Astronomers have confirmed that strong magnetic fields are frozen in place deep inside aging stars.

red giants and magnetic fields
Stars like the Sun puff up and become red giants towards the end of their lives, so they're much larger even though the masses don't really change. The red giants ("old" Suns) of the same mass as the Sun do not show strong magnetic fields in their interior, but for stars slightly more massive, up to 60% host strong magnetic fields.
University of Sydney

Stars create magnetic fields through convection, the swirling, Ferris-wheel-like motion of hot, ionized gas (or boiling water, for that matter). Where convection happens in a star depends on how massive the star is: low-mass stars, including the Sun, have convective outer envelopes around a non-convective core, but stars a little bulkier — up to a couple Suns’ worth — do have convective cores.

Recently, Jim Fuller (Caltech) and colleagues found that strong core magnetic fields could explain the oddly weak, on-and-off brightening behavior of a sample of red giant stars. These stars are low- to middle-mass and have stopped fusing hydrogen in their centers, so they don’t have convective hearts. They also often have a mismatched, variable glow, with one hemisphere brightening as the other fades. What was strange about the sample the team looked at was that this group didn’t vary as much in brightness as it should have.

Now, Dennis Stello (University of Sydney and Aarhus University, Denmark), Fuller, and their team has expanded this work to 3,600 red giants, observed with the Kepler spacecraft. The astronomers found that here, too, some red giants had “muffled” variations, but just how much they were suppressed depended on how massive the star was. For stars just above the Sun’s  mass and lighter, the stars looked normal. But for the heftiest of the sample — 1.6 to 2 solar masses — about half are “depressed,” the team reported January 6th at the American Astronomical Society meeting in Kissimmee, Florida, and in the January 21st Nature.

This mass boundary between “normal” and “depressed” red giants is also the transition point from non-convective to convective cores. So this result is a nice confirmation that astronomers can track the strength of a star’s internal magnetic field using these brightness patterns. That prospect excites researchers, because magnetic fields play a big role in stars’ evolution and death, but astronomers don’t understand the details.

However, as I noted before, red giants don’t have convective cores. But they used to, before their central hydrogen-fusion furnaces shut off. So the fields muffling the variations are fossils. Magnetic fields are like strings, Fuller says, and they get twisted and tangled by the churning, convective plasma. Once this boiling motion disappears, the field essentially freezes in place. So long as there are no big, bulk motions to disrupt the field, it should just stay put.

What the team doesn’t know is whether these fossil fields will survive once the stars kick start core helium fusion, which is the next stage in their aging process. If the fields do survive, they might be the source of the strong magnetism detected in some white dwarfs, which are the final state these red giants are approaching. The fields might also explain the “extra internal mixing” that seems to go on in some red giants and their older siblings.



Stello, Dennis et al. “A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars.” Nature. January 21, 2016.

Watch the AAS press conference: pick “Life in Clusters, Red-Giant Cores, Eta Carinae Twins, Star-Forming Galaxies” from the Meeting #227 list.


Image of Anthony Barreiro

Anthony Barreiro

January 21, 2016 at 8:45 pm

Are these frozen magnetic fields analogous to the remnant magnetic fields observed on the Moon and Mars?

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January 22, 2016 at 10:29 pm

I too need a tutorial on how you could have a frozen magnetic field in a star. From my past physics courses, I recall that magnet fields are generated by flowing charges or aligned spinning charges (such as in magnetized iron). Can someone please give a little more detail on how these 'frozen' magnetic fields could exist without convection and without having aligned spinning nuclei/electrons.

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January 25, 2016 at 3:48 pm

For a plasma, the currents are produced by the qV of the particles which results in an E=VxB electric field for a perfectly conducting plasma. The resulting MHD equations show that the magnetic flux through any closed contour moves with the plasma -- in other words it gets frozen into the plasma. My best guess is that this may be the effect being described. If there is a little bit of resistance, the magnetic field can diffuse through a plasma.

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