Lightcurve Analysis of 758 Mancunia
Abstract
Analysis of observations made independently by Warner and Behrend/ Poncy/Coliac of the main-belt asteroid 758 Mancunia indicted a period of approximately 12.7 hr. The combined data set allowed refinement of the analysis and revealed a lightcurve with a period of 12.7253 ± 0.0006 hr and amplitude of 0.26 ± 0.02 mag.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- March 2008
- Bibcode:
- 2008MPBu...35...25W