This research extends the Eclipse-Yarkovsky effect theory to exoplanet circumplanetary dust disks, developing numerical simulations and predicting observable signatures for next-gen facilities. The study identifies dynamical regimes where the EY effect alters CPD morphology, addressing gaps in exoplanet disk dynamics.
Key findings
The Eclipse-Yarkovsky effect can significantly alter circumplanetary dust disk morphology.
Three dynamical regimes are identified where the EY effect is prominent.
The research establishes predictive capabilities for observational campaigns targeting exomoon formation environments.
Limitations & open questions
The application of the EY effect to exoplanets has not been systematically explored.
Further numerical simulations and observational data are needed for validation.