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The understanding of the gravitational properties of the quantum vacuum mightbe the next scientific revolution.It was recently proposed that the quantumvacuum contains the virtual gravitational dipoles; we argue that thishypothesis might be tested within the Solar System. The key point is thatquantum vacuum ("enriched" with the gravitational dipoles) induces a retrogradeprecession of the perihelion. It is obvious that this phenomenon mighteventually be revealed by more accurate studies of orbits of planets and orbitsof the artificial Earth satellites. However, we suggest that potentialy thebest "laboratory" for the study of the gravitational properties of the quantumvacuum is the Dwarf Planet Eris and its satellite Dysnomia; the distance ofnearly 100AU makes it the unique system in which the precession of theperihelion of Dysnomia (around Eris) is strongly dominated by the quantumvacuum.

Can observations inside the Solar System reveal the gravitational properties of the quantum vacuum?