Orbit and dynamics
The path is an ellipse reaching 4.349 AU from the Sun at perihelion and 483,000 AU at aphelion, a radial span of 482,996 AU.
Applying Kepler's third law to a = 241,500 AU gives an orbital period of 118,679,499 yr, or about 43,347,686,844 days.
The high eccentricity (1) produces a strongly elongated orbit, so the object spends most of its time far from the Sun.
A steep inclination of 126.5° carries it well above and below the ecliptic plane.
Size and surface
Neither a measured diameter nor a reliable absolute magnitude is available for PANSTARRS, so its physical size remains unconstrained.
Observation record and orbit quality
The current orbit solution is based on 924 observations and has a weighted RMS residual of 0.6054 arcseconds.
About these computed values
Orbital periods, perihelion and aphelion speeds, and diameter estimates on this page are computed by SpaceAtlas from the JPL SBDB orbital elements. They are derived quantities, not values copied from the source catalogue.
Orbital Parameters
3D orbit (interactive)
Drag to rotate; scroll or pinch to zoom. The Sun is at the focus (orange), Earth's orbit is the grey ring at 1 AU, and the red dot marks the object's current position.
Close approaches
No close approaches to Earth are currently on record for this object.
Physical Parameters
Orbit Quality
Related Objects
Same object type
Similar orbit
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