Ten years after Tabby's Star's mysterious dips were traced to paradoxical dust, a tentative TESS detection of a possible super-Jupiter "dust maker" may soon be confirmed by Gaia data, validating the comet swarm hypothesis.
This episode marks ten years since the discovery of Tabby's Star (KIC 8462852), whose wildly irregular light dips—at times blocking up to 20% of its starlight—ruled out planets as the cause and fueled a decade of speculation ranging from comet swarms to alien megastructures. Dust was confirmed as the dimming culprit in 2018 through its chromatic signature, but this created a paradox: stellar radiation pressure should sweep away or destroy dust around a star like Tabby's, which fits neither young-star nor old-star categories where dust is normally seen. The leading solution invokes swarms of comets continually supplying fresh dust, flung toward the star by some massive hidden gravitational disruptor. A new paper now proposes that TESS caught the "dust maker" itself—a single, highly symmetric dip blocking about 1.1% of the star's light over roughly 20 hours, matching a giant planet on a ~3.3-year orbit at about 2.5 times Earth's distance, some 70% larger than Jupiter. Tentative spectroscopic analysis hints at a super-Jupiter of around ten Jupiter masses, though at only 2.3 sigma significance the detection remains far from confirmed and requires more radial velocity data. Confirmation may come soon, as December's Gaia astrometry release is expected to reveal the object's wobble, which would largely validate the evaporating comet swarm hypothesis. The episode closes by promoting PBS Eons' new TV series, Eons: Life and Death on Pangea, chronicling the supercontinent era and Earth's greatest mass extinction.
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