The asteroid was first observed asA916 KA at Simeiz in May 1916. The body'sobservation arc begins as1920 HA atHeidelberg Observatory in April 1920, or more than 5 years prior to its official discovery observation at Simeiz.[1]
Mussorgskia has been characterized as a commonX-type asteroid by Pan-STARRS' photometric survey. It is also characterized as a carbonaceousC-type asteroid in theSDSS-MFB (Masi Foglia Binzel) taxonomy.[4][a]
In May 2002, two rotationallightcurves ofMussorgskia were obtained fromphotometric observations by Stephen Brincat at theFlarestar Observatory in Malta and by French amateur astronomerRené Roy. Lightcurve analysis gave arotation period of 5.519 and 5.6362 hours with a brightness amplitude of 0.20 and 0.21magnitude, respectively (U=2/3).[10][11] TheCollaborative Asteroid Lightcurve Link adopts a period of 5.636 hours and a brightness variation between 0.2 and 0.21 magnitude (U=3).[4]
CALL assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a larger diameter of 36.78 kilometers based on anabsolute magnitude of 10.9.[4]
^abcSearch for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog (publication).SDSS-MFB (Masi Foglia Binzel) taxonomy (catalog).
^Schmadel, Lutz D. (2009). "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.