Late Pleistocene oceanographic and depositional variations along the Wilkes Land margin (East Antarctica) reconstructed with geochemical proxies in deep-sea sediments

2020 ◽  
Vol 184 ◽  
pp. 103045 ◽  
Author(s):  
Francisco J. Jimenez-Espejo ◽  
Massimo Presti ◽  
Gerhard Kuhn ◽  
Robert Mckay ◽  
Xavier Crosta ◽  
...  
Keyword(s):  
Late Pleistocene ◽  
Deep Sea ◽  
East Antarctica ◽  
Geochemical Proxies ◽  
Deep Sea Sediments ◽  
Wilkes Land

Late-Pleistocene Climates and Deep-Sea Sediments

Science ◽  
1956 ◽  
Vol 124 (3218) ◽  
pp. 385-389 ◽  
Author(s):  
D. B. Ericson ◽  
W. S. Broecker ◽  
J. L. Kulp ◽  
G. Wollin
Keyword(s):  
Late Pleistocene ◽  
Deep Sea ◽  
Deep Sea Sediments

Spectral Analysis of Late Pleistocene-Holocene Sediments

1973 ◽  
Vol 3 (1) ◽  
pp. 3-9 ◽  
Author(s):  
Nicklas G. Pisias ◽  
J.Paul Dauphin ◽  
Constance Sancetta
Keyword(s):  
Spectral Analysis ◽  
Late Pleistocene ◽  
North Atlantic ◽  
Deep Sea ◽  
Significant Peak ◽  
The North ◽  
Holocene Sediments ◽  
Deep Sea Sediments ◽  
The North Atlantic ◽  
Random Fluctuations

AbstractSpectral analysis of deep-sea sediments indicates that the fluctuations in compositional parameters are not random fluctuations with time. Spectra show significant peaks representing periodicities in the data of 380, 1300, and 2600 years. Two of these periods are similar to periods reported in 14C fluctuations. Analysis of a paleotemperature curve from the North Atlantic shows that the characteristics of the fluctuations within interglacial and glacial stages of the climate are similar, and that the spectrum has a significant peak at 2600 years.

scholarly journals Pliocene-Pleistocene Orbital Cyclostratigraphy and Glacial Evolution of the East Antarctic Ice Sheet from Continental Rise IODP Site U1361, Wilkes Land Margin, East Antarctica

2021 ◽  
Author(s):  
◽  
Georgia Rose Grant
Keyword(s):  
Spectral Analysis ◽  
Late Pleistocene ◽  
Gamma Ray ◽  
Physical Property ◽  
East Antarctica ◽  
Antarctic Ice Sheet ◽  
Continental Rise ◽  
Depositional Processes ◽  
Core Site ◽  
Wilkes Land

<p>Stability of the East Antarctic Ice Sheet (EAIS), in response to the orbitally-paced cooling climate of the Late Neogene, is largely unknown. The Wilkes Land margin of East Antarctica, largely grounded below sea level, has previously been proposed to respond dynamically during the warmer climate of the Pliocene, similarly to other marine based sectors of Antarctica (i.e. West Antarctica). Sediment deposition on the Wilkes Land continental rise, recovered in Integrated Ocean Drilling Program U1361A drillcore provides a distal but continuous record of EAIS fluctuations. Changes in sedimentary depositional environments at U1361A core site, were determined through analysis of lithofacies and physical property logs: natural gamma-ray (NGR), gamma-ray attenuation bulk density (GRA), magnetic susceptibility (MS) and L* colour reflectance. NGR primarily reflected biogenic content and a synchronous relationship between NGR, GRA and MS was used to identify interglacial and glacial phases, whereby decreased NGR, GRA and MS values indicated an increase in biogenic material. L* colour reflectance was more variable through time, displayed higher frequency fluctuations and a changing relationship with the other physical property logs down core. Two depositional models, based on facies interpretations and the defined physical property relationships, were produced for the Middle Late Pleistocene (last ~550 kyr; model A) and mid-Pliocene (~4.2-3.6 Ma; model B), which represent end members. Depositional processes common to both models occurred in the intervening core, spanning the Late Pliocene-Early Pleistocene (3-1 Ma). Model A, applied to the Middle Late Pleistocene, shows that alternating diatom-rich clays to silty clays in the upper 9 m of core U1361A, reflect the large amplitude ~100 kyr paced glacial-interglacial cycles, which is confirmed by spectral analysis of the physical properties for this interval. Model B, applied to the Early Pliocene, suggest that the depositional processes recorded by facies may have been less sensitive to EAIS fluctuations, probably due to the fact that the ice margin was generally more distal to the core site during glacial-interglacial cycles of advance and retreat. Nevertheless, these more subtle changes in lithology were characterised by variations in the physical property logs, and spectral analysis of these time series implied orbital pacing was still influential on depositional processes at this time (displaying power in precession and obliquity frequencies). Spectral analysis of the physical property logs and visual correlations to the benthic δ18O stack, confirmed the 4.2-1 Ma interval was paced by ~40 kyr and implies obliquity-paced oscillations of the margin of the EAIS. Precession periodicities, significant in spectra throughout the 4.2 Myr record, are proposed to be the response of phytoplankton productivity in response to seasonal insolation controlling sea-ice extent.</p>

scholarly journals Pliocene-Pleistocene Orbital Cyclostratigraphy and Glacial Evolution of the East Antarctic Ice Sheet from Continental Rise IODP Site U1361, Wilkes Land Margin, East Antarctica

2021 ◽  
Author(s):  
◽  
Georgia Rose Grant
Keyword(s):  
Spectral Analysis ◽  
Late Pleistocene ◽  
Gamma Ray ◽  
Physical Property ◽  
East Antarctica ◽  
Antarctic Ice Sheet ◽  
Continental Rise ◽  
Depositional Processes ◽  
Core Site ◽  
Wilkes Land

<p>Stability of the East Antarctic Ice Sheet (EAIS), in response to the orbitally-paced cooling climate of the Late Neogene, is largely unknown. The Wilkes Land margin of East Antarctica, largely grounded below sea level, has previously been proposed to respond dynamically during the warmer climate of the Pliocene, similarly to other marine based sectors of Antarctica (i.e. West Antarctica). Sediment deposition on the Wilkes Land continental rise, recovered in Integrated Ocean Drilling Program U1361A drillcore provides a distal but continuous record of EAIS fluctuations. Changes in sedimentary depositional environments at U1361A core site, were determined through analysis of lithofacies and physical property logs: natural gamma-ray (NGR), gamma-ray attenuation bulk density (GRA), magnetic susceptibility (MS) and L* colour reflectance. NGR primarily reflected biogenic content and a synchronous relationship between NGR, GRA and MS was used to identify interglacial and glacial phases, whereby decreased NGR, GRA and MS values indicated an increase in biogenic material. L* colour reflectance was more variable through time, displayed higher frequency fluctuations and a changing relationship with the other physical property logs down core. Two depositional models, based on facies interpretations and the defined physical property relationships, were produced for the Middle Late Pleistocene (last ~550 kyr; model A) and mid-Pliocene (~4.2-3.6 Ma; model B), which represent end members. Depositional processes common to both models occurred in the intervening core, spanning the Late Pliocene-Early Pleistocene (3-1 Ma). Model A, applied to the Middle Late Pleistocene, shows that alternating diatom-rich clays to silty clays in the upper 9 m of core U1361A, reflect the large amplitude ~100 kyr paced glacial-interglacial cycles, which is confirmed by spectral analysis of the physical properties for this interval. Model B, applied to the Early Pliocene, suggest that the depositional processes recorded by facies may have been less sensitive to EAIS fluctuations, probably due to the fact that the ice margin was generally more distal to the core site during glacial-interglacial cycles of advance and retreat. Nevertheless, these more subtle changes in lithology were characterised by variations in the physical property logs, and spectral analysis of these time series implied orbital pacing was still influential on depositional processes at this time (displaying power in precession and obliquity frequencies). Spectral analysis of the physical property logs and visual correlations to the benthic δ18O stack, confirmed the 4.2-1 Ma interval was paced by ~40 kyr and implies obliquity-paced oscillations of the margin of the EAIS. Precession periodicities, significant in spectra throughout the 4.2 Myr record, are proposed to be the response of phytoplankton productivity in response to seasonal insolation controlling sea-ice extent.</p>

scholarly journals Mechanism and Influencing Factors of REY Enrichment in Deep-Sea Sediments

Minerals ◽  
2021 ◽  
Vol 11 (2) ◽  
pp. 196
Author(s):  
Jiangbo Ren ◽  
Yan Liu ◽  
Fenlian Wang ◽  
Gaowen He ◽  
Xiguang Deng ◽  
...  
Keyword(s):  
Deep Sea ◽  
Research Progress ◽  
Bottom Current ◽  
Knowledge Map ◽  
P2o5 Content ◽  
Deep Sea Sediments ◽  
Potential Resource ◽  
And Migration ◽  
Adsorption Desorption ◽  
Sediment Interface

Deep-sea sediments with high contents of rare-earth elements and yttrium (REY) are expected to serve as a potential resource for REY, which have recently been proved to be mainly contributed by phosphate component. Studies have shown that the carriers of REY in deep-sea sediments include aluminosilicate, Fe-Mn oxyhydroxides, and phosphate components. The ∑REY of the phosphate component is 1–2 orders of magnitude higher than those of the other two carriers, expressed as ∑REY = 0.001 × [Al2O3] − 0.002 × [MnO] + 0.056 × [P2O5] − 32. The sediment P2O5 content of 1.5% explains 89.1% of the total variance of the sediment ∑REY content. According to global data, P has a stronger positive correlation with ∑REY compared with Mn, Fe, Al, etc.; 45.5% of samples have a P2O5 content of less than 0.25%, and ∑REY of not higher than 400 ppm. The ∑REY of the phosphate component reaches n × 104 ppm, much higher than that of marine phosphorites and lower than that of REY-phosphate minerals, which are called REY-rich phosphates in this study. The results of microscopic observation and separation by grain size indicate that the REY-rich phosphate component is mainly composed of bioapatite. When ∑REY > 2000 ppm, the average CaO/P2O5 ratio of the samples is 1.55, indicating that the phosphate composition is between carbonate fluoroapatite and hydroxyfluorapatite. According to a knowledge map of sediment elements, the phosphate component is mainly composed of P, Ca, Sr, REY, Sc, U, and Th, and its chemical composition is relatively stable. The phosphate component has a negative Ce anomaly and positive Y anomaly, and a REY pattern similar to that of marine phosphorites and seawater. After the early diagenesis process (biogeochemistry, adsorption, desorption, transformation, and migration), the REY enrichment in the phosphate component is completed near the seawater/sediment interface. In the process of REY enrichment, the precipitation and enrichment of P is critical. According to current research progress, the REY enrichment is the result of comprehensive factors, including low sedimentation rate, high ∑REY of the bottom seawater, a non-carbonate depositional environment, oxidation conditions, and certain bottom current conditions.

The degradation activities for three seaweed polysaccharides of Shewanella sp. WPAGA9 isolated from deep‐sea sediments

2021 ◽  
Author(s):  
Dingquan Wang ◽  
Jianxin Wang ◽  
Runying Zeng ◽  
Jie Wu ◽  
Shijia V. Michael ◽  
...  
Keyword(s):  
Deep Sea ◽  
Deep Sea Sediments
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