Ellipsoid

Definition and stakes

Portrait of Horace Lamb Horace Lamb,  1911 Encyclopædia Britannica, Volume 17… (1911)

“ The ellipsoids (41) and (43) are reciprocal polars with respect to a sphere having O as centre.
If A = B = C, the momental ellipsoid becomes a sphere; all axes through O are then principal axes, and the moment of inertia is the same for each. The mass-system is then said to possess kinetic symmetry about O.
If all the masses lie in a plane (z = 0) we have, in the notation of (25) , c2 = 0, and therefore A = Mb2, B = Ma2, C = M (a2 + b2) , so that the equation of the momental ellipsoid takes the form
b2x2 + a2y2 + (a2 + b2) z2 = ε4.
”
Source: Wikisource

Portrait of Josiah Willard Gibbs Josiah Willard Gibbs,  Scientific Papers of Josiah Willard Gibbs (1906)

“ If the medium is symmetrical with respect to a certain plane, each ellipsoid must have an axis at right angles to that plane. If the medium after a revolution of less than 180° about a certain axis is then equivalent to the medium in its first position, or symmetrical with it with respect to a plane at right angles to that axis, each ellipsoid must have an axis of revolution parallel to that axis. ”
Source: Wikisource

Various,  Encyclopaedia Britannica, 11th Edition…

“ In mechanics, the ellipsoid of gyration or inertia is such that the perpendicular from the centre to a tangent plane is equal to the radius of gyration of the given body about the perpendicular as axis; the “momental ellipsoid,” also termed the “inverse ellipsoid of inertia” or Poinsot’s ellipsoid, has the perpendicular inversely proportional to the radius of gyration; the “equimomental ellipsoid” is such that its moments of inertia about all axes are the same as those of a given body. (See Mechanics.)
ELLIPTICITY, in astronomy, deviation from a circular or spherical form
”
Source: Gutenberg

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