The number of magnetospheric solar wind charge exchange (SWCX) soft X-ray events detectable with GEO-X was estimated using the latest calibrated ACE/SWICS data on solar wind O 7+ ions. The O VII line flux at a certain solar wind O 7+ flux was calculated from an magnetohydrodynamic simulation of 2001 March 31 geomagnetic storm and scaled to the sum of emission lines from other solar wind ions based on Suzaku magnetospheric SWCX events. The instrumental background including radiation noise mainly due to energetic protons was estimated using GOES >10 MeV proton flux and our previously developed GEANT4 simulation. The number of detectable magnetospheric SWCX events that meet a criterion of signal-to-noise ratios grater than 20 peaks near solar maximum, reaching 49.7 events per year with an average duration of 2.94 hours. Assuming an observation efficiency of 30%, we found that at least one event can be detected within a 4-month time frame with a 90% probability.