magellan seamounts
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2021 ◽  
pp. 99-111
Author(s):  
S.P. Pletnev ◽  

The Paleocene-Eocene sedimentary complex is most widely developed among the sedimentary cover sediments of the Magellan Seamounts. It is made up of pelagic (nanoforaminiferal) and reef limestones, edaphogenic breccias and volcanoclastic rocks. The most widespread pelagic limestones form narrow (0.5–1.5 km) and extensive (up to 20 km) ribbon-like bodies which cover the upper parts of the slopes and the rim of the summit plateau. The maximum area of their development is marked on Fyodorov Guyot – 315 km2. Pelagic limestones and edaphogenic breccias are exposed over large areas and have mutual facies transitions. The Oligocene hiatus in sedimentation was established in the sections of the Cenozoic sedimentary cover deposits of the studied guyots.


2020 ◽  
Vol 491 (2) ◽  
pp. 199-203
Author(s):  
D. P. Savelyev ◽  
A. I. Khanchuk ◽  
O. L. Savelyeva ◽  
S. V. Moskaleva ◽  
P. E. Mikhailik

2020 ◽  
Vol 16 (3) ◽  
pp. 3-12
Author(s):  
S.P. PLETNEV ◽  
T.E. SEDYSHEVA

Fe-Mn crusts play an important role in marine mineral deposit research because of their widespread occurrence and high concentrations of valuable and rare metals. Most Fe-Mn crust deposits occur on the tens of thousands of seamounts found in the ocean. Data on the structure, texture, composition, age, and deposit characteristics will help define which factors are key for the creation of mineral accumulation and which combination of factors leads to the formation of potentially economic concentrations of metals. In this paper, we address the structure and characteristics of the oldest Fe-Mn crust stratigraphic sections (Late Cretaceous and Paleocene) collected from the Magellan seamounts. A complete section of the crusts on the Magellan Seamounts includes four layers, each 2—4 cm thickness: the Late Paleocene (?) Early Eocene layer I 1, the Mid Late Eocene layer I—2, the Miocene layer II and the Quaternary layer III. In some cases, the main CMC section is underlain by relict layers. The chemical and mineral composition of the layers was determined both by X-ray diffraction and precision methods; concentrations of the main ore components and phosphorus were determined by the methods of classical chemistry. The age of 12 samples was determined, the mineral composition of four, the chemical composition of 22 samples. The results of the relict layers analysis allow to distinguish two groups of samples among them. Among the relict layers, two age ranges are established — the second half of Late Cretaceous (R1) and the first half of Paleocene (R2). High concentrations of barium, lithium, gallium, and zinc suggest that hydrothermal sources could be the source of the material. But not through direct delivery, but via the phase of transfer of sea bottom water. Thus, the analysis of lithological and geochemical parameters and fossil fauna of foraminifera in the relict layers of the Magellan Seamounts ore section indicates two stages of their formation: Late Campan Maastricht and Early Middle Paleocene. The discreteness of the formation of relict layers in time once again proves that the sharply changing environmental conditions controlled the growth of the CMC ore section.


ZooKeys ◽  
2019 ◽  
Vol 881 ◽  
pp. 91-107 ◽  
Author(s):  
Yu Xu ◽  
Yang Li ◽  
Zifeng Zhan ◽  
Kuidong Xu

Two new species of Chrysogorgia Duchassaing & Michelotti, 1864 collected from Kocebu Guyot in the Magellan seamounts of the Pacific Ocean are described and illustrated: Chrysogorgia ramificanssp. nov. collected from a depth of 1831 m and Chrysogorgia binatasp. nov. collected from a depth of 1669 m. Chrysogorgia ramificanssp. nov. belongs to the Chrysogorgia “group A, Spiculosae” with rods distributed in body wall and tentacles, and C. binatasp. nov. belongs to the “group C, Squamosae typicae” with rods and/or spindles not present but only scales. Chrysogorgia ramificanssp. nov. differs from congeners by its main stem with 2/5R branching sequence at the bottom forming two large bottlebrush-shaped branches with 1/3R branching sequence at the top. Chrysogorgia binatasp. nov. is similar to C. scintillans Bayer & Stefani, 1988, but differs by its larger polyps, larger sclerites in the body wall, and different scales in the upper part of polyps. The mtMutS genetic distances between C. ramificanssp. nov. and C. binatasp. nov. and congeners are in the range of 0.33%–2.28% and 0.33%–2.94%, respectively, while the intraspecific distances are in the range of 0–0.16%. Molecular phylogenetic analysis indicates that C. ramificanssp. nov. is clustered with C. monticola Cairns, 2007 and C. binatasp. nov. is clustered with C. chryseis Bayer & Stefani, 1988, both with high support indicating close relationships.


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