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NASA data reveals weird x-ray changes in the exploded ruins of dead stars

NASA data reveals weird x-ray changes in the exploded ruins of dead stars This sparkling galaxy is home to a set of supernova remnants that showed variable brightnesses over 14 years of data A set of supernovae are behaving in weird ways, more than a decadeโ€™s worth of data from

NASA data reveals weird x-ray changes in the exploded ruins of dead stars
Scientific American โ€” 16 June 2026
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NASA data reveals weird x-ray changes in the exploded ruins of dead stars

This sparkling galaxy is home to a set of supernova remnants that showed variable brightnesses over 14 years of data

A set of supernovae are behaving in weird ways, more than a decadeโ€™s worth of data from NASAโ€™s Chandra X-ray Observatory reveals. Instead of slowly fading, as expected, these exploded stars have dramatically varied in brightness over the course of 14 years.

Typically, when a massive star explodes in a supernova, it leaves behind a cloud of superheated gas and debris. Over time, these stellar fireworks tend to fade, but Chandra observations of the galaxy Messier 83 (M83) from 2000 through 2014 suggests thatโ€™s not always the case. There supernova remnants that researchers had expected to have faded x-ray emissions actually showed surprising variety in the brightness of their x-rays.

The findings were published in the Astrophysical Journal this month.

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M83 is around 15 million light-years away from Earth. Also called the Southern Pinwheel, this spiral galaxy is a hotbed of star formation. โ€œWe knew that individual X-ray sources could vary dramatically,โ€ said Andrea Prestwich, an astronomer at the Catholic University of America and the studyโ€™s lead author, in a statement . โ€œBut finding that so many supernova remnants were behaving this way was a real surprise. Something unusual is going on in these objects. Pinpointing the cause remains a challenge, as M83โ€™s distance limits the detail we can observe.โ€

At least one of the odd remnants has an explanationโ€”the debris from SN 1957D, a supernova first seen almost 70 years ago, appears to be colliding with material surrounding it, leading to the increased x-ray emissions. But the cause of the other changing emissions is unclear.

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