Rotation Period Determination for 4149 Harrison and (5633) 1978 UL7
Abstract
Analysis of photometric observations of two main-belt asteroids were performed by the authors in Italy from 2015 April to June. Assuming bimodal lightcurves, the synodic periods were: 4149 Harrison, P = 3.956 ± 0.001 h and (5633) 1978 UL7 P = 7.212 ± 0.001 h.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2015
- Bibcode:
- 2015MPBu...42..281P