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Geologia Sudetica, 1999, 32:49-53.

A review of Rb-Sr isotope patterns in the Carboniferous granitoids of the Sudetes in SW Poland

Padhraig S. Kennan

1

, Helena Dziedzic

2

, Marek W. Lorenc

2

& Michat P. Mierzejewski

1 University College Dublin, Geology Department, Belfield, Dublin-4, Ireland

2 Polska Akademia Nauk, Instytut Nauk Geologicznycb, Zaklad Geologii Sudetow, 50-449 Wroclaw, ul. Podwale 75

3 Uniwersytet Wrodawski, Instytut Nauk Geologicznycb, 50-205 Wroclaw, ul Cybulskiego 30

Key words: Sudetes, Variscan granites, Rb-Sr ages, Sr-isotope systems, magma source

Abstract

Carboniferous granite intrusions are a relatively uncontroversial element in the geological history of the Sudetes in SW Poland. The Sr-isotope systems in these granites show geological scatter indicative of contamination by crustal rock, failure to homogenise during intrusion/crystallisation and inheritance from source. Rb-Sr ages are thus somewhat compromised and imprecise. The granites originated from a relatively primitive source that underlay much of the region in Carboniferous times.

Manuscript received 17 October 1998, accepted 23 April 1999

INTRODUCTION

T h e Western Sudetes appear, geologically, t o be a col- lage of discrete terranes that were d r a w n together during the complex and problematic history of a Palaeozoic oro- gen in central E u r o p e (Zelazniewicz, 1997). T h o u g h m a n y aspects of the geological history of the region remain prob- lematical, there is n o question but that in Carboniferous and early Permian times, a m a j o r post-orogenic episode of granite plutonism and coeval volcanism occurred in the Western Sudetes.

Isotopic ages suggest that igneous activity continued f o r a relatively long period, i.e., during the interval 350- 260 Ma. I m p o r t a n t intrusions n o w exposed, and w h i c h are the subject of this paper, are those of the Niemcza Zone, Strzelin, Strzegom-Sobotka and Karkonosze. N o Rb-Sr data is available f o r the related K l o d z k o - Z t o t y Stok Massif

(Fig. 1). In the discussion below, the generic term granite is widely used.

Whereas the ages of these granites in the broader scheme of things is n o t in doubt, precise Rb-Sr ages f o r the individual intrusions have proved somewhat elusive. T h e purpose of this short paper is t o review the Rb-Sr data that are available f o r these granites as a group w i t h a view to initiating f u r t h e r discussion on (a) comparisons between the individual granites, (b) any differences between the various intrusions and between these post-orogenic intru- sions and older pre 450 Ma granitoids and (c) the possibil- ity that whole-rock Sr-isotope data might reveal source variations at depth which in t u r n might help t o locate ma- jor junctions in this area of great structural complexity on the N E margin of the Bohemian Massif.

Rb-Sr WHOLE-ROCK SYSTEMS IN GRANITE: INTERPRETATION

Whole-rock Rb-Sr data f r o m m a n y places including the Sudetes have provided p o o r l y constrained ages o r have quite simply p r o v e n difficult t o interpret. W h e r e confir- m a t i o n of an age by means of, e.g., single zircon U - P b data, is available, the Rb-Sr data may be simply ignored or, at best, accorded a lesser status. Little attention is usually given t o the possible reasons f o r the failure t o obtain pre- cise ages. T h e p r o b l e m may lie not so much in the behav-

iour of R b and Sr as in the field; perhaps it m a y be over- come by good sampling strategies.

Rb-Sr whole-rock isochron ages f o r granites rely on the assumption that at the time of intrusion/crystallisa- tion, Sr-isotope homogenisation occurred, i.e., that all the samples analysed were characterised by a c o m m o n 8 7S r / Sr value at that time. It is frequent occurrence that data f r o m individual samples fail t o plot on an isochron defined

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I I O V E R S T E P S E D I M E N T S Y / A M E T A M O R P H I C ROCKS ( U N D I V I D E D ? I * * | V A R I S C A N S R A N I T O I D S L« ' I C A O O M I A N B R A N O D I O R I T E S I / ' ' ' I ORTHOONEISSES 5 0 0 MO I * I M A F I C ROCKS

THRUSTS FAULTS

Fig. 1. Outline geology of the Variscan granites in the Western Sudetes (after Zelazniewicz 1997, modified).

EFZ - Elbe Fault Zone; FSB - Fore-Sudetic Block; GSB - Gory Sowie Block; 1KB - Izera-Karkonosze Block; K - Karkonosze;

KZ - Ktodzko-Zloty Stok Massif; LG - Lausitz Granodiorite;

MZ - Moldanubian Zone; N - Niemcza Shear Zone; OFZ - Odra Fault Zone; RHZ - Rhenohercynian Zone; S - Strzelin Massif;

SMF - Sudetic Marginal Fault; SN - Snieznik gneisses; SS - Strze- gom-Sobotka Massif; STZ - Saxothuringian Zone.

by the majority of samples f r o m a single granite intrusion or that a family of samples may fail to supply an isochron at all. This is simply a reflection of the fact that, in m a n y granites, the essential condition was, f o r one reason or an- other, n o t attained. T o reject the odd sample may compro- mise any age calculated. T o consider the data set as useless may be t o lose valuable information bearing on granite source.

M a n y reasons have been proposed to explain w h y granite whole-rock Rb-Sr data might fail t o provide iso- chrons and thus fail t o support reliable ages. These include weathering and alteration, magma mixing, inheritance f o r

m e n t and fluid exchange (see, e.g., Zheng, 1989). In addi- tion, spurious ages may result if the scale of possible ho- mogenisation is ignored (e.g., Roddick & C o m p s t o n , 1977); this draws attention t o sampling strategy and the question of w h e t h e r samples chosen (or forced t o be cho- sen by, e.g., available outcrop) are likely to produce a use- ful result. In single composite intrusions, it is clear that rock composition may influence apparent ages (e.g., Stephens & Halliday, 1980). Sample size may play a crucial role. In a Caledonian granite in western Ireland, f o r exam- ple, Kennan et at, (1987) using small samples obtained a very different result f r o m that obtained by Leggo et al.

(1966) t h o u g h the very same locations were sampled. Fi- nally, in even a single granite variety supposedly part of a fractionated sequence, a cryptic initial S r /8 6S r variation with depth in an intrusion may be preserved (Mohr, 1991).

It may seem that good Rb-Sr whole-rock ages might be the exception rather than the rule. H o w e v e r , a good sam- pling strategy can overcome most of the problems briefly noted above. T h o u g h ages may be often difficult t o define precisely, the fact that Rb-Sr whole-rock data f r o m gran- ites is robust, and not as susceptible as might be t h o u g h to late post-crystallisation disturbance, is supported b y the fact that data f r o m suites of individual granites reveal ma- jor and systematic regional differences. In Ireland, Rb-Sr whole-rock data f o r Caledonian granites precisely identify regional domains ( M u r p h y et al., 1991) and reflect (and locate) m a j o r structural boundaries, e.g., the Iapetus Suture (Todd etal., 1991).

T h e Sr-isotope chemistry of m a n y granites n o t only reflects isotopic homogenisation but may clearly, at one and the same time, be an image their variable sources. A n y attempt to date granites using whole-rock Rb-Sr methods must take account of that duality.

THE CARBONIFEROUS GRANITES OF THE WESTERN SUDETES

The Karkonosze Granite is the largest of the Carbon- iferous intrusions as exposed (Fig. 1). Rb-Sr data f r o m sam- ples collected in t w o separate quarries (Huta and Michato- wice) define t w o parallel isochrons supporting ages of about 328 Ma f o r this intrusion ( D u t h o u et al., 1991).

Clearly this granite did n o t have a u n i f o r m 8 7S r /b 'Sr ratio at that time; intrusion and crystallisation did not result in large-scale Sr-isotope homogenisation. Data f r o m borehole 0akuszyce) samples, collected between 200-1000 metres depth, certainly do not define an isochron; a u n i f o r m Sr/ Sr was not achieved over that depth range. Data f r o m samples representing a short 250 metre interval of the core c o n f i r m the age of D u t h o u et al., 1991 (unpub- lished University College D u b l i n data).

These observations p r o m p t comparison w i t h the Lein- ster Granite in SE Ireland in which M o h r (1991) demon- strated significant Sr-isotope variation with depth in a granite intrusion not unlike the Karkonosze in overall structure and petrography. As the sampling was confined

t o individual quarries, the age of c. 328 Ma is p r o b a b l y accurate.

T h e Strzelin Granitoid Massif (Fig.l) is composed of small intrusions of granite, granodiorite and diorite corre- sponding t o the deeper r o o t zone of a pluton and which are hosted by Palaeozoic and Proterozoic rocks m e t a m o r - phosed and deformed during the Variscan O r o g e n y (Lorenc, 1994; Oberc-Dziedzic etal., 1994, 1996).

Rb-Sr data f r o m biotite granites give an age of about 347 Ma and, data f r o m biotite-muscovite granites, an age of about 330 Ma (Oberc-Dziedzic et al., 1994, 1996). Data f r o m m o r e basic granites failed t o give an age. H o m o g e n i - sation of these various granitoids clearly did n o t occur on a large scale.

T h e granite data plot on o r very close t o the Variscan array d r a w n on Figure 2 where, curiously, the data f o r the different Strzelin rocks appear t o bracket the data f o r the Karkonosze granite. A similar source is indicated by the similar initial ratios.

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Rb-Sr I S O T P E P A T T E R N S I N T H E C A R B O N I F E R O U S G R A N I T O I D S 51

Fig. 2. Pattern of Sr-isotope data from the Variscan granites (mostly from text references but including some unpublished data from Karkonosze). Niemcza granitoids show trend towards Gory Sowie gneiss values. Data from Karkonosze and Strzegom- Sobotka are undifferentiated but much of the latter plots below the 328 Ma references line. Rectangular boxes enclose Strzelin granite values (see text). The 450 Ma reference line is as on Fig. 5.

T h e granitoids of the N i e m c z a Z o n e (Fig.l) were em- placed syntectonically into w h a t was a m a j o r zone of re- gional shearing in Variscan times. T h e intrusions comprise n u m e r o u s small bodies w h i c h are, perhaps, connected at depth. In the field, medium-grained p o r p h y r i t i c granites and granodiorites characterised b y an abundance of en- claves are typical of the granites in the zone. These con- trast w i t h finer-grained, m o r e dioritic varieties lacking en- claves. Their present o u t c r o p is m o r e or less confined to a n u m b e r of discrete quarries in some of which, sharp con- tacts between the t w o varieties can be seen. Oliver et al.

(1993) obtained a U - P b zircon age of about 338 Ma f o r a h o r n b l e n d e syenite f r o m this suite. A complete descrip- tion of these granites and their chemistry is in preparation by Kennan, Lorenc and Dziedzic.

Rb-Sr data f o r these granites do n o t provide any rea- sonable age (Lorenc, 1998). T h e y do, however, show (a) some degree of coherence within each quarry w h e n the data are considered in the light of the U - P b zircon age. O n an isochron diagram,^the data reveal^an overall pattern ris- ing f r o m low R b / Sr and S r / Sr values t o the rela- tively high values of b o t h parameters (Fig. 3). T h e higher values apply t o granites f r o m the large quarry at Kosmin w h e r e the granite is relatively rich in enclaves. O u t c r o p observation suggests progressive digestion of the enclaves.

Rb-Sr isotope data f o r t w o enclaves (Fig. 3) seem t o indi- cate contamination by crustal material.

T h e N i e m c z a Shear Z o n e f o r m s the eastern margin of the o u t c r o p of the gneisses of the G o r y Sowie (Fig. 1). A limited a m o u n t of Rb-Sr data f o r the gneisses given by Van Breemen et al. (1982) does not rule out contamination of the N i e m c z a granites b y material f r o m these gneisses.

T h e N i e m c z a data plot at the l o w 8 7R b /8% r end of the Variscan array on Figure 2. T h e granites lacking enclaves plot closest t o the array suggesting that they and the other m a j o r granites come f r o m comparable sources if not one source. T h e enclave-rich varieties curve upwards f r o m the

Fig. 3. Pattern of Sr-isotope data for the Niemcza granites. En- clave-rich granites form a transition between values from granites lacking enclaves and enclave values. The 340 Ma reference line corresponds to a U-Pb zircon age for these granites (see text).

Variscan array towards that of the older gneisses. Some of the scatter in the data f r o m , e.g., the Karkonosze intrusion w h i c h does contain scattered enclaves, may reflect the same incorporation of enclave material.

Some granitoids (monzogranites) f r o m the Strzegom- Sobotka Granitic Massif (Fig. 1) give Rb-Sr ages of about 280 Ma (Pin et al, 1989). O n c e again, parallel isochrons suggest batches of magma w i t h distinct 8 7S r /8 6S r ratios that did not mutually homogenise. Somewhat surpris- ingly, a two-mica granite f r o m this massif gives an older age of about 326 Ma. Pin et al (1989) concluded that to- tally unrelated geodynamic causes had operated f o r differ- ent magmatic episodes contributing t o this composite in- trusion.

H o w e v e r , Pin et al. (1989) also revealed a clear spatial relationship between 8 S r /8 6S r and geographic position which is independent of petrographic type. Clearly, this is n o t an isotopically homogeneous body; model initial ra- tios at about 328 Ma clearly show this as they do the con- trast between this intrusion and, f o r instance, the Kark- onosze Granite (Fig. 4). T h e granites of b o t h intrusions have similar R b / S r values. L o w e r Sr-isotope initial ratios characterise the Strzegom-Sobotka Massif, a reflection, very likely, of a genetic relationship with nearby mafic (ophiolitc) rocks (Fig. 1).

In the light of the geographic 5 S r /8 6S r variation, the demonstrable failure to homogenise at about 328 Ma dis- played by the other Variscan granites and the relatively small n u m b e r of samples used in the age determinations, it would seem that the apparent age difference between the two-mica granite and the monzogranites should be treated with caution and confirmed. W h a t is certain is that this intrusion contains some granites with the lowest*"" S r / ! 6Sr (at 328 Ma) of all the Variscan intrusions for which data are available, lower even than the low R b / S r granitoids of Niemcza.

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KARKONOSZE O Fig. 5. Pattern of Sr-isotope data from the Izera and Snieznik gneisses. Variscan granite 328 Ma reference is shown. High Rb/Sr data and some low Rb/Sr samples are omitted for drafting pur- poses only. Weathered samples are included.

• • •

2 k 6 8 10 87Rb/86Sr

Fig. 4. Model initial ratios at 328 Ma for the Strzegom-Sobotka and Karkonosze intrusions.

OLDER GRANITOIDS

T h e Variscan Karkonosze Granite is intruded into the older Izera gneisses (Fig. 1) of the I z e r a - K A r k o n o s z e Block. Borkowska et al. (1980) determined Rb-Sr whole- rock ages in the interval 450-500 Ma f o r these gneisses and f o r the chemically indistinguishable R u m b u r k granites into w h i c h the gneisses gradationally pass. T h e scatter on the data is appreciable. T h e data f o r samples with 8 7R b /

8 6S f l 3 are plotted on Figure 5 with similar additional data f r o m the Snieznik gneisses by Borkowska etal. (1990) w h o note that their data are not in agreement with that of van Breemen et al. (1982). Data f r o m samples w i t h higher

8 7R b /8 6S r ratios than those s h o w n exhibit considerable scatter - as do similar data f r o m the Variscan granites; in these high R b / S r cases, open system behaviour may be re- sponsible.

It is clear that the later Variscan granites, t h o u g h they intruded the gneisses, did not originate f r o m the rework- ing of these gneisses. O n the ground (Fig. 1), the Izera

gneisses occur to the west and beyond, the Snieznik gneisses o u t c r o p t o the south of the K i o d z k o - Z l o t y Stok granitoid, similar gneisses occur t o the n o r t h of the Strze- g o m - S o b o t k a intrusion (at W^droze Wielkie) and the un- deformed Strzelin granites intrude an older crystalline massif.

Pin et al. (1989) inferred, on the basis of the geographic control on the Sr-isotope initial ratios, that the S t r z e g o m - Sobotka Massif straddles a m a j o r b o u n d a r y between con- trasting crustal blocks. This intrusion provides the only Sr-isotope hint of such. T h e questions raised by the re- gional occurrence of these late post-tectonic granites w i t h relatively low Sr-initial ratios, w h e n compared w i t h those of the gneisses they intrude, concern the nature, origin and extent of their source and how it came t o be below in Car- boniferous times. Rb-Sr data will n o t answer these ques- tions.

CONCLUSIONS

(1) It is more likely than n o t that all of the post-tec- tonic Carboniferous granites in the Western Sudetes de- rived f r o m a source with a similar initial 8 7S r /8 6S r and were emplaced over a short time interval about 330 Ma ago.

(2) N o n e of t h e m resulted f r o m the reworking and melting of any of the gneisses exposed in the region and f o r

w h i c h data are available. In contrast, their source was m o r e primitive w i t h m o r e juvenile mantle material in it.

(3) A t least some of the granites, most obviously those of Niemcza, are contaminated b y older crustal material (the older gneisses?) w i t h a relatively high 87 S r /8 6S r .

(4) In C a r b o n i f e r o u s times, the relatively primitive post-tectonic granites intruded.

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Rb-Sr I S O T P E P A T T E R N S I N T H E C A R B O N I F E R O U S G R A N I T O I D S 53

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MARTINEAU, F. 1990. A geochemical investigation of the age, significance and structural evolution of the Caledonian- Variscan granite-gneisses of the Snieznik metamorphic area (Central Sudetes, Poland). Geologia Sudetica, 25: 1-27.

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PARKES, M„ RYAN, P. D„ SLOAN, R. J., STILLMAN, C. J., TIETZCH-TYLER, D., TODD, S. P. & WRAFTER, J. P., 1991. Appraisal of Caledonian suspect terrains in Ire- land. Irish Journal of Earth Sciences, Irish J. Earth Sci., 11:

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COUTERIE, J. P. 1996. Age and origin of the Strzelin gra- nitoids (Fore-Sudetic Block, Poland): Rb/8 6Sr data. Neues Jahrbuch Miner. Abk, 171: 187-198.

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