From Cardiff University:
Tiny fossils hold answers to big questions on climate change
Research explores 12,000 year fossil record
The western Antarctic Peninsula is one of the fastest warming regions on the planet, and the fastest warming part of the Southern Hemisphere.
Scientists have debated the causes of this warming, particularly in light of recent instrumental records of both atmospheric and oceanic warming from the region. As the atmosphere and ocean warm, so the ice sheet (holding an equivalent of 5 metres of global sea level rise, locked up in ice) becomes vulnerable to collapse.
Now research led by Cardiff University published in Nature Geoscience has used a unique 12,000 year long record from microscopic marine algae fossils to trace glacial ice entering the ocean along the western Antarctic Peninsula.
The study has found that the atmosphere had a more significant impact on warming along the western Antarctic Peninsula than oceanic circulation in the late Holocene (from 3500-250 years ago).
This was not the case prior to 3500 years ago, and is not the case in the modern environment. The study has also shown that this late Holocene atmospheric warming was cyclic (400-500 year long cycles) and linked to the increasing strength of the El Niño – Southern Oscillation phenomenon (a climate pattern centred in the low latitude Pacific Ocean) demonstrating an equatorial influence on high latitude climate.
Dr Jennifer Pike, School of Earth and Ocean Sciences said: “Our research is helping to understand the past dynamic behaviour of the Antarctic Peninsula Ice Sheet. The implications of our findings are that the modern observations of ocean-driven warming along the western Antarctic Peninsula need to be considered as part of a natural centennial timescale cycle of climate variability, and that in order to understand climate change along the Antarctic Peninsula, we need to understand the broader climate connections with the rest of the planet.”
Ice derived from land has a very distinctive ratio of oxygen isotopes. This research is the highest resolution application in coastal Antarctic marine sediments of a technique to measure the oxygen isotope ratios of microscopic marine algae fossils (diatom silica). When a large amount of glacial ice is discharged into the coastal ocean, this alters the oxygen isotope ratio of the sea water that the marine algae are living in. This creates a clear imprint in the fossils that reveals the environmental conditions of the time. The scientists used the oxygen isotope ratio of the fossils to reconstruct the amount of glacial ice entering the coastal ocean in the past 12,000 years, and to determine whether the variations in the amount of ice being discharged were the result of changes in the ocean or atmospheric environment.
Professor Melanie Leng, from the British Geological Survey and Chair of Isotope Geosciences in the Department of Geology, University of Leicester, said: “Technologically the analysis of the oxygen isotope composition of diatom silica is extremely difficult, the British Geological Survey is one of a very few research organisations in the world that can undertake this type of analysis. For this research project the methodology has been developed over the last five years with the specific aim of investigating the different amounts of melting in the polar regions. It’s fair to say we are world leading pioneers in this technique.”
The research is co-authored with Cardiff University by the universities of Nottingham, Leicester and the British Geological Survey and was funded by the Natural Environment Research Council (NERC).
Glacial discharge along the west Antarctic Peninsula during the Holocene
The causes for rising temperatures along the Antarctic Peninsula during the late Holocene have been debated, particularly in light of instrumental records of warming over the past decades1. Suggested mechanisms range from upwelling of warm deep waters onto the continental shelf in response to variations in the westerly winds2, to an influence of El Niño–Southern Oscillation on sea surface temperatures3. Here, we present a record of Holocene glacial ice discharge, derived from the oxygen isotope composition of marine diatoms from Palmer Deep along the west Antarctic Peninsula continental margin. We assess atmospheric versus oceanic influences on glacial discharge at this location, using analyses of diatom geochemistry to reconstruct atmospherically forced glacial ice discharge and diatom assemblage4 ecology to investigate the oceanic environment. We show that two processes of atmospheric forcing—an increasing occurrence of La Niña events5 and rising levels of summer insolation—had a stronger influence during the late Holocene than oceanic processes driven by southern westerly winds and upwelling of upper Circumpolar Deepwater. Given that the evolution of El Niño–Southern Oscillation under global warming is uncertain6, its future impacts on the climatically sensitive system of the Antarctic Peninsula Ice Sheet remain to be established.
Figure 2: Morlet wavelet analysis of ODP Site 1098 δ18Odiatom record
The upper panel shows the δ18Odiatom record and the lower panel shows the wavelet power spectrum. Shaded contours represent normalized variances and black lines surround statistically significant regions that exceed 95% confidence