58 Concordia is a fairly largemain-beltasteroid that is orbiting the Sun with aperiod of 4.44 years, asemimajor axis of2.7 AU, and a loweccentricity of 0.043. It isclassified as aC-type asteroid, meaning that its surface is very dark and it is likelycarbonaceous in composition. The surface spectra displays indications ofhydrated minerals created through aqueous alteration.[5] The object is rotating with asidereal period of9.894541 h and pole orientations of (15.3°±0.7°,−4.2°±2.6°) and (195.9°±1.0°,4.8°±1.2°).[6] It belongs to theNemesis family of asteroids.
^Pilcher, Frederick (October 2016), "Rotation Determinations for 50 Virginia, 58 Concordia 307 Nike, and 339 Dorothea",The Minor Planet Bulletin,43 (4):304–306,Bibcode:2016MPBu...43..304P.
^Jiang, P. F.; Wang, X. B. (September 2018), "Photometric Study on Asteroid (58) Concordia",Acta Astronomica Sinica,59 (5): 46,Bibcode:2018AcASn..59...46J, 46.