Produced by: Mohsin Shaikh
Material from rocky planets is evaporating, creating comet-like tails as seen by JWST.
BD+05 4868 Ab displays twin dust tails, one leading and one trailing, formed by diverse grain sizes.
Planets like K2-22b lose material rapidly, leaving behind silicate and even mantle gases.
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BD+05 4868 Ab is evaporating at a moon’s mass every million years, nearing complete destruction.
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The brightest host star yet, BD+05 4868 A offers new data on disintegrating planets.
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Nitric oxide and carbon dioxide were surprisingly detected, more common in icy comets than rocky planets.
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Unique asymmetric transits reveal volatile planets with extended tails blocking starlight.
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Disintegrating planets showcase their interiors, providing insights into terrestrial evolution.
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JWST’s precision will further probe BD+05 4868 A and redefine what we know of planetary death.