SpaceAtlas Space Object Data
LINEAR
NASA JPL SBDB · 1998 VS24

LINEAR

LINEAR follows a distinctly cometary orbit: an eccentricity of 0.244 carries it from 3.405 AU at perihelion out to 5.603 AU at aphelion.

comet Observations: 48
Encyclopedia excerpt
The Lincoln Near-Earth Asteroid Research (LINEAR) project is a collaboration of the United States Air Force, NASA, and the Massachusetts Institute of Technology's Lincoln Laboratory for the systematic detection and tracking of near-Earth objects. LINEAR was responsible for the majority of asteroid discoveries from 1998 until it was overtaken by the Catalina Sky Survey in 2005. As of 15 September 2011, LINEAR had detected 231,082 new small Solar System bodies, of which at least 2,423 were near-Earth asteroids and 279 were comets. The instruments used by the LINEAR program are located at Lincoln Laboratory's Experimental Test Site (ETS) on the White Sands Missile Range (WSMR) near Socorro, New Mexico.
Orbital Period · P
9.56 yr
v(q)
18 km/s
v(Q)
10.9 km/s
TJ
2.95
Eccentricity · e
0.2439

Orbit and dynamics

Between its closest point (3.405 AU) and its farthest (5.603 AU), the heliocentric distance changes by 2.198 AU over every revolution.

One full revolution takes 9.56 yr (3,491 days), computed from the semi-major axis of 4.504 AU.

An eccentricity of 0.244 makes the orbit moderately elongated.

The orbital plane is tilted 5.03° relative to the ecliptic.

By the vis-viva equation its orbital speed rises to 18 km/s at perihelion and falls to 10.9 km/s at aphelion.

Its Tisserand parameter with respect to Jupiter is T_J = 2.95, a standard discriminator between asteroidal and cometary dynamics.

Size and surface

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

Observation record and orbit quality

Astrometry from 48 individual observations underpins this orbit; the fit leaves an RMS residual of 0.5138 arcseconds.

Condition code U = 5 indicates a moderately constrained orbit; predictions decades ahead still carry noticeable uncertainty.

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
4.504 AU
Eccentricity
0.2439
Perihelion
3.405 AU
Aphelion
5.602526 AU
Inclination
5.03°
Orbital Period
— yr
Epoch
2451149.5
Mean Anomaly
2.96°

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

Diameter
— km
Albedo
—
Density
— g/cm³
Rotation Period
— h
Absolute Magnitude
—

Orbit Quality

RMS
0.51384
Condition
5
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.

Keep exploring

Explore asteroids, comets and near-Earth objects with JPL orbital data.