On the afternoon of the 21st, The Palmer began its 13-knot transit from Rothera to Thwaites Glacier. All our fingers were crossed that the ice would not prevent the Palmer from getting close to the ice shelf. The captain maintained that weather and ice conditions would determine just how close we would get to the face of the calving front, which would in turn determine just how much data we could gather beneath the shelf front with our now very well-tested array of instruments.
The 26th of February dawns gloomy but calm, a perfect backdrop for the towering 30-40 meter wall of the eastern ice tongue, the crystalline face fractured and glowing deep teal to cobalt in the fissures and cavities. The Palmer glides slowly, 400 meters from the face of the ice shelf in front of Thwaites Glacier.
Arriving around 5 a.m., the Palmer begins to map the uncharted perimeter, the multibeam simultaneously mapping the sea floor in front and as far under the shelf as the angle of the sound pulse could extend. The weather for the next two days was expected to worsen, so this day was the perfect day to get as close to the shelf terminus as possible.
Thwaites Glacier ice shelf extends ~15 kilometers beyond the grounding line. The grounding line is where the glacier transitions from resting on the bedrock to floating ice shelf in the Amundsen Sea. Along the 150-kilometer ice front, the satellite images show two different types of ice shelf. The eastern ice shelf looks like a large solid piece of ice. Moving west along the front (down in the image) the ice changes into what looks like alligator skin. That texture is created by crevassing of the ice as it moves past the grounding line. Once they move into the sea, the ice eventually breaks along the fracture lines.
This is the first time since 2000 that the Palmer has been to Thwaites, with only one other more recent survey conducted by the Polar Stern in 2006. Neither mission made it south of 74o 50’ latitude. The Palmer mapped a new ice-free boundary that is 18 km further south than in 2006.
As of the 3rd of March, the THOR team have surveyed more than 1500 square kilometers of new sea floor. Upon reaching the eastern edge of the shelf, we gathered multibeam bathymetry and sub-bottom profiles. Sub-bottom profiles are pictures, almost like an x-ray view, of the first 10’s of meters into the sea floor. Similar to the multibeam echo sounder, sub-bottom profiles are also created from sound, but using different frequencies and computer processing to generate an image that shows sea floor structure and sedimentary layers. These profiles are collected simultaneously with the bathymetry data to help the THOR team find places to collect core samples.
The other teams are also busy deploying the ocean water CTD’s (35 in total for all of Thwaites as of 7th) and deploying gliders that collect ocean current and CTD information over a longer time period right next to the glacier. Lars Boehme and his team were gifted with a perfect day to look for seals on ice floes north of the eastern ice shelf, successfully tagging two of the four they found.
The Hugin also deployed on a 13-hour mission to conduct a survey of the sea floor. Its mission was to look for features of recent glacial retreat and measure Circumpolar Deep Water properties near the glacier front. Following its recovery on the afternoon of March 1st, the Hugin’s multibeam data revealed meter scale sea floor features, finer-scale features that complement the regional scale imagery that the multibeam bathymetry collects.
As of the 6th of March, THOR collected 14 cores from six sites, with the first three gathered in the early hours of the 27th from a site that was identified from the initial multibeam survey line at the face of the ice shelf. This first site is near what is possibly a former pinning point at the tip of the remnant Thwaites Glacier Tongue.
We wake early on the 7th to find ourselves gone from Thwaites. The Palmer is sitting quietly in the ice-free waters of western Pine Island Bay. We are there to conduct additional physical oceanography measurements and to collect moorings. Moorings are stationary instruments that collect ocean data over several years. The instruments are tethered to a weight that sinks to the bottom of the ocean. They are recovered by triggering a release mechanism that will allow the instrumentation to float up to surface for retrieval. They are sometimes hard to find because their original location may be adjusted when the weights are caught and moved by giant icebergs.
Perhaps not so surprising when we arrive is that the Pine Island calving face has also retreated several kilometers since the last survey in 2017, providing the opportunity to survey the newly exposed sea floor. The ice-free conditions ensure that we can complete the oceanographic tasks and head back to Thwaites for a few more days of surveying (and hopefully coring!) on the far east side of the Thwaites ice shelf in an area that has recently become ice free. There and gone….but going back again.