Orbit and dynamics
Between its closest point (1.296 AU) and its farthest (219,400 AU), the heliocentric distance changes by 219,399 AU over every revolution.
One full revolution takes 36,333,726 yr (13,270,893,562 days), computed from the semi-major axis of 109,700 AU.
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 27.74° carries it well above and below the ecliptic plane.
Size and surface
Neither a measured diameter nor a reliable absolute magnitude is available for MOSS, so its physical size remains unconstrained.
Observation record and orbit quality
Astrometry from 627 individual observations underpins this orbit; the fit leaves an RMS residual of 0.7074 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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