Subantarctic Macrotidal Flats, Cheniers and Beaches in San Sebastian Bay, Tierra Del Fuego, Argentina

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Subantarctic Macrotidal Flats, Cheniers and Beaches in San Sebastian Bay, Tierra Del Fuego, Argentina View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by EPrints Complutense Subantarctic macrotidal flats, cheniers and beaches in San Sebastian Bay, Tierra Del Fuego, Argentina a, b d Federico Vilas * , Alfredo Arche , Marcelo Ferrero C, Federico Isla a Universidad de Vigo, Facultad de Ciencias, Dpto. de Geociencias Marinas y Ordenacion del Territorio, Aptdo. 874, 36.200 Vigo, Spain b Instiluto de Geologia Economica, c.S.l.C.-UC.M, Facultad de Geologia, 28040 Madrid, Spain C Secretaria de Mineria. Avda. de Santa Fe 1542, 1060 Buenos Aires, Argentina d CONICET, Centro de Ge% gia de Costas y del Cuaternario, CC-722, 7600 Mar de Plata, Argentina Abstract San Sebastian Bay is a large, semicircular coastal embayment situated on the Atlantic coast of Tierra del Fuego, Argentina. It is a high-energy, subantarctic environment with a tidal range of 10.4 m, influenced by large waves of Atlantic and local origin and swept by constant, strong westerly winds. A 17 km long gravel spit protects the Northern part of the Bay giving rise to a gradient in sedimentary processes. From south to north, are seven distinct sedimentary environments. Coastal sedimentation started at least 5200 years before present (BP) and a rapid progradation related to a relative sea-level drop has infilled about 6 kilometres of the Bay with a sedimentary sequence 10-11 m thick. 14-C dating of unabraded shells in the Chenier ridges of the relict part of the complex allows for a precise reconstruction of the stages of the progradation, that has slowed from 2.35 m/year at 5000 years BP to 0.6 m/year at present. The possible causes of the sea-level drop are discussed. Keywords: Tierra del Fuego; macrotidal sedimentation; subantarctic climate; sea-level; glacio-isostatic rebound; chenier formation 1. Introduction 1980; Da\rymple et aI., 1990), among others. Some other well known examples are dominated by marine Macrotidal areas with tidal ranges over 8 m are tidal processes such as the Wash (UK) (Evans, 1965) relatively poorly studied in comparison with mesoti­ and Jade Bay (Germany) (Reineck, 1958, 1972), dal (range 2-4 m) areas, Some of them are estuarine Taizhou Bay (China) (Ren, 1986), Bohai Sea (China) in character, such as the Severn River (UK) (Kirby (Wang, 1983) and Inchon Bay (Korea) (Frey et aI., and Parker, 1982; Harris and Collins, 1985; Allen, 1988, 1989). 1987, 1988, 1990), Seine Estuary-Mont Saint Michel In the Southern Hemisphere, macrotidal areas are (France) (Larsonneur, 1982; A voine, 1986; A voine even less well known even though the tidal ranges and Larsonneur, 1987), and the Bay of Fundy and tidal flats at the Atlantic mouth of the Magellan (Canada) (Knight and Dalrymple, 1975; Amos et aI., Strait and the Atlantic Coast of Tierra del Fuego are among the largest in the world. The authors con­ ( , Corresponding author. Fax: + 34-8681-2556; E-mail: ducted surveys of San Sebastian Bay Fig. 1) be­ [email protected] tween 1985 and 1988 aimed at characterising the N - 53° 00' S. t G CERRO <I Z S···. t- ... ... .. .. Z .... / , W ,- <!) .' Il: W <I ...J .. PUNTA DE """" :r ARENAS u C '�:' BAY OF SAN SEBASTIAN PLAYA DE CHORRILLOS O IOKm. _��",=�_=, I A B Fig. I. (A) Map of situation. (B) The Bay of San Sebastian and different physiographic sectors (A to G). Dotted lines are surveyed profiles sampling stations. RG: Rio Grande, RA: Rio Gallegos, PA: PU.nta Arenas, EM: Strait of Magellan, CH: Cape Horn, US: Ushuaia. Location of profiles shown in Fig. 15 are indicated. sedimentary subenvironments, sedimentary pro­ most of them rich in organic remains, allowing for cesses, sequences, and the Quaternary evolution of C-14 dating. The quantification and interpretation of the area. the sea-level fall and its causes was another goal of The Bay presents an interesting combination of our research. physiographic features: extreme macrotidal regime, high latitude, subantarctic climate, fine-grained sedi­ mentation in a high-energy environment and related 2. Location wave- and wind-dominated areas. The bay could provide an alternative example to the classic areas 2.1. Geographic setting listed above and some guidance for the interpretation of ancient, fine-grained, marine deposits. San Sebastian Bay is a coastal embayment situ­ The San Sebastian Bay area exhibits a series of ated in the North of the Argentinean territory of the features which could be interpreted as representing a Isla Grande de Tierra del Fuego (Fig. 1); it lies Holocene fall of sea level of eustatic and/or isostatic between 63° 40' and 63° 48' long. W and 53° 00' origin, such as raised beaches and chenier ridges, and 53° 25' lat. S. « z W f-­ .....J Z I W l') U a::: « " PREVAILING BA Y OF ======:;» WIND 2 SAN SE BASTIAN , , I' N I' t " o 2 3 4 Km. , I SAN SEBASTIAN CHORRILLOS (Y. P. F. DOCK) Fig. 2. Map of the Bay. (A) Gravel beaches of Peninsula del Paramo, (B) Muddy tidal flat with tidal channels, (C) Cheniers and muddy tidal flat without tidal channels, (D) Beach complex of San Sebastian, (E) Cliffs of Punta Basilica, (F) Barrier Beach-Lagoon Complex of Chorrillos, and (G) Fossil sediments deposited during Holocene times. 1 and 2 are the surveyed profiles represented in detail in Fig. 16. The Bay is roughly semicircular in shape, measur­ cesses and rates of sedimentation in the area. Porter ing approximately 40 km from north to south and 25 et a!. (1984) described the Holocene sea level fluctu­ km from east to west (Fig. 2). Astronomic tides ations in the Magallanes-Beagle region, Heusser and range from 3A m to lOA m (Servicio de Hidrografia Rabassa (1987) described and interpreted the cli­ Naval, 1987, 1988). The average rainfall is 300-320 matic changes and glacial retreat stages in the last mm/yr, the prevailing wind comes from the west, 12,000 years in the same area and Rutter et a!. exceeding 60 km/h for more than 200 days per year, (1989) correlated the Quaternary deposits along the with occasional gusts up to 155 km/h; the stability Patagonian and Fuego coastline. of the cyclone patterns in the subantarctic region Vilas et a!. (1987) and Isla et a!. (1991) described (50' to 65' lat S) is responsible for the small varia­ the main sedimentary sequences, the sediment source tion of wind direction. Maximum summer tempera­ areas and the winter and summer wave regimes in tures reach 16°C-18°C, while in winter minimum San Sebastian Bay that occur in two areas with temperatures of - 20'C occur frequently with peri­ different characteristics: (1) a wave-dominated gravel ods of several months when the average temperature spit and (2) a tide-dominated mud flat Bujalesky et is below O°C and the sea water freezes (Servicio de a!. (1987) described the Paramo Peninsula gravel Metereol6gico Nacional, 1986). spit, and Isla (1993) described the gravel segregation and annouring processes in the Paramo Peninsula, 2.2. Geologic setting and the coastal spit that partially closed San Sebas­ tian Bay. The bedrock of the area is the Miocene Carmen The Bay is flanked to the north and the south by Silva Formation (Codignotto and Malumian, 1981) cliffs which at present are undergoing erosion; the consisting of deltaic fine sands and silts. It was northern cliffs are composed of Pleistocene Tills, deeply eroded during the first and largest Patagonian whereas the southern ones comprise the fine-grained, Glaciation (Caldenius, 1932) by a glacier coming siliciclastic, Miocene Cannen Silva Formation. Sedi­ from the Patagonian Iceshield, flowing to the NE mentation occurs in two areas with very different from Dawson Island and eroding in the last 15,000 characteristics (Fig. 2): the Peninsula del Paramo years the Inutil Bay (Chile)-San Sebastian Bay (Zone A), composed of gravel beaches, and the inner (Argentina) depression. A later, Pleistocene glacial coast of the Bay (Zones B-F), where muddy tidal period took place in the area and the Tapera Sur Till flats and sand-gravel beaches are found. As these was deposited (Codignotto, 1979, 1983). Submerged sedimentary environments prograded seawards dur­ moraines at a depth of 5 m have been recognised in ing the Holocene, these coastal sediments covered the shelf, NE of San Sebastian Bay (TOTAL AUS­ most of the much wider original San Sebastian Bay TRAL-GEOMATTER, 1980) to the west, and extensive eolian deposits cover most Raedecke (1978) made reference to several of the Holocene deposits. moraine systems, located between Bahia Inutil and This paper deals with the sedimentary processes Bahia de San Sebastian and their possible succession and deposits of the intertidal area (Fig. 2, Zones B to and Codignotto and Malumian (1981) compiled the F). The sedimentology of the Peninsula del Paramo geology of the Northern Tierra del Fuego and men­ Spit (Fig. 2, Zone A) has been discussed previously tioned the 'rhythmic topography' of the Holocene by Isla et a!. (1991) sediments in the San Sebastian Bay area. More recent research work was specifically aimed 3. Research methods at establishing the succession of glacial and inter­ glacial periods, the stratigraphy of moraines and The different subenvironments required specific coastal sediments and present-day sedimentary pro- research methods according to their dynamics and Fig. 3. (overleaf) Several aspects of the intertidal area north of the Bay. (A) Straight main tidal channel, (B) Sinuous secondary tidal channel, (C) SpideIWeb structure, (D) View across a main tidal channel. A c- - o grain size. Two methodologies were employed, one deposited during the Holocene in a phase of active for tidal flats and another for sandy and gravel coastal progradation and partly covered by eolian beaches.
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