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May 23, 2025

Pairs of stars that orbit each other exhibit unexpected magnetic activity

Comparison of magnetic activity between single and binary stars. Credit: Nature Astronomy (2025). DOI: 10.1038/s41550-025-02562-2
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Comparison of magnetic activity between single and binary stars. Credit: Nature Astronomy (2025). DOI: 10.1038/s41550-025-02562-2

A new study in Nature Astronomy, led by Dr. Jie Yu, from the Australian National University, reveals that stars in close binary systems—pairs of stars orbiting each other at close range—can exhibit unexpectedly high levels of magnetic activity.

This activity, responsible for flares, sunspots, and other energetic outbursts, is usually powered by the star's rotation. For single stars, surface increases with stellar rotation rate, but only up to a known limit, beyond which activity saturates.

Using data from China's LAMOST telescope and Europe's Gaia space observatory, Dr. Yu's team found that close binary stars break this rule. Instead of leveling off, many of these stars show even stronger magnetic activity. And in the most extreme cases—where stars spin especially fast (orbital period < 0.5 days)—the activity curiously begins to decline, a phenomenon known as supersaturation.

The findings suggest that between closely orbiting stars can amplify or reshape their magnetic behavior. Understanding these effects offers new insight into stellar evolution and the magnetic environments that surround —an important factor in determining the habitability of exoplanets.

More information: Jie Yu et al, Enhanced magnetic activity in rapidly rotating binary stars, Nature Astronomy (2025).

Journal information: Nature Astronomy

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Close binary stars display magnetic activity that exceeds the saturation limit observed in single stars, with the strongest activity found in systems with short orbital periods. However, at extremely rapid rotation rates (orbital period < 0.5 days), magnetic activity declines, indicating supersaturation. Tidal forces in these systems significantly influence stellar magnetic behavior and evolution.

This summary was automatically generated using LLM.