How and why did the Alpine Rhodope collapse during the ore‐rich Oligocene times? Jean‐Pierre BURG, ETH‐Zurich

How and why did the Alpine Rhodope
collapse
during the ore‐rich Oligocene times?
Jean‐Pierre BURG, ETH‐Zurich
Perth, June 06, 2012
A pre‐Hellenistic (Thracian) mining region
From Tonkova M. In: Geoarchaeology and Archaeomineralogy. Proceedings of the International Conference, 29‐30 October 2008 Sofia, Publishing House “St. Ivan Rilski”, 266‐270.
A pre‐Hellenistic (Thracian) mining region
Silver mine ‐ Thorikos
Mine workshop ‐ Lavrion
A still (+/‐) active mining region
Ore deposits in European Mountains
Heinrich & Neubauer 2002 Mineralium Deposita 37, 533–540
Archean “Zwischengebirge”
Rhodope Massif: simplified map
Early Paleozoic protoliths
590‐420 Ma
Mesozoic protoliths
170‐120 Ma
Paleozoic protoliths
335‐270 Ma
Jurassic rocks
160‐150 Ma
UHP and HP rocks: subduction
Metamorphic conditions
1.5‐2 GPa; 700‐800°C
Ages
from 170 to 120 Ma
Mylonitic gneiss and sense of shear
Mylonitic gneiss and sense of shear
Structural constraints: sense of shear
Late deformation pegmatites
Liati et al. 2002 Chemical Geology 184: 281‐299
Rhodope Massif: simplified map
Oldest unconformity
Maastrichtian
70‐65 Ma
Cretaceous Rhodope
Paleocene‐Eocene Rhodope
Marine (Gilbert Delta) Lutetian
(48‐40 Ma)
Geochronological constraints (as per 2012)
Protolith ages excluded
Ar‐Ar & K‐Ar
Zr rims
(eclogites?)
Ar‐Ar
Zr rims
pegmatites
HP rocks
Granites
Migmatitic domes T = 560‐680°C; P = 3‐6 kbar
Migmatitic domes T = 560‐680°C; P = 3‐6 kbar
Liati & Gebauer 1999 Contributions to Mineralogy and Petrology 135: 340‐354 This image cannot currently be display ed.
Migmatite domes: Cooling
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Extensional detachments and faulting
General cross section
Moho after Geiss 1987 Annales Geophysicae 5B(6): 623‐630
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Extension and magmatism
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Schefer et al. 2011
Int.J.Earth.Sci. 100:
1181–1206
Hydrothermal ore formation
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Hydrothermal replacement front of marble by PbS+ZnS ore
Marble
Ca‐Mn‐silicate
(“skarn")
Qz + galena + sphalerite
10 cm
(Madan, Bulgaria)
Ore precipitation and deformation
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Sphalerite‐rich vein with later calcite
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~ 20 cm
Vein sequence:
~ 20 cm
Early barren / py‐rich breccia with chl‐seric alteration, then main qtz‐ base metal sulfide veins
finally late carbonates
Ore deposits and extension
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Ore (gold) deposits and extension
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Why extension so late after orogeny?
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Van Hinsbergen et al. 2008 Earth and Planetary Science Letters 273(3‐4) 345‐358
Why a thermal flare some Ma after orogeny?
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Geological setting
Experimental migmatitic domes
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Modelling extensional core complexes
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Two extension modes
Asthenosphere‐triggered doming
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Tomography: no slab breakoff
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van Hinsbergen et al. 2005 Geology 33(4) 325‐328
Model of syn‐collision delamination
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Delamination after stagnation
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Delamination from Rhodope to Aegean
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Eocene‐Oligocene Rhodope
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In summary
• The Rhodope records Cretaceous collision.
• Only one slab preceded, participated to and
followed collision.
• The Rhodope records a southwestward migration of
mass transport, thermal events (magmatism,
metamorphic cooling, hydrothermalism) and
extension.
• The tectono‐metamorphic and magmatic history of
the Rhodope is best explained with syn‐ to post‐
collision mantle delamination (peeling off the
mantle).
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Thanks for your attention
Galena‐Chalcopyrite‐Quartz
Mine 9 of September
Madan (Bulgaria)