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Webb and Hubble Reveal Edge-On ‘Butterfly Star’ Disk With Clear Signs of Dust Settling

The multiwavelength view helps researchers gauge how efficiently grains settle toward the disk’s midplane.

Overview

  • The protostar IRAS 04302+2247 in the Taurus region lies about 525 light-years away with a protoplanetary disk roughly 65 billion kilometers across.
  • Webb’s edge-on perspective shows a thin dark dust lane and twin reflection nebulae that give the object its Butterfly Star nickname.
  • Data from JWST’s NIRCam and MIRI combined with Hubble optical imaging map small-grain distributions and nearby clumps, jets, and outflows.
  • The disk’s measured vertical thickness indicates grains have migrated toward the midplane and settled into a thin, dense layer conducive to planet formation.
  • The observations were released as a Picture of the Month and were gathered under Webb GO program #2562, which studies four edge-on disks to track dust evolution.