  We give a summary of the current state of Local Bubble research, resulting
from the discussions of a dedicated panel meeting. After more than 25 years of
intense observational and theoretical work, we are still far from a coherent
picture, although a probable one emerges at the horizon. A multi-supernova
origin seems to be the best guess, with non-equilibrium cooling and soft X-ray
emission accompanying its expansion. In addition our vantage point may force us
to accept a substantial but quantitatively unknown contribution from
heliospheric emission.
