  We estimate the rate of tidal disruption events (TDEs) that will be
detectable with future space-based gravitational wave detectors as well as the
most probable properties of these events. We find that the Laser Interferometer
Space Antenna (LISA) will be able to detect up to few 10 events, but this
number will strongly depend on our ability to disentangle the signal from the
noise. The future number of (non-)observation will add additional constraints
on the typical age of stars surrounding central black holes (BHs), however it
will not constrain the unknown regimes of the BH mass function. Most probable
events will involve 10 M$_\odot$ stars around few $10^6$ M$_\odot$ BHs and will
be detectable in the X-ray and optical part of the electromagnetic spectrum,
which may open the multi-messenger era for TDEs. The generation of detectors
following LISA will routinely detect gravitational waves from TDEs at
cosmological distances.
