Lightcurve and Rotation Period Determination for 4678 Ninian
Abstract
Photometric observations of the main-belt asteroid 4678 Ninian performed by the authors in Italy and Ireland in 2014 October and November revealed the bimodal light curve phased to 56.72 ± 0.01 hours as the most likely solution representing the synodic rotation rate for this asteroid.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- July 2015
- Bibcode:
- 2015MPBu...42..215S