(2003) SQ317

E468365

(2003) SQ317 is a small trans-Neptunian object in the Kuiper Belt, notable as a likely collisional fragment associated with the dwarf planet Haumea.

All labels observed (1)

Label Occurrences
(2003) SQ317 canonical 1

How this entity was disambiguated

Statements (31)

Predicate Object
instanceOf Kuiper Belt object ⓘ
minor planet ⓘ
small Solar System body ⓘ
trans-Neptunian object ⓘ
associatedWith Haumea ⓘ
belongsTo Haumea family ⓘ
hasAlbedo high (Haumea-family-like, inferred) ⓘ
hasCategory icy body ⓘ
outer Solar System object ⓘ
hasDiscoveryStatus numbered minor planet ⓘ
hasDiscoveryYear 2003 ⓘ
hasDynamicalClass classical Kuiper Belt object ⓘ
non-resonant trans-Neptunian object ⓘ
hasEnvironment outer Kuiper Belt ⓘ
hasObservationStatus observed at multiple oppositions ⓘ
hasOrbitalCharacteristic heliocentric orbit beyond Neptune ⓘ
low inclination (Haumea-family-like, approximate) ⓘ
moderate eccentricity (approximate) ⓘ
hasOrbitalRegion trans-Neptunian region ⓘ
hasOrigin collisional breakup of proto-Haumea (hypothesized) ⓘ
hasPhysicalProperty elongated shape (inferred from light curve, approximate) ⓘ
small size compared to major Kuiper Belt objects ⓘ
hasRelation dynamically linked to Haumea collisional family ⓘ
hasScientificInterest constrains composition of Haumea progenitor body ⓘ
tests models of Haumea collisional family formation ⓘ
hasSpectralType water-ice-dominated spectrum (inferred) ⓘ
hasSurfaceComposition water ice (inferred) ⓘ
is likely collisional fragment of Haumea family ⓘ
isPartOf Solar System ⓘ
locatedIn Kuiper Belt ⓘ
orbits Sun ⓘ

How these facts were elicited

Referenced by (1)

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

Haumea family → hasMember → (2003) SQ317 ⓘ