Study links planet spin to formation history
Astronomers using the W. M. Keck Observatory on Maunakea, Hawai’i, have measured the spins of dozens of giant planets and brown dwarfs orbiting distant stars. Their survey included 32 gas giants and brown dwarf companions, including 6 planets larger than Jupiter and 25 brown dwarf companions. The observations revealed that giant planets can spin faster than much more massive brown dwarfs, challenging simple assumptions about mass and rotation. Researchers believe magnetic interactions early in the objects’ histories may explain the difference, with stronger magnetic fields slowing rotation over time. The findings were published in The Astronomical Journal and led by scientists at Northwestern University’s Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA). The team used the Keck Planet Imager and Characterizer (KPIC) to isolate light from these distant worlds and measure subtle spectral broadening caused by rotation. Lead author Dino Chih-Chun Hsu described spin as a “fossil record” of how a planet formed. The team plans to expand the work by studying free-floating planets and using the upcoming HISPEC instrument, scheduled to begin operations in 2027.
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Sources: ScienceDaily
