We study the Kirchhoff equations for a rigid body immersed in an incom
pressible, irrotational, inviscid fluid in the case that the centers o
f buoyancy and gravity coincide. The resulting dynamical equations for
m a non-canonical Hamiltonian system with a six-dimensional phase spac
e, which may be reduced to a four-dimensional (two-degree-of-freedom,
canonical) system using the two Casimir invariants of motion. Restrict
ing ourselves to ellipsoidal bodies, we identify several completely in
tegrable subcases. In the general case, we analyze existence, linear a
nd nonlinear stability, and bifurcations of equilibria corresponding t
o steady translations and rotations, including mixed modes involving s
imultaneous motion along two body axes, some of which we show can be s
table. By perturbing from the axisymmetric, integrable case, we show t
hat slightly asymmetric ellipsoids are typically non-integrable, and w
e investigate their dynamics with a view to using motions along homo-
and -heteroclinic orbits to execute specific maneuvers in autonomous u
nderwater vehicles. (C) 1998 Elsevier Science B.V.