Chinese scientists have revealed that the halo of the Milky Way is filled with massive, doughnut-shaped magnetic fields.

Measuring 12,000 to 100,000 light-years across, these invisible magnetic doughnuts sit inside the vast gas clouds that envelop the galaxy’s bright, spinning disk, with the galaxy’s heart at their centre, according to researchers from the National Astronomical Observatories of China (NAOC) in Beijing.

While their magnetic strength was only about one-millionth of the Earth’s magnetic field, they played an instrumental part in shaping the Milky Way into what it is today, the researchers wrote in a paper published in The Astrophysical Journal last week.

“Magnetic fields are ubiquitous in our Milky Way and play a significant role in the evolution of molecular clouds, star formation and the transport of cosmic rays,” the team wrote in the paper.

The study will help determine the large-scale structure of magnetic fields in our galaxy, something that has baffled astronomers for decades – and crucial to understanding the origin and evolution of magnetism in the universe, the scientists wrote.
Magnetic forces are everywhere – from a fridge magnet, to a compass, to the Earth’s magnetic field which protects life from the attacks of high-energy solar particles and cosmic radiation.
The Milky Way is made up of a bulge at its heart, a central disk and an outer halo. Photo: Nasa/JPL-Caltech/European Space Agency

Magnetism is vital to physical processes in the universe. For instance, during the birth of new stars, magnetic forces fight gravity to slow down the gathering of hot, dense gases, so that they can form stars and do not collapse under gravity too quickly.

Scientists already knew that the magnetic fields in the Milky Way’s disk are mostly horizontal. They distribute along the galaxy’s spiral arms, with each arm resembling a huge, curved bar magnet stretching all the way from the galactic centre to its outer tip.

However, the magnetic fields of the Milky Way halo remained unclear. The halo has only 1 per cent of the galaxy’s stellar mass, and was once thought to lack a coherent, large-scale magnetic structure.

In the new study, the NAOC researchers used an indirect method known as Faraday rotation to determine the exact shape and size of magnetic fields in the galactic halo.

It works on the idea that when radio waves from distant galaxies travel through the universe, including the gas and dust between stars, the waves will change orientation because of magnetism.

By using radio telescopes on Earth, scientists can measure the direction and degree of the rotation, and work out the size and strength of the magnetic fields along the way.

This illustration shows the magnetic field structure in a galactic halo. Credit: NAOC
To do this, the Chinese team collected the Faraday rotation measurements of about 60,000 distant radio sources outside the Milky Way. They also obtained the measurements of hundreds of radio sources near the solar system inside the galaxy, including the faint ones detected by China’s FAST radio telescope in recent years.

Then the researchers subtracted the latter measurements from the former to make sure that the results reflected the true magnetic structure of the Milky Way halo.

They found that the magnetic fields extended surprisingly far into the outer part of the halo, to at least 50,000 light-years from the galactic centre. In comparison, the distance between Earth and the galactic centre is about 30,000 light years.

The researchers said that next-generation radio telescopes, such as the Square Kilometre Array (SKA) now being built in Australia and South Africa, would measure Faraday rotation more efficiently and help refine the results.

One of the SKA’s top science goals is to use its unprecedented sensitivity to study the nature of cosmic magnetism. China is a founding member of and major contributor to the SKA project.