We show how to construct non-spherically-symmetric extended bodies of uniform
density behaving exactly as pointlike masses. These ``gravitational monopoles''
have the following equivalent properties: (i) they generate, outside them, a
spherically-symmetric gravitational potential M/∣x−xO∣; (ii) their
interaction energy with an external gravitational potential U(x) is −MU(xO); and (iii) all their multipole moments (of order l≥1) with
respect to their center of mass O vanish identically. The method applies for
any number of space dimensions. The free parameters entering the construction
are: (1) an arbitrary surface Σ bounding a connected open subset
Ω of R3; (2) the arbitrary choice of the center of mass O within
Ω; and (3) the total volume of the body. An extension of the method
allows one to construct homogeneous bodies which are gravitationally equivalent
(in the sense of having exactly the same multipole moments) to any given body.Comment: 55 pages, Latex , submitted to Nucl.Phys.