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Self-Destruct
Scientific American
|October 2025
This planet triggers flares on its star—spelling its ultimate doom

STARS OFTEN WHIP their planets with stellar winds and radiation, pull them ever closer with gravity and sear them with heat. But a newfound planet exerts an unexpectedly strong-and ultimately self-destructive-influence on its star in return.
The star, HIP 67522, is slightly larger than our sun and shines roughly 408 light-years away in the Scorpius-Centaurus association. It's 17 million years old, a youngster by stellar standards, and has two orbiting planets that are even younger. The innermost of these two planets, a Jupiter-size gas giant called HIP 67522 b, orbits HIP 67522 at a distance of less than 12 times the star's radius-about one-seventh Mercury's distance in solar radii from our own sun. This in-your-face proximity, combined with HIP 67522's volatile teenage nature, creates a spectacle that astronomers have never seen before: a planet that triggers powerful flares on the surface of its host star, leading to the planet's own slow destruction.
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