From 23 February until 2 March 2006,photometric measurements were taken of the asteroid. These were used to produce alight curve showing arotation period of7.80±0.02 h with a brightness variation of0.16±0.03 inmagnitude. This result is consistent with some, but not all previous results. Some studies had suggested a longer rotation period of15.959 h; double the time measured. However, the new data is inconsistent with the longer period.[4]
In May 1979, 268 Adorea was positioned in proximity of the galaxyNGC 4517 and as a bright new light source it was identified as a potentialsupernova. However, the light was missing from a second photographic plate taken ten days later, and the source was soon identified as the asteroid.[5]
The name refers toadorea liba, theLatin name forspelt cakes produced from meal and salt offered by the Romans as a sacrifice; the name was controversial among astronomers, as all previous asteroids had been named for humans or mythological figures.[6][7]
^Stephens, Robert D. (December 2006). "Asteroid lightcurve photometry from Santana and GMARS observatories - winter and spring 2006".Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers.33 (4):100–101.Bibcode:2006MPBu...33..100S.
^West, R. (September 1979). "The Supernova that was not - 268 Adorea".The Messenger (18): 14.Bibcode:1979Msngr..18...14W.