Metallic Disk Around Hidden Companion Dims a Sun-like Star

A Sun-like star J0705+0612 dramatically dimmed between September 2024 and May 2025 due to a giant, metal-rich cloud about 1.2 billion miles from the star. The cloud appears bound to a distant companion with a few Jupiter masses—potentially a brown dwarf, giant planet, or low-mass star—carrying a circumsecondary or circumplanetary disk. Gas moves with winds of metals such as calcium and iron, measured with the GHOST spectrograph, indicating a dynamic debris disk around the companion. The star is ~3,000 light-years away, and infrared excess suggests a disk in an older system, implying a late-stage collision may have produced the cloud. This rare observation shows mature planetary systems can experience dramatic, disk-driven obscurations.