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Milky Way Magnetic Field Hides a Giant Diagonal Twist

A new radio map of the Milky Way magnetic field reveals a giant diagonal twist where the galaxy's invisible field flips the wrong way.

An artist's view of our galaxy with its magnetic field drawn as glowing lines. A new survey found that in one spiral arm, the field flips and runs the opposite way. Image: NavsoraTimes graphics.
Fig. 1 — The Milky Way and its invisible magnetic field, seen from above
An artist's view of our galaxy with its magnetic field drawn as glowing lines. A new survey found that in one spiral arm, the field flips and runs the opposite way. Image: NavsoraTimes graphics.

In This Article

  1. An Invisible Force Holding the Galaxy Together
  2. The Trick for Seeing Something Invisible
  3. How Did Scientists Spot a Twist No One Expected?
  4. What the Diagonal Twist Tells Us
  5. The Questions That Still Need Answering

Our galaxy is wrapped in something you can never see, yet it holds everything in place. It is the Milky Way magnetic field, a vast and invisible web of force. Astronomers have just drawn one of the clearest maps of it ever made, and the map held a shock: deep in one spiral arm, the field suddenly flips and runs the wrong way, cutting a giant diagonal twist across space.

An Invisible Force Holding the Galaxy Together

Think of a giant spinning plate of stars, gas, and dust. That is our galaxy. Gravity is always trying to pull all of it inward, so something has to push back and keep it steady.

One of those quiet helpers is the galaxy's magnetic field. It is far too weak to feel, but it stretches across the entire Milky Way. Scientists have long known it is there. What they lacked was a clear picture of its real shape.

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WHY THE MAGNETIC FIELD MATTERS A magnetic field is a region where magnetic force can act, like the invisible pull around a fridge magnet but spread across a whole galaxy. Researchers say that without it, the Milky Way could slowly collapse inward under its own gravity.

To map something invisible, the team needed a clever trick. And they had one.

The Trick for Seeing Something Invisible

You cannot photograph a magnetic field. So scientists watch what it does to radio waves passing through it. As those waves travel across space, electrons and magnetic fields gently twist them. That twist is called Faraday rotation.

One researcher compared it to a familiar sight: a straw in a glass of water looks bent because light changes as it passes through. By measuring how much the radio waves get twisted, the team could trace the hidden magnetic shapes behind them.

350–1030
Radio frequency range scanned, in MHz
2
Studies published from the work
Northern sky
Region of space the survey covered

The work used a new telescope in British Columbia and fed into a global project called the Global Magneto-Ionic Medium Survey, or GMIMS. Then the data showed something strange.

How Did Scientists Spot a Twist No One Expected?

Looked at from above, the Milky Way's magnetic field mostly runs in one direction, like a clock turning clockwise. The whole galaxy seems to follow that simple rule.

But in one region, the Sagittarius Arm, the field does the opposite. It runs counterclockwise. Scientists had seen hints of this reversal before, yet they could not work out how the field switched from one direction to the other.

The breakthrough came from the fresh, detailed data. The reversal was not a sharp wall. It was diagonal, slanting across space. The lead professor described the moment a colleague brought in the new data and the diagonal shape suddenly jumped out, an answer the team had been missing for years.

"We need to know what the magnetic field of the galaxy looks like now, so we can create accurate models that predict how it will evolve."

— Brown, University of Calgary · The Astrophysical Journal, 2026

What the Diagonal Twist Tells Us

A reversal is a place where the magnetic field points one way on one side and the opposite way on the other. Finding that the switch happens along a slanted, three-dimensional line is a real clue about how the galaxy is built.

One team member turned the discovery into a new 3D model. From our spot on Earth, that slanted structure is exactly what shows up as the diagonal seen in the data. It explains a puzzle that had no good answer before.

Clockwise
Direction of the main galactic field
Reversed
Field direction in the Sagittarius Arm
3D
New model shape explaining the twist
A MAP THE WHOLE WORLD CAN USE The survey did more than find one twist. It created a large, high-quality dataset of the galaxy's magnetic environment. Astronomers around the world can now use it for their own research, long after this study.

Still, a single new map cannot answer everything about a galaxy this big.

The Questions That Still Need Answering

This work maps the field as it looks today, but it does not fully explain why the reversal formed in the first place. How a galaxy grows a diagonal magnetic twist is still an open question.

The survey also covered the northern sky, so a matching look at the southern sky would complete the picture. Scientists want to know how this reversal fits into the long story of how galaxies form and slowly change over billions of years.

  • An invisible scaffold — the galaxy's magnetic field helps hold the Milky Way against the inward pull of gravity.
  • A diagonal flip — in the Sagittarius Arm the field reverses direction along a slanted, three-dimensional line.
  • A tool for everyone — the survey leaves behind a detailed magnetic map that astronomers worldwide can keep using.

"The discovery provides an important new clue about the hidden magnetic architecture of the Milky Way and could help scientists better understand how galaxies evolve." — University of Calgary, 2026.

We live inside this galaxy, yet we are still drawing its true shape for the first time. That is the quiet wonder of this work. The biggest things around us can stay hidden in plain sight, waiting for someone with the right tool and the patience to look closer.


📄 Source & Citation

Primary Source: Booth, R.A., Ordog, A., Brown, J.-A. et al. (2026). A three-dimensional model for the reversal in the local large-scale interstellar magnetic field. The Astrophysical Journal, 997(2), 304. https://doi.org/10.3847/1538-4357/ae28d1

Authors & Affiliations: Led by Rebecca A. Booth, Anna Ordog, and Jo-Anne Brown of the Department of Physics and Astronomy, University of Calgary, with international GMIMS collaborators.

Data & Code: The Faraday depth survey dataset is published openly as part of the Global Magneto-Ionic Medium Survey (GMIMS-DRAGONS).

Key Themes: Milky Way magnetic field · Magnetic reversal · Sagittarius Arm · Faraday rotation · Galaxy structure

Supporting References:

[1] Ordog, A., Booth, R.A., Landecker, T.L. et al. (2026). GMIMS-DRAGONS: a Faraday depth survey of the northern sky covering 350–1030 MHz. The Astrophysical Journal Supplement Series, 282(2):53.

[2] Dominion Radio Astrophysical Observatory, National Research Council Canada — radio survey facility.

[3] Global Magneto-Ionic Medium Survey (GMIMS) — international galactic magnetic field mapping project.

Frequently Asked Questions

What is the Milky Way magnetic field?
The Milky Way magnetic field is an invisible web of magnetic force that runs through our whole galaxy. It is weak but vast, and it helps hold the galaxy together against gravity.
What did scientists discover about the Milky Way magnetic field?
Astronomers mapped the field in fine detail and found a giant magnetic reversal in the Sagittarius Arm, where the field flips direction along a diagonal line cutting across space.
How do scientists map an invisible magnetic field?
They use a radio telescope to measure Faraday rotation, a slight twist in radio waves that happens when the waves pass through electrons and magnetic fields in space.
Why does the Milky Way magnetic field matter?
Without a magnetic field, the galaxy could collapse under its own gravity. Knowing its true shape helps scientists build accurate models of how the galaxy formed and how it will change.
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