However, Bauersfelda turns out to be a non-family asteroid from the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.
[4] Bauersfelda orbits the Sun in the outer main-belt at a distance of 2.6–3.2 AU once every 4 years and 11 months (1,810 days).
[1] It is also characterized as a S-type by PanSTARRS photometric survey,[8] which agrees with the Koronis family's overall spectral type.
In August 2012, a rotational lightcurve of this asteroid was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California.
[5][6] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 and calculates a diameter of 11.48 kilometers based on an absolute magnitude of 11.87.