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Study Ties ASASSN-24fw’s 200-Day Fade to Ringed Brown Dwarf or Super-Jupiter

A peer-reviewed model identifies a ringed sub-stellar companion as the likely cause.

Overview

  • The F-type star about 3,200 light-years away dimmed by roughly 97% for nearly nine months, making it one of the longest recorded stellar occultations.
  • Analysis of photometric and spectroscopic data favors a companion exceeding three Jupiter masses with optically thick rings extending about 0.17 astronomical units.
  • The modeled saucer-like ring structure accounts for the slow onset of dimming followed by a nearly opaque eclipse.
  • Researchers also identify a nearby red dwarf and signs of circumstellar debris unusually close to this likely older-than–1-billion-year star.
  • Follow-up observations are planned with the Very Large Telescope, the James Webb Space Telescope, and ALMA, and modeling suggests a similar event could recur in about 42–43 years.