Antarctica is no stranger to icy shenanigans – look no further than the giant spinning iceberg, or the “fingers of death” that lurk beneath the surface. In 2016, however, scientists were baffled when an unexpectedly massive hole opened up in the ice of the Weddell Sea. Now, we might know why it happened.
It’s common for areas of open water to appear within sea ice, to the extent the phenomenon has a name: a polynya. However, the 2016 Maud Rise Polynya was the largest for 40 years, reaching nearly the size of Switzerland.
Initially, meteorologists attributed the unusually large polynya to a mix of unusual ocean conditions and an epic storm – and they even recruited elephant seals to collect the data that helped them make this conclusion, strapping some fancy hats scientific equipment onto their heads.
But earlier this year, another team discovered there were more factors at play than previously thought.
An important question remained: this was the fifth time such a large polynya had been seen in the same place, but nothing so big had turned up elsewhere – why? The more recent polynyas occurred near the peak of the sea ice extent in late winter or early spring, so this was not a case of thaw coming a little earlier there.
Part of the answer lies in a large circular current known as the Weddell Gyre, which was unusually strong from 2015-2018. This brought a deep layer of warm salty water to the surface.
“This upwelling helps to explain how the sea ice might melt. But as sea ice melts this leads to a freshening of the surface water, which should in turn put a stop to the mixing. So, another process must be happening for the polynya to persist. There must be an additional input of salt from somewhere,” said study co-author Professor Fabien Roquet, of the University of Gothenburg, in a statement.
The evidence from the trusty seals, in collaboration with autonomous floats, is that salt rose in turbulent eddies as the current flowed over the Maud Rise, the undersea ridge from which the polynya gets its name.
The polynya did not form directly over the peak of the rise, however, instead being centered on its northern flank. Roquet and co-authors attribute this to Ekman transport, where water moves at right angles to the direction of the wind, rather than running before it.
“Ekman transport was the essential missing ingredient that was necessary to increase the balance of salt and sustain the mixing of salt and heat towards the surface water,” said co-author Professor Alberto Naveira Garabato of the University of Southampton. It’s not something that has been considered in previous efforts to explain polynya formation.
Climate change may not have been the cause of the Maud Rise Polynya, but that doesn’t mean they are unrelated. Ice is an insulator, blocking the transfer of energy between ocean and atmosphere. Its absence increases that exchange, and the same goes for carbon dioxide. Deep in the Antarctic winter there is little sunlight for the open sea to absorb, but that changes come spring, when the polynya can lead to additional warming. In this way the polynya can be a microcosm of the decline of southern sea ice that began in 2016 and accelerated drastically last year.
“The imprint of polynyas can remain in the water for multiple years after they’ve formed. They can change how water moves around and how currents carry heat towards the continent. The dense waters that form here can spread across the global ocean,” said co-author Professor Sarah Gille of the University of California San Diego. In 2018 some, but not all, of the conditions necessary to form polynyas were still present, and no large opening appeared.
The study is published in Science Advances.
N.B. With professors from three institutions, the list of authors on the paper is an impressive one, but we’re disappointed to see that none of the elephant seals are named as research assistants. Maybe they should unionize.
An earlier version of this article was published in May 2024.
Source Link: Eight Years Ago, A Switzerland-Sized Hole Appeared In Antarctic Sea Ice – But Why?
