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ApJS · 7 DAYS AGO
DiscoveriesNEW OBSERVATION

Stellar Factories Found Making Rare Elements

By Space.Fan Editorial Desk

Astronomers discovered that dying stars in nearby galaxies are churning out heavy metals through a unique cosmic process.

A colorful nebula with a planet and moon in the foreground.
Image · Space.Fan

The Drop

When s like our Sun reach the end of their lives, they shed their outer layers, creating beautiful glowing clouds called ary nebulae. Scientists used a powerful tool called IGRINS on the Gemini South telescope to get a closer look at 12 of these clouds in galaxies near our own. By studying the light coming from these s, they found secret stashes of rare elements like rubidium, cadmium, and tellurium. These materials are created inside s during a special process called the s-process, which happens when atoms capture tiny particles called neutrons. This study is the first time these specific elements have been spotted in ary nebulae outside of our own galaxy. The team found that some of these dying s had up to 50 times more of these heavy elements than scientists expected to see. By comparing what they saw with computer models, the researchers were able to see which s are the best at acting like cosmic chemical factories.
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Why It Matters

Understanding how s build elements is like putting together a giant puzzle of how the universe is made. By tracking these heavy metals, scientists can figure out how the material for new s and s is recycled across galaxies. This data helps experts refine their models of how s grow, change, and eventually die over billions of years.
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The Catch

While the team found many interesting results, they could not explain every they looked at. Some of the s they studied did not match any of the current computer predictions, especially those with very low amounts of metal. This means scientists still have more work to do to fully understand the complicated mixing and cooling that happens inside an aging .

Put That in Perspective

Scientists are using these findings to bridge the gap between our understanding of stars in our own Milky Way and those in smaller, neighboring galaxies. Next, they plan to use these measurements to better map out the chemical history of the entire universe.

Source September 19, 2026
ApJS

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