Scientists studying the origins of planetary systems have found that protoplanetary discs are often warped, overturning the traditional view of smooth, flat discs. The findings, published in the Astrophysical Journal Letters, show that these subtle tilts can significantly influence how planets grow and establish orbits.
The research team, using the Atacama Large Millimetre/submillimetre Ar by Sophie Jenkins
London, UK (SPX) Sep 01, 2025
Scientists studying the origins of planetary systems have found that protoplanetary discs are often warped, overturning the traditional view of smooth, flat discs. The findings, published in the Astrophysical Journal Letters, show that these subtle tilts can significantly influence how planets grow and establish orbits.
The research team, using the Atacama Large Millimetre/submillimetre Array (ALMA) as part of the exoALMA programme, discovered that many discs tilt by just half a degree to two degrees. These small misalignments resemble the inclinations between planets in our Solar System, suggesting that planetary birth environments may be more chaotic than once believed.
"Our results suggest that protoplanetary discs are slightly warped. This would be quite a change in how we understand these objects and has many consequences for how planets form. Particularly interesting is that the couple of degree warping is similar to the differences in inclination between our own Solar System planets," said Dr Andrew Winter of Queen Mary University of London.
Dr Myriam Benisty of the Max Planck Institute for Astronomy added, "exoALMA has revealed large scale structures in the planet forming discs that were completely unexpected. The warp-like structures challenge the idea of orderly planet formation and pose a fascinating challenge for the future."
The team analysed Doppler shifts in radio emissions from carbon monoxide gas, mapping motion within the discs with high precision. Careful modelling showed different regions of each disc tilted relative to one another, exposing the warps. These distortions can explain spiral patterns, turbulence, temperature variations and other large-scale gas motions observed across the discs.
Researchers believe the warps may be linked to how much material the young star accretes at its centre, pointing to a connection between stellar feeding and planet-forming regions. They could also result from gravitational forces of unseen stellar companions or dynamic interactions in the gas and dust.
The discovery provides new insight into how turbulence and mass transport in discs shape planetary formation. It challenges the notion of serene, flat nurseries for new worlds and offers a more dynamic blueprint for the creation of diverse planetary systems.
Research Report:exoALMA XVIII. Interpreting large scale kinematic structures as moderate warping
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