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Emplacement depths and radiometric ages of Paleozoic plutons of ...

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238<br />

ranging from 890 to 940 jC for Opx–Prg–Spl<br />

assembl<strong>ages</strong> (Vsˇeruby <strong>and</strong> Neukirchen olivine gabbro;<br />

Fig. 6D) <strong>and</strong> 810 to 920 jC for Opx–Cpx–Spl<br />

coronas (Hoher–Bogen olivine metagabbro; Fig. 6F).<br />

For these rocks, a pressure estimate is possible based<br />

on the reaction: Ol + Pl F H2O ! Opx + Am or Cpx +<br />

Spl. Such coronitic micr<strong>of</strong>abrics are typical features in<br />

olivine gabbros that underwent magmatic cooling or<br />

high-grade metamorphism at P =6.5–8 kbar (e.g.,<br />

Grantham et al., 1993; Jan <strong>and</strong> Karim, 1995). According<br />

to Bucher <strong>and</strong> Frey (1994), such micr<strong>of</strong>abrics are<br />

diagnostic for pressures >6 kbar. In Fig. 6D <strong>and</strong> F, the<br />

spinel-in reaction in the system CaO–MgO–Al2O3–<br />

SiO2 is illustrated according to Gasparik (1984). In<br />

natural systems containing iron (XMg = ca. 0.9), spinel<br />

may occur at some lower pressures (Bucher <strong>and</strong> Frey,<br />

1994).<br />

6. Radiometric dating<br />

For carrying out K–Ar age dating, biotite <strong>and</strong><br />

hornblende have been separated from samples <strong>of</strong> the<br />

Smrzˇovice <strong>and</strong> Teufelsberg intrusions. Light brown to<br />

greenish magnesio-hornblende sampled from finegrained<br />

hornblende–biotite diorite <strong>of</strong> the large Smrzˇovice<br />

quarry (sample SK 4, Location 2 in Fig. 1) shows<br />

weak alteration along the cleavage planes. Magnetic<br />

<strong>and</strong> unmagnetic fractions yield 547 F 7 <strong>and</strong> 549 F 7<br />

Ma, respectively (Table 2). Dark brown to reddish<br />

brown biotite separated from biotite–hornblende<br />

quartz diorite <strong>of</strong> the Smrzˇovice quarry (sample 113)<br />

shows few inclusions <strong>of</strong> plagioclase, ilmenite<br />

F hornblende. The degree <strong>of</strong> biotite alteration is<br />

very weak. In a few places, biotite is moderately<br />

altered to clinozoisite (along the cleavage planes)<br />

<strong>and</strong>/or chlorite at the margins. K–Ar dating <strong>of</strong> this<br />

biotite yields 495 F 6 Ma (Table 2).<br />

K–Ar dating <strong>of</strong> biotite <strong>of</strong> the Teufelsberg pyroxene<br />

diorite (Location 7 in Fig. 1) yields 342 F 4 Ma.<br />

Similar to the Smrzˇovice samples, the Teufelsberg<br />

biotite is relatively fresh. Rare alteration in form <strong>of</strong><br />

weak chloritization is restricted to the marginal parts.<br />

The separated zircons <strong>of</strong> the Teufelsberg diorite<br />

(Location 7 in Fig. 1) are colourless <strong>and</strong> yellow<br />

belonging to the subtypes S20 to S25 <strong>and</strong> J1 to J5<br />

according to the classification <strong>of</strong> Pupin (1980). The<br />

internal structure <strong>of</strong> the zircons is perceptible in<br />

C. Bues et al. / Tectonophysics 352 (2002) 225–243<br />

cathodoluminescence (CL) im<strong>ages</strong> oriented parallel<br />

to the zircon c-axis. The different light–dark contrasts<br />

<strong>and</strong> bright color display different amounts <strong>of</strong> trace<br />

element content. The bright color represents more or<br />

less pure zircon phase, whereas the different dark<br />

colors reflect variable amount <strong>of</strong> U <strong>and</strong> Y contents.<br />

The internal structure <strong>of</strong> all zircons is complex (e.g.,<br />

Fig. 7). A rounded heterogeneous core is surrounded<br />

by a thin discordant bright zone (A in Fig. 7), the<br />

latter suggesting a first stage <strong>of</strong> dissolution. A narrowspaced<br />

oscillatory zoning follows combined with<br />

compositional sector zoning between dark prisms<br />

<strong>and</strong> light–dark 101-pyramides until a second stage<br />

<strong>of</strong> dissolution is indicated by a thin discordant bright<br />

zone (B in Fig. 7). Towards the margin, a similar<br />

combination follows including small light–dark 211pyramids<br />

ceasing with a third stage <strong>of</strong> dissolution<br />

indicated by a thick discordant bright zone (C in Fig.<br />

7). The margin <strong>of</strong> the zircon consists <strong>of</strong> dark prisms<br />

<strong>and</strong> pyramids.<br />

The single zircons have a weight <strong>of</strong> 37–41 Ag <strong>and</strong><br />

thus, a total lead from 513 to 998 pg, resulting in high<br />

beam intensities <strong>and</strong> allowing static-mode measurements<br />

in all cases. The concordant single zircon 1 <strong>and</strong><br />

four discordant single zircons 2 to 5 define a discordia<br />

with an upper intercept at 361 F 4 Ma <strong>and</strong> a lower<br />

intercept at 16 F 12 Ma (Fig. 8F, Table 3). These data,<br />

together with the age <strong>of</strong> a concordant zircon at<br />

359 F 2 Ma, are interpreted to reflect the age <strong>of</strong> the<br />

zircon crystallization <strong>and</strong> thus, the magmatic emplacement<br />

age <strong>of</strong> the Teufelsberg diorite. Although the CL<br />

im<strong>ages</strong> show a complex core pattern in the zircons, no<br />

inherited lead could be detected (Table 3).<br />

7. Discussion <strong>and</strong> conclusions<br />

The Vsˇepadly granodiorite <strong>and</strong> the Smrzˇovice<br />

diorite <strong>of</strong> the NE part <strong>of</strong> the NKM intruded at shallow<br />

crustal levels (< 7 km depth) as is indicated by Al-in-<br />

Hbl barometry. Similar emplacement <strong>depths</strong> have<br />

been determined for the Těsovice granite <strong>of</strong> the<br />

adjacent Stod pluton (Zulauf et al., 1997). A supracrustal<br />

emplacement level is also indicated by the<br />

small differences between U–Pb zircon <strong>ages</strong> (that<br />

reflect the time <strong>of</strong> pluton emplacement) <strong>and</strong> K–Ar<br />

<strong>and</strong> Ar–Ar <strong>ages</strong> <strong>of</strong> hornblende <strong>and</strong> mica (that reflect<br />

cooling <strong>of</strong> the pluton through particular isotherms).

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