  Direct detection and characterization of Earth-like planets around Sun-like
stars is a core task for evaluating the prevalence of habitability and life in
the Universe. Here, we discuss a promising option for achieving this goal,
which is based on placing an occulter in orbit and having it project its shadow
onto the E- ELT at the surface of Earth, thus providing a sufficient contrast
for imaging and taking spectra of Earth-like planets in the habitable zones of
Sun-like stars. Doing so at a sensible fuel budget will require tailored
orbits, an occulter with a high area-to-mass ratio, and appropriate
instrumentation at the E-ELT. In this White Paper, submitted in response to the
ESA Voyage 2050 Call, we outline the fundamental aspects of the concept, and
the most important technical developments that will be required to develop a
full mission.
