Published November 2021 | Version v1
Miscellaneous

A revised age estimate for the mid-Holocene eruption of Mount Hudson (H2) using a high-resolution radiocarbon chronology

  • 1. Earth and Sustainability Science Research Centre (ESSRC), School of Biological, Earth and Environmental Sciences, University of New South Wales, Kensington, NSW (Australia)
  • 2. Chronos 14Carbon-Cycle Facility, Mark Wainwright Analytical Centre, University of New South Wales, Kensington, NSW (Australia)
  • 3. Department of Geography, Faculty of Science and Engineering, Swansea University, Wales (United Kingdom)
  • 4. Department of Geological Sciences, University of Colorado, Boulder, CO (United States)
  • 5. ARC Centre of Excellence for Australian Biodiversity and Heritage, School of Biological, Earth and Environmental Sciences, University of New South Wales, Kensington, NSW (Australia)
  • 6. EMM Consulting Pty Ltd, NSW (Australia)
  • 7. Research Laboratory for Archaeology and History of Art (RLAHA), University of Oxford (United Kingdom)
  • 8. Carbon Dating Laboratory, School of Science, University of Waikato (New Zealand)
  • 9. Department of Earth Sciences, Royal Holloway University of London (United Kingdom)

Description

Full text: Cryptotephra deposits (microscopic volcanic ash) are important geochronological tools that can be used to synchronize records of past environmental change. Here we report a distal cryptotephra from a Holocene peat sequence (Canopus Hill) in the Falkland Islands, in the South Atlantic. Using a high-resolution radiocarbon chronology and geochemical analysis (major- and trace-element) of individual volcanic glass shards, we provide a robust correlation between this cryptotephra and the large mid-Holocene explosive eruption of Mt. Hudson in Patagonia, Chile (H2; ~3.9 ka cal BP). While the commonly cited age for the H2 eruption is 3600 BP; ~3.9 ka cal yr BP, this is derived from 14C ages of bulk organic soil, sediment and peat deposits bracketing the tephra in South America. To better constrain the age of the H2 eruption, we derive a chronology from the peat sequence using a Bayesian deposition model from radiocarbon analysis of terrestrial plant macrofossils. Our age model dates the H2 tephra to 4265 ± 65 cal yr BP, suggesting that the eruption occurred slightly earlier than previously reported. The refined age and new geochemical reference dataset will facilitate the identification of the H2 tephra in other distal locations. We recommend future studies search for its presence across the sub-Antarctic islands and Antarctic Peninsula as a potentially useful chronological marker. Finally, this study improves our knowledge of the dispersion of volcanic ash from Mt. Hudson, allowing us to better understand the eruptive frequency and risks associated with the Hudson volcano.

Part of:
15th International Conference on Accelerator Mass Spectrometry. Program and abstracts

Additional details

Publishing Information

Imprint Title
15th International Conference on Accelerator Mass Spectrometry. Program and abstracts
Imprint Pagination
303 p.
Journal Page Range
p. 87
Report number
INIS-AU--0116

Conference

Title
International Accelerator Mass Spectrometry Conference
Acronym
2021 AMS-15
Dates
15-19 Nov 2021
Place
Sydney, NSW (Australia)

Optional Information

Notes
Abstract only, full text in this record Imprint:Virtual conference. Includes obituary for Alan Williams (ANSTO Organising Committee) and 'In Memoriam' presentations for Professor Didier Bourl#Latin Small Letter E With Grave#s, Robert John 'Jack' Cornett and Ken Purser.