Spin separates giant planets from 'failed stars'
SMRTR summary
Astronomers have long struggled to tell giant planets apart from brown dwarfs — objects too small to become stars but too big to be typical planets. A Northwestern University-led team discovered that spin speed is a key difference: giant planets rotate much faster than brown dwarfs. This likely reflects their different formation processes, offering scientists a powerful new tool for classifying these previously indistinguishable objects.
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