Most telescopes sit on a mountaintop and look up. This one is frozen into the ice about a mile under the South Pole, and on Tuesday it won the Nobel Prize in Physics.

The prize went to Francis Halzen, a Belgian-born physicist at the University of Wisconsin-Madison, who first pitched the idea back in 1988. His telescope is called the IceCube Neutrino Observatory, and almost none of it is visible.

All that shows on the surface is a small lab on stilts, which would fit right in with our roundup of infrastructure that looks like science fiction. The telescope itself is underneath. A full cubic kilometer of ice, strung with 5,160 glass sensors.

The IceCube Lab in deep blue twilight at the South Pole with a pale orange moon rising low on the horizon
The moon rising beside the IceCube Lab. Photo: Alicia Fattorini, IceCube/NSF
The short version
1
Space is throwing things at us
Exploding stars and black holes fire out tiny particles called neutrinos. Nearly all of them pass through the Earth as if it weren’t there.
2
Once in a while, one hits
When a neutrino does crash into something, it makes a tiny flash of blue light. In clear, dark ice, that flash can be seen.
3
The flash points home
Sensors frozen in the ice record which way the light traveled. Follow that line backward and you know where in the sky the particle came from.
IceCube, top to bottom
Depth drawn to scale
0 m
the snow
nothing
but ice
1,450 m
first sensor
2,450 m
last sensor
1 km³
of Antarctic ice, more than a billion tons of it
5,160
glass light sensors on 86 cables
7
polar summers to build, 2004 to 2010
450
scientists in 14 countries
100 trillion
neutrinos pass through your body every second

Fair warning, it took us a few reads to get our heads around all this, and we’re still not sure we fully have. So what is it looking for? Neutrinos, the shyest particles we know of. They have no charge and almost no mass, and they sail through walls, people and entire planets without touching a thing. After light itself, they’re the most common particle in the universe.

About 100 trillion of them pass through your body every second! IceCube’s own team figures a detector the size of a person would wait around a hundred years to catch just one.

Halzen’s hunch was that Antarctica had already built the detector for him. The ice deep under the pole has been squeezed for so long that the air bubbles are gone, which leaves it extremely clear. It’s also completely dark.

Every so often a neutrino does hit an atom in that ice. When it does, it kicks out particles moving faster than light can travel through ice, and they leave a faint trail of blue light that can stretch for more than a kilometer. The sensors catch that glow, and from the pattern physicists can work out where the neutrino came from.

Our favorite part is that IceCube spends much of its time looking down. Neutrinos are the only particles that can pass through a whole planet, so anything that arrives from below has to be one. It’s a telescope at the South Pole that uses the Earth as a filter to watch the northern sky. That still bends our brains a little, so we drew it.

Diagram of a neutrino from a distant galaxy passing straight through the Earth to the IceCube detector at the South Pole, while other particles stop at the surface
How a telescope at the bottom of the world watches the sky at the top. Illustration: Moss & Fog

They built it with hot water

Aerial view of the IceCube Lab and a line of red drill camp buildings on the flat white Antarctic plateau
The IceCube Lab and its drill camp from the air. Photo: Michael Rayne, ASC-ARFF

To get the sensors down there, the team melted their way in. A custom drill shot hot water through a high-pressure hose, sinking holes about 60 centimeters wide and nearly two and a half kilometers deep.

Each hole took about 48 hours and turned some 200,000 gallons of ice into water. The hose alone weighs 25,000 pounds.

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View from a drill tower at the South Pole looking down on hose reels, cables and the IceCube Lab under a deep blue sky
Hose reels and the IceCube Lab, seen from the drill tower during the 2025 to 2026 upgrade. Photo: Yuya Makino, IceCube/NSF

Then they had to hurry. Crews clipped 60 sensors onto a cable, lowered it into the water, and let the hole freeze shut around it. They did that 86 times.

Work was only possible in the polar summer, roughly November through February, so it took seven seasons. The last string went in on December 18, 2010.

Once a string freezes in, nobody can get to it again. Any fixing has to happen from the surface, by software. Fewer than 100 of the roughly 5,500 sensors have quit since.

Also, every string has a theme and every single sensor has its own name, which we find very charming!

Looking straight down a blue-white hole melted into Antarctic ice as a spherical glass light sensor is lowered into it
A newer sensor heading down a freshly melted hole during the recent IceCube Upgrade. Photo: Yuya Makino, IceCube/NSF

What it has found so far

In 2013, IceCube caught its first high-energy neutrinos from far beyond our solar system. Nobody could say what was making them.

IceCube event display from November 12, 2010, with red, orange and green spheres marking the sensors that saw light as a particle crossed the detector
What a detection looks like. Each sphere is a sensor that saw light, red first and green last. The team nicknamed this 2010 event Dr. Strangepork. Graphic: IceCube Collaboration

Then on September 22, 2017, a single neutrino lit up the array. IceCube sent out an alert, about 20 observatories on the ground and in orbit turned to look, and together they traced it to a blazar called TXS 0506+056. That’s a galaxy with a giant black hole at its center.

A second galaxy, NGC 1068, followed in 2022. That’s two so far. It’s early days for this kind of astronomy.

In 2023 came the one we like best, the first picture of our own Milky Way made with neutrinos instead of light. File it next to our look at the size of the universe.

Artist's composition of the Milky Way as a horizontal band of stars overlaid with a blue glow representing neutrino emission detected by IceCube
An artist’s composition of the Milky Way with its neutrino glow in blue. Image: IceCube Collaboration/U.S. National Science Foundation (Lily Le and Shawn Johnson)/ESO (S. Brunier)

Halzen was born in Tienen, Belgium, in 1944 and has been in Madison since 1972. That makes this a 38-year project for him, from first pitch to the phone call. Honestly, we can’t think of many ideas we’d stick with for that long.

Thirty-eight years, eight stops
1988
Halzen pitches a telescope made of polar ice
1990s
A smaller test array, AMANDA, shows the ice is clear enough
2004
Construction starts at the South Pole
2010
The 86th and last string goes in on December 18
2013
First high-energy neutrinos from deep space
2017
One neutrino is traced back to a distant blazar
2023
The Milky Way, pictured in neutrinos
2026
The Nobel Prize in Physics

He won it alone, too, which hasn’t happened in physics in more than thirty years.

He took the committee’s call in Italy and said the news felt “strange.” Then he gave the credit to his collaborators.

“A celebration of a very unusual project.”
Francis Halzen, on the prize

They aren’t done, either. An upgrade went in over the last polar summer, and there’s a proposal for a successor called IceCube-Gen2 with eight times the volume.

Two people from the team stay at the pole all year to look after it, right through the long, dark winter. And the ice they’re standing on slides about ten meters a year, all in one piece. So the whole telescope is very slowly on the move.

A lone figure stands in front of the red-lit IceCube Lab during the polar night, with the Milky Way and green aurora overhead
One of the two winterovers outside the lab during the polar night. Photo: Josh Veitch-Michaelis, IceCube/NSF

Images courtesy of the IceCube Collaboration and the U.S. National Science Foundation. See more from our Science archive.

By Moss & Fog Staff

Author

Ben VanderVeen is the founder and editor of Moss & Fog, one of the web’s longest-running visual culture destinations. Since 2009, he’s been finding and framing the most beautiful, surprising, and thought-provoking work in art, architecture, design, and nature — reaching over 325,000 readers each month. He lives in Portland, Oregon.

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