KnowraHill sphereLinked fromLinked fromThe 19 pages that link to Hill sphere, each with the reason it gives.All 19Related 12Narrower topic 1Compared with 6Roche limitCompared with: It concerns gravitational control of orbiting objects, not whether a satellite is torn apart.Lagrange pointCompared with: It describes a body's gravitational domain, not a force-balance location in the rotating frame.Tidal interactionCompared with: It concerns orbital stability, unlike the internal deformation central to tidal interaction.Tidal strippingRelated: Material beyond this gravitational domain is especially vulnerable to removal.Restricted three-body problemRelated: Its boundaries approximate where a small body can remain bound to one primary.Natural satelliteRelated: A satellite generally must orbit within its primary's Hill sphere to remain bound.Roche lobeCompared with: It describes gravitational dominance in a different orbital setup, not the binary equipotential boundary.Trojan asteroidRelated: A planet’s Hill sphere helps set the scale of its gravitational influence on nearby co-orbitals.Galactic tideCompared with: It describes a related gravitational boundary, usually for a body orbiting another body.ExomoonRelated: An exomoon must orbit within its planet's region of gravitational dominance.Irregular satelliteNarrower topic: A planet can retain distant satellites only within the gravitational domain set by its Hill sphere.Moons of JupiterRelated: It helps explain the space within which Jupiter can keep moons in orbit.Space rendezvousRelated: Near a target, its local gravitational influence helps frame relative motion and approach behavior.Horseshoe orbitRelated: Close encounters and orbital reversals depend on the scale of each co-orbital body's gravitational influence.Tisserand parameterCompared with: The parameter describes global orbital constraints, not the spatial boundary of a planet's gravitational influence.Moon (astronomy)Related: A planet’s Hill sphere constrains the orbits in which its moons can remain bound.ProtoplanetRelated: It approximates the region from which a protoplanet can gravitationally gather material.Dermott's lawRelated: The size and stability limits of a satellite system constrain which orbital spacings are possible.Minor-planet moonRelated: A moon must remain within its minor planet's gravitational domain despite solar perturbations.
KnowraHill sphereLinked fromLinked fromThe 19 pages that link to Hill sphere, each with the reason it gives.All 19Related 12Narrower topic 1Compared with 6Roche limitCompared with: It concerns gravitational control of orbiting objects, not whether a satellite is torn apart.Lagrange pointCompared with: It describes a body's gravitational domain, not a force-balance location in the rotating frame.Tidal interactionCompared with: It concerns orbital stability, unlike the internal deformation central to tidal interaction.Tidal strippingRelated: Material beyond this gravitational domain is especially vulnerable to removal.Restricted three-body problemRelated: Its boundaries approximate where a small body can remain bound to one primary.Natural satelliteRelated: A satellite generally must orbit within its primary's Hill sphere to remain bound.Roche lobeCompared with: It describes gravitational dominance in a different orbital setup, not the binary equipotential boundary.Trojan asteroidRelated: A planet’s Hill sphere helps set the scale of its gravitational influence on nearby co-orbitals.Galactic tideCompared with: It describes a related gravitational boundary, usually for a body orbiting another body.ExomoonRelated: An exomoon must orbit within its planet's region of gravitational dominance.Irregular satelliteNarrower topic: A planet can retain distant satellites only within the gravitational domain set by its Hill sphere.Moons of JupiterRelated: It helps explain the space within which Jupiter can keep moons in orbit.Space rendezvousRelated: Near a target, its local gravitational influence helps frame relative motion and approach behavior.Horseshoe orbitRelated: Close encounters and orbital reversals depend on the scale of each co-orbital body's gravitational influence.Tisserand parameterCompared with: The parameter describes global orbital constraints, not the spatial boundary of a planet's gravitational influence.Moon (astronomy)Related: A planet’s Hill sphere constrains the orbits in which its moons can remain bound.ProtoplanetRelated: It approximates the region from which a protoplanet can gravitationally gather material.Dermott's lawRelated: The size and stability limits of a satellite system constrain which orbital spacings are possible.Minor-planet moonRelated: A moon must remain within its minor planet's gravitational domain despite solar perturbations.