Overview
- The planet, WISPIT 2b, orbits a young sun-like star about 430 light years away, sits in a disk gap at roughly 56 astronomical units, and is estimated to be about 5 million years old.
- ESO’s Very Large Telescope captured the object in near-infrared light, while a University of Arizona instrument detected hydrogen-alpha emission in visible light that signals ongoing gas accretion.
- Researchers report the first unambiguous planet detection within a multi-ringed protoplanetary disk, with the surrounding disk extending to about 380 astronomical units and the source confirmed as co-moving with the star.
- The finding arose from a five-year snapshot survey led by teams at Leiden University, the University of Galway, and the University of Arizona, with results published in The Astrophysical Journal Letters.
- Outlets differ on the planet’s mass, describing it as Jupiter-like or several times more massive, and teams plan follow-up spectroscopy and monitoring, with Arizona researchers also noting a second candidate inside the disk’s inner cavity.