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		Geology  
    Apuan Alps interpretation 
 
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	The current interpretation model 
	of the Apuan Alps was defined in 1990 when Carmignani and Kligfield (and, 
	separately, Coli) noted closes analogies between the evolution of the Apuan-Apennine 
	area and northern American Core Complex, where more recent structures 
	of extensional tectonics superimposed upon older compressive deformations.
	 
	Nowadays, almost the 
	entire scientific community agrees on the interpretation of the Apuan Alps 
	and the Northern Apennines as the complex result of two different and 
	subsequent deformation phases: the first compressional-collisional and the 
	second extensional. 
	
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			The 
	Apuan Alps and the Northern Apennines belong to the same thrust and 
	fold mountain belt originated during the Cenozoic by the overthrusting of 
	the Ligurian Units, derived from the ocean (Alpine Tethys) internal domain, 
			onto the external Tuscan and Umbria-Marche continental margin 
			domains.  
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			Tectonic map of the Northern Apennines (Carmignani 
			et al., 
			2006)  | 
		
		 
		
		The 
		complex tectonic evolution of the area showed a first phase of 
		deformation and metamorphism within a collisional geodynamic context. It was then 
	followed by a second phase within an extensional tectonic regime, 
	characterized by the development of low-angle shear zones and normal faults 
	responsible for the uplift and exhumation of the deepest structural units. 
		
			
			In the light of crustal 
	plate movements in the Mediterranean area, the tectonic events began in the 
	Late Cretaceous when the European and Apulian (-African) continental margins 
	sutured the Tethys Ocean. In particular, during the Late Oligocene, the 
	Briançonnais microcontinent (before belonging to the European plate) moved 
	towards East and collided with the Adria microplate with the subduction of 
	the Apulian lithosphere underneath the Corsica-Sardinia block.  
			Thus, the Apuan Alps and the Northern Apennines underwent a first phase of 
	structuration during a compressional tectonic phase characterized by crustal 
	shortening and nappe emplacement towards the Apulian foreland. Since the 
	Tortonian onwards, the subduction process contributed to the development of 
	back-arc oceanic basins and therefore the opening of the Thyrrenian Sea, 
	within crustal extensional processes which are clearly recognizable in the 
	extensional features of macro and microstructures. 
			
			
			A large tectonic window 
	formed in the Apuan Alps, thus exposing the ‘Metamorphic Complex of the 
	Apuan Alps’. It is the deepest structural level outcropping in the internal 
	parts of the Northern Apennines and it is therefore a key area to understand 
	mechanisms and geodynamic processes which led to the formation of the 
	Apenninic range. 
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			In particular, two 
	superposed units, both belonging to the metamorphic succession of the Tuscan 
	Domain, are identifiable in the Apuan tectonic window. The lower unit is the 
			"Autochthonous" Auct. with extensive outcrops across the main ridge, both on 
	the coastal and inland mountainsides, whereas the Massa Unit, on top of it, 
	is only found in the westernmost part of the tectonic window.  
	The Massa Unit is 
	composed of a Paleozoic basement on which lays in unconformity a thick 
	Triassic sedimentary sequence characterized by Ladinian basic metavolcanic 
	rocks. The Mesozoic cover begins with quartz metaconglomerates associated 
	with metasandstones, metasiltstones and black phyllites which can be 
	interpreted as continental and/or coastal siliciclastic deposits. Upward, 
	they are followed by mainly calcareous rocks (marbles, metabreccias, 
	calcareous schists and carbonate phyllites), deriving from carbonate shelf 
	and neritic-pelagic deposits, intercalated with alkaline metabasites. The 
	sequence ended with Carnian phyllites of continental-coastal origin and 
	levels of anagenites: metaconglomerates with mainly quartz and quartzite 
	clasts. 
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			The "Autochthonous" 
			Auct. too is formed by a Paleozoic basement, deriving from 
			previous orogenic structures, with an initial age presumably dating 
			back to the Cambrian. A metasedimentary sequence, showing ages from 
			the Late Triassic up to the Oligocene, unconformably lies upon the 
			crystalline basement, like in the Massa Unit. 
			The 
			Meso-Cenozoic cover begins with a classic “Verrucano” characterized 
			by polygenic conglomerates, calcareous metasandstones and 
			siliciclastic dolomites intercalated with metabreccias (VIN) presumably 
			deriving from a transitional (from continental to littoral) 
			depositional environment. They are followed by the “Grezzoni” 
			dolomites (GRE) of the Late Triassic carbonate shelf, which are followed 
			by micritic fossiliferous metalimestones of the “Colonnata” limestones and marlstones. 
			They are then followed 
			by the Megalodont-bearing Marbles (MMG) intercalated with polygenic metabreccias 
			(BSE) and chloritoid schists 
			(BSEa) which testify episodes of 
			emersion of the carbonate platform with the formation of lateritic-bauxitic 
			layers and the deposition of debris flows at the bottom of the 
			tectonically active scarps. 
			Marbles with different dolomitization levels, crystalline dolomites, 
			marbles and monogenic metabreccias are typical of the overlying 
			formations of Dolomitic marbles (MDD) and Marbles s.s. 
			(MAA), witnessing to the 
			development of a new carbonate platform formed after that of the 
			“Grezzoni” dolomites in the Late Triassic. Upward, pinkish marbles (MRZ), metalimestones with cherts 
			(CLF), calcschists 
			(CCI) and 
			jaspers (DSD) are a sign of 
			the drowning of the marble carbonate platform and the beginning of 
			an hemipelagic sedimentation. 
			
			Possible time 
			displacement among the different subsiding blocks brought about the 
			formation of very different depositional environments with “reduced” 
			and/or “condensed” sequences, the first evidence of which is 
			polygenic metabreccias characterized by a phyllitic matrix. The 
			sequence ends with metalimestones with cherty bands and nodules (ENT), calcschists, Nummulite limestones, sericitic phyllites 
			(SSR) and quartz-feldspatic 
			metasandstones (PSM) belonging respectively to pelagic and foredeep 
			deposits reaching the Late Oligocene. 
			
			In conclusion, 
			there is a strong correlation between the rocks of the Paleozoic 
			basement of the Massa Unit and those of the "Autochthonous" Auct. 
			which show analogous deformation and a similar greenschist facies 
			metamorphism owing to the Hercynian orogeny. The same situation 
			repeats when comparing the two metasedimentary covers because, 
			despite the first being less thick than the second, their rocks are 
			characterized by the same Alpine metamorphism, whose greenschist 
			facies paragenesis shows differences in temperature and pressure 
			conditions, higher in the Massa Unit. 
			In the proposed Geopark territory, rocks of the non-Metamorphic 
			Succession of Tuscan Domain outcrop beyond the borders of the 
			tectonic window. They are related to a single unit, commonly known 
			as Tuscan Nappe geometrically overlying the Metamorphic Complex of 
			the Apuan Alps (made up by the Massa Unit and the "Autochthonous" 
			Auct.). The Tuscan Nappe rocks belong to the Meso-Cenozoic 
			cover, the Paleozoic basement not being present at all. There are 
			closed and frequent correlations as regards lithology, depositional 
			environment and age between the geological formations of 
			"Autochthonous" Auct. and Tuscan Nappe. The main difference 
			lays in the degree of metamorphism which is absent or very weak in 
			the Tuscan Nappe. 
			 
			
			
			The Tuscan Nappe is in 
	turn overthrusted by the Ligurian Units s.l., which crop out mainly 
	in the northern part of the Geopark area, being represented by Helminthoid 
	Flysch (Late Cretaceous) with basal complex characterized by ophiolitic 
	detritism and olistolites and by shaly-calcereous deposits and calcareous 
	turdidites ranging in age from Late Cretaceous to Eocene. 
	The proposed territory is also characterized by post-orogenic deposits which 
	cover the whole time frame from the Late Miocene to today. This is 
	particularly the case of polygenic Breccias of Metato (which derived from 
	formations of the Tuscan Domaine cover), glacial and fluvio-glacial deposits 
	(Middle-Late Pleistocene) as well as alluvial, slope and landslide deposits 
	(Holocene).  | 
		
		 
			  
			 
			
			Stratigraphic column 
			of the 
			
			 "Autochthonous"
			Auct.(Carmignani et al., 
			2006) 
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	The detailed description of the formations above mentioned is here omitted, 
	referring to the legend of the enclosed geological map. 
	The complex geological history of the Apuan Alps is responsible for the 
	great geodiversity of rocks and minerals of the territory. The composition 
	of lithotypes, the Hercynian and Alpine deformations, metamorphism and 
	hydrothermalism brought about a remarkable variety of minerals. Witness the 
	large number of minerals found in the area, achieving the total of about 
	275. 
	For the first time 
			30 mineral species have been discovered and described in the Apuan Alps [allanite-(La), 
	apuanite, bottinoite, carraraite, dessauite, garavellite, grumiplucite, 
	marrucciite, meneghinite, moëloite, pellouxite, pillaite, rouxelite, 
	scainiite, versiliaite, volaschioite, zaccagnaite, 
	zincalstibite, etc.] most of which are exclusive to this area. 
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			Tectonic map of the Apuan Alps (Carmignani 
			et al., 
			2006) 
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