Lightcurve Determination of 3151 Talbot and 4666 Dietz
Abstract
CCD photometry observations of 3151 Talbot and 4666 Dietz were obtained at the Bigmuskie Observatory, Italy, during 2011 June and July. Analysis found a rotation period of 19.49 ± 0.01 h for 3151 Talbot and a period of 2.953 ± 0.003 h for 4666 Dietz.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2011
- Bibcode:
- 2011MPBu...38..223F