
If there were such a thing as a photo album of the universe, it might include snapshots of pancake-like disks of gas and dust, swirling around newly formed stars across the Milky Way. Known as planet-forming disks, they are believed to be a short-lived feature around most, if not all, young stars, providing the raw materials for planets to form.
Most of these planetary nurseries are short-lived, typically lasting only about 10 million years—a fleeting existence by cosmic standards. Now, in a surprising find, researchers at the University of Arizona have discovered that disks can grace their host stars much longer than previously thought, provided the stars are small—one-tenth of the sun’s mass or less.
In a paper published in the Astrophysical Letters Journal, a research tea...
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