In an articlepublished Aug. 28 in Nature Astronomy, a collaboration led by Sui Ann Mao, the Minerva Research Group leader at the Max Planck Institute for Radio Astronomy and a former postdoctoral Jansky Fellow at the University of Wisconsin–Madison, reports the discovery of large, well-ordered magnetic fields in a galaxy far, far away. Because of the time it takes light to travel such immense distances, astrophysicists observe cosmologically distant magnetic fields as they were 4.6 billion years ago. The new observations provide hints at how magnetic fields have grown into galactic-sized structures since the beginning of the universe.

Like the humble refrigerator magnet, astronomical objects such as galaxies, stars, and even our own Earth have magnetic fields that attract and repel other magnets and electrically charged matter. Understanding magnetic fields is essential to understanding fundamental questions about the universe. Among other things, magnetic fields play a crucial role in the processes that form stars out of interstellar gas, determine how stars affect their surroundings, and indicate whether planets may or may not be habitable.

In the Big Bang theory for the origin of the universe, there were no magnetic fields in the cosmos. So when and how did magnetic fields arise? Scientists, including Mao’s team, aim to answer the question by observing the strength and organization of magnetic fields in galaxies as far away — and therefore as far back in time — as possible, when the universe was much younger.

“By catching magnetic fields when they’re so young, we can rule out some of the theories of where they come from,” explains Ellen Zweibel, a professor of astronomy and physics at UW–Madison and a co-author of the new study.

Astronomers had measured large, well-ordered magnetic fields in our own Milky Way and in galaxies in our cosmic neighborhood before. But Mao’s team is the first to successfully measure the magnetic field structure of a galaxy so distant in both space and time, pushing the boundaries of what’s capable with current radio telescope technology and analysis techniques. With the National Radio Astronomy Obesrvatory’s Very Large Array, a collection of 27 radio telescopes in New Mexico arranged to function together as a single enormous telescope, Mao observed a distant galaxy with a specific configuration optimal for measuring the galaxy’s magnetic fields.

The galaxy lies in front of a quasar, one of the brightest objects in the sky. The light from the quasar appears as two distinct images around the foreground galaxy, bent and magnified by the galaxy’s mass in a phenomenon called gravitational lensing. Mao and her team measured how properties of the two images of the quasar differed, affected by the magnetic fields of the galaxy, to determine the strength and organization of those magnetic fields.

“It’s a beautiful experiment,” Zweibel says of Mao’s experimental design.

Zweibel explains that the setup eliminates the need to account for how looking through different parts of the Milky Way would affect the observations. Since the two views of the quasar are observed along two very close lines of sight through the Milky Way, they are affected in the same way and can be compared.

Mao first proposed this experiment to Zweibel when she was a postdoctoral scientist at UW–Madison. She says Madison is a stimulating environment for studying and discussing magnetic fields in the universe because of a critical mass of scientists researching the phenomenon and the annual Midwest Magnetic Fields Workshop that takes place in Madison.

“Madison is the magnetic fields capital of the USA — it’s the place to go if you want to study magnetism,” says Mao.