Abstract
The timing of Triassic magmatism of the Ditrău Alkaline Massif (Eastern Carpathians, Romania) is important for constraining the tectonic framework and emplacement context of this igneous suite during the closure of Paleotethys and coeval continental rifting, as well as formation of back-arc basins.
Our latest geochronological data refine the previously reported ages ranging between 237.4 ± 9.1 and 81.3 ± 3.1 Ma. New K/Ar and U–Pb age data combined with all recently (post-1990) published ages indicate a relatively short magmatic span (between 238.6 ± 8.9 Ma and 225.3 ± 2.7 Ma; adding that the most relevant U–Pb ages scatter around ∼230 Ma) of the Ditrău Alkaline Massif. The age data complemented by corresponding palinspastic reconstructions shed light on the paleogeographic environment wherein the investigated igneous suite was formed.
The magmatism of the Ditrău Alkaline Massif could be associated with an intra-plate, rift-related extensional tectonic setting at the southwestern margin of the East European Craton during the Middle–Late Triassic (Ladinian–Norian) period.
Introduction
The Ditrău Alkaline Massif (DAM), located in the Eastern Carpathians (Romania), is an igneous suite characterized by complex structure and lithology. Since its first mention by Lilienbach (1833) the DAM has been studied, including its petrotectonic environment, petrogenetic relations and the timing of magmatism (e.g. Koch, 1876, 1879; Streckeisen, 1938, 1960; Codarcea et al., 1957, 1958; Bagdasarian, 1972; Streckeisen and Hunziker, 1974; Pál-Molnár and Árva-Sós, 1995; Dallmeyer et al., 1997; Kräutner and Bindea, 1998; Morogan et al., 2000; Pál-Molnár, 2000, 2010a; Pană et al., 2000; Batki et al., 2004, 2014, 2018; Fall et al., 2007; Pál-Molnár et al., 2015a, 2015b).
Several analyses have been conducted with various dating methods (e.g., K/Ar, 40Ar/39Ar and U–Pb age determinations) on different rock types and mineral phases of the Ditrău Alkaline Massif. The interpretation of the results led to contradictory hypotheses on the genesis of the igneous complex and its rock associations. In order to better understand the evolution and magmatic processes of the massif, these data needed to be reconsidered and supplemented by additional, up-to-date age determination.
The aim of our study – based on the revision of previous age data and interpretation of new amphibole and biotite K/Ar, as well as titanite and zircon U–Pb ages of amphibole- and pyroxene-rich cumulate, syenite, nepheline syenite and granite samples – is to review and specify the age, time span and sequence of the open-system magmatic processes (e.g., Batki et al., 2018) that played an important role in the formation of the Ditrău Alkaline Massif.
Geologic setting
The Ditrău Alkaline Massif is located in the southern and southwestern part of the Giurgeu Mountains (Eastern Carpathians, Romania) and crops out in an area of ca. 225 km2 (Fig. 1A). The DAM consists of diverse rock types in an elaborate structural relationship. The most common rock types of the massif are as follows: mafic-ultramafic cumulates (e.g., hornblendite, olivine-rich cumulate, amphibole- and pyroxene-rich cumulate, amphibole-rich cumulate), alkali gabbro, alkali diorite, monzodiorite, monzonite, monzosyenite, syenite, nepheline syenite, quartz syenite and alkali granite (Fig. 1B). These rocks are cross-cut by lamprophyre, tinguaite and syenite dykes (Pál-Molnár, 2000; Batki et al., 2014; Pál-Molnár et al., 2015a, 2015b).
The DAM had intruded into the Mesozoic crystalline rocks of the Eastern Carpathians and was subjected to nappe-forming Alpine tectonic events (Pál-Molnár, 1994a, 1994b; Pál-Molnár and Árva-Sós, 1995). The Central Eastern Carpathian Zone or Crystalline Mesozoic Zone is an east-verging nappe system that was formed during the Austrian tectogenesis. It derives from the marginal part of the Getic microcontinent that forms the basement of the Transylvanian Basin. The nappe system is referred to as Median Dacides (Săndulescu, 1984) or Eastern Getides (Balintoni, 1997). According to Săndulescu (1984), the Median Dacides can be divided into three Alpine nappes (Infrabucovinian, Subbucovinian and Bucovinian), composed of pre-Alpine metamorphic rocks and Permo-Mesozoic cover sequences. Pre-Alpine, west-verging, petrographically uniform tectonic units of the Subbucovinian and Bucovinian Nappes and their respective metamorphic terranes (or alternatively: litogroups) are as follows: Rodna (Rebra Terrane), Pietrosu Bistriţei (Negrişoara Terrane), Putna (Tulgheş Terrane) and Rarău Nappe (Bretila Terrane and Hăghimaş Granitoids) (Balintoni et al., 1983; Vodă and Balintoni, 1994; Balintoni, 1997).
The Ditrău Alkaline Massif belongs structurally to the Bucovinian Nappe and is in direct contact with four of its pre-Alpine metamorphic units (Bretila, Tulgheş, Negrişoara and Rebra Terrane) (Fig. 2) (Pál-Molnár, 2000; Pál-Molnár, 2010b). The massif was uprooted during the Alpine tectonic events and cut by the Bucovinian shear zone at a depth of ca. 1800–2000 m. Hence, the Subbucovinian Nappe and the DAM are bounded by a tectonic unconformity (Kräutner and Bindea, 1995).
Timing of the Ditrău magmatism – previous work
Early investigations – based on field and structural observations (e.g., Reinhardt, 1911; Streckeisen, 1952, 1954; Codarcea et al., 1957) – were complemented and specified by modern instrumental analytical techniques providing more precise data (Table 1). Sample locations of former studies are either unknown, or the descriptions are constrained to the name of valleys alone. Since the previous sampling points are not accurately retraceable, these data are not marked on the geologic map.
Results of previously conducted age determinations
Source | Rock type | Locality | Method | Studied sample | Age (Ma) |
Bagdasarian (1972) | Hornblendite | West of the conjunction of Teasc and Jolotca creeks | K/Ar | whole rock | 196 ± 6 |
Hornblendite | West of the conjunction of Jolotca and Simo creeks | K/Ar | whole rock | 161 ± 2 | |
Hornblendite | West of the conjunction of Jolotca and Holoşag creeks | K/Ar | whole rock | 161 ± 10 | |
Hornblendite | Ditrău-valley and the spring area of the Putna creek | K/Ar | whole rock | 177 ± 1 | |
Syenite | East from the conjunction of Jolotca and Simo creeks | K/Ar | whole rock | 128 ± 3 | |
Syenite | Central part of the Jolotca-valley | K/Ar | whole rock | 121 ± 2 | |
Syenite | Road between Ditrău-valley and Putna creek | K/Ar | whole rock | 121.5 ± 0.5 | |
Syenite pegmatite | East of the conjunction of Teasc and Jolotca creeks | K/Ar | whole rock | 142 ± 7 | |
Nepheline syenite | Road between Ditrău-valley and Putna creek | K/Ar | whole rock | 152 ± 1 | |
Leucogranite | Conjuction of Jolotca and Hompot creeks | K/Ar | whole rock | 125 ± 10 | |
Mica schist | Basin of Putna creek, Ditrău-Tulgheş road, km 20 | K/Ar | whole rock | 284 ± 14 | |
Streckeisen and Hunziker (1974) | Nepheline syenite | Comarnic plateau | K/Ar | biotite | 151 ± 9 |
Nepheline syenite | Ditrău creek, gallery I. | K/Ar | biotite | 153 ± 3 | |
Tinguaite | Cianodul, 500 m E | K/Ar | whole rock | 161 ± 7 | |
Tinguaite | Prişca, 500 m NE | K/Ar | whole rock | 156 ± 6 | |
Hornfels | Teasc creek, 750 m SE | K/Ar | biotite | 150 ± 6 | |
Mînzatu and Ardeleanu (1980); Mînzatu et al. (1981) | Biotitized hornblendite | Jolotca-valley | K/Ar | biotite | 161.0 ± 6.3 |
Biotite hornblendite | Jolotca-valley | K/Ar | biotite | 134.5 ± 5.2 | |
Biotite syenite | Ditrău-valley | K/Ar | whole rock | 112 | |
biotite | 117 | ||||
Biotite syenite | Ditrău-valley, gallery VII. | K/Ar | whole rock | 131 | |
biotite | 134.3 ± 4.8 | ||||
Biotite syenite | Ditrău-Tulgheş road, km 11 | K/Ar | whole rock | 136 | |
biotite | 139.3 ± 5.1 | ||||
Biotite syenite | Ditrău-valley, quarry | K/Ar | biotite | 113.6 ± 4.6 | |
Syenite pegmatite | Hereb-valley, gallery VI. | K/Ar | muscovite | 161.8 ± 6.1 | |
Biotite syenite with cancrinite | Cianodul-valley | K/Ar | biotite | 126.0 ± 5.0 | |
Syenite with sodalite (vein) | Ditrău-Tulgheş road, km 7 | K/Ar | biotite | 120.0 ± 4.5 | |
Nepheline syenite | Ditrău-valley | K/Ar | nepheline | 150.9 ± 5.8 | |
Pegmatoidic nepheline syenite | Ditrău-valley, quarry | K/Ar | nepheline | 116.1 ± 4.4 | |
Nepheline syenite with cancrinite | Ditrău-valley | K/Ar | nepheline | 147.4 ± 6.0 | |
Nepheline syenite with cancrinite | Ditrău-valley | K/Ar | biotite | 136.9 ± 5.1 | |
Liebneritized nepheline syenite | Ditrău-valley | K/Ar | nepheline | 81.3 ± 3.1 | |
Aplite granite | Borehole 120, m 2 | K/Ar | whole rock | 141.9 ± 5.5 | |
Tinguaite | Conjunction of Aurora and Belcina creeks | K/Ar | whole rock | 172.0 ± 6.6 | |
Tinguaite | Aurora-valley | K/Ar | whole rock | 159.3 ± 6.1 | |
Tinguaite | Cianodul-valley | K/Ar | whole rock | 141.9 ± 5.5 | |
Biotite hornfels | Aurora, borehole F 144. | K/Ar | whole rock | 138 | |
Biotite hornfels | Aurora-valley, gallery VII. | K/Ar | whole rock | 172 | |
Phlogopite marble | Lazarea, borehole, 141, m 137 | K/Ar | biotite | 150.0 ± 6.0 | |
Pál-Molnár and Árva-Sós (1995) | Hornblendite with textural ordering | Jolotca, Tarniţa de Sus creek | K/Ar | amphibole | 237.4 ± 9.1 |
Hornblendite with textural ordering | Jolotca, Pietrarilor creek | K/Ar | amphibole | 216.0 ± 8.8 | |
Hornblendite without textural ordering | Jolotca, gallery VI. | K/Ar | amphibole | 226.0 ± 9.6 | |
Pegmatoidic hornblendite | Jolotca, Tarniţa de Sus creek, gallery XXV. | K/Ar | amphibole | 234.7 ± 10.8 | |
plagioclase | 161.3 ± 9.8 | ||||
biotite | 162.4 ± 6.1 | ||||
biotite | 168.3 ± 7.2 | ||||
Meladiorite with textural ordering | Jolotca, Teasc creek | K/Ar | amphibole | 208.3 ± 8.3 | |
feldspar | 138.2 ± 5.8 | ||||
Diorite with textural ordering | Jolotca, Teasc creek | K/Ar | amphibole | 176.6 ± 6.7 | |
feldspar | 137.4 ± 5.5 | ||||
Diorite with feldspar aggregates | Jolotca, Tarniţa de Jos creek | K/Ar | amphibole | 218.7 ± 8.3 | |
feldspar | 155.4 ± 5.8 | ||||
Syenite | Jolotca, Teasc creek, gallery XIX. | K/Ar | biotite | 107.6 ± 4.1 | |
K-feldspar | 182.7 ± 6.9 | ||||
Alkaline feldspar syenite | Jolotca, Simo creek | K/Ar | biotite | 102.6 ± 4.0 | |
K-feldspar | 113.5 ± 4.3 | ||||
Sodalite nepheline syenite | Jolotca, Teasc creek | K/Ar | biotite | 182.4 ± 6.9 | |
nepheline + sodalite | 232.7 ± 8.8 | ||||
Granite | Jolotca, Turcului creek | K/Ar | biotite | 217.6 ± 8.3 | |
feldspar | 146.0 ± 5.6 | ||||
Granite | Jolotca, Teasc creek | K/Ar | biotite | 213.5 ± 8.2 | |
K-feldspar | 139.1 ± 5.4 | ||||
Granite | Jolotca, Creanga Mare creek | K/Ar | biotite | 206.3 ± 7.8 | |
K-feldspar | 142.7 ± 5.7 | ||||
Dallmeyer et al. (1997) | Gabbro | Jolotca-valley | 40Ar/39Ar | amphibole | 227.1 ± 0.1 |
Hornblende diorite | Ditrău-Tulgheş road, km 7 | 40Ar/39Ar | amphibole | 231.5 ± 0.1 | |
Pană et al. (2000) | Syenite | Jolotca, Jolotca creek | U–Pb | zircon | 229.6 +1.7/−1.2 |
The first K/Ar dating of whole rock samples (hornblendite, syenite, granite, nepheline syenite) was carried out by Bagdasarian (1972): hornblendite yielded K/Ar mean ages of 196 ± 6 – 161 ± 2 Ma. The age of syenite ranges between 142 ± 7 and 121.5 ± 0.5 Ma. Granite was suggested to be formed 125 ± 10 Ma ago. Nepheline syenite gave a K/Ar age of 152 ± 1 Ma.
According to the results of Streckeisen and Hunziker (1974), the K/Ar ages of biotite crystals from nepheline syenite are 153 ± 3 and 151 ± 9 Ma. An age of 150 ± 6 Ma was determined for the biotite of the contact metamorphic rock (hornfels). Whole rock samples of tinguaite yielded K/Ar ages of 161 ± 7 and 156 ± 6 Ma. In their hypothesis, Streckeisen and Hunziker (1974) assumed the following formation sequence for the different rock types of the massif: (1) intrusion of dioritic and gabbroic magmas into the crystalline country rocks; (2) intrusion of syenitic magma and formation of granitoid rocks by assimilation in the marginal zones of the massif; (3) intrusion of nepheline syenite magma, accompanied by metasomatism and hybridization; (4) formation of lamprophyre, pegmatite and aplite dykes.
Considering the results of formerly conducted K/Ar age determinations, Kräutner et al. (1976) assumed that the emplacement age of the DAM is 135 Ma.
Mînzatu and Ardeleanu (1980), as well as Mînzatu et al. (1981) performed K/Ar analyses on minerals and whole rock samples as well. Muscovite separated from syenite yielded a K/Ar age of 161.8 ± 6.1 Ma, whereas the age of biotite ranges between 139.3 ± 5.1 and 113.6 ± 4.6 Ma. Whole rock samples of syenite gave K/Ar ages of 136 – 112 Ma. The ages of biotite of metasomatically altered syenite are 126.0 ± 5 and 120.0 ± 4.5 Ma. An age of 141.9 ± 5.5 Ma was obtained for whole rock samples of granite aplite. Biotite of hornblendite yielded K/Ar ages of 161.0 ± 6.3 and 134.5 ± 5.2 Ma. Measured ages of nephelines from nepheline syenite are 150.9 ± 5.8 and 116.1 ± 4.4 Ma. Biotite of metasomatically altered nepheline syenite gave a K/Ar age of 136.9 ± 5.1 Ma, while the ages of nephelines are 147.4 ± 6 and 81.3 ± 3.1 Ma. Whole rock ages of tinguaite range from 172.0 ± 6.6 to 141.9 ± 5.5 Ma. Whole rock samples of the contact rock (hornfels) yielded a K/Ar age of 138 Ma, whereas the age of biotite is 156.8 ± 5.9 Ma.
Based on Popescu (1985), the Rb–Sr whole rock age of ultrabasic rocks and syenite is 200 and 160 Ma, respectively.
Zincenco (1991) reinterpreted the available K/Ar and Rb–Sr data. According to his hypothesis, the DAM entered the subsolidus stage 171 ± 3 Ma ago. Pneumatolytic and hydrothermal phases ended 165 ± 5 and 154 Ma ago, respectively. Based on supplementary Rb–Sr whole rock data, Zincenco et al. (1994) proposed an emplacement age of 201 ± 1 Ma.
Pál-Molnár and Árva-Sós (1995) determined the K/Ar age of minerals of different rock types (cumulate rocks, diorite, granite, nepheline syenite, syenite and alkaline feldspar syenite). Amphiboles of cumulate rocks gave K/Ar ages of 237.4 ± 9.1 – 216.0 ± 8.8 Ma. Amphiboles of diorite display various ages between 218.7 ± 8.3 and 176.6 ± 6.7 Ma. The obtained K/Ar age of biotite and feldspar of syenite is 107.6 ± 4.1 and 182.7 ± 6.9 Ma, respectively. Biotite and alkaline feldspar of alkaline feldspar syenite yielded a K/Ar age of 102.6 ± 4 and 113.5 ± 4.3 Ma, respectively. Biotite and nepheline + sodalite of sodalite nepheline syenite reached their closure temperature at 182.4 ± 6.9 and 232.7 ± 8.8 Ma, respectively. K/Ar ages of biotite of granite range from 217.6 ± 8.3 to 206.3 ± 7.8 Ma, whereas the age of alkaline feldspar is 142.7 ± 5.7 – 139.1 ± 5.4 Ma. Based on the above results, Pál-Molnár and Árva-Sós (1995) developed a two-stage evolution history for the massif: (1) Middle Triassic–Lower Jurassic (hornblendite, nepheline syenite, granite); (2) Middle Jurassic–Lower Cretaceous (syenite, alkaline feldspar syenite, diorite).
Dallmeyer et al. (1997) estimated the age of hornblendes with the 40Ar/39Ar method. The 40Ar/39Ar plateau age of amphibole from hornblendite and gabbro is 231.5 ± 0.1 and 227.1 ± 0.1 Ma, respectively.
Copious age data by Bagdasarian (1972), Streckeisen and Hunziker (1974), Kräutner et al. (1976), Mînzatu and Ardeleanu (1980), Mînzatu et al. (1981), Popescu (1985), Zincenco (1991), Zincenco et al. (1994), Pál-Molnár and Árva-Sós (1995), and Dallmeyer et al. (1997) were summarized and interpreted by Kräutner and Bindea (1998). According to their hypothesis, the DAM was formed by a five-stage magmatic process: (1) generation of a mantle-derived gabbroic-dioritic magma in an extensional tectonic environment (at 230 Ma); (2) 215 Ma ago the subsolidus gabbroic-dioritic magma intruded into the crust and interacted with the crustal syenitic melt. Hybrid rocks were formed as a consequence of magma mixing and mingling; (3) parental melt of nepheline syenite was formed by the opening of the Civcin-Severin Rift Zone (160 Ma ago). Mafic, feldspathoid-bearing rocks [ditro-essexite (alkali gabbro or monzodiorite with essexitic-theralitic chemistry)] were generated by hybridization and partial metasomatic substitution; (4) the magmatic system cooled to below 300 °C at 135 Ma. The hydrothermal activity ceased 115 Ma ago; (5) closure of the Ar-system (115 Ma) can be attributed to tectonic uplift caused by nappe transport (Kräutner and Bindea, 1998).
Pană et al. (2000) conducted U–Pb analyses on zircons of syenite; 116 separated grains were examined by Thermal Ionization Mass Spectrometry (TIMS). An age of 229.6 +1.7/−1.2 Ma (Mean Square of Weighted Deviations, MSWD = 1.7) was reported for the syenite. They concluded that the syenite intruded almost at the same time as gabbro and diorite; hence the magmatic evolution of the massif was considerably shorter than previously presumed (e.g., by Pál-Molnár and Árva-Sós, 1995; Kräutner and Bindea, 1998).
Sampling and analytical techniques
Sampling and petrography
Eight rock samples (1 cumulate, 2 syenites, 2 nepheline syenites and 3 granites) were collected from surface outcrops of the DAM. The cumulate rock (VRG6546/b), syenite (VRG7404, VRG7425) and nepheline syenite (VRG6836, VRG7546) were sampled in the valleys of the Tarniţa, Teasc, Holoşag and Fagului Plat creeks. The granite samples (VRG6827, VRG6831, VRG6853) were collected in the valleys of the Turcului and Creanga Mare creeks (Fig. 1B). Petrographic observations were carried out at the Department of Mineralogy, Geochemistry and Petrology, University of Szeged, Szeged, Hungary with optical microscopes. Mineral phases were identified with a THERMO Scientific DXR Raman microscope. Modal compositions (V/V%) in petrographic descriptions were estimated from thin sections. Radiometric age data were classified by the Geologic Time Scale of the ICS (2018/08) (Cohen et al., 2013, updated).
K/Ar geochronology
For the purpose of K/Ar age determination, the least-altered rocks were selected from more than 100 samples. Investigations were performed on separated mineral phases (amphibole and biotite) at the Institute for Nuclear Research, Hungarian Academy of Sciences, Debrecen, Hungary, using a digital flame photometer and a magnetic mass spectrometer. The Asia-1/65 Russian, GL-O French, LP-6 American and HD-B1 German reference materials were used as external standards. Given errors only represent analytical errors (standard deviation); consequently, geologic factors (e.g., Argon-loss, excess Argon) cannot be identified. Description of the equipment, methodology of the analysis and calibration of the device can be found in studies by Balogh (1985) and Odin et al. (1982).
U–Pb geochronology
Titanite (VRG7404) and zircon (VRG7425) crystals were separated from two syenite samples and from one nepheline syenite sample (VRG7546) from the northern part of the DAM (Fig. 1B). Sample preparation for U–Pb geochronology included standard gravity and magnetic separation from the 63–500 µm size fractions. Zircon and titanite crystals were mounted in epoxy resin mounts and were polished to a 1 µm finish. All mineral species were investigated and mapped by optical microscopy, cathodoluminescence (CL) and back-scattered (BSE) imaging. CL and BSE images of mineral separates from nepheline syenite were obtained at the Department of Petrology and Geochemistry, Eötvös Loránd University, Budapest, Hungary using an AMRAY 1830 SEM equipped with GATAN MiniCL (3 nA, 10 kV setup). Imaging of crystals separated from syenite was carried out at the Department of Geosciences, Johann Wolfgang Goethe University, Frankfurt, Germany. In situ U–Pb geochronology was performed at the GÖochron Laboratories, Georg-August University of Göttingen, Göttingen, Germany, using an excimer laser and a Thermo Finnigan Element2 sector field mass spectrometer.
The spot diameters were 23 and 33 µm with an ablation system of ASI Resolution 155. The method employed for analysis is described in detail by Frei and Gerdes (2009). GJ-1 reference zircon (Jackson et al., 2004) was used as "primary standard" and Plešovice zircon (Sláma et al., 2008) and 91500 zircon (Wiedenbeck et al., 1995) were measured as secondary reference materials along with unknown zircon crystals. The MKED1 reference material (Spandler et al., 2016) was used as primary titanite standard, whereas the OLT1 (Kennedy et al., 2010) and BLS (Aleinikoff et al., 2007) were applied as secondary reference materials.
The concordia plots were constructed by IsoplotR (Vermeesch, 2018).
Petrography of the dated samples
Amphibole- and pyroxene-rich cumulate
Amphibole- and pyroxene-rich cumulate (VRG6546/b) consists of idiomorphic–hypidiomorphic cumulus amphibole (Fig. 3A) with variable grain size (macrocrysts ≤11 mm; microcrysts: 100–500 μm). Amphibole oikocrysts (larger than 10 mm) are rich in clinopyroxene, titanite, magnetite and apatite inclusions. Some of the amphiboles alter to epidote and chlorite. Clinopyroxene (≤16 V/V%) occurs as macrocrysts or as inclusions in amphibole oikocrysts, and often shows alteration to secondary amphibole, chlorite or epidote. Hypidiomorphic biotite occurs in small amount (1–20 V/V%). Hypidiomorphic–xenomorphic intercumulus plagioclase (≤12 V/V%) fills up residual space between mafic minerals. Magnetite (≤5 V/V%), primary titanite (≤3 V/V%) and apatite (≤5 V/V%) occur as inclusions in cumulus minerals and as intergranular crystals.
Syenite
Syenite (VRG7404, VRG7425) is phaneritic with a medium to coarse-grained, inequigranular, serial and hypidiomorphic texture. It consists of alkaline feldspar (67–81 V/V%) and plagioclase (18–26 V/V%), accompanied by muscovite (0–1 V/V%), cancrinite (0–7 V/V%) and primary accessory minerals (apatite, zircon and titanite) (0–4 V/V%) (Fig. 3B). Mafic minerals of the groundmass occur in negligible amounts (biotite: 0–1 V/V%). Mafic components form aggregates enclosed in the syenite, comprising amphibole (4–83 V/V%), biotite (3–59 V/V%), clinopyroxene (0–7 V/V%), minor amounts of alkaline and plagioclase feldspars (1–13 and 1–10 V/V%, respectively), accessory- (apatite, zircon and titanite; 0–22 V/V%) and opaque minerals (1–14 V/V%).
Nepheline syenite
Nepheline syenite (VRG6836, VRG7546) is holocrystalline and displays an equigranular, medium to coarse-grained texture. The most common rock-forming minerals are idiomorphic nepheline (7–35 V/V%) and hypidiomorphic–xenomorphic alkaline feldspar (59–90 V/V%) (Fig. 3C). Nepheline is 5–15 mm in size, albeit it often occurs as microcrystals (∼0.5 mm). Along cracks and fissures nepheline is replaced by cancrinite, sodalite or analcime. The amount of plagioclase is negligible (≤10 V/V%). The dominant mafic components are biotite (2–10 V/V%), clinopyroxene (2–7 V/V%) and amphibole (2–5 V/V%). Titanites occur in two generations: 0.1–0.3 and 2.1–2.5 mm in size. Additional magmatic accessory phases are apatite, zircon, magnetite and ilmenite (3–5 V/V%).
Granite
Granite (VRG6827, VRG6831, VRG6853) is phaneritic and inequigranular. It is composed of alkaline feldspar (24–45 V/V%), plagioclase (21–35 V/V%) and quartz (17–31 V/V%) (Fig. 3D). Microcline is often poikilitic and encloses plagioclase, quartz and biotite. Two generations of plagioclases can be recognized: (a) megacrystalline, zoned and sericitic; (b) smaller sized and myrmekitic. Mafic constituents (3–25 V/V%) are represented by biotite and amphibole. Altered amphibole is often accompanied by opaque minerals, biotite and epidote. Secondary rutile and titanite aggregates occur along the cleavage faces of altered biotite. Zircon, titanite, apatite and magnetite are the most common primary accessory minerals.
Results
K/Ar geochronology
Results of K/Ar age dating can be found in Fig. 5 and Table 2. Amphibole of amphibole- and pyroxene-rich cumulate yielded a K/Ar mean age of 238.6 ± 8.9 Ma. An age of 216.0 ± 8.1 Ma was determined for amphibole of nepheline syenite. K/Ar ages of biotite from granite are 201.4 ± 7.6 and 198.3 ± 7.5 Ma. Amphibole of granite gave K/Ar mean ages of 197.3 ± 7.4 and 196.3 ± 7.4 Ma.
Results of K/Ar age dating
Sample | Rock type | Locality and GPS coordinates | Studied fraction | K-content (%) | 40Arrad/g (ncm3/g) | 40Arrad (%) | Age (Ma) |
VRG6546/b | Amphibole- and pyroxene-rich cumulate | Jolotca, Tarniţa de Sus creek 46.87454, 25.49871 | amphibole | 1.16 | 1.15·10−5 | 78.1 | 238.6 ± 8.9 |
VRG6836 | Nepheline syenite | Jolotca, Fagului Plat creek 46.86841, 25.55315 | amphibole | 1.62 | 1.4450·10−5 | 94.8 | 216.0 ± 8.1 |
VRG6827 | Granite | Jolotca, Turcului creek 46.8706, 25.55029 | amphibole | 3.41 | 2.7641·10−5 | 93.6 | 197.3 ± 7.4 |
VRG6831 | Granite | Jolotca, Turcului creek 46.88141, 25.55258 | amphibole | 1.33 | 1.0719·10−5 | 87.7 | 196.3 ± 7.4 |
biotite | 3.46 | 2.8194·10−5 | 92.4 | 198.3 ± 7.5 | |||
VRG6853 | Granite | Jolotca, Creanga Mare creek 46.8743, 25.59169 | biotite | 4.04 | 3.3468·10−5 | 95 | 201.4 ± 7.6 |
U–Pb geochronology
The textural homogeneity of the studied titanite and zircon crystals was inspected using CL and BSE images. The ideal spots for analyses were selected based on these images, in order to avoid crystal parts containing inclusions, different texture or cracks. CL images usually show normal magmatic zoning of the examined titanite and zircon grains. Older or texturally disparate crystal domains were only observed in the case of zircon samples.
Syenite
In-situ U–Pb dating was performed on 15 rim and 16 core domains of titanite crystals. The different growth zones did not yield distinguishable ages within uncertainty. The amount of non-radiogenic 206Pb isotope is high; thus, one can consider the matrix-corrected lower intercept age of 225.3 ± 1.5 Ma with an MSWD value of 1.1 on the Tera-Wasserburg diagram as a relevant datum (n = 31; Fig. 4A), and an interpreted main crystallization age of 225.3 ± 2.7 Ma (with 1% external uncertainties; Table 3).
Summary of U–Pb titanite and zircon ages of the studied syenite and nepheline syenite samples from the Ditrău Alkaline Massif
Sample | Rock type | Locality and GPS coordinates | Studied fraction | Number of measured data/concordant data | Lower intercept age (Ma) | MSWD | Concordia age (number of dates included) | MSWD | Interpreted main crystallisation age (Ma) with uncertainty (including 1% external uncertainties) |
VRG7404 | Syenite | Teasc creek 46.88086, 25.51715 | titanite | 30/0 | 225.3 ± 1.5 | 1.1 | n.d. | n.d. | 225.3 ± 2.7 |
VRG7546 | Nepheline syenite | Teasc creek 46.88461, 25.5132 | titanite | 25/0 | 230.6 ± 2.6 | 1.5 | n.d. | n.d. | 230.6 ± 3.5 |
VRG7425 | Syenite | Holoşag creek 46.87458, 25.53758 | zircon | 32/15 | n.d. | n.d. | 232.4 ± 2.4 (15) | 14 | 232.4 ± 3.3 |
VRG7546 | Nepheline syenite | Teasc creek 46.88461, 25.5132 | zircon | 105/82 | n.d. | n.d. | 230.6 ± 0.8 (81) | 6.9 | 230.6 ± 2.4 |
In-situ U–Pb dates of 32 zircon spots on 12 crystals were measured. The obtained data were filtered according to their discordance (<5%) and resulted in 15 concordant dates, varying between 238.1 and 226.3 Ma. The calculated concordia age is 232.4 ± 2.4 Ma that has a relatively high (14) MSWD value (overdispersion is included in the uncertainty; Vermeesch, 2018; Fig. 4B). The interpreted main zircon crystallization age is 232.4 Ma, with an uncertainty of ± 3.3 Ma (including 1% external uncertainties; Table 3).
Nepheline syenite
The analyzed titanite crystals show around 10% non-radiogenic 206Pb contents; thus, one can apply the fractionation-corrected lower intercept age of 230.6 ± 2.6 Ma with an MSWD value of 1.7 on the Tera-Wasserburg diagram as a relevant datum (Fig. 4C) and an interpreted crystallization age of 230.6 ± 3.5 Ma (n = 25; with external uncertainties; Table 3).
In-situ U–Pb dating was performed on two grain-size fractions of zircon crystals. The obtained 105 data were filtered according to their discordance (<5%). There was no difference in age between the grain size fractions. Analyses yielded 82 concordant ages, ranging between 238.7 and 220.1 Ma. One older, xenocrystic date of 757.8 Ma was detected. The concordia age is 230.6 ± 0.8 Ma, with an MSWD of 6.9 (uncertainty includes the overdispersion of MSWD; Vermeesch, 2018; Fig. 4D). The main zircon crystallization age is 230.6 Ma, with an uncertainty of ± 2.4 Ma (including 1% external uncertainties; Table 3).
Discussion
According to our field structural and petrographic observations, the following inferences can be drawn: (a) based on petrographic and genetic aspects, cumulate rocks (e.g., hornblendite, olivine-rich cumulate, amphibole- and pyroxene-rich cumulate, amphibole-rich cumulate), gabbro and diorite should not be classified into different rock-complexes (e.g., Anastasiu and Constantinescu, 1979; Zólya and Zólya, 1985, 1986; Pál-Molnár, 1988). It can be noticed that these rock types occur adjacently (Fig. 1B) with either abrupt or gradual transition to each other. After Pál-Molnár (2000), the rock association of this structurally and tectonically complex lithostratigraphic unit is referred to as the Tarniţa Complex. Detailed petrogenetic interpretation of this unit can be found in Pál-Molnár et al. (2015b) and Heincz et al. (2018); (b) the gradual transition between diorite, monzodiorite, monzonite and syenite is difficult to trace in the field; (c) transition between syenite, quartz syenite and granite can also be continuous; (d) different-sized metamorphic xenoliths occur in syenite and granite; (e) rocks of the Tarniţa Complex, diorite-syenite and syenite-granite transition zones are cross-cut by nepheline syenite; (f) syenite intruded into the Tarniţa Complex; (g) nepheline syenite and rocks of (a)–(f) are cross-cut by tinguaite dykes; (h) lamprophyre dykes intersect all other rock types of the massif.
Geochronological data
Comparing the results of previous work with our new K/Ar and U–Pb data (Tables 1–3) the diversity of obtained ages, ranging between 238.6 ± 8.9 Ma and 81.3 ± 3.1 (Fig. 5) can be observed. This phenomenon can be explained by the fact that different authors performed K/Ar analyses on various minerals with different closure temperature; however, interpretation of these data should be carried out with caution. Bagdasarian (1972), Streckeisen and Hunziker (1974), Mînzatu and Ardeleanu (1980), as well as Mînzatu et al. (1981) determined whole rock ages. The results of these analyses are mostly mixed ages, due to the different closure temperature and resistance of the minerals. K/Ar data of biotite and feldspars – considering the low closure temperature of these phases – yield the age of postmagmatic events. This means that the ages obtained from minerals with higher closure temperature for the K/Ar decay system [i.e., amphibole: 510 ± 25 °C (Harrison, 1981); Pál-Molnár and Árva-Sós, 1995; Dallmeyer et al., 1997] and the U–Pb ages of titanite and zircon (Pană et al., 2000; this study) could provide the most relevant information about the timing of the magmatic events. The K/Ar age of amphiboles yield reliable information solely when the solidus of the crystallizing magma and the closure temperature of amphibole are comparable. It must be noticed that the amphibole of this study dated by K/Ar method originates from a cumulate rock that – based on previous thermobarometric calculations of Almási et al. (2015) and Pál-Molnár et al. (2015b) – crystallized at considerably higher temperatures (900–1050 °C) than the typical closure temperature of amphibole. Hence, the K/Ar age of the studied amphibole sample displays the minimum crystallization age of the amphibole- and pyroxene-rich cumulate rock. The analyzed titanite and zircon crystallization dates of syenite and nepheline syenite samples are mostly equal within uncertainty and are concordant with the 229.6 +1.7/−1.2 Ma ID-TIMS age of the zircon crystals from a syenite sample published by Pană et al. (2000). This is also in age-agreement with the amphibole data of hornblendite determined by Pál-Molnár and Árva-Sós (1995) and with amphibole data of gabbro and diorite analyzed by Dallmeyer et al. (1997).
The emplacement sequence of the different rock types of the massif – considering field occurrences and overlapping age data – is as follows: cumulate rocks, diorite, monzodiorite, monzonite, syenite, quartz syenite, granite, nepheline syenite, tinguaite, lamprophyre.
Taking into account all age data from the examined rock types in this study, they reveal a slightly broad age span, from 238.6 ± 8.9 Ma (amphibole from cumulate rock by K/Ar method) to 196.3 ± 7.4 Ma (amphibole from granite by K/Ar method). Nevertheless, the younger dates are possibly affected by post-magmatic fluids, similarly to those younger ages from previous studies using K/Ar and Rb–Sr methods. Therefore, the lower limit of the magmatic event age is questionable, since both the archive data and the new K/Ar ages exhibit wide scattering. The upper limit is also ambiguous, as the highest age-value (238.6 ± 8.9 Ma of amphibole from amphibole- and pyroxene-rich cumulate; this study) was determined by the K/Ar method and shows a significant error, overlapping the U–Pb ages.
According to these, it can be concluded that the igneous event age could be most plausible between 238.6 ± 8.9 Ma (amphibole from amphibole- and pyroxene-rich cumulate; this study) and 225.3 ± 2.7 Ma (titanite from syenite; this study), keeping in mind that the most significant U–Pb data scatter around ∼230 Ma.
Using the methodology we have so far, there is no resolvable age difference between the early emplaced cumulate rocks and the late nepheline syenite.
These data contradict the age-range of the multi-stage evolution theory of the DAM proposed by Morogan et al. (2000) and disprove the age-range of the two and multi-stage formation hypothesis of Pál-Molnár and Árva-Sós (1995), Kräutner and Bindea (1998), as well as of Pál-Molnár (2000, 2008).
Palinspastic reconstruction
Based on previous geochemical results (e.g., Morogan et al., 2000; Pál-Molnár 2000, 2010b; Batki et al., 2014; Pál-Molnár et al., 2015b) the DAM was emplaced in an intra-plate, rift-related tectonic environment. Considering the age- and geochemical data, the formation of the massif can be attributed to the evolution of Western-Tethys. Several authors (e.g., Kozur, 1991; Stampfli and Borel, 2002, 2004; Hoeck et al., 2009; Pană, 2010) have made attempts to interpret the rifting and subducting events of the separate oceanic basins of Tethys. Contrasting palinspastic reconstructions have been developed due to the complex structure and tectonic evolution of the area. The formation of the Alps and Carpathians is coherent with the evolution of Meliata-Maliac/Vardar Oceans (Stampfli and Borel, 2002).
According to Stampfli and Borel (2002), the Neotethys started to open in the Late Carboniferous–Early Permian period. This process initiated the drifting of the Cimmerian Block from Pangea and the subduction of Paleotethys in the Middle–Late Triassic period. Slab roll-back of Paleotethys resulted in the formation of back-arc basins along the southern Eurasian margin. Some of these basins evolved into an oceanic basin. Several back-arc basins (e.g., Karakaya, Küre) closed due to the Cimmerian collision in the Jurassic. The Meliata, Maliac and Pindos oceanic branches remained open until the Late Jurassic. Their subduction initiated the opening of further back-arc basins (e.g., Vardar). Subduction of the Küre Ocean was accompanied by the closure of the Meliata-Maliac Ocean in the Late Triassic–Early Jurassic (Stampfli and Borel, 2002).
Kozur (1991) made two Middle–Late Triassic palinspastic reconstructions for the Eastern Carpathians: (a) the postulated Central Dinaric Ocean was situated between the High Karst Zone and the Lim/Bosnian Zone. The two branches of this ocean were the Hallstatt and Meliata Oceans. The Transylvanian–Pieniny Ocean occupied an adjacent but separate basin; (b) according to the second hypothesis of Kozur (1991), a triple junction was formed in the Eastern Carpathians. One of its branches, the Pieniny Ocean, opened up during the Early Anisian, whereas Meliata evolved in the Middle Anisian. The Transylvanian Ocean extended through the Strandzha Zone to the Pontides. Based on Kozur (1991), the Meliata Ocean closed in the Late Jurassic (Oxfordian); its remnants are represented by obducted nappes enclosing ophiolites.
Middle–Late Triassic ophiolite breccias and olistholites occur in the Late Barremian–Early Albian Wildflysch of Rarău, Hăghimaş and Perşani Mountains (Eastern Carpathians). Hoeck et al. (2009) proposed that these rocks are remnants of a subducted oceanic crust, formerly located between the Bucovinian, Infrabucovinian and Northern Apuseni continental panels. The emplacement of the DAM can be attributed to the opening of the oceanic basin. Analogous Middle Triassic intrusions occur in the Southern Alps (Castellarin et al., 1982) and Dinarides (Pamić, 1984). The opening of the Vardar Ocean induced the subduction of the oceanic branch beneath the Northern Apuseni and Infrabucovinian units. The ocean closed in the Late Triassic–Early Jurassic (Hoeck et al., 2009).
Pană (2010) did not agree with the hypothesis of Hoeck et al. (2009), considering (a) that the entire ophiolite suite is not represented, (b) that the studied rocks are located in an intra-continental tectonic setting and (c) that the reported age data are not precise enough. Pană (2010) questioned the credibility of the palinspastic reconstruction of Hoeck et al. (2009). According to Hoeck et al. (2009), the Northern Apuseni block was located north of the Meliata Ocean, albeit Triassic sediments and volcanic rocks of the Northern Apuseni Mountains can be correlated with rocks formed south of the Meliata Ocean (Channell and Kozur, 1997). In the absence of geologic evidence, Pană (2010) argued the hypothesis that the oceanic crust subducted beneath the Northern Apuseni and Infrabucovinian continental domains in the Late Triassic–Early Jurassic.
Geochronological data are in correspondence with the reviewed palinspastic reconstructions and petrogenesis of the DAM. Considering this information, the Ditrău Alkaline Massif was formed in an intra-plate, rift-related extensional tectonic setting at the southwestern margin of the East European Craton (Fig. 6; the postulated area of emplacement is marked by a red rectangle) during the Middle–Late Triassic.
Concluding remarks
Previous, mostly K/Ar geochronological data of the Ditrău Alkaline Massif have been supplemented and refined by new, more precise K/Ar and U–Pb age data. U–Pb geochronology of accessory minerals is the most reliable method to determine the age of magmatic processes, while postmagmatic thermal events can be traced by the K/Ar decay system.
A K/Ar age of 238.6 ± 8.9 Ma was obtained for amphibole of the amphibole- and pyroxene-rich cumulate. Based on in-situ U–Pb dating, titanite and zircon from syenite were formed at 225.3 ± 2.7 Ma and 232.4 ± 3.3 Ma, respectively. Nepheline syenite yielded a K/Ar age of 216.0 ± 8.1 Ma, as well as U–Pb titanite and zircon age of 230.6 ± 3.5 and 230.6 ± 2.4 Ma, respectively. K/Ar age of biotite from granite ranges from 201.4 ± 7.6 to 196.3 ± 7.4 Ma. Considering new and previous (post-1990) K/Ar and U–Pb data, the crystallization of the massif took place between 238.6 ± 8.9 and 225.3 ± 2.7 Ma (noting that the most relevant U–Pb ages scatter around ∼230 Ma).
Age data and tectonic analogies suggest a short magmatic span (Middle–Late Triassic, Ladinian–Norian) of the Ditrău Alkaline Massif. Magmatism could be associated with an intra-plate, rift-related extensional tectonic setting at the southwestern margin of the East European Craton.
Acknowledgements
The authors are grateful to the staff of ‘Vulcano’ Petrology and Geochemistry Research Group, Department of Mineralogy, Geochemistry and Petrology, University of Szeged, Szeged, Hungary and to the technician of the MTA-ELTE Volcanology Research Group. Axel Gerdes of Goethe University, Frankfurt, Germany is gratefully acknowledged for his assistance with preliminary U–Pb analyses. A thorough review, helpful comments and valuable suggestions of Zsolt Benkó (Institute for Nuclear Research, Hungarian Academy of Sciences, Debrecen, Hungary) and of an anonymous reviewer are highly appreciated. Gábor Dobosi is gratefully acknowledged for his editorial work on the manuscript.
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Appendices
Appendix A Results of U–Pb dating of titanites and zircons from syenite
Isotopic data | Ages | RDC age | ||||||||||||||||||
Rock Nr. | Spot Nr. | Studied fraction | U (ppm) | Pb (ppm) | 207Pb/235U | ±1σ (%) | 206Pb/238U | ±1σ (%) | rho | 207Pb/206Pb | ±1σ (%) | 207Pb/235U | ±2σ (Ma) | 206Pb/238U | ±2σ (Ma) | 207Pb/206Pb | ±2σ (Ma) | Disc. (%) | 206Pb/238U | ±2σ (Ma) |
VRG7404 | 136 | titanite (core) | 23 | 135 | 0.72685 | 3.7 | 0.03653 | 1.6 | 0.42 | 0.14433 | 3.4 | 554.7 | 32.0 | 231.3 | 7.1 | 2,279.8 | 58.4 | 58.3 | n.d. | n.d. |
137 | 25 | 110 | 0.75060 | 3.5 | 0.03912 | 1.6 | 0.45 | 0.13916 | 3.1 | 568.6 | 30.6 | 247.4 | 7.6 | 2,216.9 | 54.5 | 56.5 | n.d. | n.d. | ||
138 | 24 | 134 | 0.73909 | 4.4 | 0.03820 | 1.5 | 0.35 | 0.14033 | 4.1 | 561.9 | 38.0 | 241.7 | 7.1 | 2,231.3 | 71.1 | 57.0 | n.d. | n.d. | ||
139 | 23 | 118 | 0.79848 | 3.9 | 0.03866 | 1.8 | 0.45 | 0.14982 | 3.5 | 596.0 | 35.6 | 244.5 | 8.5 | 2,343.9 | 60.2 | 59.0 | n.d. | n.d. | ||
143 | 23 | 118 | 0.77044 | 3.8 | 0.03878 | 1.4 | 0.37 | 0.14408 | 3.6 | 580.0 | 34.3 | 245.3 | 6.9 | 2,276.9 | 61.9 | 57.7 | n.d. | n.d. | ||
144 | 24 | 116 | 0.80808 | 3.6 | 0.03705 | 1.6 | 0.45 | 0.15820 | 3.2 | 601.4 | 33.0 | 234.5 | 7.4 | 2,436.6 | 55.1 | 61.0 | n.d. | n.d. | ||
145 | 25 | 189 | 0.72811 | 3.4 | 0.03788 | 1.4 | 0.41 | 0.13939 | 3.1 | 555.4 | 29.4 | 239.7 | 6.6 | 2,219.7 | 54.3 | 56.8 | n.d. | n.d. | ||
146 | 22 | 112 | 0.97697 | 3.6 | 0.04056 | 1.8 | 0.49 | 017471 | 3.2 | 692.1 | 36.6 | 256.3 | 8.8 | 2,603.3 | 53.2 | 63.0 | n.d. | n.d. | ||
147 | 22 | 133 | 0.76930 | 4.2 | 0.03853 | 1.8 | 0.43 | 0.14482 | 3.8 | 579.4 | 37.0 | 243.7 | 8.5 | 2,285.7 | 65.0 | 57.9 | n.d. | n.d. | ||
148 | 21 | 130 | 0.74806 | 4.7 | 0.03774 | 1.8 | 0.38 | 0.14376 | 4.3 | 567.1 | 41.1 | 238.8 | 8.2 | 2,273.1 | 74.9 | 57.9 | n.d. | n.d. | ||
149 | 22 | 129 | 0.71685 | 4.2 | 0.03714 | 1.8 | 0.43 | 0.13998 | 3.8 | 548.8 | 36.3 | 235.1 | 8.3 | 2,227.0 | 66.8 | 57.2 | n.d. | n.d. | ||
150 | 19 | 119 | 0.74282 | 4.3 | 0.03785 | 1.8 | 0.43 | 0.14235 | 3.9 | 564.0 | 37.6 | 239.5 | 8.7 | 2,256.1 | 67.5 | 57.5 | n.d. | n.d. | ||
151 | 19 | 126 | 0.78341 | 3.8 | 0.03881 | 1.7 | 0.46 | 0.14641 | 3.4 | 587.4 | 34.1 | 245.4 | 8.3 | 2,304.5 | 58.2 | 58.2 | n.d. | n.d. | ||
152 | 21 | 142 | 0.75546 | 4.6 | 0.03755 | 1.9 | 0.41 | 0.14592 | 4.2 | 571.4 | 40.6 | 237.6 | 8.8 | 2,298.7 | 72.3 | 58.4 | n.d. | n.d. | ||
153 | 23 | 100 | 0.90703 | 3.8 | 0.03936 | 1.7 | 0.46 | 0.16712 | 3.4 | 655.5 | 36.8 | 248.9 | 8.4 | 2,529.0 | 56.8 | 62.0 | n.d. | n.d. | ||
154 | 26 | 119 | 0.83752 | 3.3 | 0.03831 | 1.6 | 0.48 | 0.15856 | 2.9 | 617.8 | 31.2 | 242.3 | 7.6 | 2,440.4 | 50.2 | 60.8 | n.d. | n.d. | ||
155 | titanite (external rim zone) | 19 | 124 | 0.73359 | 4.4 | 0.03749 | 2.0 | 0.46 | 0.14192 | 3.9 | 558.7 | 37.7 | 237.2 | 9.3 | 2,250.9 | 67.1 | 57.5 | n.d. | n.d. | |
156 | 20 | 131 | 0.68042 | 4.5 | 0.03771 | 1.8 | 0.40 | 0.13086 | 4.1 | 527.0 | 37.5 | 238.6 | 8.4 | 2,109.5 | 72.9 | 54.7 | n.d. | n.d. | ||
157 | 20 | 128 | 0.72551 | 3.9 | 0.03708 | 1.6 | 0.41 | 0.14191 | 3.5 | 553.9 | 33.4 | 234.7 | 7.3 | 2,250.7 | 61.4 | 57.6 | n.d. | n.d. | ||
158 | 19 | 119 | 0.75104 | 4.6 | 0.03814 | 1.8 | 0.40 | 0.14282 | 4.2 | 568.8 | 40.2 | 241.3 | 8.7 | 2,261.7 | 72.6 | 57.6 | n.d. | n.d. | ||
159 | 18 | 122 | 0.79154 | 4.6 | 0.03882 | 1.9 | 0.41 | 0.14789 | 4.2 | 592.0 | 42.1 | 245.5 | 9.1 | 2,321.8 | 73.0 | 58.5 | n.d. | n.d. | ||
163 | 23 | 121 | 0.82517 | 4.3 | 0.03842 | 1.8 | 0.41 | 0.15577 | 3.9 | 610.9 | 39.9 | 243.0 | 8.4 | 2,410.3 | 67.0 | 60.2 | n.d. | n.d. | ||
164 | 68 | 409 | 0.45308 | 3.0 | 0.03603 | 1.2 | 0.39 | 0.09120 | 2.8 | 379.4 | 19.1 | 228.2 | 5.3 | 1,450.8 | 52.7 | 39.9 | n.d. | n.d. | ||
165 | 21 | 132 | 1.04638 | 4.0 | 0.04026 | 1.6 | 0.40 | 0.18850 | 3.7 | 727.1 | 42.1 | 254.4 | 8.0 | 2,729.2 | 60.9 | 65.0 | n.d. | n.d. | ||
166 | 21 | 132 | 0.70461 | 4.1 | 0.03727 | 1.6 | 0.40 | 0.13712 | 3.8 | 541.5 | 35.0 | 235.9 | 7.6 | 2,191.2 | 66.2 | 56.4 | n.d. | n.d. | ||
167 | 19 | 148 | 0.69969 | 4.6 | 0.03817 | 1.6 | 0.35 | 0.13295 | 4.3 | 538.6 | 38.7 | 241.5 | 7.7 | 2,137.3 | 75.3 | 55.2 | n.d. | n.d. | ||
168 | 19 | 126 | 0.79403 | 4.3 | 0.03852 | 1.4 | 0.33 | 0.14950 | 4.1 | 593.5 | 39.5 | 243.7 | 6.8 | 2,340.3 | 70.6 | 58.9 | n.d. | n.d. | ||
169 | 25 | 183 | 0.64632 | 4.1 | 0.03778 | 1.5 | 0.37 | 012409 | 3.8 | 506.2 | 32.6 | 239.0 | 7.1 | 2.015.9 | 67.1 | 52.8 | n.d. | n.d. | ||
170 | 22 | 165 | 0.70375 | 4.3 | 0.03734 | 1.8 | 0.42 | 0.13669 | 3.9 | 541.0 | 36.1 | 236.3 | 8.3 | 2,185.7 | 67.8 | 56.3 | n.d. | n.d. | ||
171 | 76 | 405 | 0.47834 | 2.4 | 0.03593 | 1.0 | 0.42 | 0.09657 | 2.2 | 396.9 | 15.7 | 227.5 | 4.5 | 1,558.9 | 41.0 | 42.7 | n.d. | n.d. | ||
173 | 19 | 121 | 0.80402 | 5.2 | 0.03884 | 2.1 | 0.41 | 0.15015 | 4.8 | 599.1 | 47.9 | 245.6 | 10.3 | 2,347.7 | 81.9 | 59.0 | n.d. | n.d. | ||
VRG7425 | 186 | zircon | 110 | 90 | 0.26723 | 2.9 | 0.03563 | 0.9 | 0.31 | 0.05440 | 2.7 | 240.5 | 12.3 | 225.7 | 3.9 | 387.8 | 61.5 | 6.2 | 228.0 | 5.5 |
187 | 613 | 1,014 | 0.35413 | 1.4 | 0.03677 | 0.7 | 0.49 | 0.06986 | 1.2 | 307.8 | 7.6 | 232.8 | 3.2 | 924.2 | 26.1 | 24.4 | 233.9 | 5.0 | ||
188 | 269 | 453 | 0.35170 | 2.2 | 0.04026 | 0.8 | 0.36 | 0.06336 | 2.0 | 306.0 | 11.6 | 254.4 | 3.9 | 720.5 | 43.5 | 16.9 | 256.2 | 5.8 | ||
189 | 143 | 163 | 0.50105 | 2.2 | 0.03831 | 0.9 | 0.38 | 0.09485 | 2.1 | 412.4 | 15.2 | 242.4 | 4.1 | 1,525.1 | 39.2 | 41.2 | 244.6 | 5.9 | ||
190 | 63 | 29 | 0.25208 | 4.0 | 0.03671 | 1.1 | 0.28 | 0.04980 | 3.9 | 228.3 | 16.6 | 232.4 | 5.2 | 185.9 | 90.3 | -1.8 | 235.1 | 6.4 | ||
191 | 76 | 37 | 0.27668 | 2.8 | 0.03580 | 1.0 | 0.36 | 0.05604 | 2.6 | 248.0 | 12.5 | 226.8 | 4.5 | 454.2 | 58.7 | 8.6 | 229.4 | 5.8 | ||
192 | 527 | 1,503 | 0.26969 | 1.6 | 0.03744 | 0.7 | 0.45 | 0.05224 | 1.4 | 242.4 | 6.9 | 236.9 | 3.3 | 296.1 | 32.8 | 2.3 | 238.1 | 5.1 | ||
193 | 550 | 1,240 | 0.25668 | 1.6 | 0.03649 | 0.7 | 0.41 | 0.05102 | 1.5 | 232.0 | 6.7 | 231.0 | 3.0 | 241.6 | 34.0 | 0.4 | 232.2 | 4.9 | ||
194 | 455 | 923 | 0.25928 | 1.5 | 0.03662 | 0.7 | 0.45 | 0.05136 | 1.3 | 234.1 | 6.3 | 231.8 | 3.1 | 256.9 | 31.2 | 1.0 | 233.1 | 5.0 | ||
195 | 52 | 21 | 0.26020 | 4.6 | 0.03607 | 1.2 | 0.25 | 0.05232 | 4.5 | 234.8 | 19.5 | 228.4 | 5.3 | 299.3 | 102.4 | 2.7 | 231.3 | 6.6 | ||
196 | 66 | 33 | 0.51201 | 3.2 | 0.03880 | 1.2 | 0.37 | 0.09571 | 3.0 | 419.8 | 22.0 | 245.4 | 5.7 | 1,542.2 | 55.8 | 41.5 | 248.2 | 7.1 | ||
197 | 65 | 27 | 0.31322 | 3.5 | 0.03551 | 1.1 | 0.32 | 0.06398 | 3.3 | 276.7 | 17.0 | 224.9 | 4.9 | 741.0 | 70.2 | 18.7 | 227.6 | 6.2 | ||
198 | 588 | 476 | 0.25556 | 1.5 | 0.03578 | 0.7 | 0.44 | 0.05180 | 1.3 | 231.1 | 6.2 | 226.6 | 2.9 | 276.6 | 31.2 | 1.9 | 227.9 | 4.8 | ||
199 | 145 | 110 | 0.29792 | 2.0 | 0.03829 | 0.9 | 0.43 | 0.05643 | 1.8 | 264.8 | 9.4 | 242.2 | 4.1 | 469.3 | 40.6 | 8.5 | 244.5 | 5.9 | ||
203 | 52 | 22 | 1.02762 | 2.5 | 0.04170 | 1.1 | 0.43 | 0.17871 | 2.3 | 717.7 | 26.0 | 263.4 | 5.6 | 2,641.0 | 38.2 | 63.3 | 266.5 | 7.2 | ||
204 | 784 | 1,286 | 0.25988 | 1.5 | 0.03602 | 0.7 | 0.45 | 0.05232 | 1.3 | 234.6 | 6.1 | 228.1 | 2.9 | 299.6 | 30.1 | 2.7 | 229.1 | 4.9 | ||
205 | 539 | 1,703 | 0.26807 | 1.6 | 0.03719 | 0.7 | 0.42 | 0.05228 | 1.5 | 241.1 | 7.0 | 235.4 | 3.1 | 297.7 | 34.2 | 2.4 | 236.5 | 5.0 | ||
206 | 406 | 866 | 0.29035 | 1.7 | 0.03628 | 0.7 | 0.44 | 0.05805 | 1.5 | 258.8 | 7.7 | 229.7 | 3.3 | 531.7 | 33.1 | 11.3 | 231.1 | 4.9 | ||
207 | 237 | 336 | 0.26695 | 2.0 | 0.03549 | 0.7 | 0.38 | 0.05456 | 1.8 | 240.3 | 8.4 | 224.8 | 3.3 | 394.2 | 40.7 | 6.4 | 226.6 | 4.8 | ||
208 | 63 | 31 | 0.25580 | 3.8 | 0.03823 | 1.2 | 0.31 | 0.04853 | 3.6 | 231.3 | 15.7 | 241.8 | 5.5 | 125.4 | 85.0 | -4.6 | 244.7 | 7.0 | ||
209 | 251 | 247 | 0.25428 | 2.1 | 0.03544 | 0.8 | 0.35 | 0.05204 | 2.0 | 230.0 | 8.8 | 224.5 | 3.3 | 287.0 | 46.1 | 2.4 | 226.3 | 5.1 | ||
210 | 626 | 849 | 0.26920 | 1.5 | 0.03631 | 0.6 | 0.42 | 0.05377 | 1.4 | 242.1 | 6.5 | 229.9 | 2.9 | 361.4 | 31.2 | 5.0 | 231.1 | 4.6 | ||
211 | 59 | 23 | 0.32810 | 4.1 | 0.03641 | 1.2 | 0.29 | 0.06536 | 4.0 | 288.1 | 20.8 | 230.5 | 5.3 | 786.1 | 83.3 | 20.0 | 233.3 | 6.7 | ||
212 | 228 | 150 | 0.25211 | 2.2 | 0.03576 | 0.8 | 0.35 | 0.05113 | 2.1 | 228.3 | 9.2 | 226.5 | 3.5 | 246.8 | 48.5 | 0.8 | 228.4 | 5.2 | ||
213 | 293 | 182 | 0.27302 | 1.8 | 0.03559 | 0.8 | 0.43 | 0.05563 | 1.6 | 245.1 | 7.8 | 225.5 | 3.4 | 437.7 | 36.3 | 8.0 | 227.2 | 5.1 | ||
214 | 74 | 48 | 0.72322 | 2.9 | 0.03765 | 1.2 | 0.42 | 0.13931 | 2.6 | 552.6 | 24.9 | 238.3 | 5.7 | 2,218.7 | 46.0 | 56.9 | 240.9 | 6.9 | ||
215 | 153 | 297 | 0.35895 | 2.4 | 0.03658 | 0.8 | 0.35 | 0.07118 | 2.2 | 311.4 | 12.9 | 231.6 | 3.8 | 962.5 | 45.9 | 25.6 | 233.6 | 5.3 | ||
216 | 58 | 22 | 0.25210 | 4.0 | 0.03649 | 1.1 | 0.28 | 0.05011 | 3.9 | 228.3 | 16.6 | 231.0 | 5.2 | 200.1 | 90.0 | -1.2 | 233.8 | 6.3 | ||
217 | 1,464 | 3,459 | 0.25582 | 1.3 | 0.03640 | 0.6 | 0.45 | 0.05098 | 1.2 | 231.3 | 5.6 | 230.5 | 2.8 | 239.8 | 28.1 | 0.4 | 231.0 | 4.6 | ||
277 | 133 | 130 | 0.30481 | 2.5 | 0.03862 | 1.0 | 0.39 | 0.05724 | 2.3 | 270.1 | 12.1 | 244.3 | 4.7 | 500.8 | 51.9 | 9.6 | 246.6 | 6.3 | ||
278 | 1,336 | 2,526 | 0.26004 | 1.4 | 0.03635 | 0.6 | 0.46 | 0.05189 | 1.2 | 234.7 | 5.7 | 230.1 | 2.9 | 280.5 | 28.1 | 1.9 | 230.8 | 4.6 | ||
279 | 512 | 770 | 0.25622 | 1.7 | 0.03709 | 0.8 | 0.45 | 0.05010 | 1.6 | 231.6 | 7.3 | 234.8 | 3.7 | 199.9 | 36.5 | −1.4 | 236.1 | 5.3 |
Appendix B Results of U–Pb dating of titanites and zircons from nepheline syenite
Isotopic data | Ages | RDC age | ||||||||||||||||||
Rock Nr. | Spot Nr. | Studied fraction | U (ppm) | Pb (ppm) | 207Pb/235U | ±1σ (%) | 206Pb/238U | ±1σ (%) | rho | 207Pb/206Pb | ±1σ (%) | 207Pb/235U | ±2σ (Ma) | 206Pb/238U | ±2σ (Ma) | 207Pb/206Pb | ±2σ (Ma) | Disc. (%) | 206Pb/238U | ±2σ (Ma) |
VRG7546 | 212 | titanite | 66 | 155 | 1.54659 | 2.8 | 0.04607 | 1.6 | 0.59 | 0.24346 | 2.2 | 949.1 | 34.5 | 290.4 | 9.3 | 3142.8 | 36.5 | 69.4 | n.d. | n.d. |
213 | 31 | 120 | 0.77526 | 4.9 | 0.03948 | 2.0 | 0.41 | 0.14243 | 4.4 | 582.8 | 43.6 | 249.6 | 9.8 | 2257.0 | 76.7 | 57.2 | n.d. | n.d. | ||
214 | 40 | 158 | 0.71918 | 4.2 | 0.03807 | 2.1 | 0.50 | 0.13701 | 3.7 | 550.2 | 36.2 | 240.9 | 10.0 | 2189.8 | 63.9 | 56.2 | n.d. | n.d. | ||
215 | 39 | 165 | 0.67799 | 5.3 | 0.03652 | 2.2 | 0.41 | 0.13464 | 4.8 | 525.6 | 43.7 | 231.2 | 9.8 | 2159.5 | 84.1 | 56.0 | n.d. | n.d. | ||
216 | 37 | 143 | 0.74720 | 4.7 | 0.03777 | 2.1 | 0.45 | 0.14347 | 4.2 | 566.6 | 41.6 | 239.0 | 9.9 | 2269.6 | 73.4 | 57.8 | n.d. | n.d. | ||
217 | 41 | 137 | 0.86524 | 3.6 | 0.04055 | 1.9 | 0.53 | 0.15474 | 3.1 | 633.0 | 34.4 | 256.3 | 9.7 | 2399.0 | 52.6 | 59.5 | n.d. | n.d. | ||
218 | 38 | 137 | 1.64935 | 3.3 | 0.04719 | 1.9 | 0.60 | 0.25350 | 2.6 | 989.3 | 41.6 | 297.2 | 11.3 | 3206.8 | 41.9 | 70.0 | n.d. | n.d. | ||
219 | 25 | 127 | 0.67242 | 5.8 | 0.03860 | 2.5 | 0.42 | 0.12634 | 5.3 | 522.2 | 48.0 | 244.2 | 11.8 | 2047.7 | 93.2 | 53.2 | n.d. | n.d. | ||
223 | 24 | 137 | 0.71374 | 5.1 | 0.03837 | 2.1 | 0.42 | 0.13492 | 4.6 | 547.0 | 43.6 | 242.7 | 10.2 | 2163.1 | 81.1 | 55.6 | n.d. | n.d. | ||
224 | 55 | 223 | 0.74245 | 3.6 | 0.03774 | 1.6 | 0.46 | 0.14266 | 3.2 | 563.8 | 31.0 | 238.8 | 7.7 | 2259.8 | 54.7 | 57.6 | n.d. | n.d. | ||
225 | 75 | 289 | 0.68795 | 3.2 | 0.03925 | 1.5 | 0.48 | 0.12712 | 2.8 | 531.6 | 26.7 | 248.2 | 7.5 | 2058.5 | 49.9 | 53.3 | n.d. | n.d. | ||
226 | 27 | 121 | 0.70438 | 5.1 | 0.03791 | 2.1 | 0.41 | 0.13477 | 4.6 | 541.4 | 43.2 | 239.8 | 9.9 | 2161.1 | 81.2 | 55.7 | n.d. | n.d. | ||
227 | 24 | 130 | 0.85630 | 5.4 | 0.03958 | 2.5 | 0.46 | 0.15689 | 4.8 | 628.1 | 51.3 | 250.3 | 12.2 | 2422.5 | 81.8 | 60.2 | n.d. | n.d. | ||
228 | 24 | 134 | 0.77055 | 5.3 | 0.03900 | 2.1 | 0.40 | 0.14330 | 4.8 | 580.1 | 47.2 | 246.6 | 10.3 | 2267.5 | 83.5 | 57.5 | n.d. | n.d. | ||
229 | 20 | 117 | 0.72592 | 5.8 | 0.03821 | 2.3 | 0.39 | 0.13780 | 5.4 | 554.2 | 50.6 | 241.7 | 10.9 | 2199.7 | 93.6 | 56.4 | n.d. | n.d. | ||
230 | 50 | 160 | 0.68620 | 4.1 | 0.03795 | 1.9 | 0.46 | 0.13113 | 3.6 | 530.5 | 34.3 | 240.1 | 9.0 | 2113.2 | 64.2 | 54.7 | n.d. | n.d. | ||
231 | 37 | 138 | 0.71482 | 5.3 | 0.03725 | 2.3 | 0.45 | 0.13916 | 4.7 | 547.6 | 45.0 | 235.8 | 10.9 | 2216.9 | 81.9 | 56.9 | n.d. | n.d. | ||
232 | 32 | 128 | 0.61333 | 4.2 | 0.03810 | 2.0 | 0.46 | 0.11676 | 3.7 | 485.7 | 32.9 | 241.0 | 9.3 | 1907.3 | 67.6 | 50.4 | n.d. | n.d. | ||
233 | 22 | 120 | 2.14270 | 3.9 | 0.05327 | 2.2 | 0.55 | 0.29170 | 3.3 | 1162.7 | 55.2 | 334.6 | 14.2 | 3426.7 | 51.5 | 71.2 | n.d. | n.d. | ||
234 | 21 | 118 | 0.73199 | 6.4 | 0.03692 | 2.3 | 0.36 | 0.14380 | 6.0 | 557.7 | 55.5 | 233.7 | 10.5 | 2273.5 | 102.8 | 58.1 | n.d. | n.d. | ||
235 | 21 | 114 | 0.66111 | 6.3 | 0.03738 | 2.2 | 0.34 | 0.12829 | 5.9 | 515.3 | 51.6 | 236.5 | 10.1 | 2074.7 | 104.5 | 54.1 | n.d. | n.d. | ||
236 | 31 | 122 | 0.67883 | 4.9 | 0.03804 | 2.2 | 0.45 | 0.12944 | 4.4 | 526.1 | 41.0 | 240.6 | 10.6 | 2090.4 | 77.6 | 54.3 | n.d. | n.d. | ||
237 | 50 | 167 | 1.04936 | 3.1 | 0.04245 | 1.9 | 0.60 | 0.17929 | 2.5 | 728.6 | 32.7 | 268.0 | 9.8 | 2646.4 | 42.0 | 63.2 | n.d. | n.d. | ||
238 | 50 | 173 | 0.74667 | 3.7 | 0.03987 | 1.6 | 0.44 | 0.13581 | 3.3 | 566.3 | 32.3 | 252.1 | 7.9 | 2174.5 | 58.2 | 55.5 | n.d. | n.d. | ||
239 | 47 | 169 | 0.75969 | 3.8 | 0.03881 | 1.7 | 0.44 | 0.14197 | 3.4 | 573.8 | 33.3 | 245.5 | 8.0 | 2251.4 | 58.7 | 57.2 | n.d. | n.d. | ||
2 | zircon | 163 | 123 | 0.29791 | 3.1 | 0.03647 | 1.1 | 0.35 | 0.05924 | 2.9 | 264.8 | 14.4 | 230.9 | 4.9 | 575.8 | 63.0 | 12.8 | 233.0 | 6.3 | |
8 | 719 | 588 | 0.25134 | 1.7 | 0.03622 | 0.7 | 0.38 | 0.05032 | 1.6 | 227.7 | 7.1 | 229.4 | 3.0 | 209.7 | 37.5 | -0.8 | 230.6 | 4.9 | ||
9 | 396 | 183 | 0.25785 | 2.6 | 0.03641 | 0.8 | 0.30 | 0.05136 | 2.5 | 232.9 | 10.8 | 230.6 | 3.5 | 257.0 | 56.8 | 1.0 | 232.1 | 5.2 | ||
10 | 260 | 115 | 0.25341 | 2.6 | 0.03638 | 1.0 | 0.38 | 0.05051 | 2.4 | 229.3 | 10.5 | 230.4 | 4.4 | 218.7 | 55.0 | -0.5 | 232.2 | 5.9 | ||
11 | 758 | 481 | 0.25583 | 2.0 | 0.03731 | 0.8 | 0.38 | 0.04973 | 1.8 | 231.3 | 8.2 | 236.1 | 3.5 | 182.5 | 43.0 | -2.1 | 237.3 | 5.4 | ||
12 | 122 | 87 | 0.35852 | 3.5 | 0.03783 | 1.4 | 0.39 | 0.06873 | 3.3 | 311.1 | 19.1 | 239.4 | 6.6 | 890.6 | 67.5 | 23.0 | 241.7 | 7.7 | ||
13 | 815 | 825 | 0.25133 | 1.9 | 0.03642 | 0.7 | 0.37 | 0.05005 | 1.8 | 227.7 | 7.9 | 230.6 | 3.2 | 197.4 | 41.8 | -1.3 | 231.7 | 4.9 | ||
14 | 273 | 411 | 0.39439 | 2.4 | 0.04008 | 1.0 | 0.43 | 0.07136 | 2.1 | 337.6 | 13.6 | 253.4 | 5.1 | 967.8 | 43.9 | 24.9 | 255.1 | 6.5 | ||
15 | 2338 | 4194 | 0.25599 | 1.4 | 0.03642 | 0.6 | 0.40 | 0.05098 | 1.3 | 231.4 | 6.0 | 230.6 | 2.7 | 239.8 | 30.8 | 0.4 | 230.9 | 4.6 | ||
16 | 632 | 830 | 0.30083 | 2.1 | 0.03800 | 0.7 | 0.33 | 0.05740 | 2.0 | 267.1 | 10.0 | 240.5 | 3.3 | 507.1 | 44.2 | 10.0 | 241.7 | 5.1 | ||
17 | 513 | 370 | 0.25407 | 1.8 | 0.03636 | 0.9 | 0.47 | 0.05067 | 1.6 | 229.9 | 7.5 | 230.3 | 3.9 | 226.0 | 37.6 | -0.2 | 231.6 | 5.6 | ||
18 | 346 | 190 | 0.23856 | 2.3 | 0.03601 | 0.8 | 0.35 | 0.04804 | 2.1 | 217.2 | 9.0 | 228.1 | 3.6 | 101.3 | 51.0 | -5.0 | 229.7 | 5.2 | ||
19 | 58 | 19 | 0.27159 | 5.7 | 0.03527 | 1.6 | 0.28 | 0.05585 | 5.5 | 244.0 | 24.8 | 223.4 | 7.1 | 446.4 | 121.3 | 8.4 | 226.2 | 8.0 | ||
20 | 58 | 22 | 0.25220 | 5.1 | 0.03528 | 1.4 | 0.28 | 0.05185 | 4.9 | 228.4 | 21.1 | 223.5 | 6.3 | 278.6 | 113.1 | 2.1 | 226.2 | 7.2 | ||
21 | 614 | 566 | 0.28735 | 2.0 | 0.03626 | 0.7 | 0.35 | 0.05747 | 1.8 | 256.5 | 8.9 | 229.6 | 3.1 | 509.7 | 40.5 | 10.5 | 230.9 | 4.9 | ||
22 | 428 | 336 | 0.24654 | 2.3 | 0.03588 | 0.8 | 0.35 | 0.04983 | 2.1 | 223.8 | 9.2 | 227.3 | 3.6 | 187.1 | 49.8 | -1.6 | 228.7 | 5.2 | ||
27 | 303 | 235 | 0.34566 | 2.3 | 0.03696 | 0.8 | 0.35 | 0.06783 | 2.2 | 301.5 | 12.3 | 234.0 | 3.8 | 863.3 | 45.9 | 22.4 | 235.7 | 5.3 | ||
28 | 145 | 84 | 0.83472 | 2.0 | 0.04177 | 1.2 | 0.62 | 0.14493 | 1.6 | 616.2 | 18.8 | 263.8 | 6.4 | 2287.0 | 28.2 | 57.2 | 266.2 | 7.6 | ||
29 | 684 | 358 | 0.26225 | 1.7 | 0.03752 | 0.6 | 0.36 | 0.05069 | 1.6 | 236.5 | 7.1 | 237.4 | 2.8 | 227.0 | 36.4 | -0.4 | 238.7 | 4.8 | ||
30 | 883 | 534 | 0.26774 | 1.8 | 0.03691 | 0.7 | 0.37 | 0.05260 | 1.7 | 240.9 | 7.8 | 233.7 | 3.1 | 311.8 | 38.6 | 3.0 | 234.7 | 5.0 | ||
31 | 187 | 97 | 0.25814 | 2.9 | 0.03574 | 1.0 | 0.36 | 0.05238 | 2.7 | 233.2 | 12.1 | 226.4 | 4.7 | 302.0 | 61.8 | 2.9 | 228.4 | 5.8 | ||
32 | 410 | 245 | 0.25477 | 2.3 | 0.03615 | 0.7 | 0.32 | 0.05111 | 2.2 | 230.4 | 9.5 | 229.0 | 3.3 | 245.7 | 50.3 | 0.6 | 230.5 | 4.9 | ||
33 | 321 | 213 | 0.24952 | 2.6 | 0.03669 | 0.9 | 0.33 | 0.04932 | 2.4 | 226.2 | 10.5 | 232.3 | 3.9 | 163.0 | 57.1 | -2.7 | 234.0 | 5.6 | ||
34 | 356 | 321 | 0.25461 | 2.6 | 0.03638 | 0.7 | 0.26 | 0.05075 | 2.5 | 230.3 | 10.6 | 230.4 | 3.0 | 229.6 | 57.5 | 0.0 | 232.0 | 4.9 | ||
35 | 329 | 318 | 0.25435 | 2.4 | 0.03601 | 0.9 | 0.35 | 0.05123 | 2.3 | 230.1 | 10.1 | 228.1 | 3.8 | 251.1 | 52.7 | 0.9 | 229.7 | 5.5 | ||
36 | 182 | 158 | 0.24532 | 3.5 | 0.03471 | 1.0 | 0.29 | 0.05125 | 2.6 | 222.8 | 14.0 | 220.0 | 4.3 | 252.2 | 76.9 | 1.2 | 221.9 | 5.7 | ||
37 | 295 | 375 | 0.24633 | 2.8 | 0.03531 | 0.9 | 0.34 | 0.05060 | 2.6 | 223.6 | 11.2 | 223.7 | 4.2 | 222.6 | 60.5 | 0.0 | 225.3 | 5.4 | ||
38 | 205 | 215 | 0.29938 | 2.8 | 0.03565 | 0.8 | 0.30 | 0.06091 | 2.6 | 265.9 | 12.9 | 225.8 | 3.7 | 636.0 | 56.6 | 15.1 | 227.7 | 5.1 | ||
39 | 978 | 796 | 0.26487 | 1.8 | 0.03655 | 0.7 | 0.36 | 0.05255 | 1.7 | 238.6 | 7.7 | 231.5 | 3.0 | 309.3 | 38.4 | 3.0 | 232.4 | 4.9 | ||
40 | 1064 | 845 | 0.25724 | 1.6 | 0.03617 | 0.7 | 0.41 | 0.05157 | 1.5 | 232.4 | 6.8 | 229.1 | 3.0 | 266.4 | 34.5 | 1.4 | 230.0 | 4.9 | ||
41 | 779 | 825 | 0.25774 | 1.6 | 0.03640 | 0.7 | 0.47 | 0.05135 | 1.4 | 232.8 | 6.5 | 230.5 | 3.4 | 256.7 | 32.1 | 1.0 | 231.6 | 4.9 | ||
42 | 167 | 39 | 0.27072 | 3.2 | 0.03657 | 1.0 | 0.32 | 0.05369 | 3.1 | 243.3 | 14.0 | 231.5 | 4.7 | 358.1 | 69.3 | 4.8 | 233.7 | 6.0 | ||
47 | 213 | 58 | 0.24678 | 3.2 | 0.03625 | 0.9 | 0.28 | 0.04936 | 3.1 | 224.0 | 13.1 | 229.6 | 4.2 | 165.2 | 72.7 | -2.5 | 231.6 | 5.6 | ||
48 | 65 | 23 | 0.26598 | 4.4 | 0.03566 | 1.5 | 0.33 | 0.05410 | 4.1 | 239.5 | 18.7 | 225.9 | 6.5 | 375.1 | 92.6 | 5.7 | 228.6 | 7.7 | ||
49 | 65 | 26 | 0.28945 | 4.6 | 0.03597 | 1.2 | 0.26 | 0.05835 | 4.5 | 258.1 | 21.2 | 227.9 | 5.4 | 542.9 | 97.9 | 11.7 | 230.6 | 6.6 | ||
50 | 235 | 191 | 0.25644 | 2.5 | 0.03552 | 0.8 | 0.33 | 0.05236 | 2.4 | 231.8 | 10.4 | 225.0 | 3.6 | 301.2 | 54.3 | 2.9 | 226.8 | 5.1 | ||
51 | 571 | 720 | 0.25764 | 2.0 | 0.03677 | 0.7 | 0.36 | 0.05082 | 1.9 | 232.8 | 8.5 | 232.8 | 3.3 | 232.5 | 44.1 | 0.0 | 234.0 | 5.0 | ||
52 | 551 | 677 | 0.24864 | 2.0 | 0.03646 | 0.7 | 0.34 | 0.04946 | 1.9 | 225.5 | 8.0 | 230.9 | 3.0 | 169.6 | 43.6 | -2.4 | 232.1 | 4.9 | ||
53 | 306 | 147 | 0.25863 | 2.5 | 0.03588 | 0.8 | 0.30 | 0.05227 | 2.4 | 233.6 | 10.6 | 227.3 | 3.5 | 297.1 | 55.3 | 2.7 | 229.0 | 5.2 | ||
54 | 315 | 198 | 0.24386 | 2.1 | 0.03561 | 0.9 | 0.40 | 0.04966 | 1.9 | 221.6 | 8.5 | 225.6 | 3.8 | 179.0 | 45.6 | -1.8 | 227.3 | 5.5 | ||
55 | 133 | 51 | 0.25036 | 3.7 | 0.03603 | 1.1 | 0.29 | 0.05039 | 3.6 | 226.9 | 15.2 | 228.2 | 4.9 | 213.2 | 82.7 | -0.6 | 230.5 | 6.2 | ||
56 | 577 | 1293 | 0.26913 | 2.1 | 0.03632 | 0.8 | 0.39 | 0.05373 | 1.9 | 242.0 | 9.0 | 230.0 | 3.7 | 359.8 | 43.8 | 4.9 | 231.2 | 5.2 | ||
57 | 219 | 189 | 0.25893 | 2.7 | 0.03533 | 0.9 | 0.34 | 0.05315 | 2.5 | 233.8 | 11.3 | 223.8 | 4.0 | 335.4 | 57.7 | 4.3 | 225.7 | 5.4 | ||
58 | 429 | 253 | 0.25053 | 2.1 | 0.03627 | 0.9 | 0.44 | 0.05010 | 1.9 | 227.0 | 8.7 | 229.7 | 4.2 | 199.6 | 44.4 | -1.2 | 231.2 | 5.5 | ||
59 | 216 | 197 | 0.25083 | 3.0 | 0.03587 | 0.9 | 0.30 | 0.05071 | 2.9 | 227.3 | 12.4 | 227.2 | 4.1 | 227.8 | 67.2 | 0.0 | 229.1 | 5.5 | ||
60 | 361 | 220 | 0.25474 | 2.0 | 0.03617 | 0.8 | 0.37 | 0.05107 | 1.9 | 230.4 | 8.4 | 229.1 | 3.4 | 244.2 | 43.8 | 0.6 | 230.7 | 5.2 | ||
61 | 519 | 375 | 0.25554 | 2.1 | 0.03596 | 0.7 | 0.33 | 0.05154 | 2.0 | 231.1 | 8.7 | 227.7 | 3.1 | 265.1 | 45.9 | 1.4 | 229.1 | 4.9 | ||
62 | 384 | 256 | 0.27256 | 2.3 | 0.03625 | 0.7 | 0.33 | 0.05452 | 2.2 | 244.7 | 10.0 | 229.6 | 3.4 | 392.8 | 48.6 | 6.2 | 231.1 | 4.9 | ||
66 | 27 | 12 | 1.10886 | 4.5 | 0.12338 | 1.3 | 0.30 | 0.06518 | 4.7 | 757.6 | 48.7 | 750.0 | 19.1 | 780.2 | 90.6 | 1.0 | 757.8 | 22.1 | ||
67 | 303 | 166 | 0.24457 | 2.6 | 0.03599 | 0.8 | 0.31 | 0.04927 | 2.5 | 222.2 | 10.5 | 228.0 | 3.6 | 161.0 | 58.5 | -2.6 | 229.7 | 5.2 | ||
68 | 483 | 803 | 0.25976 | 1.8 | 0.03710 | 0.7 | 0.42 | 0.05077 | 1.6 | 234.5 | 7.5 | 234.9 | 3.4 | 230.6 | 37.6 | -0.2 | 236.2 | 5.0 | ||
69 | 248 | 170 | 0.24450 | 3.1 | 0.03592 | 1.0 | 0.31 | 0.04936 | 2.9 | 222.1 | 12.4 | 227.6 | 4.3 | 164.8 | 68.8 | -2.5 | 229.4 | 5.8 | ||
70 | 69 | 28 | 0.28168 | 4.8 | 0.03614 | 1.5 | 0.30 | 0.05652 | 4.6 | 252.0 | 21.6 | 228.9 | 6.6 | 472.9 | 101.7 | 9.2 | 231.6 | 7.8 | ||
71 | 126 | 70 | 0.26269 | 3.5 | 0.03634 | 1.1 | 0.33 | 0.05242 | 3.3 | 236.8 | 14.7 | 230.1 | 5.1 | 303.9 | 74.9 | 2.8 | 232.4 | 6.3 | ||
72 | 967 | 1462 | 0.25258 | 1.7 | 0.03593 | 0.8 | 0.44 | 0.05098 | 1.5 | 228.7 | 7.0 | 227.6 | 3.4 | 239.8 | 35.8 | 0.5 | 228.5 | 5.2 | ||
73 | 296 | 284 | 0.26067 | 2.4 | 0.03706 | 0.8 | 0.34 | 0.05101 | 2.3 | 235.2 | 10.2 | 234.6 | 3.8 | 241.2 | 52.6 | 0.3 | 236.3 | 5.3 | ||
74 | 143 | 51 | 0.24486 | 3.3 | 0.03552 | 1.2 | 0.37 | 0.04999 | 3.0 | 222.4 | 13.1 | 225.0 | 5.3 | 194.6 | 70.9 | -1.2 | 227.2 | 6.5 | ||
75 | 696 | 688 | 0.26251 | 1.9 | 0.03601 | 0.7 | 0.39 | 0.05287 | 1.7 | 236.7 | 7.9 | 228.1 | 3.3 | 323.3 | 39.2 | 3.6 | 229.2 | 4.9 | ||
76 | 149 | 28 | 0.24971 | 3.7 | 0.03543 | 1.1 | 0.29 | 0.05111 | 3.5 | 226.3 | 15.0 | 224.5 | 4.7 | 245.7 | 81.1 | 0.8 | 226.7 | 6.1 | ||
77 | 890 | 424 | 0.24788 | 1.7 | 0.03577 | 0.7 | 0.41 | 0.05025 | 1.6 | 224.9 | 7.0 | 226.6 | 3.2 | 206.6 | 37.0 | -0.8 | 227.7 | 4.8 | ||
78 | 446 | 121 | 0.25187 | 2.0 | 0.03572 | 0.8 | 0.38 | 0.05113 | 1.9 | 228.1 | 8.3 | 226.3 | 3.5 | 246.9 | 43.6 | 0.8 | 227.8 | 5.1 | ||
79 | 378 | 102 | 0.26057 | 2.2 | 0.03704 | 0.9 | 0.38 | 0.05102 | 2.1 | 235.1 | 9.5 | 234.5 | 4.0 | 241.6 | 48.0 | 0.3 | 236.1 | 5.7 | ||
80 | 517 | 711 | 0.24154 | 2.1 | 0.03541 | 0.7 | 0.35 | 0.04947 | 1.9 | 219.7 | 8.1 | 224.3 | 3.2 | 170.2 | 45.0 | -2.1 | 225.6 | 4.8 | ||
81 | 859 | 922 | 0.26900 | 1.8 | 0.03631 | 0.7 | 0.37 | 0.05372 | 1.7 | 241.9 | 7.7 | 230.0 | 3.0 | 359.5 | 37.9 | 4.9 | 231.0 | 4.9 | ||
82 | 810 | 882 | 0.25301 | 1.8 | 0.03571 | 0.7 | 0.39 | 0.05137 | 1.7 | 229.0 | 7.5 | 226.2 | 3.2 | 257.6 | 39.1 | 1.2 | 227.3 | 4.8 | ||
347 | 788 | 843 | 0.25886 | 1.9 | 0.03673 | 1.0 | 0.50 | 0.05112 | 1.7 | 233.7 | 8.0 | 232.5 | 4.3 | 246.3 | 38.5 | 0.5 | 233.6 | 6.0 | ||
348 | 220 | 104 | 0.26570 | 2.6 | 0.03712 | 1.1 | 0.42 | 0.05192 | 2.3 | 239.3 | 11.0 | 234.9 | 5.0 | 282.0 | 53.9 | 1.8 | 236.9 | 6.4 | ||
349 | 540 | 409 | 0.25685 | 2.1 | 0.03729 | 1.0 | 0.46 | 0.04995 | 1.8 | 232.1 | 8.6 | 236.0 | 4.5 | 192.9 | 43.0 | -1.7 | 237.4 | 6.0 | ||
350 | 538 | 443 | 0.25604 | 2.0 | 0.03610 | 0.9 | 0.46 | 0.05143 | 1.8 | 231.5 | 8.4 | 228.6 | 4.2 | 260.4 | 41.5 | 1.2 | 230.0 | 5.5 | ||
351 | 1138 | 547 | 0.25040 | 1.9 | 0.03584 | 1.0 | 0.51 | 0.05067 | 1.6 | 226.9 | 7.6 | 227.0 | 4.3 | 225.9 | 37.4 | 0.0 | 227.9 | 5.8 | ||
352 | 1209 | 661 | 0.26116 | 1.8 | 0.03589 | 0.9 | 0.49 | 0.05277 | 1.6 | 235.6 | 7.7 | 227.3 | 4.0 | 319.0 | 36.8 | 3.5 | 228.2 | 5.5 | ||
353 | 1102 | 564 | 0.25674 | 1.8 | 0.03638 | 1.0 | 0.53 | 0.05118 | 1.6 | 232.0 | 7.6 | 230.4 | 4.4 | 249.0 | 36.1 | 0.7 | 231.3 | 5.9 | ||
354 | 286 | 286 | 0.24608 | 2.7 | 0.03603 | 1.1 | 0.42 | 0.04953 | 2.5 | 223.4 | 10.9 | 228.2 | 5.0 | 173.0 | 57.5 | -2.2 | 229.9 | 6.2 | ||
355 | 435 | 494 | 0.26319 | 2.3 | 0.03680 | 1.0 | 0.43 | 0.05187 | 2.1 | 237.2 | 9.7 | 233.0 | 4.5 | 279.6 | 47.5 | 1.8 | 234.4 | 6.0 | ||
356 | 134 | 46 | 0.26488 | 3.8 | 0.03556 | 1.1 | 0.30 | 0.05402 | 3.6 | 238.6 | 16.0 | 225.3 | 5.0 | 371.8 | 80.7 | 5.6 | 227.5 | 6.2 | ||
358 | 252 | 255 | 0.25008 | 2.5 | 0.03630 | 1.0 | 0.40 | 0.04997 | 2.3 | 226.6 | 10.3 | 229.9 | 4.6 | 193.5 | 54.2 | -1.4 | 231.6 | 5.9 | ||
359 | 168 | 74 | 0.24981 | 3.2 | 0.03608 | 1.1 | 0.33 | 0.05022 | 3.0 | 226.4 | 13.0 | 228.5 | 4.7 | 205.1 | 70.2 | -0.9 | 230.6 | 6.2 | ||
364 | 150 | 69 | 0.16750 | 4.8 | 0.03571 | 1.2 | 0.24 | 0.03402 | 4.6 | 157.3 | 14.0 | 226.2 | 5.2 | 0.1 | 0.0 | -43.8 | 228.3 | 6.5 | ||
365 | 412 | 304 | 0.24596 | 2.6 | 0.03548 | 1.1 | 0.41 | 0.05029 | 2.4 | 223.3 | 10.5 | 224.7 | 4.8 | 208.3 | 55.2 | -0.6 | 226.2 | 6.1 | ||
367 | 120 | 66 | 0.21858 | 4.1 | 0.03522 | 1.2 | 0.30 | 0.04501 | 3.9 | 200.7 | 14.9 | 223.1 | 5.4 | 0.1 | 0.2 | -11.2 | 225.4 | 6.5 | ||
368 | 447 | 299 | 0.24771 | 2.7 | 0.03657 | 1.2 | 0.43 | 0.04913 | 2.5 | 224.7 | 11.0 | 231.5 | 5.3 | 154.0 | 57.8 | -3.0 | 233.0 | 6.7 | ||
369 | 300 | 215 | 0.25628 | 2.9 | 0.03739 | 1.1 | 0.38 | 0.04971 | 2.7 | 231.7 | 12.2 | 236.6 | 5.2 | 181.7 | 63.3 | -2.1 | 238.4 | 6.4 | ||
370 | 419 | 377 | 0.25357 | 2.1 | 0.03715 | 1.0 | 0.47 | 0.04951 | 1.9 | 229.5 | 8.8 | 235.1 | 4.6 | 172.1 | 44.3 | -2.5 | 236.6 | 6.0 | ||
371 | 755 | 596 | 0.25527 | 2.2 | 0.03588 | 1.0 | 0.46 | 0.05160 | 1.9 | 230.8 | 9.0 | 227.2 | 4.5 | 267.8 | 44.6 | 1.6 | 228.4 | 5.8 | ||
372 | 1302 | 1870 | 0.26212 | 1.8 | 0.03642 | 0.9 | 0.49 | 0.05221 | 1.6 | 236.4 | 7.7 | 230.6 | 4.1 | 294.5 | 36.5 | 2.5 | 231.3 | 5.5 | ||
373 | 321 | 221 | 0.26007 | 2.7 | 0.03058 | 1.1 | 0.41 | 0.06167 | 2.5 | 234.7 | 11.5 | 194.2 | 4.3 | 662.8 | 53.5 | 17.3 | 195.7 | 5.3 | ||
374 | 508 | 322 | 0.25522 | 2.2 | 0.03647 | 1.0 | 0.48 | 0.05075 | 1.9 | 230.8 | 9.0 | 230.9 | 4.8 | 229.7 | 44.1 | 0.0 | 232.3 | 5.9 | ||
375 | 447 | 260 | 0.25287 | 2.4 | 0.03598 | 1.0 | 0.41 | 0.05097 | 2.2 | 228.9 | 9.8 | 227.9 | 4.4 | 239.5 | 50.2 | 0.4 | 229.4 | 5.8 | ||
376 | 845 | 506 | 0.25212 | 2.0 | 0.03588 | 0.9 | 0.46 | 0.05096 | 1.7 | 228.3 | 8.0 | 227.3 | 4.0 | 239.0 | 40.1 | 0.5 | 228.3 | 5.5 | ||
377 | 226 | 131 | 0.27130 | 4.0 | 0.03662 | 1.2 | 0.31 | 0.05373 | 3.8 | 243.7 | 17.3 | 231.9 | 5.5 | 359.9 | 85.4 | 4.9 | 233.8 | 6.7 | ||
378 | 747 | 454 | 0.25565 | 2.0 | 0.03654 | 0.9 | 0.46 | 0.05074 | 1.8 | 231.2 | 8.4 | 231.4 | 4.2 | 229.0 | 41.9 | -0.1 | 232.5 | 5.6 | ||
379 | 390 | 247 | 0.24105 | 2.6 | 0.03581 | 1.0 | 0.38 | 0.04882 | 2.4 | 219.3 | 10.5 | 226.8 | 4.5 | 139.1 | 57.6 | -3.4 | 228.4 | 5.8 | ||
383 | 368 | 134 | 0.25856 | 2.2 | 0.03557 | 1.0 | 0.46 | 0.05272 | 2.0 | 233.5 | 9.2 | 225.3 | 4.4 | 316.6 | 44.7 | 3.5 | 226.9 | 5.8 | ||
384 | 353 | 154 | 0.24551 | 2.6 | 0.03595 | 1.0 | 0.37 | 0.04954 | 2.5 | 222.9 | 10.6 | 227.7 | 4.3 | 173.4 | 57.3 | -2.1 | 229.3 | 5.8 | ||
385 | 210 | 109 | 0.24320 | 3.3 | 0.03443 | 1.2 | 0.35 | 0.05124 | 3.1 | 221.0 | 13.3 | 218.2 | 5.0 | 251.5 | 71.8 | 1.3 | 220.1 | 6.3 | ||
386 | 181 | 41 | 0.26851 | 3.4 | 0.03588 | 1.1 | 0.31 | 0.05427 | 3.2 | 241.5 | 14.6 | 227.3 | 4.7 | 382.4 | 72.5 | 5.9 | 229.3 | 6.2 | ||
387 | 219 | 154 | 0.24940 | 3.4 | 0.03547 | 1.3 | 0.38 | 0.05100 | 3.1 | 226.1 | 13.9 | 224.7 | 5.8 | 240.9 | 72.6 | 0.6 | 226.6 | 6.9 | ||
388 | 56 | 19 | 0.19895 | 7.6 | 0.03552 | 1.6 | 0.22 | 0.04063 | 7.4 | 184.2 | 25.7 | 225.0 | 7.2 | 0.1 | 0.1 | -22.1 | 227.8 | 8.1 | ||
389 | 355 | 452 | 0.27273 | 2.5 | 0.03676 | 1.0 | 0.41 | 0.05380 | 2.2 | 244.9 | 10.8 | 232.7 | 4.6 | 362.8 | 50.9 | 5.0 | 234.4 | 6.0 | ||
390 | 65 | 27 | 0.27183 | 4.7 | 0.03519 | 1.7 | 0.37 | 0.05602 | 4.3 | 244.2 | 20.3 | 223.0 | 7.6 | 453.2 | 96.1 | 8.7 | 225.6 | 8.4 | ||
391 | 61 | 23 | 0.25265 | 6.6 | 0.03455 | 1.5 | 0.23 | 0.05303 | 6.5 | 228.7 | 27.4 | 219.0 | 6.6 | 330.3 | 146.5 | 4.3 | 221.6 | 7.5 | ||
392 | 66 | 22 | 0.22581 | 5.2 | 0.03558 | 1.4 | 0.28 | 0.04603 | 5.0 | 206.7 | 19.5 | 225.4 | 6.4 | 0.1 | 9.6 | -9 | 228.1 | 7.3 | ||
393 | 179 | 199 | 0.26902 | 3.6 | 0.03580 | 1.1 | 0.30 | 0.05451 | 3.4 | 241.9 | 15.4 | 226.7 | 4.8 | 392.1 | 76.3 | 6.3 | 228.7 | 6.2 | ||
394 | 253 | 307 | 0.24991 | 3.1 | 0.03537 | 1.1 | 0.36 | 0.05125 | 2.9 | 226.5 | 12.8 | 224.0 | 5.0 | 252.2 | 67.6 | 1.1 | 225.8 | 6.1 | ||
395 | 145 | 69 | 0.24820 | 3.4 | 0.03574 | 1.2 | 0.36 | 0.05037 | 3.2 | 225.1 | 13.8 | 226.4 | 5.4 | 212.2 | 73.8 | -0.6 | 228.5 | 6.5 |