Honda

Eccentricity · e

1.0

Orbit and dynamics

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 127.9° carries it well above and below the ecliptic plane.

Size and surface

Neither a measured diameter nor a reliable absolute magnitude is available for Honda, so its physical size remains unconstrained.

Observation record and orbit quality

The current orbit solution is based on 35 observations and has a weighted RMS residual of 0.5142 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

Semi-Major Axis

— AU

Eccentricity

1.0

Perihelion

1.099 AU

Aphelion

— AU

Inclination

127.91°

Orbital Period

— yr

Epoch

2440151.5

Mean Anomaly

—°

Close approaches

No close approaches to Earth are currently on record for this object.

Physical Parameters

Diameter

— km

Albedo

—

Density

— g/cm³

Rotation Period

— h

Absolute Magnitude

—

Orbit Quality

RMS

0.51422

Condition

—

Orbit ID

—

Data source: NASA JPL Small-Body Database . 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.

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