Rotation Period Determination for 5401 Minamioda
Abstract
Photometric observations of the main-belt asteroid 5401 Minamioda in 2015 November revealed a monomodal lightcurve phased to 3.949 ± 0.001 hours as the more likely solution for the synodic rotation period of the asteroid, although a bimodal solution phased to 7.897 ± 0.003 hours cannot be ruled out completely.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- April 2016
- Bibcode:
- 2016MPBu...43..188M