β Pic b shows coherent sub-percent brightness cycles with a 9.00 ± 0.13 hr period in two JWST bands — interpreted as its rotation — with a spin axis consistent with edge-on viewing and spin-orbit alignment.
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Photometric Variability and Rotation of Beta Pictoris b from JWST NIRCam Coronagraphic Imaging
β Pic b shows coherent sub-percent brightness cycles with a 9.00 ± 0.13 hr period in two JWST bands — interpreted as its rotation — with a spin axis consistent with edge-on viewing and spin-orbit alignment.