2016 MB1
2016 MB1 belongs to the Apollo group of near-Earth asteroids, whose orbits cross the path of Earth; with a semi-major axis of 1.172 AU it takes 1.27 yr to circle the Sun.
Orbit and dynamics
Between its closest point (0.594 AU) and its farthest (1.75 AU), the heliocentric distance changes by 1.156 AU over every revolution.
One full revolution takes 1.27 yr (463 days), computed from the semi-major axis of 1.172 AU.
The high eccentricity (0.493) produces a strongly elongated orbit, so the object spends most of its time far from the Sun.
A steep inclination of 53.26° carries it well above and below the ecliptic plane.
By the vis-viva equation its orbital speed rises to 47.2 km/s at perihelion and falls to 16 km/s at aphelion.
Because q < 1 AU and Q > 1 AU, this orbit geometrically intersects the region of Earth's orbit.
Size and surface
No direct size measurement is available; from an absolute magnitude of H = 19.86 and an assumed geometric albedo of 0.14, the diameter works out to roughly 0.38 km.
Observation record and orbit quality
Astrometry from 46 individual observations underpins this orbit; the fit leaves an RMS residual of 0.5202 arcseconds.
Condition code U = 1 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.
