Edinburgh Research Archive >
Geosciences, School of >
Earth and Planetary Science Research Institute >
Earth and Planetary Science Research Institute publications >
Please use this identifier to cite or link to this item:
|Title: ||Origin of clasts and matrix within the Milano and Napoli mud volcanoes, Mediterranean Ridge accretionary complex|
|Authors: ||Robertson, Alastair H F|
|Issue Date: ||1998|
|Citation: ||Robertson, A.H.F., Emeis, K.-C., Richter, C., and Camerlenghi, A. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 160|
|Publisher: ||Ocean Drilling Program|
|Abstract: ||Petrographic and mineralogical studies of clasts and matrix in the Milano and Napoli mud volcanoes drilled during Ocean
Drilling Program Leg 160 provide important clues about depositional processes, provenance, and the tectonic setting of deepsea
sediments that accumulated before genesis of the Mediterranean Ridge mud volcanoes.
The clasts recovered from both mud volcanoes are mainly mudstone and claystone, calcareous siltstone, quartzose sandstone
and siltstone, shallow-water–derived limestone, and pelagic carbonate. Biostratigraphic evidence indicates mainly early
and middle Miocene ages for fossiliferous clasts, with the older microfossils being reworked. Textural evidence (grading) suggests
that the clastic lithologies are turbidites. Sources of the sandstones were mainly plutonic igneous and subordinate metamorphic
rocks. Sporadic, exceptionally well-rounded, quartz grains may be of eolian origin and were probably derived from the
Precambrian basement of North Africa. Shallow-water–derived carbonates were also redeposited as calciturbidites, with variable
admixing with siliciclastic and pelagic carbonate, which indicates shared depositional pathways. Pelagic carbonates (packstones)
were redeposited basinward as calciturbidites from a deep-sea carbonate slope that formed part of the North African
continental margin. During the middle Miocene, the background sedimentation was in situ pelagic carbonate. In addition, relatively
rare, texturally immature, lithic sandstones include serpentinite, basalt, and radiolarian chert, of ophiolite-related origin.
This material was derived from the orogenic areas to the north, possibly originally from the higher thrust sheets of Crete, before
late Miocene and subsequent erosion and extensional downfaulting.
The texture and composition of the mud and clay matrix provide clues about the mode of the mud volcanism. The matrix of
the mud debris flows includes numerous, small, angular clasts of unfossiliferous claystone and shardlike fragments, which
show pseudolamination, microshearing, and crosscutting veinlets, features that are taken as evidence for the involvement of
high fluid pressure in clast and matrix formation (hyrofracturing|
|Keywords: ||mud volcanoes|
|Appears in Collections:||Earth and Planetary Science Research Institute publications|
Items in ERA are protected by copyright, with all rights reserved, unless otherwise indicated.