Riemann ellipsoid

E468356

A Riemann ellipsoid is a rotating, self-gravitating fluid mass in ellipsoidal equilibrium whose internal motion and figure are analyzed in Riemann’s extension of classical ellipsoidal models in celestial mechanics.

All labels observed (2)

Label Occurrences
Riemann ellipsoids 3
Riemann ellipsoid canonical 1

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf astrophysical fluid configuration ⓘ
ellipsoidal equilibrium configuration ⓘ
equilibrium figure ⓘ
rotating fluid body ⓘ
self-gravitating fluid mass ⓘ
analyzedUsing ellipsoidal harmonics and tensor methods ⓘ
appearsIn theory of dynamical stability of rotating fluids ⓘ
assumes Newtonian gravity in the standard formulation ⓘ
ideal (non-viscous) fluid in the classical treatment ⓘ
definedBy Riemann’s extension of Dirichlet’s ellipsoidal figures ⓘ
definedIn 19th-century work of Bernhard Riemann on rotating fluid masses ⓘ
equilibriumCondition balance of self-gravity, pressure, and inertial forces ⓘ
ellipsoidal surfaces of constant density and pressure ⓘ
extends classical ellipsoidal models of rotating masses ⓘ
theory of equilibrium figures of rotating fluids ⓘ
generalizes Jacobi ellipsoid ⓘ
Maclaurin spheroid ⓘ
hasComponent centrifugal forces due to rotation ⓘ
pressure gradients in the fluid ⓘ
self-gravity ⓘ
hasInternalMotion linear velocity field in spatial coordinates ⓘ
uniform vorticity in the fluid interior (in Riemann’s construction) ⓘ
hasParameter angular velocity of figure rotation ⓘ
internal vorticity or circulation parameter ⓘ
mass density ⓘ
three principal semi-axes of the ellipsoid ⓘ
total mass ⓘ
hasProperty ellipsoidal figure maintained in time ⓘ
internal fluid motion ⓘ
rotating ⓘ
self-gravitating ⓘ
stationary in a rotating frame ⓘ
time-independent shape in equilibrium ⓘ
uniform density (in the classical model) ⓘ
hasShape ellipsoid ⓘ
triaxial ellipsoid ⓘ
namedAfter Bernhard Riemann ⓘ
relatedTo Dirichlet ellipsoids ⓘ
Poincaré’s theory of rotating fluid masses ⓘ
equilibrium figures of rotating homogeneous masses ⓘ
satisfies Euler equations for an incompressible rotating fluid (in the classical idealization) ⓘ
Poisson equation for the gravitational potential ⓘ
studiedIn astrophysical fluid dynamics ⓘ
celestial mechanics ⓘ
gravitational theory of rotating bodies ⓘ
usedAsModelFor idealized galactic cores ⓘ
rotating gaseous planets ⓘ
rotating stars ⓘ

How these facts were elicited

Referenced by (4)

Full triples — surface form annotated when it differs from this entity's canonical label.

Jacobi ellipsoid → isRelatedTo → Riemann ellipsoid ⓘ
Roche–Riemann ellipsoids → subclassOf → Riemann ellipsoids ⓘ
linked to: Riemann ellipsoid
Roche–Riemann ellipsoids → relatedTo → Riemann ellipsoids ⓘ
linked to: Riemann ellipsoid
Chandrasekhar’s theory of ellipsoidal figures of equilibrium → studies → Riemann ellipsoids ⓘ
linked to: Riemann ellipsoid