(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.
Statements (31)
| Predicate | Object |
|---|---|
| instanceOf |
Kuiper Belt object
ⓘ
minor planet ⓘ small Solar System body ⓘ trans-Neptunian object ⓘ |
| associatedWith | Haumea NERFINISHED ⓘ |
| belongsTo | Haumea family NERFINISHED ⓘ |
| 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 NERFINISHED ⓘ |
| locatedIn | Kuiper Belt NERFINISHED ⓘ |
| orbits | Sun NERFINISHED ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.