Produced by: Mohsin Shaikh
New analysis suggests Jupiter-like exoplanets formed in just 1–2 million years—half the time scientists once believed, challenging the slow-build model of planetary evolution.
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Gas giants appear to gather mass in the very earliest stages of a protoplanetary disk, when solids and gases are still plentiful—far earlier than previous models proposed.
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Researchers used atmospheric metallicity to decode accretion history. High levels of heavy elements indicate rapid, early formation when solid material was most abundant.
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Researchers studied just seven gas giants, yet all pointed to massive solid accretion—each planet formed from the equivalent of 50 Earth masses of solids.
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These findings align with emerging evidence about our own solar system: Jupiter likely formed earlier than expected, shifting the timing models for all giant planets.
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Theories built on “core accretion” now face serious questions. If planets form faster, current frameworks must adapt—or be replaced.
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Gas giants don't just grow—they reshape. Their early formation impacts the positioning and size of rocky planets, possibly even pushing Mercury and shrinking Mars.
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The study introduces a statistical framework to estimate solid accretion in exoplanets—potentially unlocking clues about countless other worlds.
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All data used was archival. But with tools like the James Webb Space Telescope, future studies could validate and expand these early formation patterns.