Rotation Period Determination for 671 Carnegia
Abstract
Analysis of photometric observations of the main-belt asteroid 671 Carnegia from 2014 January-March revealed a bimodal lightcurve with a period of 8.332 ± 0.001 hours as the most likely solution. However, a trimodal solution of 12.50 hours still could not be formally ruled out.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2014
- Bibcode:
- 2014MPBu...41..261B