A Determination of the Rotational Period of 8882 Sakaetamura
Abstract
CCD Observations of 8882 Sakaetamura were taken on nine nights between 2012 Jan 7 and 29. Analysis of the data found a synodic period of 4.874 ± 0.002 h with a lightcurve amplitude of 0.60 ± 0.1.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2012
- Bibcode:
- 2012MPBu...39..206W