Researchers believe a gigantic ring system surrounding a brown dwarf or super-Jupiter could have blocked the star's light, causing an extremely rare fading star phenomenon. The dimming lasted nearly 200 days, making it one of the longest ever observed.
SourceRoyal Astronomical Society·JournalMonthly Notices of the Royal Astronomical Society·DateFeb 11, 2026
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Researchers at the University of Washington have discovered a unique binary star system where a small companion star is surrounded by a large disk of dusty material. The companion star caused a seven-year-long eclipse of the main star, Gaia17bpp, which is one of the longest recorded eclipses.
A University of Sydney graduate student has reconstructed images of the star CW Leo, which appears to be a changing 'inkblot pattern' due to dust and gas ejections. The star's appearance evolved over eight years, revealing it is not buried under its own dust as previously thought.
SourceUniversity of Sydney·JournalMonthly Notices of the Royal Astronomical Society·DateDec 3, 2015
A team of researchers from MIT has detected optical features around Chiron that may signal the presence of a ring system, jets, or a shell of dust. The findings are based on observations of a stellar occultation in 2011, which revealed symmetrical and sharp features near the start and end of the event.
SourceMassachusetts Institute of Technology·JournalIcarus·DateMar 16, 2015
A team of astronomers from MIT and Williams College observed the light from a star as it disappeared behind Charon and reappeared on the other side. They determined Charon's radius to be 606 ± 8 km, roughly twice the width of Massachusetts, and established a density of 1.72 g/cm3.