In March 1984, the first but poorly rated rotational
lightcurve of
Summa was obtained from photometric observations by American astronomer
Richard Binzel. It gave a
rotation period of 9.66 hours with a brightness amplitude of 0.14
magnitude (). In August 2012, a refined yet ambiguous lightcurve with a period of 6.855 hours and an amplitude of 0.13 was obtained by Larry E. Owings at the Barnes Ridge Observatory in California (). Lightcurve analysis also considered that
Summa might be a
binary system. One month later, the so-far best rated lightcurve from British astronomer Kevin Hills using the remote controlled Riverland Dingo Observatory in Australia, gave a period of 6.8549 hours with a brightness amplitude of 0.18 (). == Diameter an albedo ==