model (Gallagher 1995). The geographical location of the samples and the results are presented in Fig. 3 and Tables 1 to 5.

Fig. 3
figure 3

Geological map of the Kraishte area (Fig. 2) with location and FT ages of the analysed samples. Lines AB and CD are the sections in Fig. 8.

Table 1 Fission-track analysis

Morava and Struma units

All samples from the Morava and Struma units yield pre-Cenozoic zircon FT ages (119–69 Ma; Tables 1 and 2). Apatite FT ages from both units can be divided into two groups: (a) 66–56 Ma for samples that have relatively short mean track length (13.18–12.15 μm) and standard deviations of 2.5–1.36 μm; and (b) 40–29 Ma for samples with longer mean track length (14.7–14.29 μm) and standard deviations of 1.54–0.86 μm.

Table 2 Fission-track analysis

Osogovo–Lisets Complex

Eleven samples from the Osogovo–Lisets Complex were analysed. The majority of the samples cluster between 47 and 39 Ma for zircon and between 46 and 38 Ma for apatite (Fig. 3, Table 3). Exceptions are apatite ages from samples AK218, K1067a, and AK45, which are between 30 and 27 Ma (Fig. 3, Table 3).

Table 3 Fission-track analysis

In general, samples from the Osogovo–Lisets Complex have long mean track lengths (14.65–13.72 μm) and yield similar zircon and apatite ages (Table 3). Compilation of the modelled time-temperature (T–t) paths (Gallagher 1995) reveals two groups with different thermal histories (Fig. 4). One group underwent fast cooling through both the zircon and apatite closure temperatures from 47 to 38 Ma, while the other cooled more slowly below 110°C after 30 Ma.

Fig. 4
figure 4

Modelled T–t paths for footwall samples (crystalline rocks of the Osogovo–Lisets Complex) of the detachment system. For details of modelling see the Appendix. Group “a” shows fast cooling from 47 to 38 Ma. Group “b” underwent relatively slower cooling after 30 Ma. The apatite partial annealing zone is within the temperature limits assigned by Laslett et al. (1987). The modelled T–t paths are extended into the zircon partial annealing zone (Yamada et al. 1995) where grey squares represent the zircon FT ages of the modelled samples.

Paleogene sediments

By applying the FT technique to apatites, the timing and the temperature of burial of the sediments as well as the final inversion of each basin can often be assessed.

Five volcanic ashes were dated both by FT and U/Pb SHRIMP on zircons to better constrain the timing of sedimentation in the basins (Table 4). The zircon FT ages range between 35 and 32 Ma (AK72, AK125, AK167, AK199, AK245; Table 4) in statistical agreement with the U/Pb SHRIMP ages obtained from samples AK199(33.46±0.22 Ma) and AK245(33.07±0.28 Ma) (Fig. 5; Kounov 2003).

Table 4 Fission-track analysis
Fig. 5
figure 5

Tera-Wasserburg diagrams (Tera and Wasserburg 1972) for sample AK245 and sample AK199 (for locations see Fig. 3). Filled ellipses on the diagrams to the right are those used for age calculations. Data-point error ellipses: 68.3% confidence for all diagrams.

Three sandstone samples from the stratigraphically deepest section of the Pianets basin (AK8, AK9, AK65; Fig. 6) each contain only one apatite population, with ages ranging between 48 and 40 Ma and with mean-track lengths from 13 to 12 μm. These ages are very close to the estimated age of deposition (middle Eocene = Bartonian; Kounov 2003). Thermal modelling of these samples (Fig. 7) reveals that there has been post-depositional heating to about 90°C. A similar thermal history may be suggested for the granite clast from a breccia at the base of the small basin N of Kjustendil (AK106, Fig. 3). This sample yields an apatite age of 65±9 Ma with a mean track length of 12.58±0.2 μm and a bimodal length distribution (Fig. 7).

Fig. 6
figure 6

Detrital and volcanic ash population ages vs. stratigraphic position from the Paleogene sediments in the Kraishte area. Different age populations were separated using the method of Sambridge and Compston (1994). Bold sample numbers are pyroclastics. Time-scale of Berggren et al. (1995). Formation and member names after Kounov (2003).

Fig. 7
figure 7

Left column: modelled thermal histories for the terrigenous sediments of Paleogene basins. The apatite partial annealing zone is within the temperature limits assigned by Laslett et al. (1987). For details of modelling see the Appendix. Boxes constrain the (T–t) space permitted for the modelled paths. Grey arrows represent potential paths of cooling before sedimentation. The shaded vertical area represents the probable heating event at 45–35 Ma. Right column: apatite FT length histograms. n number of track lengths measured. Var is percent variation from pooled age.

Upwards in the section of the Pianets basin, the apparent apatite ages, except for the uppermost sample (AK234), are older than the depositional age. Attempts to statistically split these into sub populations failed in many cases. This was specifically a problem in some ash layers (e.g. AK73 and AK76, Fig. 6) where the mean ages are at least 10 million years older than the age of sedimentation and hence it was suspected that older detrital populations might be a contaminant. In sample AK76A, the sandstone layer resting on tuff AK76 (Fig. 6), two populations were present in the 50 dated apatite grains (Table 4). The AFT age of the youngest population is 36±1 Ma, which corresponds to the age of the lowermost ash layer AK72 (35.1±3.6) from the same section, as well as to that of a pyroclastic flow AK125 (35.0± 3.0) from the Prekolnitsa basin (W of Kjustendil, Figs. 2 and 3). The second population has an age of 49±5 Ma, an age which is slightly older than the oldest age from the Osogovo–Lisets Complex.

All clastic horizons, as well as some of the pyroclastics, contain zircons older than the age of sedimentation; however, there is a general younging trend in these detrital ages upwards in the section (Fig. 6).

Magmatic rocks

Three samples from Cenozoic granites and dykes were dated (Table 5).

Table 5 Fission-track analysis

The FT analysis of the Osogovo granite yields identical apatite and zircon ages of 31±3 Ma and 31±2 Ma (AK50; Fig. 3), respectively. The mean track length in apatite is 14.53±0.10 μm. These ages are concordant with the U/Pb zircon single crystal ages of Graf (2001). Rhyolitic dykes yield zircon FT ages of 32±3 and 29±2 Ma (AK308 and AK56; Fig. 3) and an apatite age of 29±4 Ma (AK56)with a mean track length of 15.07±0.1 μm.

Interpretation

This discussion refers to the structural frame summarised above, whereby the Osogovo–Lisets Dome represents the footwall of a Cenozoic extension system characterised by the major Eleshnitsa detachment and the Morava and Struma units forming, along with the sedimentary basins, the hanging wall.

Thermal history of the footwall

Compilation of the modelled T–t paths from the Osogovo–Lisets Complex reveals two groups with different thermal histories (Fig. 4). Group “a” had very rapid cooling from 260 to 60°C between 47 and 38 Ma. This rapid cooling is also confirmed by the almost identical ages of the zircons and apatites. Samples from group “b” yielded similar zircon ages. We suggest that they also followed path “a” until they reached 60°C and afterwards they underwent a heating event prior to 30 Ma before cooling to the surface from that time on. Rhyolitic dykes and small igneous bodies ubiquitously intruded the detachments at 31 Ma and most likely caused local heating to temperatures >110°C (K1067a, AK45, AK218), resetting any previous apatite ages (Fig. 4, path “b”). Effects of such intrusions are by chance of sampling. Thus the FT ages of group “b” are considered to indicate such local thermal perturbations on the overall general cooling pattern.

The cooling path “a” traces rapid exhumation of the Osogovo–Lisets Complex, which reflects a major tectonic event. Extension-related exhumation along the Eleshnitsa detachment is the most likely interpretation, and began before 47 Ma. Progressive southwestward unroofing and cooling along this detachment is observed through the decreasing zircon and apatite FT ages (Fig. 8). A maximum extension rate may be derived, using the width of the exhumed rocks along which the younging trend is measured. This yields an average of 2 mm/year over 7 million year. We emphasise that this value might be overestimated by as much as 40% (Ehlers et al. 2001), yet is a reasonable figure in terms of tectonic processes.

Fig. 8
figure 8

Sections AB and CD (Fig. 3) with apatite and zircon FT ages. Lithological key as in Fig. 2.

Thermal history of the hanging wall

Morava and Struma units

The two groups of apatite FT ages from the Morava and Struma units are interpreted as follows:

  • The modelled T–t paths of the 66–56 Ma samples (path “c”, Fig. 9) take into account that the sample sites were just underneath the Paleogene sediments and that clasts from the Morava and Struma units are present in these sediments. Thus the Morava and Struma units are assumed to have been at or very close to the surface during the Paleogene. The thermal histories reveal a period of heating to a maximum of 100°C between 48 and 35 Ma before cooling again to the surface today.

  • The second group “d”, reveals a period of cooling through the apatite partial annealing zone over the last 40 million year.

Fig. 9
figure 9

Modelled T–t paths for the hanging wall samples of the detachment system. Black squares represent the zircon FT ages of the modelled samples. Dashed lines within the apatite partial annealing zone represent the probable earlier T–t path for the samples from group “d” fully reset during the extension by high heat flow from the footwall or late magmatic activity respectively.

The timing of this heating phase in the hanging wall is coincident with the extension phase that exhumed the Osogovo–Lisets Complex. We suggest that this heating event is most likely due to heat advecting from the rising hot footwall rocks.

Basins

The syn-sedimentary volcanic rocks have zircon ages between 35 and 32 Ma (Fig. 6). Therefore, the oldest sediments must be older than 35 Ma. A straight line extrapolation to the oldest units extends the age of sedimentation to at the latest 40 Ma, (middle Eocene = Bartonian) and puts an upper limit on the initiation of the basins (Zagorchev 2001). This is at least 7 million years after the beginning of extension as determined above.

Thermal history

Thermal modelling of the apatite FT data from four sedimentary horizons below the ashes (Figs. 3, 6 and 7; samples AK8, AK9, AK65 and AK106) supports the conclusion that the detrital apatites in the lower layers of the basin were partially reset (to between 80 and 100°C) during the time period of 45–35 Ma. This heating event took place almost immediately after sedimentation and lasted until about 35 Ma, when cooling began and lasted until today.

This then implies that the sediments younger than 35 Ma have not been reset. The first line of evidence for lack of resetting in these sediments is the presence of mixed apatite age populations. Secondly, the youngest apatite population in sandstone sample AK76a has an age of 36 Ma (Fig.6). This age is statistically coincident with the volcanic age of the ash AK72 (35 Ma) about 300 m beneath sandstone AK76a. In addition, the sedimentary overburden, which is estimated to be at most 1,500 m (the thickness of sediments younger than 35 Ma), cannot explain the 80–100°C heating recorded prior to 35 Ma in the bottom sediments.

Sediment source

The older detrital zircon ages, dominantly in the lower section but also partly represented higher in the stratigraphic section (Fig. 6) are most likely due to input from the Morava and Struma units, which have older exhumation histories (Table 1).

Sample AK76a has three populations of apatites, 36, 49 and 79 Ma. The first corresponds to the age of the ash immediately below, AK72. The second population is slightly older than the oldest age from the Osogovo–Lisets Complex at the surface today (compare Tables 3 and 4). Thus, it is probable that second population grains are derived from the Osogovo–Lisets Complex. These ages represent the time at which the sample was at a temperature of approximately 110°C and was exposed later after further erosion or tectonic denudation, with a lag time of approximately 15 million years. The third population was probably derived from the Morava and Struma units because the age corresponds to the ages obtained from these units at the surface today.

Some sediment samples have single population AFT ages at about 30 Ma (AK234, AK261c, AK167, AK302); Table 1; Fig. 3). These ages are younger than the estimated stratigraphic age of the enclosing sediments (Kounov 2003) and may again reflect heat advection from igneous activity, which was pervasive at that time (Harkovska and Pecskay 1997).

Comparative cooling

A comparison of the temperature-time path of the footwall with that of the hanging wall (Fig. 10) reveals that heating in the hanging wall, i.e. the Morava and Struma units as well as the sediments, is contemporaneous with the fastest cooling in the footwall. This clearly suggests that heat derived from the rising hot footwall was conducted into the hanging wall as it has been argued in other natural examples (e.g. Van Den Driessche and Brun 1991–1992; Grasemann and Mancktelow 1993; Ehlers et al. 2001).

Fig. 10
figure 10

Modelled T–t paths for the samples from the footwall and hanging wall of the detachment system including those of the sedimentary basins and path “b” of the hanging wall samples (dashed black line).

Thermotectonic evolution

The Osogovo–Lisets Dome has the structural and thermal characteristics of a core complex exhumed during early Cenozoic extension. A retrogressive metamorphic overprint of greenschist-facies (chlorite-ilmenite-clinozoisite) is related to hydrothermal activity during the formation of extensional shear bands, crenulation cleavage, cohesive breccias in which Pb–Zn-ores crystallised (Vardev 1987), and gouges. This overprint mostly affects the cataclastic part of the detachment zone (top of the footwall). The old mineral assemblages show little retrogressive overprint in the deepest structural levels. Probably part of the retrogressive metamorphism (chloritisation and epidotisation) is also associated with the younger magmatic phase, when hydrothermal activity was present.

Fission-track data document rapid cooling in the Osogovo–Lisets Complex in the middle Eocene (Fig. 11a). The younging direction of the FT ages further indicates that the bulk movement along the Eleshnitsa detachment was top-to-the-SW, which is consistent with the relative displacement inferred from slickenside lineations, secondary fractures and shear bands. The Eleshnitsa detachment was the main detachment. The younger Dragovishtitsa detachment was the antithetic fault accommodating the dome formation (Fig. 11b).

Fig. 11
figure 11

Proposed evolutionary model of the Kraishte area from middle Eocene to present times.

In the basins, formation of the alluvial fans was related to faulting along their borders, where large olistoliths were shed from the fault scarps. Formation of the half-graben basins in the hanging wall of the detachments was related to the W–E to SW–NE extension and the resulting NW–SE trending faults controlling sedimentation. By the end of the Eocene, sediments had sealed the inactive detachments. This inactivity may actually correspond to a major change in extension tectonics since it also was the time of marine transgression and volcanic activity (35–32 Ma; Fig. 11c). Furthermore, this also correlates with the termination of the heating phase in the hanging wall.

Extension may have been accompanied by ductile flow and anatexis in the lower crust but these levels were not exhumed in the Osogovo–Lisets core complex (Fig. 11c, d). However, the emplacement of the 32–29 Ma rhyolitic to dacitic subvolcanic bodies and dykes into the Paleogene sediments and their basement, along with intrusion of the Osogovo granite, are strong evidence for melting of the lower crust during the Cenozoic (Graf 2001). The dykes cut the detachments (Fig. 11d), which also suggests a major change in extension tectonics at about 30 Ma.

Post-Oligocene (Miocene?) brittle deformation (Fig. 11d) was associated with the formation of NW–SE and NNW–SSE sets of normal and strike-slip faults (Bonchev et al. 1960; Moskovski 1969, 1971; Moskovski and Harkovska 1973; Kounov 2003).

Discussion

Our new FT ages indicate that Paleogene extension in the Kraishte lasted between 47 and 30 Ma. This is consistent with the late Eocene sedimentary cover on the detachment and 30 Ma dykes that crosscut the detachment. This extension is much younger than the Late Cretaceous Sredna Gora back arc basin (Aiello et al. 1977) and therefore is not related to the corresponding arc system. On the other hand, such timing is similar to the extension associated with Late Eocene to Late Oligocene magmatism reported in the Balkan and adjacent segments of the Alpine orogenic system (Burchfiel et al. 2000) and orogen-parallel extension in the southern Carpathians (Schmid et al. 1998). It is also contemporaneous with and has a similar trend to the early Cenozoic extension in the Rhodope (Burg et al. 1996; Ricou et al. 1998). Accordingly, Eocene–Oligocene SW–NE extension was active all around the Carpatho-Balkanic orocline.

It is difficult to decide whether coeval events in the Kraishte and the Rhodope have the same cause. In both cases, early Cenozoic extension fits neither the trend nor the age of the N–S Aegean extension, which dominated the eastern Mediterranean realm since ca. 25 Ma (e.g. Gautier et al. 1999; Burchfiel et al. 2000). It is an older event that might reflect transtension during northeastward drifting, lateral extrusion and rotation of continental fragments around the western boundary of Moesia (Boccaletti et al. 1974; Tapponnier 1977; Burchfiel 1980; Schmid et al. 1998). In the Osogovo–Lisets Complex, the lack of Mesozoic, high-grade mylonitic deformation documented throughout the Rhodope (Burg et al. 1996; Krohe and Mposkos 2002) and the absence of Paleozoic–Mesozoic cover in the Rhodope lead us to suggest, following Gealey (1988), that the continental fragments around western Moesia, found as slivers in the eastern Carpathians, have a Serbo-Macedonian rather than a Rhodopian affinity.

While extension was taking place in the Kraishte, convergence that dominated the Mediterranean realm led to the closure of the Vardar Ocean and further obduction of its remnants onto the Pelagonian continental fragment (Ricou et al. 1998). Owing to the dominantly rhyolitic and very short-lived magmatism, we do not concur with Burchfiel et al. (2000) that extension took place within a subduction-related arc. Orogen-normal extension of a thickened and thermally weakened continental crust is the most plausible explanation for the formation of the Osogovo–Lisets Complex. This extension event may have been triggered by the shift of the subduction from the Vardar to its current position in the exterior of the Dinaric–Hellenic Belt (Fig. 1).

Conclusions

Examination of the Osogovo–Lisets core complex in the Kraishte, western Bulgaria revealed:

  1. 1.

    Cenozoic extension began before 47 Ma, associated with formation of low-angle detachment faults between the Morava and Struma units in the hanging wall and the Osogovo–Lisets complex in the footwall.

  2. 2.

    Progressive southwestward unroofing and cooling of the Osogovo–Lisets basement along the Eleshnitsa detachment dominated crustal extension and controlled the formation of half-graben sedimentary basins filled initially with continental deposits.

  3. 3.

    During rapid cooling of the hot Osogovo–Lisets footwall, heat was transferred to the hanging wall.

  4. 4.

    Rhyolitic magmatism accompanied syn-extension sedimentation between 35 and 32 Ma.

  5. 5.

    Segments of the detachments were no longer active by the latest Eocene, when sedimentation became marine. Inactivation of the detachment system preceded the emplacement of rhyolitic dykes and magmatic bodies such as the Osogovo granite (31–30 Ma), which caused local heating in the region.

  6. 6.

    Crustal thinning led to the denudation and exhumation of the Precambrian-early Cambrian basement rocks exposed in high-altitude culminations (Osogovo and Lisets Mountains) between low-altitude basins.

We conclude that the Kraishte region underwent a major extensional event in the middle Eocene-early Oligocene. This extension in the southern Balkan is older than, and separated from, the Miocene to Quaternary Aegean extension. Eocene–Oligocene extension was controlled by the distribution of earlier crustal thickening all around the Carpatho-Balkanic orocline, earlier thickening being represented by the Cretaceous emplacement of the Morava Nappe in the Kraishte. The presence of a thickened crust is consistent with the massive rhyolitic volcanism that sealed extension structures in the Kraishte as in the Rhodope. This rhyolitic magmatism reveals voluminous crustal melting in deep root zones and subsequent mass and heat transfer in the crust.