Mikeanderson is a member the Eos family (606),[3] the largest asteroid family in the outer asteroid belt consisting of nearly 10,000 asteroids. It orbits the Sun in the outer main-belt at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,903 days; semi-major axis of 3.01 AU). Its orbit has an eccentricity of 0.11 and an inclination of 10° with respect to the ecliptic.[1]
The body's observation arc begins with a precovery taken at Palomar Observatory in October 1960, more than 40 years prior to its official discovery observation.[5]
Physical characteristics
The asteroid's spectral type is unknown. Typically, members of the Eos family are K-type asteroids. Mikeanderson's measured albedo also agrees with this spectral classification (see below).[6]: 23
Rotation period
As of 2017, no rotational lightcurve of Mikeanderson has been obtained from photometric observations. The asteroid's rotation period, poles and shape remain unknown.[1][7]