The French-Italian collaboration VIRGO is presently building an interf
erometric gravitational wave detector aimed at measuring spectral stra
ins in vacuo as small as 10(-23)/root Hz in the bandwidth 5 - 10(4)Hz.
Elimination of thermal noise effects poses new challenges to internal
friction experts. VIRGO requirements and strategies are outlined here
with the purpose of stimulating discussion, advice and, possibly, col
laboration.