Lightcurve Inversion for 65 Cybele
Abstract
We present a shape and spin axis model for main-belt asteroid 65 Cybele. The model was obtained with lightcurve inversion process, using combined dense photometric data obtained during fifteen apparitions from 1977 to 2014 and sparse data from USNO Flagstaff. Analysis of the resulting data found a sidereal period P = 6.081434 ± 0.000005 hours and two possible pole solutions: (l = 208°, b = -7°) and (l = 27°, b = -14°) with an error of ±15 degrees.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- July 2015
- Bibcode:
- 2015MPBu...42..204F