Hostname: page-component-8448b6f56d-wq2xx Total loading time: 0 Render date: 2024-04-25T00:31:05.907Z Has data issue: false hasContentIssue false

Mid-Holocene macrofossil-bearing raised marine beaches at Potter Peninsula, King George Island, South Shetland Islands

Published online by Cambridge University Press:  17 February 2003

RODOLFO A. DEL VALLE
Affiliation:
Instituto Antártico Argentino, Dirección Nacional del Antártico, Cerrito 1248, 1010 Buenos Aires, Argentina
DIEGO MONTALTI
Affiliation:
Instituto Antártico Argentino, Dirección Nacional del Antártico, Cerrito 1248, 1010 Buenos Aires, Argentina
MOSHE INBAR
Affiliation:
Haifa University, Department of Geography, Mount Carmel, Haifa 31 905, Israel

Abstract

A 2.7 m thick mid-Holocene sedimentary succession composed of alluvial fan and marine beach deposits is exposed at 14.4–17.1 m above sea level (a.s.l.) on the south-eastern coast of Potter Peninsula, King George Island (South Shetland Islands, Antarctica). The raised marine beach deposits contain a subfossil assemblage that includes remains of Adélie (Pygoscelis adeliae) and gentoo (P. papua) penguins, skua (Catharacta sp), seals (elephant seal Mirounga sp), and seaweed fragments. The palaeontological and palaeogeographical evidence allows us to infer that penguin rookeries were active on high cliffs of the Potter Peninsula during the marine beach sedimentation, which is dated to c. 4540–4450 reservoir-corrected 14C yr BP on the basis of radiocarbon dating on penguin bones. The data presented in this paper are in agreement with the Holocene palaeoenvironmental chronology known from Potter Peninsula, and suggest that marine birds and seals inhabited the coastal areas of King George Island probably during a mid- Holocene period of seasonally open marine conditions, which may coincide with a cooling period around Antarctica estimated from ice core records between 8000–4000 yr BP that preceded the “climate optimum” in the Antarctic Peninsula (4000–3000 yr BP).

Type
Research Article
Copyright
© Antarctic Science Ltd 2002

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)