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The Star That Shouldn't Exist! đŸŒŸđŸ’„
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126 vues7J'aime41NextLevelFacts-f4ctVersion originale : 2026-05-15

HD 222697 is a 2.7 solar mass star that appears young and bright despite being in a 2.5 billion-year-old star cluster, because it formed from a violent collision between two stars rather than through normal stellar aging; this merger created a hybrid star with a metal-poor surface like a newborn but a metal-rich interior like an old giant, spinning at 180 km per second as evidence of its violent origin, with such collisions occurring roughly once every 1,000 years to rejuvenate star clusters.

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