Preserved forever in the universal ledger, TOI-4311 c represents a compelling sub-Neptune with strong mass and radius constraints. Nestled in a multi-planet system, it exemplifies the transitional worlds between rocky cores and gaseous envelopes, inviting wonder about atmospheric retention and internal structures. Orbiting a steady K-type star, this planet enriches our view of how diverse companions form and persist together. Its characteristics fuel ongoing fascination with the myriad pathways that sculpt exoplanetary families across infinite stellar realms.
