Earth–Moon Lagrange region

E1010249

The Earth–Moon Lagrange region comprises the gravitationally stable and semi-stable points in the Earth–Moon system where spacecraft can maintain position with minimal fuel, making it valuable for observation, navigation, and future space infrastructure.

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Statements (45)

Predicate Object
instanceOf Lagrange point system
celestial mechanics region
coordinateFrame rotating frame of Earth–Moon system
definedIn restricted three-body problem
enables continuous observation of Earth–Moon system
long-duration cislunar presence
governedBy Newtonian gravity NERFINISHED
hasApplication future space infrastructure
space navigation
space observation
spacecraft positioning
hasComponent Earth–Moon L1 point NERFINISHED
Earth–Moon L2 point NERFINISHED
Earth–Moon L3 point NERFINISHED
Earth–Moon L4 point NERFINISHED
Earth–Moon L5 point NERFINISHED
hasDynamicalStructure invariant manifolds
hasNumberOfLagrangePoints 5
hasPotentialUse assembly nodes for spacecraft
communication relay hubs
navigation beacons
propellant depots
hasPrimaryBody Earth NERFINISHED
hasProperty contains gravitational equilibrium points
contains semi-stable points
contains stable points
enables low-fuel station-keeping
hasSecondaryBody Moon NERFINISHED
hasSemiStablePoint Earth–Moon L1 point NERFINISHED
Earth–Moon L2 point NERFINISHED
Earth–Moon L3 point NERFINISHED
hasStablePoint Earth–Moon L4 point NERFINISHED
Earth–Moon L5 point NERFINISHED
partOf Earth–Moon system NERFINISHED
relatedTo Sun–Earth Lagrange points NERFINISHED
cislunar space
relevantTo astrodynamics
mission design
space logistics
studiedIn celestial mechanics
space mission analysis
supports Lissajous orbits NERFINISHED
halo orbits
usedFor cislunar space operations
deep-space gateway concepts

Referenced by (1)

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

EQUULEUS CubeSat targetRegion Earth–Moon Lagrange region
subject surface form: EQUULEUS