Preferred mechanism of planet formation
Determine whether core accretion or gravitational instability is the preferred mechanism of planet formation in young planetary systems, focusing on establishing which scenario best explains observational evidence from directly imaged planets and protoplanets.
References
Direct imaging provides then a whole picture of a newly formed system, giving the opportunity to investigate which is the preferred mechanism of planet formation, a debate that still remains open.
Another possibility is that the observed GEMS are the result of disk fragmentation (A. P. Boss 2006; A. P. Boss & S. Kanodia 2023), although the efficiency of this mechanism around low-mass stars remains unconstrained.
How these substellar companions form and how their formation pathways differ from exoplanets is still a major question in astronomy.