Planetary systems are built by planets and planetesimals formed in circumstellar disks surrounding young pre-main sequence stars. Once in the main-sequence collisions of planetesimals produce small dust particles giving rise to the so-called debris disks. The mutual interaction among planets, planetesimals and debris disks, and with their host stars determines the fate of planetary systems.

    Currently thousands of main-sequence stars are known to host planets and
    debris disks. The Solar System with its peculiarities is just one of
    such planetary systems. However, only few tens of stars are known to
    host simultaneously both planets and debris disks. Therefore, the
    study of those systems is particularly valuable to widen our knowledge
    of planetary systems and their evolution.

    This page just collects some of the properties of the known, to our knowledge,
     solar-type stars hosting both planets and debris disk.