Amundsen Sea sediment drifts: Archives of modifications in oceanographic and climatic conditions
Highlights
► Four depositional stages related to changes in oceanography/climate for the Cenozoic. ► Sediment drifts indicate bottom current activity already in Eocene/Oligocene times. ► Intensified bottom currents during the period 21–15 Ma. ► Increased sediment input following 15 Ma represents the major onset of glaciations. ► A change in ice regime from wet- to dry-based after 4 Ma
Introduction
During the last years the West Antarctic Ice Sheet (WAIS) has been reported to undergo significant changes, especially in the area of Pine Island Bay, Amundsen Sea Embayment, where large glaciers draining the ice sheet have shown rapid flow acceleration, increased thinning, and grounding line retreat (Rignot and Jacobs, 2002, Shepherd et al., 2004, Thomas et al., 2004). In order to better understand the dynamics of the WAIS and be able to provide reliable constraints for numerical simulations of a possible future behaviour of the ice sheet, information on the development of the WAIS is needed. This, especially for the early phase, is still under debate and not known in much detail both chronologically and regionally. While good progress has been made over the last years in reconstructing the development of the ice sheet since the late Miocene for the western Antarctic Peninsula and Bellingshausen Sea, the Pliocene for the Ross Sea area and the late Quaternary for Pine Island Bay, little is known from the greater Amundsen Sea, which lies between the Ross and Bellingshausen Seas under the east setting Antarctic Circumpolar Current (ACC) (Orsi et al., 1995, Carter et al., 2009).
The Amundsen Sea is located along the southern Pacific margin of West Antarctica (Fig. 1). This part of the southern Pacific was created by rift and breakup processes and the formation of the earliest oceanic crust between Campbell Plateau/Chatham Rise and Marie Byrd Land/Thurston Island Block at 90–80 Ma (Eagles et al., 2004, Gohl et al., 2007, and references therein). The emplacement of the Marie Byrd Seamounts (MBS) was a result of magmatic activity at 65–55 Ma or older (Kipf et al., 2008, Kipf et al., submitted for publication). Up to 4 km of sediment have been deposited on top of basement. These sediment deposits have been subject to extensive reworking by oceanic currents and, on the shelf, advance-retreat cycles of the ice sheet.
Presently, the Amundsen Sea lies under the flow of Antarctic Bottom Water (AABW), which here is formed mainly in the western Ross Sea (Gordon et al., 2009, Orsi and Wiederwohl, 2009) and participates in the cyclonic circulation of the Subpolar gyres once it has reached the oceanic domain (Orsi et al., 1999). Circumpolar Deep Water (CDW) is observed to flow onto the shelf areas of the Amundsen Sea via bathymetric troughs (Jacobs et al., 1996, Thoma et al., 2008). In the Bellingshausen Sea, a southwest setting flow of bottom water has been observed close to the continental slope as far west as 83°W (see Hillenbrand et al. (2008) for a detailed presentation). Based on the study of sediment drifts, Scheuer et al. (2006b) and Hillenbrand et al. (2003) inferred that this bottom water flow extends even farther west to 93°W.
The work presented here will provide insight on the palaeoceanographic evolution of the greater Amundsen Sea, which represents one of the outflow regions of the Ross Sea gyre into the deep Pacific–Antarctic Basin (Orsi, 2010) and into which the glaciers of the Pine Island Bay area drain, by analysing sedimentary features observed in seismic reflection data.
Section snippets
Geological setting
No direct evidence for an ice sheet extending onto the West Antarctic continental shelves could be detected for the early Cenozoic (Anderson, 1999). A cooling of the surface waters has been reported for the Eocene by Anderson (1999), which may be due to an already existing proto-Ross Gyre as proposed by Huber et al. (2004). A direct relationship between tectonic movements and the onset of massive glaciations can be ruled out because both the opening of the Drake Passage commencing in the middle
Database
Multichannel seismic reflection data gathered by the Alfred-Wegener-Institut (AWI) in 1994 and 2006 form the base of this study (Fig. 1). Details of field parameters and processing of the seismic data can be found in Gohl et al. (1997), Nitsche et al. (2000) and Uenzelmann-Neben et al. (2007). No gain was applied to the data, neither during processing nor for display. Differences in reflection amplitude discussed in the following thus are real. Additional seismic data (Yamaguchi et al., 1988)
Sedimentary features observed
Before describing the sedimentary units observed in our data in detail we define the three sedimentary features primarily observed.
Observations
Our seismic data show an up to 3400 ms TWT (~ 4.2 km using a conversion velocity of vp = 2.5 km/s) thick pile of sediments on top of oceanic basement. We can distinguish up to four sedimentary units (units I–IV) based on seismic reflection characteristics and sedimentary features observed.
The oldest sedimentary unit I shows a thickness of 100–1600 ms TWT (~ 0.1–2 km) depending of the underlying basement topography. Unit I mainly fills depressions between basement highs and thus levels out the basement
Discussion
The sedimentary structures observed in the seismic data show a distinct distribution for the different sedimentary units and migration from one unit to the other. We are aware of the fact that only few seismic lines cover this huge area and the sedimentary structures may have been imaged obliquely. This limits the validity of the inferred sediment transport directions. We still analyse the geometry of the sediment drifts and channel–levee systems to derive a working hypothesis for the
Conclusions
Analysing seismic reflection data with respect to sedimentary structures on the continental rise of the southern Amundsen Sea, we observe sediment drifts, mass transport deposits such as debris flows, and channel–levee systems as predominant features showing a distinct regional and chronological development. We can identify four major stages in sediment deposition related to modification in the oceanographic and climatic system (Table 1).
Sediment drifts have already been formed in the oldest
Acknowledgements
We are grateful to the captains, crews and scientists for their support during the RV Polarstern cruises ANT-XI/3 (1994) and ANT-XXIII/4 (2006) during which the data used in this paper were collected. We further thank the helpful comments of three reviewers and Dr. D. Piper. This is AWI publication No. 25584.
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