Orbit and dynamics
Between its closest point (1.148 AU) and its farthest (2.026 AU), the heliocentric distance changes by 0.878 AU over every revolution.
One full revolution takes 2.00 yr (730 days), computed from the semi-major axis of 1.587 AU.
An eccentricity of 0.277 makes the orbit moderately elongated.
The orbital plane is tilted 17.24° relative to the ecliptic.
By the vis-viva equation its orbital speed rises to 31.4 km/s at perihelion and falls to 17.8 km/s at aphelion.
Its perihelion lies just outside Earth's orbit, which is why it is classed as Earth-approaching rather than Earth-crossing.
Size and surface
The measured diameter is 1.96 km, a value from direct size determination rather than from brightness alone.
A geometric albedo of 0.105 points to a comparatively bright, reflective surface.
Observation record and orbit quality
Astrometry from 1,971 individual observations underpins this orbit; the fit leaves an RMS residual of 0.5661 arcseconds.
Condition code U = 0 means the orbit is very well determined, leaving only a small uncertainty in the future ephemeris.
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
Orbit diagram
The Sun sits at the focus (orange). Earth's orbit is the grey circle at 1 AU. The red dot marks the object's position at the catalog epoch.
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 size
Similar orbit
Keep exploring
Explore asteroids, comets and near-Earth objects with JPL orbital data.