Neptune's regular inner satellites

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Neptune's regular inner satellites are a closely packed group of small, faint moons orbiting near the planet, shaped and influenced by its strong gravitational and ring system dynamics.

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Statements (44)

Predicate Object
instanceOf astronomical object group
group of natural satellites
associatedWith Neptune's ring arcs NERFINISHED
discoveredBy Voyager 2 NERFINISHED
dynamicallyInteractsWith Neptune's rings NERFINISHED
hasComposition likely water ice and rock mixture
hasDynamicalRole confinement of ring arcs
shepherding of ring material
hasEnvironment strong Neptunian radiation and magnetospheric environment
hasExplorationStatus no dedicated orbiter mission as of 2024
only briefly imaged by Voyager 2 in 1989
hasNamingTheme Greek sea deities
hasObservationChallenge faintness and proximity to bright Neptune
small angular separation from Neptune in the sky
hasOrbitalCharacteristic closely packed orbits
low orbital inclinations
nearly circular orbits
prograde orbits
short orbital periods
hasOrbitalRegion inside Proteus's orbit
inside Triton's orbit
hasOrbitalStability long-term stability affected by mutual perturbations
hasPhysicalProperty faint brightness
irregular shapes
low albedo
small size
hasPopulation six known moons
hasScientificInterest constraints on Neptune's ring origin
study of ring–moon interactions
study of tidal evolution in the Neptunian system
influencedBy Neptune's gravitational field
Neptune's ring system dynamics
mutual gravitational interactions
locatedIn inner Neptunian system
member Despina NERFINISHED
Galatea NERFINISHED
Hippocamp NERFINISHED
Larissa NERFINISHED
Naiad NERFINISHED
Thalassa NERFINISHED
observedBy Hubble Space Telescope NERFINISHED
ground-based telescopes with adaptive optics
orbits Neptune NERFINISHED
partOf Neptunian satellite system NERFINISHED

Referenced by (1)

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

Despina belongsTo Neptune's regular inner satellites