A deep canyon at the front of the Vanderford Glacier in East Antarctica has been mapped for the first time by acousticians on board RSV Nuyina. The previously unknown canyon, more than 2,200 metres deep, 2,000 metres wide and at least 55 kilometres long, was discovered after the ship left Casey research station following its refuelling operation.
As the ship navigated Vincennes Bay in front of the glacier, acousticians Jill Brouwer, Alison Herbert and Floyd Howard switched on the ship’s EM122 multibeam echosounder and were surprised by what they saw. “Although we’ve been visiting this region for decades on the Aurora Australis, we haven’t had the capability to do this sort of detailed mapping before,” Mr Howard said. “As a result, current navigational charts of this area are based on fairly limited surveys. Our work has shown that the seafloor is deeper and more complex than we thought.”
Building a Picture of the Seafloor
The multibeam echosounder sends out pings of sound in a fan shape beneath the ship and ‘listens’ to the returning echoes to build a picture of the seafloor. The sideways projection of sound also allowed the team to map the canyon underneath the glacier for up to three and a half kilometres from the front.
Voyage Leader Lloyd Symons said it’s not unusual to see interesting features in front of glaciers, which scour the seafloor as they advance or retreat and drop rocks or ‘erratics’ along the way. But he wasn’t expecting a canyon this deep. “It is truly mind-boggling to look northward to the nearby Browning Peninsula and know that there is 2,200 metres of water underneath the keel.”
“It will be really interesting to see how we can use Nuyina’s acoustic capabilities to improve our understanding of the seafloor bathymetry around our other stations in the future, particularly the approach to Mawson, which has a deep, narrow channel surrounded by pinnacles of rock.”
Measuring Changes in Water Properties
The technical team on board also sampled the water in the canyon using a conductivity, temperature, depth (CTD) instrument, deployed to just three metres above the seafloor. CTDs are used by oceanographers to measure changes in water properties – including ocean temperature and salinity near glaciers, to understand how warming water contributes to glacial melt from below. The data from this and other mapping efforts on board Nuyina will feed into global efforts to map the world’s oceans by 2030.
Acoustics experts and science systems engineers on the ship are from the AAD’s Technology and Innovation Branch, funded by the Australian government to manage the suite of world-leading science systems on board RSV Nuyina.
About RSV Nuyina
The icebreaker RSV Nuyina is the main lifeline to Australia’s Antarctic and sub-Antarctic research stations and the central platform of the Antarctic and Southern Ocean scientific research. Nuyina makes it possible to cross thousands of kilometres of the world’s stormiest seas, navigate through Antarctica’s formidable sea ice barrier, and live and work for extended periods on the coldest, driest and windiest continent on Earth – some of the harshest conditions in the world.
Nuyina, pronounced noy-yee-nah, means ‘southern lights’ in palawa kani, the language of Tasmanian Aborigines.