From “CSIROscope” (AU) At CSIRO (AU)-Commonwealth Scientific and Industrial Research Organization : “Getting to the bottom of Antarctic Bottom Water”
At
CSIRO (AU)-Commonwealth Scientific and Industrial Research Organization
1.25.23
Dr Alix Post | Geoscience Australia
Associate Professor Helen Bostock | The University of Queensland
Matt Marrison | CSIRO
A team of scientists is plumbing the depths in East Antarctica to increase our understanding of Antarctic Bottom Water.
R/V Investigator [below] is once again sailing south to conduct important research in Antarctica. Called “CANYONS”, scientists on this 47-day voyage will investigate Antarctic Bottom Water in the Cape Darnley region of East Antarctica.
This is what you need to know about Antarctic Bottom Water.
Voyage Chief Scientist Dr Alix Post from Geoscience Australia will lead the 47-day voyage to East Antarctica. Image: Asaesja Young.
What is Antarctic Bottom Water?
You probably haven’t heard about Antarctic Bottom Water before but it’s very important for our oceans and climate. Put simply, Antarctic Bottom Water is dense, cold, oxygen-rich water that forms in just a few places around the Antarctic continent.
This water forms as cold winds blowing off Antarctica cool the ocean surface and form sea ice. As fresh sea ice forms, the salt in the seawater is ‘rejected’ (released). As a consequence, very salty and cold water is left behind. The same winds blowing off Antarctica then blow the sea ice away, exposing the ocean and forming new sea ice. This process further increases the saltiness of the water. This water then sinks through the water column forming Antarctic Bottom Water in the deepest parts of the ocean.
These bodies of open water, which are called polynya, can be thought of as sea ice factories.
The most important thing to know about Antarctic Bottom Water is that it’s the densest water on the planet. As the densest water mass, Antarctic Bottom Water flows down the Antarctic continental margin and north across the seafloor. In fact, it’s been found to occupy depths below 4000 metres in all ocean basins that have a connection to the Southern Ocean.
For this reason, it has a significant influence on the circulation of the world’s oceans.
Why is it so important?
The flow of Antarctic Bottom Water drives ocean circulation, assists in carbon capture and storage, and also carries oxygen to the deep ocean. As such, Antarctic Bottom Water ventilates the deep ocean.
However, climate change and the melting of the Antarctic ice sheet has led to increased fresh water flowing into the oceans around Antarctica. This has reduced the formation of Antarctic Bottom Water as it impedes the process to make cold, salty water. This reduction is likely to continue as the climate continues to warm.
Potentially, a complete shutdown of Antarctic Bottom Water formation is possible in the future. If this happens, it will likely have dramatic effects on ocean circulation. This will have consequences for weather patterns and the global climate. Moreover, a shutdown would likely create additional warming of the climate, including from reduced carbon capture and storage.
The CTD (conductivity, temperature and depth instrument) on R/V Investigator will be used to collect water samples and photograph seafloor life in Antarctica. Image Rod Palmer.
Where are we going and why?
The Cape Darnley region of East Antarctica is one of only four regions where the cold, salty and dense Antarctic Bottom Water forms. Scientists on this voyage aim to determine the flow pathways of this dense water mass down the rugged submarine canyons of the seafloor in this region. At the same time, they will also investigate its impact on seafloor life and ecosystems.
Importantly, they are also seeking insights into Antarctic Bottom Water sensitivity to changes in climate. This will help us predict how a warming climate will influence its future formation and impact on ocean circulation. Changes in the water mass have been detected over recent decades.
However, changes in this region have been little studied.
To address this, a multidisciplinary team of scientists from Australian research institutions and universities has been assembled on board R/V Investigator. This team will be led by Dr Alix Post from Geoscience Australia and A/Prof Helen Bostock from The University of Queensland.
Putting together pieces of an icy puzzle
Scientists want to better understand the tipping points that influence the production of Antarctic Bottom Water by investigating different climate states in the past climate record. To achieve this, the team on R/V Investigator will undertake detailed seafloor mapping of this area for the first time. Complete seafloor maps will reveal where Antarctic Bottom Water flows through the rugged submarine canyons. This will enable realistic ocean, climate and ecosystem models to be developed.
Multibeam sonar systems on R/V Investigator will be used to map the seafloor to study how features in the region, such as deep canyons, influence the flow of Antarctic Bottom Water.
In addition, they will also collect long sediment cores, analyze seawater samples and use deep sea cameras to image seafloor life.
Long sediment cores will reveal past changes in sea ice, ice-sheets and ocean circulation. These records will unlock the history of Antarctic dense water formation during periods of Earth’s history that were warmer than today. As a result, we will gain important insights into how our global climate is likely to respond to changes in the future.
Furthermore, the team will also collect large volumes of Antarctic seawater. Importantly, this will give us valuable insights into the processes controlling the distribution of trace metals in Antarctic waters. It will also contribute to developing new geochemical tracers for past ocean and ice sheet change.
Protecting Antarctica’s ecosystems
The area is one of three regions proposed as Antarctic Marine Protected Areas on the East Antarctic margin. Scientists will use deep sea cameras to take the first images of the seafloor life in this remote part of Antarctica. Altogether, the information they collect will help ensure this region can be protected into the future.
Join us in the south
The team will be bringing their research to life through photography, video, blogs and podcasts. These will be released through the Australian Centre for Excellence in Antarctic Science. We’ll share updates across our social channels with #RVInvestigator.
See the full article here .
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CSIRO (AU)-Commonwealth Scientific and Industrial Research Organization , is Australia’s national science agency and one of the largest and most diverse research agencies in the world.
CSIRO works with leading organizations around the world. From its headquarters in Canberra, CSIRO maintains more than 50 sites across Australia and in France, Chile and the United States, employing about 5,500 people.
Federally funded scientific research began in Australia 104 years ago. The Advisory Council of Science and Industry was established in 1916 but was hampered by insufficient available finance. In 1926 the research effort was reinvigorated by establishment of the Council for Scientific and Industrial Research (CSIR), which strengthened national science leadership and increased research funding. CSIR grew rapidly and achieved significant early successes. In 1949 further legislated changes included renaming the organization as CSIRO.
Notable developments by CSIRO have included the invention of atomic absorption spectroscopy; essential components of Wi-Fi technology; development of the first commercially successful polymer banknote; the invention of the insect repellent in Aerogard and the introduction of a series of biological controls into Australia, such as the introduction of myxomatosis and rabbit calicivirus for the control of rabbit populations.
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Australia Telescope National Facility – radio telescopes in the Facility include the Australia Telescope Compact Array, the Parkes Observatory, Mopra Radio Telescope Observatory and the Australian Square Kilometre Array Pathfinder.
CSIRO Australia Compact Array (AU), six radio telescopes at the Paul Wild Observatory, is an array of six 22-m antennas located about twenty five kilometres (16 mi) west of the town of Narrabri in Australia.
CSIRO-Commonwealth Scientific and Industrial Research Organization (AU) Parkes Observatory [Murriyang, the traditional Indigenous name], located 20 kilometres north of the town of Parkes, New South Wales, Australia, 414.80m above sea level.
NASA Canberra Deep Space Communication Complex, AU, Deep Space Network. Credit: The National Aeronautics and Space Agency
ESA DSA 1, hosts a 35-metre deep-space antenna with transmission and reception in both S- and X-band and is located 140 kilometres north of Perth, Western Australia, near the town of New Norcia
CSIRO-Commonwealth Scientific and Industrial Research Organization (AU)CSIRO R/V Investigator.
UK Space NovaSAR-1 satellite (UK) synthetic aperture radar satellite.
CSIRO Pawsey Supercomputing Centre AU)
Magnus Cray XC40 supercomputer at Pawsey Supercomputer Centre Perth Australia
Galaxy Cray XC30 Series Supercomputer at at Pawsey Supercomputer Centre Perth Australia
Pausey Supercomputer CSIRO Zeus SGI Linux cluster
Others not shown
Australia Telescope National Facility – radio telescopes included in the Facility include the Australia Telescope Compact Array, the Parkes Observatory, Mopra Radio Telescope Observatory and the Australian Square Kilometre Array Pathfinder.
Haystack Observatory EDGES telescope in a radio quiet zone at the Inyarrimanha Ilgari Bundara Murchison Radio-astronomy Observatory (MRO), on the traditional lands of the Wajarri peoples.
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