Mozartia orbits the Sun in the inner main-belt at a distance of 1.7–2.9 AU once every 3 years and 6 months (1,268 days). Its orbit has an eccentricity of 0.26 and an inclination of 4° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation in 1924.[6]
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Mozartia measures 7.919 kilometers in diameter and its surface has an albedo of 0.250.[5]
Lightcurves
As of 2017, no rotational lightcurve of Mozartia has been obtained. The body's rotation period and shape remain unknown.[1][7]
^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN978-3-642-01964-7.