Recently, astronomers used radio and optical telescopes to study double planetary disks around binary stars, showing differences in their disks whether they formed together or not.
The collection of material around binary stars, called "protoplanetary disks," formed from raw materials as parent stars.
DF Tau, situated over 400 light-years away in the constellation Taurus, has peculiar characteristics where its ‘double’ planetary disks show distinct differences and only the primary star has an active inner disk.
The research around the system suggests that the dispersal of circumstellar disks is complex and there is more to disk evolution than just time.
Planetary disks are giant wheels spinning in molecular clouds forming planetesimals and ultimately planets.
Finding planetary disks around other stars gives an insight into the early stages of the formation and evolution process.
The survey conducted by the astronomers will shed some light on the process of planetary formation in paired disks and help understand their evolution.
Their data may highlight the individual viscosities of the disks and the presence of a substellar companion carving out gaps around the secondary star to explain the dissipation differences.
Research surrounding the processes of planetary formation and circumstellar evolution should help understand the realms with respect to planet formation.
Checking out more binaries should give us a better understanding of binary star and planet evolution.