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The next generation magnetic spectrometer in space, AMS-100, is designed tohave a geometrical acceptance of $100\,\mathrm{m}^2\,\mathrm{sr}$ and to beoperated for at least ten years at the Sun-Earth Lagrange Point 2. Compared toexisting experiments, it will improve the sensitivity for the observation ofnew phenomena in cosmic rays, and in particular in cosmic antimatter, by atleast a factor of 1000. The magnet design is based on high temperaturesuperconductor tapes, which allow the construction of a thin solenoid with ahomogeneous magnetic field of 1 Tesla inside. The inner volume is instrumentedwith a silicon tracker reaching a maximum detectable rigidity of 100 TV and acalorimeter system that is 70 radiation lengths deep, equivalent to fournuclear interaction lengths, which extends the energy reach for cosmic-raynuclei up to the PeV scale, i.e. beyond the cosmic-ray knee. Covering most ofthe sky continuously, AMS-100 will detect high-energy gamma rays in thecalorimeter system and by pair conversion in the thin solenoid, reconstructedwith excellent angular resolution in the silicon tracker.

AMS-100: The Next Generation Magnetic Spectrometer in Space -- An International Science Platform for Physics and Astrophysics at Lagrange Point 2