Jacobi ellipsoid

A Jacobi ellipsoid is a triaxial (i.e. scalene) ellipsoid under hydrostatic equilibrium which arises when a self-gravitating fluid body of uniform density rotates with a constant angular velocity. It is named after the German mathematician Carl Gustav Jacob Jacobi.
History.
Before Jacobi, the Maclaurin spheroid, which was formulated in 1742, was considered to be the only type of ellipsoid which can be in equilibrium. Lagrange in 1811 considered the possibility of a tri-axial ellipsoid being in equilibrium, but concluded that the two equatorial axes of the ellipsoid must be equal, leading back to the solution of Maclaurin spheroid. But Jacobi realized that Lagrange's demonstration is a sufficiency condition, but not necessary. He remarked:
"One would make a grave mistake if one supposed that the spheroids of revolution are the only admissible figures of equilibrium even under the restrictive assumption of second degree surfaces" (...) "In fact a simple consideration shows that ellipsoids with three unequal axes can very well be figures of equilibrium; and that one can assume an ellipse of arbitrary shape for the equatorial section and determine the third axis (which is also the least of the three axes) and the angular velocity of rotation such that the ellipsoid is a figure of equilibrium."
Jacobi formula.
For an ellipsoid with equatorial semi-principal axes formula_1 and polar semi-principal axis formula_2, the angular velocity formula_3 about formula_2 is given by
where formula_6 is the density and formula_7 is the gravitational constant, subject to the condition
For fixed values of formula_9 and formula_10, the above condition has solution for formula_2 such that 
The integrals can be expressed in terms of incomplete elliptic integrals. In terms of the Carlson symmetric form elliptic integral formula_13, the formula for the angular velocity becomes
and the condition on the relative size of the semi-principal axes formula_15 is
The angular momentum formula_17 of the Jacobi ellipsoid is given by
where formula_19 is the mass of the ellipsoid and formula_20 is the "mean radius", the radius of a sphere of the same volume as the ellipsoid.
Relationship with Dedekind ellipsoid.
The Jacobi and Dedekind ellipsoids are both equilibrium figures for a body of rotating homogeneous self-gravitating fluid. However, while the Jacobi ellipsoid spins bodily, with no internal flow of the fluid in the rotating frame, the Dedekind ellipsoid maintains a fixed orientation, with the constituent fluid circulating within it. This is a direct consequence of Dedekind's theorem.
For any given Jacobi ellipsoid, there exists a Dedekind ellipsoid with the same semi-principal axes formula_15 and same mass and with a flow velocity field of
where formula_23 are Cartesian coordinates on axes formula_24 aligned respectively with the formula_15 axes of the ellipsoid. Here formula_26 is the vorticity, which is uniform throughout the spheroid (formula_27). The angular velocity formula_3 of the Jacobi ellipsoid and vorticity of the corresponding Dedekind ellipsoid are related by
That is, each particle of the fluid of the Dedekind ellipsoid describes a similar elliptical circuit in the same period in which the Jacobi spheroid performs one rotation.
In the special case of formula_30, the Jacobi and Dedekind ellipsoids (and the Maclaurin spheroid) become one and the same; bodily rotation and circular flow amount to the same thing. In this case formula_31, as is always true for a rigidly rotating body.
In the general case, the Jacobi and Dedekind ellipsoids have the same energy, but the angular momentum of the Jacobi spheroid is the greater by a factor of