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We suggest that major Luminous Blue Variable (LBV) eruptions are a result ofa periastron passage interaction with the secondary star. The interaction musttake place when the primary envelope is in an unstable phase. In our model themass transferred to the secondary accounts for the energy and light curve ofthe eruption. We propose that all major LBV eruptions are triggered by stellarcompanions, and that in extreme cases a short duration event with a huge masstransfer rate can lead to a bright transient event on time scales of weeks tomonths (a `supernova impostor')

LBV Eruptions Triggered and Powered by Binary Interaction