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New orbital clue reveals how hot Jupiters really formed

Hot Jupiters were once cosmic oddities, but unraveling how they moved so close to their stars has remained a stubborn mystery. Scientists have long debated whether these giants were violently flung inward or peacefully drifted through their birth disks. A new approach from researchers in Tokyo cracks open this puzzle by using the timescale of orbital circularization as a diagnostic.

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