Jacobi ellipsoid

E105603

A Jacobi ellipsoid is a rotating, self-gravitating fluid body in equilibrium that takes on a triaxial ellipsoidal shape due to its rapid spin.

All labels observed (1)

Label Occurrences
Jacobi ellipsoid canonical 5

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf equilibrium figure ⓘ
rotating fluid body ⓘ
self-gravitating body ⓘ
triaxial ellipsoid ⓘ
belongsToFamily Roche–Riemann ellipsoids ⓘ
differsFrom Maclaurin spheroid by having three unequal axes ⓘ
fieldOfStudy astrophysics ⓘ
celestial mechanics ⓘ
fluid dynamics ⓘ
gravitational physics ⓘ
generalizes Maclaurin spheroid ⓘ
hasApplication constraining densities of small Solar System bodies ⓘ
interpreting light curves of elongated asteroids ⓘ
hasAxisConfiguration three unequal principal axes ⓘ
hasEquilibriumCondition balance between centrifugal force and self-gravity ⓘ
hasForceBalance gradient of total potential equals zero on surface ⓘ
hasHistoricalContext 19th-century mathematical physics ⓘ
hasLimitingCase Maclaurin spheroid at lower rotation ⓘ
hasMathematicalDescription ellipsoidal figure with constant density and uniform rotation ⓘ
hasParameter angular velocity ⓘ
axis ratio a:b:c ⓘ
mass density ⓘ
hasPotential gravitational potential satisfying Poisson equation ⓘ
hasProperty hydrostatic equilibrium ⓘ
rapid rotation ⓘ
rigid-body rotation ⓘ
self-gravity dominated ⓘ
uniform density ⓘ
hasShape triaxial ellipsoid ⓘ
hasSymmetry no rotational symmetry about any principal axis ⓘ
isDiscussedIn theory of figures of equilibrium of rotating masses ⓘ
isExampleOf self-consistent rotating equilibrium configuration ⓘ
isNamedAfter Carl Gustav Jacob Jacobi ⓘ
isRelatedTo Chandrasekhar’s theory of ellipsoidal figures of equilibrium ⓘ
Riemann ellipsoid ⓘ
Roche ellipsoid ⓘ
isSolutionOf equations of rotating self-gravitating fluid equilibrium ⓘ
isStableFor certain ranges of angular velocity ⓘ
isUnstableFor sufficiently high rotation rates ⓘ
occursAt higher angular momentum than Maclaurin spheroid ⓘ
requiresAssumption barotropic equation of state ⓘ
inviscid fluid ⓘ
usedToModel rapidly rotating planets ⓘ
rapidly rotating stars ⓘ
rotating asteroids ⓘ
rotating minor planets ⓘ

How these facts were elicited

Referenced by (5)

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

Haumea → equilibriumFigure → Jacobi ellipsoid ⓘ
Maclaurin spheroid → relatedTo → Jacobi ellipsoid ⓘ
Roche–Riemann ellipsoids → generalizes → Jacobi ellipsoid ⓘ
Riemann ellipsoid → generalizes → Jacobi ellipsoid ⓘ
Roche ellipsoid → generalizationOf → Jacobi ellipsoid ⓘ