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Magnetic fields may be the secret behind binary star formation

Date:
June 5, 2026
Source:
National Institutes of Natural Sciences
Summary:
Scientists have uncovered a surprising force that may help explain how binary star systems form so quickly. New supercomputer simulations show that magnetic fields surrounding newborn stars can act like a cosmic brake, stripping away angular momentum and allowing two still-forming protostars to spiral closer together instead of drifting apart.
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Many stars are born inside vast clouds of gas and dust in space. As parts of these clouds collapse under gravity, they create dense regions known as molecular cloud cores where new stars begin to take shape.

Star formation often occurs in groups rather than in isolation. In some cases, two newborn stars become gravitationally bound, creating what astronomers call a binary star system. Observations indicate that many of these systems form very early, before the stars themselves have fully developed. However, researchers have long struggled to understand how two growing protostars can move close enough together to become a binary pair within such a short period of time.

Simulations Reveal the Importance of Magnetic Fields

To investigate this mystery, researchers carried out advanced simulations using several supercomputers, including the National Astronomical Observatory of Japan's ATERUI III system and its predecessor, ATERUI II.

The results showed that magnetic fields threading through the surrounding gas can help draw protostars closer together. Interactions between the magnetic field and the gas remove angular momentum from the pair, allowing the two objects to spiral inward and form a binary system within a realistic timescale.

The simulations also highlighted just how important magnetic fields are to the process. In a test run that excluded magnetic fields entirely, the protostars moved farther apart instead of closer together.

Possible Implications for Black Hole Mergers

The researchers found that a similar mechanism could operate in much larger systems. Massive binary black holes located in the gas rich centers of newly formed galaxies may also lose angular momentum through interactions involving magnetic fields.

Such a process could help explain how pairs of giant black holes move close enough together to eventually merge. These mergers are thought to be an important step in the formation of supermassive black holes after galaxies collide and combine.

Directly simulating the long-term evolution of massive binary black holes remains computationally difficult because of the enormous timescales involved. As a result, researchers say that further studies will be needed to fully determine how magnetic fields influence the behavior and merger of these extreme objects.


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Materials provided by National Institutes of Natural Sciences. Note: Content may be edited for style and length.


Journal Reference:

  1. Tomoaki Matsumoto, Kenta Hotokezaka, Kohei Inayoshi. Magnetic-field-induced inspiral of binaries with circumbinary disc: black hole and protostellar systems. Monthly Notices of the Royal Astronomical Society, 2026; 548 (2) DOI: 10.1093/mnras/stag669

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National Institutes of Natural Sciences. "Magnetic fields may be the secret behind binary star formation." ScienceDaily. ScienceDaily, 5 June 2026. <www.sciencedaily.com/releases/2026/06/260605023355.htm>.
National Institutes of Natural Sciences. (2026, June 5). Magnetic fields may be the secret behind binary star formation. ScienceDaily. Retrieved June 5, 2026 from www.sciencedaily.com/releases/2026/06/260605023355.htm
National Institutes of Natural Sciences. "Magnetic fields may be the secret behind binary star formation." ScienceDaily. www.sciencedaily.com/releases/2026/06/260605023355.htm (accessed June 5, 2026).

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