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Rogue Planet Caught in Record Growth Spurt, Accreting Like a Young Star

Multi-facility observations reveal magnetic funneling with fleeting water vapor signatures that point to a star-like origin.

Overview

  • The free-floating object Cha 1107-7626, about 5–10 times Jupiter’s mass and roughly 620–630 light-years away, reached a peak accretion rate of around 6 billion metric tons per second in August 2025.
  • The outburst was about eight times stronger than in the preceding months and marks the fastest planet-scale growth ever recorded.
  • Spectra taken from late June through August show hotter, brighter emission and the temporary appearance of water vapor in the surrounding disk that was absent before the burst.
  • Signatures indicate material was funneled along magnetic fields, mirroring rare growth episodes in young stars and informing how some rogue planets may form.
  • Findings draw on ESO’s Very Large Telescope with support from JWST archives and SINFONI, are published in Astrophysical Journal Letters, and follow-up monitoring is planned with archival hints of a similar episode in 2016.