ALMA Makes First Observations of a Magnetic Field in a Protoplanetary Disk

ALMA 0.9mm observations of the protoplanetary disk in the HD 142527 system with the magnetic field structure superimposed on the image. Credit: ALMA (ESO/NAOJ/NRAO), S. Ohashi et al.
A research group led by Satoshi Ohashi at the NAOJ have used ALMA Band 3, 4, 6 and 7 data (spanning a wavelength range of 0.87-2.7 mm or a frequency range of 111-345 GHz) to measure polarized thermal dust emission from the protoplanetary disk in the HD 142527 system. This represents the first time that polarized dust emission and hence magnetic fields have been measured within a protoplanetary disk. These results have revealed that the magnetic fields have a complex three-dimensional structure and have also provided valuable data that had been missing from theoretical models of these dust disks. See the press release from ALMA or the paper in Nature Astronomy for more information.
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