Unusual planet configurations in binary star systems may arise from material transfer during white dwarf formation or from orbital destabilization effects.
Unusual planet configurations in binary star systems may arise from material transfer during white dwarf formation or from orbital destabilization effects.
A retrograde planet in a tight binary star system with a white dwarf
In binary systems, the interactions between stars and their surrounding disks significantly influence the dynamics of planet formation, particularly through resonances and disk gap sizes.