(120178) 2003 OP32
E468359
(120178) 2003 OP32 is a trans-Neptunian object in the Kuiper Belt, notable as a likely collisional fragment of the dwarf planet Haumea.
Statements (30)
| Predicate | Object |
|---|---|
| instanceOf |
Haumea family member
ⓘ
Kuiper belt object ⓘ collisional fragment ⓘ minor planet ⓘ trans-Neptunian object ⓘ |
| absoluteMagnitude | 4.1 ⓘ |
| albedo | high ⓘ |
| aphelionDistance | approximately 52 AU ⓘ |
| associatedWith | dwarf planet Haumea NERFINISHED ⓘ |
| belongsTo | Solar System NERFINISHED ⓘ |
| belongsToPopulation | outer Solar System small bodies ⓘ |
| discoveredIn | 2003 ⓘ |
| dynamicalClass | classical Kuiper belt object ⓘ |
| eccentricity | approximately 0.13 ⓘ |
| hasColor | neutral ⓘ |
| hasOrbitalResonance | none strong with Neptune ⓘ |
| hasRotation | yes ⓘ |
| inclination | approximately 27 degrees ⓘ |
| likelyOrigin | collision involving Haumea ⓘ |
| locatedIn | Kuiper belt NERFINISHED ⓘ |
| minorPlanetNumber | 120178 ⓘ |
| orbitalPeriod | approximately 310 years ⓘ |
| orbits | Sun ⓘ |
| partOf | Haumea collisional family NERFINISHED ⓘ |
| perihelionDistance | approximately 41 AU ⓘ |
| semiMajorAxis | approximately 46 AU ⓘ |
| similarTo |
Haumea in composition
ⓘ
other Haumea family objects ⓘ |
| spectralType | water-ice rich ⓘ |
| surfaceComposition | water ice ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.