In order to get diffraction limited imaging on large telescopes using Laser
Guide Stars one needs to Ire several such artificial beacons angularly dis
placed with respect to the science target. Such displacement scales with th
e diameter of the telescope. It is pointed out that when this angle exceeds
some given figure it can be more efficient to use directly some off-axis N
atural Guide Stars. With realistic assumptions it turns out that next gener
ation giant telescopes could benefit from this technique and could not requ
ire any Laser Guide Star.