| 
       
		Petrology and geochemistry of basic-ultrabasic 
		forearc ophiolite banded complexes. 
		
		Raisa M.Yurkova, Boris J.Voronin 
		
		Institute of oil and gas 
		problems RAS, 
		
		bivrmyrzb@mty-net.ru 
		  
		
		The present paper is based on the results of the 
		study of ultrabasic-basic banded ophiolite complexes in the 
		northwestern  segment of the active continental margin of the Pacific 
		Ocean: Sakhalin, Kamchatka and the Koryak Ridge. A  banded rock series 
		was formed upon polycyclic intrusion of mafic gabbronorite magma along 
		dyke-like channels into lherzolite,  wehrlite, apodunite-harzburgite, 
		serpentinite bands affected by the extension of the arch of an uplifting 
		mantle diapir  in the primitive island arc-trough transition zone [3]. 
		Magma is assumed to have crystallized dynamically to form pyroxenites  
		[4]. Depths varied from 20-30 to 10-12 km. These conditions were 
		conducive to the formation of differenttemperature  bimetasomatic beds: 
		1) apogabbronorite beds (T=900oC) consisting of bronzite, 
		diopside and pargasitic hornblende; 
		
		2) apolherzolite beds (T=550-700 oC) 
		composed typically of diopside, pargasitic hornblende, grossular-andradite  
		and herzinite. The presence of herzinite suggests high-pressure 
		conditions. Aposerpentinite beds are formed of lizardite,  pentlandite 
		and chrome-spinellid. Gabbronorites and pyroxenites were subjected to 
		autometamorphic amphibolization  (T=700-800oC) to form 
		various combinations of edenite, edenitic, high-Mg and tschermakitic 
		hornblende and magnesiohastingsite.  Gabbronorites, screened by 
		serpentinites in solid-ductile condition, were recrystallized under 
		granulite-facies metamorphic  conditions (T=830-880oC). As a 
		result, the following mineral associations were formed: anorthite, 
		bronzite-hypersthene, diopsidesalite 
		
		and titaniferous magnetite. The orientation of 
		metamorphic banding in the rocks and the arrangement of multiple 
		twinned  bands suggest that the recrystallization of gabbronorites was 
		induced by shear strain and sliding deformations directed along the  gabbronorite-ultrabasic 
		rock contact. Screening is indicated by a lower degree of multiple 
		mineral alterations of recrystallized gabbronorites  in comparison with 
		non-recrystallized igneous types of these rocks. In addition, screening 
		seems to have contributed to  the persistence of relatively low 
		strontium isotope ratios in recrystallized gabbronorites (Table 1). 
		These values exceed the upper  limit of 87Sr/86Sr 
		ratios in MORB and are characteristic of rocks from most modern island 
		arcs and active continent margins [2].  The destruction of diopside 
		lamellae upon recrystallization of bronzite resulted in the increased 
		role of „R„p cations in plagioclase  and Fe in newly-formed pyroxenes. 
		These trends are more conspicuous in contact-reaction interrelations 
		with ultrabasic rocks. 
		
		Recrystallized gabbronorites typically show a 
		well-defined negative Eu anomaly, suggesting their non-cumulate genesis. 
		Nonrecrystallized  gabbronorites exhibit both positive and negative Eu 
		anomalies. The Eu-anorthite molecule ratio in plagioclase from  these 
		rocks is noteworthy. The incipient relationship might be accidental. 
		Data are presented in the order of collecting (see Table  1). 
		 
		
		Table 1.  87Sr/Sr 86  
		variations gabbronorite plagioclases. 
		Geological Institute RAS laboratories.  Electron microprobe analysis. 
		
			
				| 
				 
				Rock tipe  | 
				
				 
				magmatic  | 
				
				 
				metamorphic  | 
			 
			
				| 
				 
				Plagioclases (%An)
				  | 
				
				 
				85-88  | 
				
				 
				85-88  | 
				
				 
				83-92  | 
				
				 
				92-94  | 
				
				 
				92-94  | 
				
				 
				95-100  | 
				
				 
				95-100  | 
				
				 
				95-100  | 
			 
			
				| 
				 
				87Sr/Sr 
				86 (±0.00006 
				– 0.00010)  | 
				
				 
				0.70446  | 
				
				 
				0.70511  | 
				
				 
				0.70493  | 
				
				 
				0.70501  | 
				
				 
				0.70503  | 
				
				 
				0.70400  | 
				
				 
				0.70393  | 
				
				 
				0.70384  | 
			 
			
				| 
				 
				Eu, 
				г/т  | 
				
				 
				no  | 
				
				 
				0,047  | 
				
				 
				0,056  | 
				
				 
				no  | 
				
				 
				no  | 
				
				 
				0,127  | 
				
				 
				0,226  | 
				
				 
				0,094  | 
			 
		 
		  
		  
		  
		  
		
		Garnet amphibolites and eclogite-like rocks were 
		formed step by step under dynamothermal metamorphic conditions in 
		locally  elevated temperature (C=700-800oC) and pressure (P>5 
		kbar) zones. These rocks occur as band-like and lens-shaped granoblastic- 
		
		textured rocks, 2.0 x 0.8 m2 in size, oriented 
		subconcordantly with banding in websterite beds. Garnet-bearing 
		phyllonites,  formed after granet amphibolites and eclogite-like rocks, 
		and other types of phyllonites are characteristic of foliation zones 
		in   banded complexes. Almandine porphyroblasts in phyllonites have a 
		low pyrope molecule concentration (Table 2). The smaller  pyrope minal 
		content of phyllonite garnet in comparison with that of original rocks 
		is attributed to its recrystallization under lowertemperature  
		dynamometamorphic conditions. The polygenetic nature of banded 
		complexes, in which gabbronorites are not coeval  with lherzolites and 
		their host apodunitic-harzburgitic serpentinites, is thus revealed. 
		Gabbronorites and lherzolites intruded serpentinites  at different 
		depths („Q„S- conditions). In this sense, banded complexes can be 
		interpreted as polygenic basic-hyperbasic plutons.  The composition of 
		spinel suggests that lherzolites were crystallized at elevated 
		pressures. The equilibrium ortho- and clinopyroxene  formation 
		temperature (T = 950oC), calculated with L.L. Perchuk?f 
		geothermometer [1], and the stability limits of spinelperidotite  facies 
		suggest that lherzolites from the banded complex were formed at a depth 
		of 30-55 km and a pressure of 8-10 kbar  [5]. Serpentinites can exist 
		under such conditions [3]. Gabbronorites were recrystallized at a 
		temperature of 880-925oC, based on  the above estimates. The 
		stability conditions of plagioclase-pyroxene parageneses indicate that 
		they were produced at a depth of  20-30 km and a pressure of up to 7-8 
		kbar. Banding is attributed to the gdyke within a dykeh intrusion of 
		differentiated melt, which  gave rise to endocontact and 
		high-temperature zones in the form of thin (1-1.5 cm), relatively 
		melanocratic bands. Both hightemperature  bimetasomatic and magmatic 
		geneses (in particular, dynamic crystallization from melt) are assumed 
		for intermediate  rocks (wehrlites, pyroxenites) at our present level of 
		knowledge [4]. The formation of granulitic (recrystallized) 
		gabbronorites,  eclogite-like rocks and high-temperature garnet and 
		plagioclase amphibolites was associated with deep local post-solidus  
		(C=800oC) dynamometamorphism of gabbronorites and 
		bimetasomatic rocks. These alterations were coeval with the 
		autometamorphic  alteration of gabbronorites in zones unaffected by 
		intense autometamorphic dynamic stress. Local dynamothermal 
		metamorphism  varied from high-temperature(C=800oC) and 
		high-pressure (>5 kbar) to low-temperature subsurface (phyllonites) 
		conditions.  This evidence is consistent with the concept of the 
		protrusive-diapir evolution of ophiolite assemblages [3].  The time span 
		from the beginning of formation to the intrusion of an ophiolite diapir, 
		estimated at 200±10 Ma, is within  the time span of an Alpine tectonic 
		cycle and in the more frequent magnetic inversion interval (a second 
		geon). The lifetime of  the diapir nearly coincides with the period 
		(212-215 Ma) of rotation of the solar system around the core of the 
		Galaxy.  The time 
		span from the beginning of formation to the intrusion of an ophiolite 
		diapir, estimated at 200±10 Ma, is within  the time span of an Alpine 
		tectonic cycle and in the more frequent magnetic inversion interval (a 
		second geon). The lifetime of  the diapir nearly coincides with the 
		period (212-215 Ma) of rotation of the solar system around the core of 
		the Galaxy. 
		
		          Literature 
		
		1.    
		Perchuk L.L. Cotexistence  of minerals. L. Nedra  1971, 413 p. 
		(in Russian)  
		
		2.    
		Sharaskin A.Y., Bogdanov N.A., Zakariadze G.S. 
		Geochemistry   and   timing   of the   marginal basin and arc agmatism 
		in the Philippine Sea // Plilos. Trans. Roy. Soc. London A. 1981. Vol. 
		300. P. 287-297. 
		
		3.    
		Yurkova R.M., Voronin B.J. Uplift and transformation mantle 
		hydrocarbon fluds connetcted with ophiolite diapor formation // Genesis 
		of hydrocarbon fluids and deposids. М.:Geos, 
		2006. p. 56-67.  (in Russian) 
		
		4.    
		Irving A. Petrology and geochemistry of composite ultramafic 
		xenoliths in alcalic basalts and implications for magmatic processes 
		within the mantle // Amer. J. Sci. A. 1980. Vol. 280. P. 989- 426. 
		
		5.    
		O'Hara M.J. Mineral paragenesis in ultrabasic 'rocks // 
		Ultramafic and related rocks. N.Y.: Blackwall, 1967, P. 393-408.  |