Produced by: Manoj Kumar
Sub-Neptunes—mysterious, gassy planets—are the most common in our galaxy, yet none orbit our Sun.
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Until now, their thick, hazy atmospheres blocked chemical readings, leaving scientists puzzled.
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NASA’s James Webb Telescope pierced the haze of TOI-421 b, revealing detailed atmospheric data.
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At 1,340°F, TOI-421 b’s heat may burn off haze—finally exposing its molecular makeup.
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Water vapor, carbon monoxide, and sulfur dioxide were detected—revealing a chemical fingerprint.
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Scientists were stunned to find TOI-421 b’s atmosphere dominated by hydrogen—unlike other sub-Neptunes.
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This unique composition hints at different evolutionary paths among sub-Neptunes across the galaxy.
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Why don’t these common exoplanets exist in our solar system? Webb’s findings bring us closer to answers.
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Hotter sub-Neptunes may be the key to unlocking atmospheric secrets and classifying unknown planets.
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