In November, scientists arrived at the South Pole in planes outfitted with skis to pull off a construction project seven years in the making.
They had a short summer window — November to early February — to drill six new holes at least a mile and a half deep into the Antarctic ice and install long cables, beaded with hundreds of orb-shaped light detectors. This dense network of eyes is an upgrade to the IceCube Neutrino Observatory, a massive 15-year-old system made up of more than 5,000 sensors embedded in a gigaton of ice.
These devices are all looking for the fleeting footprints of neutrinos, the most mysterious in the pantheon of known particles.
Neutrinos are often called “ghost particles” because most of the time, they stream through and by us unnoticed. They have no charge and very little mass. They are abundant — generated by fusion reactions in the sun, showering down when cosmic rays interact with Earth’s atmosphere and also racing across the cosmos, ejected from the most explosive events. Neutrinos may seem like esoteric, subatomic minutiae, but they are connected to some of the most fundamental questions about our existence: They govern how a supernova explodes, they play a role in our understanding of the Big Bang, and they can help answer basic questions about why we are made of matter, not antimatter.
Because of their ghostlike nature, neutrinos streak across great distances unperturbed and can provide a new kind of telescope into the cataclysms that shape the evolution of galaxies. Until now, IceCube has largely been focused on trying to capture evidence of these extremely high-energy neutrinos. The upgrade expands its capabilities, allowing scientists to ask even more basic questions about these particles, including how they morph from one flavor of neutrino into another, and providing an opportunity to study the most elusive neutrino of all — the tau neutrino.
The newly completed upgrade will give the detector greater sensitivity to probe lower-energy neutrinos, allowing scientists to learn more about what happens as atmospheric neutrinos change from one type to another. It will also help them to understand more about how light travels within the ice to improve all the data the observatory collects.
“I think it’s really cool — a totally new way to see things,” said Erin O’Sullivan, an associate professor of physics at Uppsala University in Sweden and a spokesperson for the project. If human eyes saw neutrinos and not visible light, “the sun would be shining all the time, and it would be coming up through the floor and through our eyelids.”
IceCube can’t directly see these enigmatic particles, but its thousands of sensors can detect what happens after they interact with matter. When they do, the neutrinos produce charged particles that travel through the ice at nearly the speed of light, creating a blue glow called Cherenkov radiation.
In 2017, IceCube detected a high-energy neutrino from a blazar, a galaxy with a supermassive black hole at its center, 4 billion light-years away off the left shoulder of the constellation Orion. In 2022, scientists reported that an active galaxy called NGC 1068, in the constellation named after the sea monster Cetus, was spewing high-energy neutrinos our way from the supermassive black hole that powered it. Most recently, scientists reported that neutrinos were coming from inside our own galaxy, the Milky Way.
In the Trump administration’s budget request, the observatory’s National Science Foundation funding would have been cut in half, as part of a large reduction to the agency’s overall budget. Congress rejected the president’s budget proposal for the NSF, funding the agency at nearly the same level as last year.
Albrecht Karle, principal investigator of the upgrade, has been making trips to Antarctica since the 1990s. He works at the University of Wisconsin at Madison, but he left home the day before Thanksgiving for the South Pole. He arrived at the observatory in December, a week before drilling was to begin.
Most of the anticipation around IceCube is for the data it will collect for years to come, but the update of the observatory — in the planning for seven years — was a tense time for the scientists working on the ice.
“Drilling is never a piece of cake. … This drill is the most powerful hot-water drill on Earth of its kind. You can never leave it alone. It’s minus 30 degrees Celsius, and if water sits more than 45 minutes, it starts freezing,” Karle said.
The team worked to melt holes in the ice quickly — but quick is relative. To drill holes a mile and a half deep takes about 30 hours, and 18 more hours to return to the surface. Then, the race begins because almost immediately, the hole starts to shrink as the water refreezes.
“If it takes too much time, the instruments don’t fit in anymore. That’s always a concern,” Karle said. “So we do careful calculations to predict what we call the lifetime of the hole. If it takes us longer to get the instruments deployed into the hole, then we risk the strings [getting] stuck. That can be nerve-racking.”
The sixth hole was completed on Jan. 20.
“Within the first couple years, we should be making much better measurements,” O’Sullivan said. “There’s hope to expand the detector, by an order of magnitude in volume, so the important thing there is we’re not just seeing a few neutrino point sources, but we’re starting to be a true telescope. … That’s really the dream.”
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