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Astronomers Unveil Disintegrating Exoplanet with Record-Breaking Dust Tail

MIT researchers using NASA's TESS have identified BD+05 4868 Ab, a rocky planet evaporating into a 9-million-kilometer mineral tail, with plans for JWST observations to analyze its composition.

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Overview

  • BD+05 4868 Ab, located 140 light-years away in the Pegasus constellation, is rapidly disintegrating due to extreme proximity to its star, completing an orbit every 30.5 hours.
  • The planet's surface, heated to nearly 3,000 °F, is covered in molten magma that evaporates into space, forming the longest known comet-like tail of mineral dust at 9 million kilometers.
  • Each orbit causes the planet to lose a Mount Everest’s worth of material, with researchers predicting complete disintegration in 1–2 million years.
  • The discovery, made using NASA's TESS, marks BD+05 4868 Ab as the fourth known disintegrating exoplanet, with the most catastrophic evaporation rate and deepest transit signals observed.
  • Upcoming James Webb Space Telescope observations aim to analyze the mineral composition of the planet's dust trail, offering insights into rocky planet interiors and formation processes.