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High-energy astrophysical neutrinos, discovered by IceCube, are now regularlyobserved, albeit at a low rate due to their low flux. As a result, openquestions about high-energy neutrino astrophysics and particle physics remainlimited by statistics at best, or unanswered at worst. Fortunately, thissituation will improve soon: in the next few years, a host of new neutrinotelescopes, currently under planning and construction, will come online. It isnatural to combine their collected observing power: we propose the PlanetaryNeutrino Monitoring System (PLE$\nu$M), a concept for a global repository ofhigh-energy neutrino observations, in order to finally give firm answers toopen questions. PLE$\nu$M will reach up to four times the exposure availabletoday by combining the exposures of current and future neutrino telescopesdistributed around the world -- IceCube, IceCube-Gen2, Baikal-GVD, KM3NeT, andP-ONE. Depending on the declination and spectral index, PLE$\nu$M will improvethe sensitivity to astrophysical neutrinos by up to two orders of magnitude. Wepresent first estimates on the capability of PLE$\nu$M to discover Galactic andextragalactic sources of astrophysical neutrinos and to characterize thediffuse flux of high-energy neutrinos in unprecedented detail.

PLE$\nu$M: A global and distributed monitoring system of high-energy astrophysical neutrinos